The following information is also available:
Time column is TIME ORDERED-> Determining observation start and end
Offset of 153175090.419100 from 1993-01-01 00:00:00 is date and time (including leapseconds) = 1997-11-08 20:38:06.41909 Modified Julian Day = 50760.859796517361247-> leapsec.fits already present in current directory
Offset of 153201042.336900 from 1993-01-01 00:00:00 is date and time (including leapseconds) = 1997-11-09 03:50:38.33690 Modified Julian Day = 50761.160165936344129-> Observation begins 153175090.4191 1997-11-08 20:38:06
ATTITUDE_V0.9j
reading attitude file:./merged.tmp
open asc output file:out.tmp
AVERAGE ASPECT AND OFFSET FOR THIS ATTITUDE FILE:
Attitude file start and stop ascatime : 153175090.419000 153201042.336900
Data file start and stop ascatime : 153175090.419000 153201042.336900
Aspecting run start and stop ascatime : 153175090.419093 153201042.336828
Time interval averaged over (seconds) : 25951.917735
Total pointing and manuver time (sec) : 15584.483398 10367.477539
Mean boresight Euler angles : 296.685359 65.155080 192.174421
RA DEC SUN ANGLE
Mean solar position (deg) : 223.16 -16.52
Mean aberration (arcsec) : -7.92 12.87
Mean sat X-axis (deg) : 143.864384 62.503614 99.79
Mean sat Y-axis (deg) : 211.864846 -11.032767 12.26
Mean sat Z-axis (deg) : 296.685359 24.844921 82.69
RA DEC ROLL OFFSET
(deg) (deg) (deg) (arcmin)
Average 296.445557 24.662233 102.264328 1.254106
Minimum 296.443604 24.659649 102.013405 0.014505
Maximum 296.663849 25.023891 102.278931 24.741486
Sigma (RMS) 0.001626 0.000593 0.034569 3.805211
Number of ASPECT records processed = 12808
Aspecting to RA/DEC : 296.44555664 24.66223335
closing output file...
closing attitude file...
-> Standard Output From STOOL checkatt:
Opening file: ./out.tmp
***************** Observation Info ******************
RA (J2000 deg): 296.446 DEC: 24.662
START TIME: SC 153175090.4191 = UT 1997-11-08 20:38:10
****** Definition of Attitude SENSOR Bit Flags ******
Sensors used in the attitude determination and attitude control mode
1: USED, 0: NOT USED
B0:STT-A, B1:STT-B, B2:NSAS, B3:GAS, B4:SSAS-SA, B5:SSAS-SB,
B6:IRU-X, B7:IRU-Y, B8:IRU-Z, B9:IRU-S1, B10:IRU-S2,
B11: Attitude control mode 1: coarse, 0: fine
B12: Sun presence 1: day, 0: night
B13: STT-A earth occultation 1: earth occultation, 0: no occultation
B14: STT-B earth occultation 1: earth occultation, 0: no occultation
B16,17,18: STT-A track stars no.1,2,3, 1: USED, 0: NOT USED
B19,20,21: STT-B track stars no.1,2,3, 1: USED, 0: NOT USED
B22,23: always 0
******** Attitude File Reconstruction Summary *******
S S N G S S I I I I I A S S S S S
T T S A S S R R R R R C U T T T T
T T A S A A U U U U U M N T T T T
- - S . A A - - - - - . . - - - -
A B . . - - X Y Z S S . . A B A B
. . . . S S . . . 1 2 . . O O S S
offset_time separation sensor . . . . A B . . . . . . . C C T T
(sec) (arcmin) . . . . . . . . . . . . . C C R R
BIT: 0 1 2 3 4 5 6 7 8 9 A B C D E
0.500110 16.709 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
276.499207 15.708 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
295.999176 14.686 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
314.499146 13.661 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
329.999115 12.653 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
346.998962 11.631 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
362.998962 10.614 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
380.998779 9.595 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
398.998779 8.579 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
419.498718 7.567 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
441.498718 6.566 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
466.998596 5.559 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
497.498627 4.553 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
535.498291 3.550 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
586.498230 2.542 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
661.998047 1.538 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
828.497498 0.538 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
1563.995239 0.063 8403 1 1 0 0 0 0 0 0 0 0 1 0 0 0 0 0 0
5083.984375 0.084 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
7323.977051 0.121 1C8443 1 1 0 0 0 0 1 0 0 0 1 0 0 0 0 4 3
10843.965820 0.162 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
13083.958984 0.065 1C8443 1 1 0 0 0 0 1 0 0 0 1 0 0 0 0 4 3
16603.947266 0.056 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
18779.941406 0.067 1C8443 1 1 0 0 0 0 1 0 0 0 1 0 0 0 0 4 3
22315.929688 0.079 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0
24539.921875 0.162 1C8443 1 1 0 0 0 0 1 0 0 0 1 0 0 0 0 4 3
25951.917969 24.741 9603 1 1 0 0 0 0 0 0 0 1 1 0 1 0 0 0 0
Attitude Records: 12808
Attitude Steps: 27
Maneuver ACM time: 10367.49 sec
Pointed ACM time: 15584.5 sec
-> Calculating aspect point90 125 count=182 sum1=53997.1 sum2=11856.9 sum3=34975.2 90 126 count=10401 sum1=3.08583e+06 sum2=677677 sum3=1.9988e+06 91 122 count=14 sum1=4153.77 sum2=911.661 sum3=2690.18 91 123 count=111 sum1=32933.2 sum2=7228.89 sum3=21329.8 91 124 count=146 sum1=43317.1 sum2=9509.76 sum3=28056.1 91 125 count=157 sum1=46580.3 sum2=10227.4 sum3=30170.4 91 126 count=599 sum1=177717 sum2=39028.2 sum3=115112 92 120 count=38 sum1=11274.8 sum2=2473.69 sum3=7301.47 92 121 count=62 sum1=18395.6 sum2=4036.55 sum3=11913.2 92 122 count=55 sum1=16318.5 sum2=3581.29 sum3=10568.4 93 117 count=24 sum1=7121.21 sum2=1561.61 sum3=4611.05 93 118 count=38 sum1=11275.1 sum2=2472.87 sum3=7301.02 93 119 count=40 sum1=11868.4 sum2=2603.41 sum3=7685.49 93 120 count=18 sum1=5340.75 sum2=1171.65 sum3=3458.54 94 114 count=5 sum1=1483.64 sum2=325.193 sum3=960.553 94 115 count=31 sum1=9198.5 sum2=2016.4 sum3=5955.55 94 116 count=28 sum1=8308.21 sum2=1821.54 sum3=5379.37 94 117 count=14 sum1=4154.07 sum2=910.863 sum3=2689.74 95 112 count=19 sum1=5638 sum2=1235.32 sum3=3649.85 95 113 count=23 sum1=6824.87 sum2=1495.58 sum3=4418.36 95 114 count=21 sum1=6231.33 sum2=1365.71 sum3=4034.26 96 109 count=6 sum1=1780.49 sum2=389.934 sum3=1152.48 96 110 count=23 sum1=6825.14 sum2=1494.9 sum3=4417.94 96 111 count=21 sum1=6231.57 sum2=1365.11 sum3=4033.89 96 112 count=6 sum1=1780.43 sum2=390.066 sum3=1152.56 97 98 count=14 sum1=4154.56 sum2=908.299 sum3=2688.78 97 99 count=1 sum1=296.758 sum2=64.881 sum3=192.051 97 107 count=16 sum1=4748.11 sum2=1039.47 sum3=3073.05 97 108 count=20 sum1=5935.07 sum2=1299.5 sum3=3841.42 97 109 count=15 sum1=4451.25 sum2=974.754 sum3=2881.15 98 99 count=33 sum1=9793.25 sum2=2141.15 sum3=6337.33 98 104 count=3 sum1=890.304 sum2=194.82 sum3=576.144 98 105 count=19 sum1=5638.56 sum2=1233.95 sum3=3648.97 98 106 count=20 sum1=5935.24 sum2=1299.1 sum3=3841.15 98 107 count=6 sum1=1780.56 sum2=389.772 sum3=1152.37 99 99 count=134 sum1=39767.6 sum2=8694.77 sum3=25731.7 99 102 count=1 sum1=296.777 sum2=64.919 sum3=192.032 99 103 count=19 sum1=5638.73 sum2=1233.57 sum3=3648.67 99 104 count=25 sum1=7419.27 sum2=1623.36 sum3=4801.07 100 99 count=126 sum1=37394.4 sum2=8175.96 sum3=24194.6 100 100 count=176 sum1=52234.4 sum2=11420.8 sum3=33794.5 100 101 count=30 sum1=8903.49 sum2=1947.18 sum3=5760.65 100 102 count=22 sum1=6529.15 sum2=1428.12 sum3=4224.64 101 100 count=45 sum1=13355.5 sum2=2920.1 sum3=8640.52 112 90 count=1 sum1=296.905 sum2=64.794 sum3=191.911 0 out of 12808 points outside bin structure-> Euler angles: 296.686, 65.1548, 192.174
Interpolating 40 records in time interval 153201018.337 - 153201042.337
Dropped 1st C2 read after clocking change in ft971108_2038_0350S100201H.fits Dropped 1st C3 read after clocking change in ft971108_2038_0350S100201H.fits Dropped 1st C0 read after clocking change in ft971108_2038_0350S100201H.fits Dropped 1st C1 read after clocking change in ft971108_2038_0350S100201H.fits Dropped 1st C1 read after clocking change in ft971108_2038_0350S100401H.fits Dropping SF 1383 with synch code word 1 = 195 not 243 Dropping SF 1384 with inconsistent datamode 0/31 639.998 second gap between superframes 1518 and 1519 Dropped 1st C3 read after clocking change in ft971108_2038_0350S000901H.fits Dropped 1st C0 read after clocking change in ft971108_2038_0350S000901H.fits Dropped 1st C1 read after clocking change in ft971108_2038_0350S001101H.fits 3212 of 3214 super frames processed-> Removing the following files with NEVENTS=0
ft971108_2038_0350G200170H.fits[0] ft971108_2038_0350G201170H.fits[0] ft971108_2038_0350G201270H.fits[0] ft971108_2038_0350G202470L.fits[0] ft971108_2038_0350G202570L.fits[0] ft971108_2038_0350G203270M.fits[0] ft971108_2038_0350G203370L.fits[0] ft971108_2038_0350G203470L.fits[0] ft971108_2038_0350G204170M.fits[0] ft971108_2038_0350G300170H.fits[0] ft971108_2038_0350G300270H.fits[0] ft971108_2038_0350G300370H.fits[0] ft971108_2038_0350G301270H.fits[0] ft971108_2038_0350G302370M.fits[0] ft971108_2038_0350G302470M.fits[0] ft971108_2038_0350G302570L.fits[0] ft971108_2038_0350G302670L.fits[0] ft971108_2038_0350G303470M.fits[0] ft971108_2038_0350G303570L.fits[0] ft971108_2038_0350G303670L.fits[0] ft971108_2038_0350G304370M.fits[0] ft971108_2038_0350G304470M.fits[0] ft971108_2038_0350S002101L.fits[0] ft971108_2038_0350S102101L.fits[0]-> Checking for empty GTI extensions
ft971108_2038_0350S000101H.fits[2] ft971108_2038_0350S000201H.fits[2] ft971108_2038_0350S000301L.fits[2] ft971108_2038_0350S000401H.fits[2] ft971108_2038_0350S000501L.fits[2] ft971108_2038_0350S000601L.fits[2] ft971108_2038_0350S000701L.fits[2] ft971108_2038_0350S000801H.fits[2] ft971108_2038_0350S000901H.fits[2] ft971108_2038_0350S001001H.fits[2] ft971108_2038_0350S001101H.fits[2] ft971108_2038_0350S001201L.fits[2] ft971108_2038_0350S001301M.fits[2] ft971108_2038_0350S001401H.fits[2] ft971108_2038_0350S001501M.fits[2] ft971108_2038_0350S001601L.fits[2] ft971108_2038_0350S001701L.fits[2] ft971108_2038_0350S001801L.fits[2] ft971108_2038_0350S001901M.fits[2] ft971108_2038_0350S002001L.fits[2] ft971108_2038_0350S002201L.fits[2] ft971108_2038_0350S002301M.fits[2] ft971108_2038_0350S002401L.fits[2] ft971108_2038_0350S002501M.fits[2]-> Merging GTIs from the following files:
ft971108_2038_0350S100101H.fits[2] ft971108_2038_0350S100201H.fits[2] ft971108_2038_0350S100301H.fits[2] ft971108_2038_0350S100401H.fits[2] ft971108_2038_0350S100501L.fits[2] ft971108_2038_0350S100601H.fits[2] ft971108_2038_0350S100701L.fits[2] ft971108_2038_0350S100801L.fits[2] ft971108_2038_0350S100901L.fits[2] ft971108_2038_0350S101001H.fits[2] ft971108_2038_0350S101101H.fits[2] ft971108_2038_0350S101201L.fits[2] ft971108_2038_0350S101301M.fits[2] ft971108_2038_0350S101401H.fits[2] ft971108_2038_0350S101501M.fits[2] ft971108_2038_0350S101601L.fits[2] ft971108_2038_0350S101701L.fits[2] ft971108_2038_0350S101801L.fits[2] ft971108_2038_0350S101901M.fits[2] ft971108_2038_0350S102001L.fits[2] ft971108_2038_0350S102201L.fits[2] ft971108_2038_0350S102301M.fits[2] ft971108_2038_0350S102401L.fits[2] ft971108_2038_0350S102501M.fits[2]-> Merging GTIs from the following files:
ft971108_2038_0350G200270H.fits[2] ft971108_2038_0350G200370H.fits[2] ft971108_2038_0350G200470H.fits[2] ft971108_2038_0350G200570H.fits[2] ft971108_2038_0350G200670L.fits[2] ft971108_2038_0350G200770H.fits[2] ft971108_2038_0350G200870H.fits[2] ft971108_2038_0350G200970H.fits[2] ft971108_2038_0350G201070H.fits[2] ft971108_2038_0350G201370L.fits[2] ft971108_2038_0350G201470L.fits[2] ft971108_2038_0350G201570H.fits[2] ft971108_2038_0350G201670L.fits[2] ft971108_2038_0350G201770M.fits[2] ft971108_2038_0350G201870M.fits[2] ft971108_2038_0350G201970M.fits[2] ft971108_2038_0350G202070M.fits[2] ft971108_2038_0350G202170H.fits[2] ft971108_2038_0350G202270M.fits[2] ft971108_2038_0350G202370M.fits[2] ft971108_2038_0350G202670L.fits[2] ft971108_2038_0350G202770L.fits[2] ft971108_2038_0350G202870M.fits[2] ft971108_2038_0350G202970M.fits[2] ft971108_2038_0350G203070M.fits[2] ft971108_2038_0350G203170M.fits[2] ft971108_2038_0350G203570L.fits[2] ft971108_2038_0350G203670L.fits[2] ft971108_2038_0350G203770M.fits[2] ft971108_2038_0350G203870M.fits[2] ft971108_2038_0350G203970M.fits[2] ft971108_2038_0350G204070M.fits[2] ft971108_2038_0350G204270L.fits[2] ft971108_2038_0350G204370L.fits[2] ft971108_2038_0350G204470M.fits[2] ft971108_2038_0350G204570M.fits[2] ft971108_2038_0350G204670M.fits[2] ft971108_2038_0350G204770M.fits[2]-> Merging GTIs from the following files:
ft971108_2038_0350G300470H.fits[2] ft971108_2038_0350G300570H.fits[2] ft971108_2038_0350G300670L.fits[2] ft971108_2038_0350G300770H.fits[2] ft971108_2038_0350G300870H.fits[2] ft971108_2038_0350G300970H.fits[2] ft971108_2038_0350G301070H.fits[2] ft971108_2038_0350G301170H.fits[2] ft971108_2038_0350G301370L.fits[2] ft971108_2038_0350G301470L.fits[2] ft971108_2038_0350G301570H.fits[2] ft971108_2038_0350G301670L.fits[2] ft971108_2038_0350G301770M.fits[2] ft971108_2038_0350G301870M.fits[2] ft971108_2038_0350G301970M.fits[2] ft971108_2038_0350G302070M.fits[2] ft971108_2038_0350G302170H.fits[2] ft971108_2038_0350G302270M.fits[2] ft971108_2038_0350G302770L.fits[2] ft971108_2038_0350G302870L.fits[2] ft971108_2038_0350G302970M.fits[2] ft971108_2038_0350G303070M.fits[2] ft971108_2038_0350G303170M.fits[2] ft971108_2038_0350G303270M.fits[2] ft971108_2038_0350G303370M.fits[2] ft971108_2038_0350G303770L.fits[2] ft971108_2038_0350G303870L.fits[2] ft971108_2038_0350G303970M.fits[2] ft971108_2038_0350G304070M.fits[2] ft971108_2038_0350G304170M.fits[2] ft971108_2038_0350G304270M.fits[2] ft971108_2038_0350G304570L.fits[2] ft971108_2038_0350G304670L.fits[2] ft971108_2038_0350G304770M.fits[2] ft971108_2038_0350G304870M.fits[2] ft971108_2038_0350G304970M.fits[2] ft971108_2038_0350G305070M.fits[2]
GISSORTCODE:LO:Start program GISSORTCODE:LO:End program-> Standard Error Output From STOOL gissortsplit:
GISSORTSPLIT:LO:Start program GISSORTSPLIT:LO:g200170h.prelist merge count = 1 photon cnt = 1 GISSORTSPLIT:LO:g200270h.prelist merge count = 1 photon cnt = 3 GISSORTSPLIT:LO:g200370h.prelist merge count = 1 photon cnt = 2 GISSORTSPLIT:LO:g200470h.prelist merge count = 4 photon cnt = 3442 GISSORTSPLIT:LO:g200570h.prelist merge count = 1 photon cnt = 2 GISSORTSPLIT:LO:g200670h.prelist merge count = 1 photon cnt = 2 GISSORTSPLIT:LO:g200770h.prelist merge count = 1 photon cnt = 1 GISSORTSPLIT:LO:g200170l.prelist merge count = 1 photon cnt = 11 GISSORTSPLIT:LO:g200270l.prelist merge count = 3 photon cnt = 112 GISSORTSPLIT:LO:g200370l.prelist merge count = 6 photon cnt = 5382 GISSORTSPLIT:LO:g200170m.prelist merge count = 1 photon cnt = 1 GISSORTSPLIT:LO:g200270m.prelist merge count = 5 photon cnt = 6571 GISSORTSPLIT:LO:g200370m.prelist merge count = 4 photon cnt = 64 GISSORTSPLIT:LO:g200470m.prelist merge count = 1 photon cnt = 24 GISSORTSPLIT:LO:g200570m.prelist merge count = 1 photon cnt = 18 GISSORTSPLIT:LO:g200670m.prelist merge count = 1 photon cnt = 20 GISSORTSPLIT:LO:g200770m.prelist merge count = 1 photon cnt = 16 GISSORTSPLIT:LO:g200870m.prelist merge count = 1 photon cnt = 35 GISSORTSPLIT:LO:g200970m.prelist merge count = 1 photon cnt = 29 GISSORTSPLIT:LO:g201070m.prelist merge count = 1 photon cnt = 10 GISSORTSPLIT:LO:g201170m.prelist merge count = 1 photon cnt = 8 GISSORTSPLIT:LO:Total filenames split = 38 GISSORTSPLIT:LO:Total split file cnt = 21 GISSORTSPLIT:LO:End program-> Creating ad55014000g200170m.unf
---- cmerge: version 1.6 ---- A total of 5 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971108_2038_0350G202070M.fits 2 -- ft971108_2038_0350G202270M.fits 3 -- ft971108_2038_0350G203170M.fits 4 -- ft971108_2038_0350G204070M.fits 5 -- ft971108_2038_0350G204770M.fits Merging binary extension #: 2 1 -- ft971108_2038_0350G202070M.fits 2 -- ft971108_2038_0350G202270M.fits 3 -- ft971108_2038_0350G203170M.fits 4 -- ft971108_2038_0350G204070M.fits 5 -- ft971108_2038_0350G204770M.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad55014000g200270l.unf
---- cmerge: version 1.6 ---- A total of 6 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971108_2038_0350G200670L.fits 2 -- ft971108_2038_0350G201470L.fits 3 -- ft971108_2038_0350G201670L.fits 4 -- ft971108_2038_0350G202770L.fits 5 -- ft971108_2038_0350G203670L.fits 6 -- ft971108_2038_0350G204370L.fits Merging binary extension #: 2 1 -- ft971108_2038_0350G200670L.fits 2 -- ft971108_2038_0350G201470L.fits 3 -- ft971108_2038_0350G201670L.fits 4 -- ft971108_2038_0350G202770L.fits 5 -- ft971108_2038_0350G203670L.fits 6 -- ft971108_2038_0350G204370L.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad55014000g200370h.unf
---- cmerge: version 1.6 ---- A total of 4 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971108_2038_0350G200570H.fits 2 -- ft971108_2038_0350G201070H.fits 3 -- ft971108_2038_0350G201570H.fits 4 -- ft971108_2038_0350G202170H.fits Merging binary extension #: 2 1 -- ft971108_2038_0350G200570H.fits 2 -- ft971108_2038_0350G201070H.fits 3 -- ft971108_2038_0350G201570H.fits 4 -- ft971108_2038_0350G202170H.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Ignoring the following files containing 000000112 events
ft971108_2038_0350G202670L.fits ft971108_2038_0350G203570L.fits ft971108_2038_0350G204270L.fits-> Ignoring the following files containing 000000064 events
ft971108_2038_0350G201970M.fits ft971108_2038_0350G203070M.fits ft971108_2038_0350G203970M.fits ft971108_2038_0350G204670M.fits-> Ignoring the following files containing 000000035 events
ft971108_2038_0350G202870M.fits-> Ignoring the following files containing 000000029 events
ft971108_2038_0350G202970M.fits-> Ignoring the following files containing 000000024 events
ft971108_2038_0350G204470M.fits-> Ignoring the following files containing 000000020 events
ft971108_2038_0350G203770M.fits-> Ignoring the following files containing 000000018 events
ft971108_2038_0350G204570M.fits-> Ignoring the following files containing 000000016 events
ft971108_2038_0350G203870M.fits-> Ignoring the following files containing 000000011 events
ft971108_2038_0350G201370L.fits-> Ignoring the following files containing 000000010 events
ft971108_2038_0350G201770M.fits-> Ignoring the following files containing 000000008 events
ft971108_2038_0350G201870M.fits-> Ignoring the following files containing 000000003 events
ft971108_2038_0350G200370H.fits-> Ignoring the following files containing 000000002 events
ft971108_2038_0350G200770H.fits-> Ignoring the following files containing 000000002 events
ft971108_2038_0350G200970H.fits-> Ignoring the following files containing 000000002 events
ft971108_2038_0350G200470H.fits-> Ignoring the following files containing 000000001 events
ft971108_2038_0350G200870H.fits-> Ignoring the following files containing 000000001 events
ft971108_2038_0350G202370M.fits-> Ignoring the following files containing 000000001 events
ft971108_2038_0350G200270H.fits-> Collecting GIS3 event files by mode
GISSORTCODE:LO:Start program GISSORTCODE:LO:End program-> Standard Error Output From STOOL gissortsplit:
GISSORTSPLIT:LO:Start program GISSORTSPLIT:LO:g300170h.prelist merge count = 1 photon cnt = 1 GISSORTSPLIT:LO:g300270h.prelist merge count = 1 photon cnt = 1 GISSORTSPLIT:LO:g300370h.prelist merge count = 4 photon cnt = 3122 GISSORTSPLIT:LO:g300470h.prelist merge count = 1 photon cnt = 1 GISSORTSPLIT:LO:g300570h.prelist merge count = 1 photon cnt = 1 GISSORTSPLIT:LO:g300670h.prelist merge count = 1 photon cnt = 2 GISSORTSPLIT:LO:g300170l.prelist merge count = 1 photon cnt = 10 GISSORTSPLIT:LO:g300270l.prelist merge count = 3 photon cnt = 90 GISSORTSPLIT:LO:g300370l.prelist merge count = 6 photon cnt = 4845 GISSORTSPLIT:LO:g300170m.prelist merge count = 1 photon cnt = 1 GISSORTSPLIT:LO:g300270m.prelist merge count = 5 photon cnt = 6207 GISSORTSPLIT:LO:g300370m.prelist merge count = 4 photon cnt = 67 GISSORTSPLIT:LO:g300470m.prelist merge count = 1 photon cnt = 20 GISSORTSPLIT:LO:g300570m.prelist merge count = 1 photon cnt = 13 GISSORTSPLIT:LO:g300670m.prelist merge count = 1 photon cnt = 20 GISSORTSPLIT:LO:g300770m.prelist merge count = 1 photon cnt = 26 GISSORTSPLIT:LO:g300870m.prelist merge count = 1 photon cnt = 13 GISSORTSPLIT:LO:g300970m.prelist merge count = 1 photon cnt = 16 GISSORTSPLIT:LO:g301070m.prelist merge count = 1 photon cnt = 49 GISSORTSPLIT:LO:g301170m.prelist merge count = 1 photon cnt = 31 GISSORTSPLIT:LO:Total filenames split = 37 GISSORTSPLIT:LO:Total split file cnt = 20 GISSORTSPLIT:LO:End program-> Creating ad55014000g300170m.unf
---- cmerge: version 1.6 ---- A total of 5 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971108_2038_0350G302070M.fits 2 -- ft971108_2038_0350G302270M.fits 3 -- ft971108_2038_0350G303270M.fits 4 -- ft971108_2038_0350G304270M.fits 5 -- ft971108_2038_0350G305070M.fits Merging binary extension #: 2 1 -- ft971108_2038_0350G302070M.fits 2 -- ft971108_2038_0350G302270M.fits 3 -- ft971108_2038_0350G303270M.fits 4 -- ft971108_2038_0350G304270M.fits 5 -- ft971108_2038_0350G305070M.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad55014000g300270l.unf
---- cmerge: version 1.6 ---- A total of 6 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971108_2038_0350G300670L.fits 2 -- ft971108_2038_0350G301470L.fits 3 -- ft971108_2038_0350G301670L.fits 4 -- ft971108_2038_0350G302870L.fits 5 -- ft971108_2038_0350G303870L.fits 6 -- ft971108_2038_0350G304670L.fits Merging binary extension #: 2 1 -- ft971108_2038_0350G300670L.fits 2 -- ft971108_2038_0350G301470L.fits 3 -- ft971108_2038_0350G301670L.fits 4 -- ft971108_2038_0350G302870L.fits 5 -- ft971108_2038_0350G303870L.fits 6 -- ft971108_2038_0350G304670L.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad55014000g300370h.unf
---- cmerge: version 1.6 ---- A total of 4 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971108_2038_0350G300570H.fits 2 -- ft971108_2038_0350G301070H.fits 3 -- ft971108_2038_0350G301570H.fits 4 -- ft971108_2038_0350G302170H.fits Merging binary extension #: 2 1 -- ft971108_2038_0350G300570H.fits 2 -- ft971108_2038_0350G301070H.fits 3 -- ft971108_2038_0350G301570H.fits 4 -- ft971108_2038_0350G302170H.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Ignoring the following files containing 000000090 events
ft971108_2038_0350G302770L.fits ft971108_2038_0350G303770L.fits ft971108_2038_0350G304570L.fits-> Ignoring the following files containing 000000067 events
ft971108_2038_0350G301970M.fits ft971108_2038_0350G303170M.fits ft971108_2038_0350G304170M.fits ft971108_2038_0350G304970M.fits-> Ignoring the following files containing 000000049 events
ft971108_2038_0350G302970M.fits-> Ignoring the following files containing 000000031 events
ft971108_2038_0350G303070M.fits-> Ignoring the following files containing 000000026 events
ft971108_2038_0350G304070M.fits-> Ignoring the following files containing 000000020 events
ft971108_2038_0350G303970M.fits-> Ignoring the following files containing 000000020 events
ft971108_2038_0350G304770M.fits-> Ignoring the following files containing 000000016 events
ft971108_2038_0350G301870M.fits-> Ignoring the following files containing 000000013 events
ft971108_2038_0350G301770M.fits-> Ignoring the following files containing 000000013 events
ft971108_2038_0350G304870M.fits-> Ignoring the following files containing 000000010 events
ft971108_2038_0350G301370L.fits-> Ignoring the following files containing 000000002 events
ft971108_2038_0350G300870H.fits-> Ignoring the following files containing 000000001 events
ft971108_2038_0350G300770H.fits-> Ignoring the following files containing 000000001 events
ft971108_2038_0350G300970H.fits-> Ignoring the following files containing 000000001 events
ft971108_2038_0350G300470H.fits-> Ignoring the following files containing 000000001 events
ft971108_2038_0350G303370M.fits-> Ignoring the following files containing 000000001 events
ft971108_2038_0350G301170H.fits-> Collecting SIS0 event files by mode
SIS0SORTCODE:LO:Start program SIS0SORTCODE:LO:End program-> Standard Error Output From STOOL sis0sortsplit:
SIS0SORTSPLIT:LO:Start program SIS0SORTSPLIT:LO:s000101h.prelist merge count = 6 photon cnt = 5881 SIS0SORTSPLIT:LO:s000201h.prelist merge count = 2 photon cnt = 4343 SIS0SORTSPLIT:LO:s000301l.prelist merge count = 9 photon cnt = 13167 SIS0SORTSPLIT:LO:s000401l.prelist merge count = 2 photon cnt = 112 SIS0SORTSPLIT:LO:s000501m.prelist merge count = 5 photon cnt = 22596 SIS0SORTSPLIT:LO:Total filenames split = 24 SIS0SORTSPLIT:LO:Total split file cnt = 5 SIS0SORTSPLIT:LO:End program-> Creating ad55014000s000101m.unf
---- cmerge: version 1.6 ---- A total of 5 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971108_2038_0350S001301M.fits 2 -- ft971108_2038_0350S001501M.fits 3 -- ft971108_2038_0350S001901M.fits 4 -- ft971108_2038_0350S002301M.fits 5 -- ft971108_2038_0350S002501M.fits Merging binary extension #: 2 1 -- ft971108_2038_0350S001301M.fits 2 -- ft971108_2038_0350S001501M.fits 3 -- ft971108_2038_0350S001901M.fits 4 -- ft971108_2038_0350S002301M.fits 5 -- ft971108_2038_0350S002501M.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad55014000s000201l.unf
---- cmerge: version 1.6 ---- A total of 9 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971108_2038_0350S000301L.fits 2 -- ft971108_2038_0350S000501L.fits 3 -- ft971108_2038_0350S000701L.fits 4 -- ft971108_2038_0350S001201L.fits 5 -- ft971108_2038_0350S001601L.fits 6 -- ft971108_2038_0350S001801L.fits 7 -- ft971108_2038_0350S002001L.fits 8 -- ft971108_2038_0350S002201L.fits 9 -- ft971108_2038_0350S002401L.fits Merging binary extension #: 2 1 -- ft971108_2038_0350S000301L.fits 2 -- ft971108_2038_0350S000501L.fits 3 -- ft971108_2038_0350S000701L.fits 4 -- ft971108_2038_0350S001201L.fits 5 -- ft971108_2038_0350S001601L.fits 6 -- ft971108_2038_0350S001801L.fits 7 -- ft971108_2038_0350S002001L.fits 8 -- ft971108_2038_0350S002201L.fits 9 -- ft971108_2038_0350S002401L.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad55014000s000301h.unf
---- cmerge: version 1.6 ---- A total of 6 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971108_2038_0350S000101H.fits 2 -- ft971108_2038_0350S000201H.fits 3 -- ft971108_2038_0350S000401H.fits 4 -- ft971108_2038_0350S000801H.fits 5 -- ft971108_2038_0350S001101H.fits 6 -- ft971108_2038_0350S001401H.fits Merging binary extension #: 2 1 -- ft971108_2038_0350S000101H.fits 2 -- ft971108_2038_0350S000201H.fits 3 -- ft971108_2038_0350S000401H.fits 4 -- ft971108_2038_0350S000801H.fits 5 -- ft971108_2038_0350S001101H.fits 6 -- ft971108_2038_0350S001401H.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad55014000s000401h.unf
---- cmerge: version 1.6 ---- A total of 2 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971108_2038_0350S000901H.fits 2 -- ft971108_2038_0350S001001H.fits Merging binary extension #: 2 1 -- ft971108_2038_0350S000901H.fits 2 -- ft971108_2038_0350S001001H.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Ignoring the following files containing 000000112 events
ft971108_2038_0350S000601L.fits ft971108_2038_0350S001701L.fits-> Collecting SIS1 event files by mode
SIS1SORTCODE:LO:Start program SIS1SORTCODE:LO:End program-> Standard Error Output From STOOL sis1sortsplit:
SIS1SORTSPLIT:LO:Start program SIS1SORTSPLIT:LO:s100101h.prelist merge count = 6 photon cnt = 12737 SIS1SORTSPLIT:LO:s100201h.prelist merge count = 2 photon cnt = 16896 SIS1SORTSPLIT:LO:s100301l.prelist merge count = 9 photon cnt = 16140 SIS1SORTSPLIT:LO:s100401l.prelist merge count = 2 photon cnt = 112 SIS1SORTSPLIT:LO:s100501m.prelist merge count = 5 photon cnt = 38543 SIS1SORTSPLIT:LO:Total filenames split = 24 SIS1SORTSPLIT:LO:Total split file cnt = 5 SIS1SORTSPLIT:LO:End program-> Creating ad55014000s100101m.unf
---- cmerge: version 1.6 ---- A total of 5 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971108_2038_0350S101301M.fits 2 -- ft971108_2038_0350S101501M.fits 3 -- ft971108_2038_0350S101901M.fits 4 -- ft971108_2038_0350S102301M.fits 5 -- ft971108_2038_0350S102501M.fits Merging binary extension #: 2 1 -- ft971108_2038_0350S101301M.fits 2 -- ft971108_2038_0350S101501M.fits 3 -- ft971108_2038_0350S101901M.fits 4 -- ft971108_2038_0350S102301M.fits 5 -- ft971108_2038_0350S102501M.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad55014000s100201h.unf
---- cmerge: version 1.6 ---- A total of 2 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971108_2038_0350S100201H.fits 2 -- ft971108_2038_0350S100301H.fits Merging binary extension #: 2 1 -- ft971108_2038_0350S100201H.fits 2 -- ft971108_2038_0350S100301H.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad55014000s100301l.unf
---- cmerge: version 1.6 ---- A total of 9 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971108_2038_0350S100501L.fits 2 -- ft971108_2038_0350S100701L.fits 3 -- ft971108_2038_0350S100901L.fits 4 -- ft971108_2038_0350S101201L.fits 5 -- ft971108_2038_0350S101601L.fits 6 -- ft971108_2038_0350S101801L.fits 7 -- ft971108_2038_0350S102001L.fits 8 -- ft971108_2038_0350S102201L.fits 9 -- ft971108_2038_0350S102401L.fits Merging binary extension #: 2 1 -- ft971108_2038_0350S100501L.fits 2 -- ft971108_2038_0350S100701L.fits 3 -- ft971108_2038_0350S100901L.fits 4 -- ft971108_2038_0350S101201L.fits 5 -- ft971108_2038_0350S101601L.fits 6 -- ft971108_2038_0350S101801L.fits 7 -- ft971108_2038_0350S102001L.fits 8 -- ft971108_2038_0350S102201L.fits 9 -- ft971108_2038_0350S102401L.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad55014000s100401h.unf
---- cmerge: version 1.6 ---- A total of 6 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971108_2038_0350S100101H.fits 2 -- ft971108_2038_0350S100401H.fits 3 -- ft971108_2038_0350S100601H.fits 4 -- ft971108_2038_0350S101001H.fits 5 -- ft971108_2038_0350S101101H.fits 6 -- ft971108_2038_0350S101401H.fits Merging binary extension #: 2 1 -- ft971108_2038_0350S100101H.fits 2 -- ft971108_2038_0350S100401H.fits 3 -- ft971108_2038_0350S100601H.fits 4 -- ft971108_2038_0350S101001H.fits 5 -- ft971108_2038_0350S101101H.fits 6 -- ft971108_2038_0350S101401H.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Ignoring the following files containing 000000112 events
ft971108_2038_0350S100801L.fits ft971108_2038_0350S101701L.fits-> Tar-ing together the leftover raw files
a ft971108_2038_0350G200270H.fits 31K a ft971108_2038_0350G200370H.fits 31K a ft971108_2038_0350G200470H.fits 31K a ft971108_2038_0350G200770H.fits 31K a ft971108_2038_0350G200870H.fits 31K a ft971108_2038_0350G200970H.fits 31K a ft971108_2038_0350G201370L.fits 31K a ft971108_2038_0350G201770M.fits 31K a ft971108_2038_0350G201870M.fits 31K a ft971108_2038_0350G201970M.fits 31K a ft971108_2038_0350G202370M.fits 31K a ft971108_2038_0350G202670L.fits 31K a ft971108_2038_0350G202870M.fits 31K a ft971108_2038_0350G202970M.fits 31K a ft971108_2038_0350G203070M.fits 31K a ft971108_2038_0350G203570L.fits 31K a ft971108_2038_0350G203770M.fits 31K a ft971108_2038_0350G203870M.fits 31K a ft971108_2038_0350G203970M.fits 31K a ft971108_2038_0350G204270L.fits 31K a ft971108_2038_0350G204470M.fits 31K a ft971108_2038_0350G204570M.fits 31K a ft971108_2038_0350G204670M.fits 31K a ft971108_2038_0350G300470H.fits 31K a ft971108_2038_0350G300770H.fits 31K a ft971108_2038_0350G300870H.fits 31K a ft971108_2038_0350G300970H.fits 31K a ft971108_2038_0350G301170H.fits 31K a ft971108_2038_0350G301370L.fits 31K a ft971108_2038_0350G301770M.fits 31K a ft971108_2038_0350G301870M.fits 31K a ft971108_2038_0350G301970M.fits 31K a ft971108_2038_0350G302770L.fits 31K a ft971108_2038_0350G302970M.fits 31K a ft971108_2038_0350G303070M.fits 31K a ft971108_2038_0350G303170M.fits 31K a ft971108_2038_0350G303370M.fits 31K a ft971108_2038_0350G303770L.fits 31K a ft971108_2038_0350G303970M.fits 31K a ft971108_2038_0350G304070M.fits 31K a ft971108_2038_0350G304170M.fits 31K a ft971108_2038_0350G304570L.fits 31K a ft971108_2038_0350G304770M.fits 31K a ft971108_2038_0350G304870M.fits 31K a ft971108_2038_0350G304970M.fits 31K a ft971108_2038_0350S000601L.fits 29K a ft971108_2038_0350S001701L.fits 31K a ft971108_2038_0350S100801L.fits 29K a ft971108_2038_0350S101701L.fits 31K-> Checking OBJECT keywords in HK and event files
temp2gain v4.3 'ft971108_2038.0350' is successfully opened Data Start Time is 153175088.42 (19971108 203804) Time Margin 2.0 sec included Sync error detected in 1382 th SF 'ft971108_2038.0350' EOF detected, sf=3214 Data End Time is 153201044.34 (19971109 035040) Gain History is written in ft971108_2038_0350.ghf-> Stdout output from ISAS program temp2gain
leapsec FITS data was successfully read-> Checking if column CAL_START in ft971108_2038_0350.ghf[1] is in order
Time column is TIME ORDERED-> Checking if column CAL_STOP in ft971108_2038_0350.ghf[1] is in order
Time column is TIME ORDERED-> Calculating attitude correction from ft971108_2038_0350CMHK.fits
The sum of the selected column is 9565.0000 The mean of the selected column is 93.774510 The standard deviation of the selected column is 1.2812962 The minimum of selected column is 92.000000 The maximum of selected column is 96.000000 The number of points used in calculation is 102-> Standard Output From FTOOL fstatistic:
The sum of the selected column is 9565.0000 The mean of the selected column is 93.774510 The standard deviation of the selected column is 1.2812962 The minimum of selected column is 92.000000 The maximum of selected column is 96.000000 The number of points used in calculation is 102
ASCALIN_V0.9u(mod)-> Checking if ad55014000g200270l.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000g200370h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000g300170m.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000g300270l.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000g300370h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s000101m.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s000102m.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s000112m.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s000201l.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s000202l.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s000212l.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s000301h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s000302h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s000312h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s000401h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s000402h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s000412h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s100101m.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s100102m.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s100112m.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s100201h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s100202h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s100212h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s100301l.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s100302l.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s100312l.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s100401h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s100402h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad55014000s100412h.unf is covered by attitude file
ASCALIN_V0.9u(mod)
S0-HK file: ft971108_2038_0350S0HK.fits S1-HK file: ft971108_2038_0350S1HK.fits G2-HK file: ft971108_2038_0350G2HK.fits G3-HK file: ft971108_2038_0350G3HK.fits Date and time are: 1997-11-08 20:38:02 mjd=50760.859750 Orbit file name is ./frf.orbit.241 Epoch of Orbital Elements: 1997-11-03 21:59:59 Rigidity Data File: ./rigidity.data.1.23 Attitude FRF: fa971108_2038.0350 output FITS File: ft971108_2038_0350.mkf Total 812 Data bins were processed.-> Checking if column TIME in ft971108_2038_0350.mkf is in order
Time column is TIME ORDERED-> Calculating dead time values for filter file
The sum of the selected column is 3340.1043 The mean of the selected column is 17.306240 The standard deviation of the selected column is 7.0236451 The minimum of selected column is 4.1875138 The maximum of selected column is 44.750141 The number of points used in calculation is 193-> Using the following selection criteria:
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S0_PIXL1>0 && S0_PIXL1<38.3 ) ) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Filtering ad55014000s000112m.unf into ad55014000s000112m.evt
The sum of the selected column is 3340.1043 The mean of the selected column is 17.306240 The standard deviation of the selected column is 7.0236451 The minimum of selected column is 4.1875138 The maximum of selected column is 44.750141 The number of points used in calculation is 193-> Using the following selection criteria:
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S0_PIXL1>0 && S0_PIXL1<38.3 ) ) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Skipping ad55014000s000201l.unf because of mode
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S0_PIXL1>0) )&&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Deleting ad55014000s000202l.evt since it contains 0 events
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S0_PIXL1>0) )&&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Deleting ad55014000s000212l.evt since it contains 0 events
The sum of the selected column is 1007.9032 The mean of the selected column is 16.256503 The standard deviation of the selected column is 5.7886036 The minimum of selected column is 6.0937691 The maximum of selected column is 33.968857 The number of points used in calculation is 62-> Using the following selection criteria:
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S0_PIXL1>0 && S0_PIXL1<33.6 ) ) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Filtering ad55014000s000312h.unf into ad55014000s000312h.evt
The sum of the selected column is 1007.9032 The mean of the selected column is 16.256503 The standard deviation of the selected column is 5.7886036 The minimum of selected column is 6.0937691 The maximum of selected column is 33.968857 The number of points used in calculation is 62-> Using the following selection criteria:
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S0_PIXL1>0 && S0_PIXL1<33.6 ) ) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Skipping ad55014000s000401h.unf because of mode
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S0_PIXL0>0)&&(S0_PIXL3>0) )&&( (S0_SATF3<1) ||(S0_SATF3>1)) &&( (S0_SATF0<1) ||(S0_SATF0>1)) &&( (S0_SATF3<1) ||(S0_SATF3>1)) &&( (S0_SATF0<1) ||(S0_SATF0>1)) &&((T_DY_NT<0)||(T_DY_NT>32)) &&((T_SAA <0)||(T_SAA >32))-> Filtering ad55014000s000412h.unf into ad55014000s000412h.evt
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S0_PIXL0>0)&&(S0_PIXL3>0) )&&( (S0_SATF3<1) ||(S0_SATF3>1)) &&( (S0_SATF0<1) ||(S0_SATF0>1)) &&( (S0_SATF3<1) ||(S0_SATF3>1)) &&( (S0_SATF0<1) ||(S0_SATF0>1)) &&((T_DY_NT<0)||(T_DY_NT>32)) &&((T_SAA <0)||(T_SAA >32))-> Skipping ad55014000s100101m.unf because of mode
The sum of the selected column is 4577.4833 The mean of the selected column is 26.157047 The standard deviation of the selected column is 8.9424686 The minimum of selected column is 9.8437824 The maximum of selected column is 70.062721 The number of points used in calculation is 175-> Using the following selection criteria:
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S1_PIXL1>0 && S1_PIXL1<52.9 ) ) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Filtering ad55014000s100112m.unf into ad55014000s100112m.evt
The sum of the selected column is 4577.4833 The mean of the selected column is 26.157047 The standard deviation of the selected column is 8.9424686 The minimum of selected column is 9.8437824 The maximum of selected column is 70.062721 The number of points used in calculation is 175-> Using the following selection criteria:
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S1_PIXL1>0 && S1_PIXL1<52.9 ) ) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Skipping ad55014000s100201h.unf because of mode
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S1_PIXL0>0)&&(S1_PIXL1>0)&&(S1_PIXL2>0)&&(S1_PIXL3>0) )&&( (S1_SATF2<1) ||(S1_SATF2>1)) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&( (S1_SATF0<1) ||(S1_SATF0>1)) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&((T_DY_NT<0)||(T_DY_NT>64)) &&((T_SAA <0)||(T_SAA >64))-> Filtering ad55014000s100212h.unf into ad55014000s100212h.evt
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S1_PIXL0>0)&&(S1_PIXL1>0)&&(S1_PIXL2>0)&&(S1_PIXL3>0) )&&( (S1_SATF2<1) ||(S1_SATF2>1)) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&( (S1_SATF0<1) ||(S1_SATF0>1)) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&((T_DY_NT<0)||(T_DY_NT>64)) &&((T_SAA <0)||(T_SAA >64))-> Skipping ad55014000s100301l.unf because of mode
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S1_PIXL1>0) )&&( (S1_SATF1<1) ||(S1_SATF1>1)) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Deleting ad55014000s100302l.evt since it contains 0 events
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S1_PIXL1>0) )&&( (S1_SATF1<1) ||(S1_SATF1>1)) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Deleting ad55014000s100312l.evt since it contains 0 events
The sum of the selected column is 1794.9119 The mean of the selected column is 29.424785 The standard deviation of the selected column is 14.098761 The minimum of selected column is 13.781293 The maximum of selected column is 80.125252 The number of points used in calculation is 61-> Using the following selection criteria:
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S1_PIXL1>0 && S1_PIXL1<71.7 ) ) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Filtering ad55014000s100412h.unf into ad55014000s100412h.evt
The sum of the selected column is 1794.9119 The mean of the selected column is 29.424785 The standard deviation of the selected column is 14.098761 The minimum of selected column is 13.781293 The maximum of selected column is 80.125252 The number of points used in calculation is 61-> Using the following selection criteria:
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S1_PIXL1>0 && S1_PIXL1<71.7 ) ) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&( (S1_SATF1<1) ||(S1_SATF1>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Filtering ad55014000g200170m.unf into ad55014000g200170m.evt
(SAA==0)&& (COR>4)&& (G2_H0+G2_H2+G3_H0+G3_H2<45)&& (G2_H0+G2_H2+G3_H0+G3_H2<0.45*COR**2-13*COR+125)&& (RBM_CONT<100)&& (ELV>5)&& (ACS==0)&& (ANG_DIST>0)&& (ANG_DIST<0.01)&& (G2_L1>0)-> Filtering ad55014000g200270l.unf into ad55014000g200270l.evt
(SAA==0)&& (COR>4)&& (G2_H0+G2_H2+G3_H0+G3_H2<45)&& (G2_H0+G2_H2+G3_H0+G3_H2<0.45*COR**2-13*COR+125)&& (RBM_CONT<100)&& (ELV>5)&& (ACS==0)&& (ANG_DIST>0)&& (ANG_DIST<0.01)&& (G2_L1>0)-> Filtering ad55014000g200370h.unf into ad55014000g200370h.evt
(SAA==0)&& (COR>4)&& (G2_H0+G2_H2+G3_H0+G3_H2<45)&& (G2_H0+G2_H2+G3_H0+G3_H2<0.45*COR**2-13*COR+125)&& (RBM_CONT<100)&& (ELV>5)&& (ACS==0)&& (ANG_DIST>0)&& (ANG_DIST<0.01)&& (G2_L1>0)-> Filtering ad55014000g300170m.unf into ad55014000g300170m.evt
(SAA==0)&& (COR>4)&& (G2_H0+G2_H2+G3_H0+G3_H2<45)&& (G2_H0+G2_H2+G3_H0+G3_H2<0.45*COR**2-13*COR+125)&& (RBM_CONT<100)&& (ELV>5)&& (ACS==0)&& (ANG_DIST>0)&& (ANG_DIST<0.01)&& (G3_L1>0)-> Filtering ad55014000g300270l.unf into ad55014000g300270l.evt
(SAA==0)&& (COR>4)&& (G2_H0+G2_H2+G3_H0+G3_H2<45)&& (G2_H0+G2_H2+G3_H0+G3_H2<0.45*COR**2-13*COR+125)&& (RBM_CONT<100)&& (ELV>5)&& (ACS==0)&& (ANG_DIST>0)&& (ANG_DIST<0.01)&& (G3_L1>0)-> Filtering ad55014000g300370h.unf into ad55014000g300370h.evt
(SAA==0)&& (COR>4)&& (G2_H0+G2_H2+G3_H0+G3_H2<45)&& (G2_H0+G2_H2+G3_H0+G3_H2<0.45*COR**2-13*COR+125)&& (RBM_CONT<100)&& (ELV>5)&& (ACS==0)&& (ANG_DIST>0)&& (ANG_DIST<0.01)&& (G3_L1>0)
-ANNULUS(128.5,128.5,192,88) -ELLIPSE(167.5,220,24.66,28.95,245.298)-> gis2_ano_on_flf_180295.fits already present in current directory
ASCAEXPO_V0.9b
reading data file: ad55014000g200170m.evt
reading gti ext: STDGTI
reading cal file: gis2_ano_on_flf_180295.fits
reading inst file: GIS2_REGION256.4_regionmap.tmp
making an inst map...
rebin gis: 1
multiply inst map...
reading att file: ./fa971108_2038.0350
making an exposure map...
Aspect RA/DEC/ROLL : 296.4460 24.6625 102.2741
Mean RA/DEC/ROLL : 296.4459 24.6880 102.2741
Pnt RA/DEC/ROLL : 296.4441 24.6380 102.2741
Image rebin factor : 1
Attitude Records : 12849
GTI intervals : 5
Total GTI (secs) : 7791.874
Max attitude excursion (arcsecs) : 5.000
0 Percent Complete: Total/live time: 0.00 0.00
10 Percent Complete: Total/live time: 944.00 944.00
20 Percent Complete: Total/live time: 4055.94 4055.94
30 Percent Complete: Total/live time: 4055.94 4055.94
40 Percent Complete: Total/live time: 4059.88 4059.88
50 Percent Complete: Total/live time: 4059.88 4059.88
60 Percent Complete: Total/live time: 7023.87 7023.87
70 Percent Complete: Total/live time: 7023.87 7023.87
80 Percent Complete: Total/live time: 7027.79 7027.79
90 Percent Complete: Total/live time: 7776.38 7776.38
100 Percent Complete: Total/live time: 7791.88 7791.88
Number of attitude steps used: 36
Number of attitude steps avail: 3723
Mean RA/DEC pixel offset: 32.0986 34.8485
writing expo file: ad55014000g200170m.expo
closing attitude file...
closing data file...
-> Generating low and high energy images for ad55014000g200170m.evt
ASCAEXPO_V0.9b
reading data file: ad55014000g200270l.evt
reading gti ext: STDGTI
reading cal file: gis2_ano_on_flf_180295.fits
reading inst file: GIS2_REGION256.4_regionmap.tmp
making an inst map...
rebin gis: 1
multiply inst map...
reading att file: ./fa971108_2038.0350
making an exposure map...
Aspect RA/DEC/ROLL : 296.4460 24.6625 102.2757
Mean RA/DEC/ROLL : 296.4465 24.6888 102.2757
Pnt RA/DEC/ROLL : 296.4423 24.6402 102.2757
Image rebin factor : 1
Attitude Records : 12849
GTI intervals : 3
Total GTI (secs) : 71.987
Max attitude excursion (arcsecs) : 5.000
0 Percent Complete: Total/live time: 0.00 0.00
10 Percent Complete: Total/live time: 7.99 7.99
20 Percent Complete: Total/live time: 19.99 19.99
30 Percent Complete: Total/live time: 64.01 64.01
40 Percent Complete: Total/live time: 64.01 64.01
50 Percent Complete: Total/live time: 67.99 67.99
60 Percent Complete: Total/live time: 67.99 67.99
70 Percent Complete: Total/live time: 71.99 71.99
100 Percent Complete: Total/live time: 71.99 71.99
Number of attitude steps used: 6
Number of attitude steps avail: 4292
Mean RA/DEC pixel offset: -10.8833 -2.1726
writing expo file: ad55014000g200270l.expo
closing attitude file...
closing data file...
-> Generating low and high energy images for ad55014000g200270l.evt
ASCAEXPO_V0.9b
reading data file: ad55014000g200370h.evt
reading gti ext: STDGTI
reading cal file: gis2_ano_on_flf_180295.fits
reading inst file: GIS2_REGION256.4_regionmap.tmp
making an inst map...
rebin gis: 1
multiply inst map...
reading att file: ./fa971108_2038.0350
making an exposure map...
Aspect RA/DEC/ROLL : 296.4460 24.6625 102.2652
Mean RA/DEC/ROLL : 296.4382 24.6660 102.2652
Pnt RA/DEC/ROLL : 296.5333 24.9073 102.2652
Image rebin factor : 1
Attitude Records : 12849
GTI intervals : 3
Total GTI (secs) : 2307.980
Max attitude excursion (arcsecs) : 5.000
0 Percent Complete: Total/live time: 0.00 0.00
10 Percent Complete: Total/live time: 1539.98 1539.98
20 Percent Complete: Total/live time: 1539.98 1539.98
30 Percent Complete: Total/live time: 1540.48 1540.48
40 Percent Complete: Total/live time: 1540.48 1540.48
50 Percent Complete: Total/live time: 2288.48 2288.48
60 Percent Complete: Total/live time: 2288.48 2288.48
70 Percent Complete: Total/live time: 2307.98 2307.98
100 Percent Complete: Total/live time: 2307.98 2307.98
Number of attitude steps used: 5
Number of attitude steps avail: 4832
Mean RA/DEC pixel offset: -10.6728 -2.2846
writing expo file: ad55014000g200370h.expo
closing attitude file...
closing data file...
-> Generating low and high energy images for ad55014000g200370h.evt-ANNULUS(128.5,128.5,192,88) -ELLIPSE(217,95,21.56,25.92,169.216)-> gis3_ano_on_flf_180295.fits already present in current directory
ASCAEXPO_V0.9b
reading data file: ad55014000g300170m.evt
reading gti ext: STDGTI
reading cal file: gis3_ano_on_flf_180295.fits
reading inst file: GIS3_REGION256.4_regionmap.tmp
making an inst map...
rebin gis: 1
multiply inst map...
reading att file: ./fa971108_2038.0350
making an exposure map...
Aspect RA/DEC/ROLL : 296.4460 24.6625 102.2754
Mean RA/DEC/ROLL : 296.4494 24.6640 102.2754
Pnt RA/DEC/ROLL : 296.4410 24.6627 102.2754
Image rebin factor : 1
Attitude Records : 12849
GTI intervals : 5
Total GTI (secs) : 7791.874
Max attitude excursion (arcsecs) : 5.000
0 Percent Complete: Total/live time: 0.00 0.00
10 Percent Complete: Total/live time: 944.00 944.00
20 Percent Complete: Total/live time: 4055.94 4055.94
30 Percent Complete: Total/live time: 4055.94 4055.94
40 Percent Complete: Total/live time: 4059.88 4059.88
50 Percent Complete: Total/live time: 4059.88 4059.88
60 Percent Complete: Total/live time: 7023.87 7023.87
70 Percent Complete: Total/live time: 7023.87 7023.87
80 Percent Complete: Total/live time: 7027.79 7027.79
90 Percent Complete: Total/live time: 7776.38 7776.38
100 Percent Complete: Total/live time: 7791.88 7791.88
Number of attitude steps used: 36
Number of attitude steps avail: 3723
Mean RA/DEC pixel offset: 44.1772 36.0484
writing expo file: ad55014000g300170m.expo
closing attitude file...
closing data file...
-> Generating low and high energy images for ad55014000g300170m.evt
ASCAEXPO_V0.9b
reading data file: ad55014000g300270l.evt
reading gti ext: STDGTI
reading cal file: gis3_ano_on_flf_180295.fits
reading inst file: GIS3_REGION256.4_regionmap.tmp
making an inst map...
rebin gis: 1
multiply inst map...
reading att file: ./fa971108_2038.0350
making an exposure map...
Aspect RA/DEC/ROLL : 296.4460 24.6625 102.2771
Mean RA/DEC/ROLL : 296.4496 24.6642 102.2771
Pnt RA/DEC/ROLL : 296.4392 24.6649 102.2771
Image rebin factor : 1
Attitude Records : 12849
GTI intervals : 3
Total GTI (secs) : 71.987
Max attitude excursion (arcsecs) : 5.000
0 Percent Complete: Total/live time: 0.00 0.00
10 Percent Complete: Total/live time: 7.99 7.99
20 Percent Complete: Total/live time: 19.99 19.99
30 Percent Complete: Total/live time: 64.01 64.01
40 Percent Complete: Total/live time: 64.01 64.01
50 Percent Complete: Total/live time: 67.99 67.99
60 Percent Complete: Total/live time: 67.99 67.99
70 Percent Complete: Total/live time: 71.99 71.99
100 Percent Complete: Total/live time: 71.99 71.99
Number of attitude steps used: 6
Number of attitude steps avail: 4292
Mean RA/DEC pixel offset: -0.8178 -1.1726
writing expo file: ad55014000g300270l.expo
closing attitude file...
closing data file...
-> Generating low and high energy images for ad55014000g300270l.evt
ASCAEXPO_V0.9b
reading data file: ad55014000g300370h.evt
reading gti ext: STDGTI
reading cal file: gis3_ano_on_flf_180295.fits
reading inst file: GIS3_REGION256.4_regionmap.tmp
making an inst map...
rebin gis: 1
multiply inst map...
reading att file: ./fa971108_2038.0350
making an exposure map...
Aspect RA/DEC/ROLL : 296.4460 24.6625 102.2666
Mean RA/DEC/ROLL : 296.4414 24.6414 102.2666
Pnt RA/DEC/ROLL : 296.5303 24.9320 102.2666
Image rebin factor : 1
Attitude Records : 12849
GTI intervals : 3
Total GTI (secs) : 2307.980
Max attitude excursion (arcsecs) : 5.000
0 Percent Complete: Total/live time: 0.00 0.00
10 Percent Complete: Total/live time: 1539.98 1539.98
20 Percent Complete: Total/live time: 1539.98 1539.98
30 Percent Complete: Total/live time: 1540.48 1540.48
40 Percent Complete: Total/live time: 1540.48 1540.48
50 Percent Complete: Total/live time: 2288.48 2288.48
60 Percent Complete: Total/live time: 2288.48 2288.48
70 Percent Complete: Total/live time: 2307.98 2307.98
100 Percent Complete: Total/live time: 2307.98 2307.98
Number of attitude steps used: 5
Number of attitude steps avail: 4832
Mean RA/DEC pixel offset: -1.0099 -1.3247
writing expo file: ad55014000g300370h.expo
closing attitude file...
closing data file...
-> Generating low and high energy images for ad55014000g300370h.evt
ASCAEXPO_V0.9b
reading data file: ad55014000s000102m.evt
reading gti ext: STDGTI
reading hp ext: HOT_PIXELS
reading cal file: s0_teldef_ascalin.fits
making an inst map...
SIS AREA DISC ENABL OFF
CHIP: 0 1 2 3
CCD POWER ON/OFF: OFF ON OFF OFF
AREA DISC IN/OUT: OUT OUT IN IN
AREA DISC H START: 6 6 6 316
AREA DISC H STOP: 425 425 200 425
AREA DISC V START: 2 2 2 2
AREA DISC V STOP: 422 422 150 112
reading att file: ./fa971108_2038.0350
making an exposure map...
Aspect RA/DEC/ROLL : 296.4460 24.6625 102.2823
Mean RA/DEC/ROLL : 296.4644 24.6795 102.2823
Pnt RA/DEC/ROLL : 296.4272 24.6468 102.2823
Image rebin factor : 4
Attitude Records : 12849
Hot Pixels : 9
GTI intervals : 17
Total GTI (secs) : 6111.462
Max attitude excursion (arcsecs) : 5.000
0 Percent Complete: Total/live time: 0.00 0.00
10 Percent Complete: Total/live time: 1151.85 1151.85
20 Percent Complete: Total/live time: 3263.67 3263.67
30 Percent Complete: Total/live time: 3263.67 3263.67
40 Percent Complete: Total/live time: 3267.61 3267.61
50 Percent Complete: Total/live time: 3267.61 3267.61
60 Percent Complete: Total/live time: 5791.67 5791.67
70 Percent Complete: Total/live time: 5791.67 5791.67
80 Percent Complete: Total/live time: 5795.59 5795.59
90 Percent Complete: Total/live time: 5795.59 5795.59
100 Percent Complete: Total/live time: 6111.46 6111.46
Number of attitude steps used: 36
Number of attitude steps avail: 3336
Mean RA/DEC pixel offset: 353.5318 258.8842
writing expo file: ad55014000s000102m.expo
closing attitude file...
closing data file...
-> Generating low and high energy images for ad55014000s000102m.evt
ASCAEXPO_V0.9b
reading data file: ad55014000s000302h.evt
reading gti ext: STDGTI
reading hp ext: HOT_PIXELS
reading cal file: s0_teldef_ascalin.fits
making an inst map...
SIS AREA DISC ENABL OFF
CHIP: 0 1 2 3
CCD POWER ON/OFF: OFF ON OFF OFF
AREA DISC IN/OUT: OUT OUT IN IN
AREA DISC H START: 6 6 6 316
AREA DISC H STOP: 425 425 200 425
AREA DISC V START: 2 2 2 2
AREA DISC V STOP: 422 422 150 112
reading att file: ./fa971108_2038.0350
making an exposure map...
Aspect RA/DEC/ROLL : 296.4460 24.6625 102.2705
Mean RA/DEC/ROLL : 296.4546 24.6503 102.2705
Pnt RA/DEC/ROLL : 296.5178 24.9134 102.2705
Image rebin factor : 4
Attitude Records : 12849
Hot Pixels : 7
GTI intervals : 5
Total GTI (secs) : 1915.861
Max attitude excursion (arcsecs) : 5.000
0 Percent Complete: Total/live time: 0.00 0.00
10 Percent Complete: Total/live time: 1211.86 1211.86
20 Percent Complete: Total/live time: 1211.86 1211.86
30 Percent Complete: Total/live time: 1211.99 1211.99
40 Percent Complete: Total/live time: 1211.99 1211.99
50 Percent Complete: Total/live time: 1915.86 1915.86
100 Percent Complete: Total/live time: 1915.86 1915.86
Number of attitude steps used: 4
Number of attitude steps avail: 4037
Mean RA/DEC pixel offset: -48.7873 -68.2039
writing expo file: ad55014000s000302h.expo
closing attitude file...
closing data file...
-> Generating low and high energy images for ad55014000s000302h.evt
ASCAEXPO_V0.9b
reading data file: ad55014000s100102m.evt
reading gti ext: STDGTI
reading hp ext: HOT_PIXELS
reading cal file: s1_teldef_ascalin.fits
making an inst map...
SIS AREA DISC ENABL OFF
CHIP: 0 1 2 3
CCD POWER ON/OFF: OFF ON OFF OFF
AREA DISC IN/OUT: OUT OUT OUT OUT
AREA DISC H START: 6 6 6 6
AREA DISC H STOP: 425 425 425 425
AREA DISC V START: 2 2 2 2
AREA DISC V STOP: 422 422 422 422
reading att file: ./fa971108_2038.0350
making an exposure map...
Aspect RA/DEC/ROLL : 296.4460 24.6625 102.2751
Mean RA/DEC/ROLL : 296.4471 24.6772 102.2751
Pnt RA/DEC/ROLL : 296.4445 24.6493 102.2751
Image rebin factor : 4
Attitude Records : 12849
Hot Pixels : 21
GTI intervals : 29
Total GTI (secs) : 5567.462
Max attitude excursion (arcsecs) : 5.000
0 Percent Complete: Total/live time: 0.00 0.00
10 Percent Complete: Total/live time: 927.85 927.85
20 Percent Complete: Total/live time: 2911.67 2911.67
30 Percent Complete: Total/live time: 2911.67 2911.67
40 Percent Complete: Total/live time: 2915.61 2915.61
50 Percent Complete: Total/live time: 2915.61 2915.61
60 Percent Complete: Total/live time: 5215.67 5215.67
70 Percent Complete: Total/live time: 5215.67 5215.67
80 Percent Complete: Total/live time: 5219.59 5219.59
90 Percent Complete: Total/live time: 5219.59 5219.59
100 Percent Complete: Total/live time: 5567.46 5567.46
Number of attitude steps used: 36
Number of attitude steps avail: 3336
Mean RA/DEC pixel offset: 349.0877 330.7350
writing expo file: ad55014000s100102m.expo
closing attitude file...
closing data file...
-> Generating low and high energy images for ad55014000s100102m.evt
ASCAEXPO_V0.9b
reading data file: ad55014000s100402h.evt
reading gti ext: STDGTI
reading hp ext: HOT_PIXELS
reading cal file: s1_teldef_ascalin.fits
making an inst map...
SIS AREA DISC ENABL OFF
CHIP: 0 1 2 3
CCD POWER ON/OFF: OFF ON OFF OFF
AREA DISC IN/OUT: OUT OUT OUT OUT
AREA DISC H START: 6 6 6 6
AREA DISC H STOP: 425 425 425 425
AREA DISC V START: 2 2 2 2
AREA DISC V STOP: 422 422 422 422
reading att file: ./fa971108_2038.0350
making an exposure map...
Aspect RA/DEC/ROLL : 296.4460 24.6625 102.2633
Mean RA/DEC/ROLL : 296.4390 24.6535 102.2633
Pnt RA/DEC/ROLL : 296.5352 24.9158 102.2633
Image rebin factor : 4
Attitude Records : 12849
Hot Pixels : 18
GTI intervals : 4
Total GTI (secs) : 1911.861
Max attitude excursion (arcsecs) : 5.000
0 Percent Complete: Total/live time: 0.00 0.00
10 Percent Complete: Total/live time: 1143.86 1143.86
20 Percent Complete: Total/live time: 1143.86 1143.86
30 Percent Complete: Total/live time: 1143.99 1143.99
40 Percent Complete: Total/live time: 1143.99 1143.99
50 Percent Complete: Total/live time: 1911.86 1911.86
100 Percent Complete: Total/live time: 1911.86 1911.86
Number of attitude steps used: 4
Number of attitude steps avail: 4037
Mean RA/DEC pixel offset: -52.1205 -14.3156
writing expo file: ad55014000s100402h.expo
closing attitude file...
closing data file...
-> Generating low and high energy images for ad55014000s100402h.evtad55014000s000102m.expo ad55014000s000302h.expo ad55014000s100102m.expo ad55014000s100402h.expo-> Summing the following images to produce ad55014000sis32002_all.totsky
ad55014000s000102m.img ad55014000s000302h.img ad55014000s100102m.img ad55014000s100402h.img-> Summing the following images to produce ad55014000sis32002_lo.totsky
ad55014000s000102m_lo.img ad55014000s000302h_lo.img ad55014000s100102m_lo.img ad55014000s100402h_lo.img-> Summing the following images to produce ad55014000sis32002_hi.totsky
ad55014000s000102m_hi.img ad55014000s000302h_hi.img ad55014000s100102m_hi.img ad55014000s100402h_hi.img-> Running XIMAGE to create ad55014000sis32002.gif
No of detectors read in: 20 ![1]XIMAGE> read/fits ad55014000sis32002_all.totsky Reading an image Telescope ASCA SIS0 Image display size = 320 Done, closing file Largest, Smallest 2.00000 0. Bscale, Bzero from file 1.0000000000000 0. After internal scaling Bscale and Bzero 1.0000000000000 0. Image level, max: 2 min: 0 ![2]XIMAGE> read/exp_map ad55014000sis32002.totexpo Reading an image Telescope ASCA SIS0 Image display size = 320 Done, closing file Largest, Smallest 134.301 0. Bscale, Bzero from file 1.0000000000000 0. After internal scaling Bscale and Bzero 1.0000000000000 0. Image level, max: 134 min: 0 ![3]XIMAGE> smooth ![4]XIMAGE> cpd /ppm ![5]XIMAGE> cey 2000 ![6]XIMAGE> title "RIDGE_EDGE5" ![7]XIMAGE> title/lower "ASCA SIS0,SIS1 November 8, 1997 Exposure: 15506.6 s" ![8]XIMAGE> disp/correct/noframe Displaying image The image is exposure corrected Min = 0 max = 32767 ![9]XIMAGE> grid ![10]XIMAGE> scale scal_f, min_inten 1.00000 0. i,inten,mm,pp 1 0. 0 0 i,inten,mm,pp 2 4.00000 40 -1 i,inten,mm,pp 3 8.00000 80 -1 i,inten,mm,pp 4 45.0000 45 0 ![11]XIMAGE> exit-> Summing gis images
ad55014000g200170m.expo ad55014000g200270l.expo ad55014000g200370h.expo ad55014000g300170m.expo ad55014000g300270l.expo ad55014000g300370h.expo-> Summing the following images to produce ad55014000gis25670_all.totsky
ad55014000g200170m.img ad55014000g200270l.img ad55014000g200370h.img ad55014000g300170m.img ad55014000g300270l.img ad55014000g300370h.img-> Summing the following images to produce ad55014000gis25670_lo.totsky
ad55014000g200170m_lo.img ad55014000g200270l_lo.img ad55014000g200370h_lo.img ad55014000g300170m_lo.img ad55014000g300270l_lo.img ad55014000g300370h_lo.img-> Summing the following images to produce ad55014000gis25670_hi.totsky
ad55014000g200170m_hi.img ad55014000g200270l_hi.img ad55014000g200370h_hi.img ad55014000g300170m_hi.img ad55014000g300270l_hi.img ad55014000g300370h_hi.img-> Running XIMAGE to create ad55014000gis25670.gif
No of detectors read in: 20 ![1]XIMAGE> read/fits ad55014000gis25670_all.totsky Reading an image Telescope ASCA GIS2 Image display size = 256 Done, closing file Largest, Smallest 5.00000 0. Bscale, Bzero from file 1.0000000000000 0. After internal scaling Bscale and Bzero 1.0000000000000 0. Image level, max: 5 min: 0 ![2]XIMAGE> read/exp_map ad55014000gis25670.totexpo Reading an image Telescope ASCA GIS2 Image display size = 256 Done, closing file Largest, Smallest 339.061 0. Bscale, Bzero from file 1.0000000000000 0. After internal scaling Bscale and Bzero 1.0000000000000 0. Image level, max: 339 min: 0 ![3]XIMAGE> smooth ![4]XIMAGE> cpd /ppm ![5]XIMAGE> cey 2000 ![6]XIMAGE> title "RIDGE_EDGE5" ![7]XIMAGE> title/lower "ASCA GIS2,GIS3 November 8, 1997 Exposure: 20343.6 s" ![8]XIMAGE> disp/correct/noframe Displaying image The image is exposure corrected Min = 0 max = 32767 ![9]XIMAGE> grid ![10]XIMAGE> scale scal_f, min_inten 1.00000 0. i,inten,mm,pp 1 0. 0 0 i,inten,mm,pp 2 4.00000 40 -1 i,inten,mm,pp 3 8.00000 80 -1 i,inten,mm,pp 4 52.0000 52 0 ![11]XIMAGE> exit
96 116 6.5206e-05 124 14 5.59424-> Smoothing ad55014000gis25670_hi.totsky with ad55014000gis25670.totexpo
96 116 3.51976e-05 124 11 5.06714-> Smoothing ad55014000gis25670_lo.totsky with ad55014000gis25670.totexpo
98 113 2.39683e-05 123 16 4.59793-> Determining extraction radii
96 116 24 T-> Sources with radius >= 2
96 116 24 T-> Standard Output From STOOL colorpic:
color plane 0 color plane 1 color plane 2 writing image image written-> Creating fits catalog of sources: ad55014000gis25670.src
-> Standard Output From STOOL colorpic:
color plane 0 color plane 1 color plane 2 writing image image written-> Creating fits catalog of sources: ad55014000sis32002.src
The sum of the selected column is 854.00000 The mean of the selected column is 142.33333 The standard deviation of the selected column is 1.5055453 The minimum of selected column is 141.00000 The maximum of selected column is 145.00000 The number of points used in calculation is 6-> Standard Output From FTOOL fstatistic:
The sum of the selected column is 584.00000 The mean of the selected column is 97.333333 The standard deviation of the selected column is 1.2110601 The minimum of selected column is 96.000000 The maximum of selected column is 99.000000 The number of points used in calculation is 6-> Converting (96.0,116.0,2.0) to g3 detector coordinates
The sum of the selected column is 1336.0000 The mean of the selected column is 148.44444 The standard deviation of the selected column is 1.1303883 The minimum of selected column is 147.00000 The maximum of selected column is 150.00000 The number of points used in calculation is 9-> Standard Output From FTOOL fstatistic:
The sum of the selected column is 884.00000 The mean of the selected column is 98.222222 The standard deviation of the selected column is 1.3944334 The minimum of selected column is 96.000000 The maximum of selected column is 100.00000 The number of points used in calculation is 9
1 ad55014000s000102m.evt 422 1 ad55014000s000302h.evt 422-> Standard Output From STOOL group_event_files:
1 ad55014000s000112m.evt 463 1 ad55014000s000312h.evt 463-> Standard Output From STOOL group_event_files:
1 ad55014000s100102m.evt 515 1 ad55014000s100402h.evt 515-> Fetching SIS1_NOTCHIP0.1
ad55014000s100102m.evt ad55014000s100402h.evt-> Grouping ad55014000s110102_0.pi to 40 counts/bin
------------------------- MANDATORY KEYWORDS/VALUES ------------------------- -------------------------------------------------------------------- -------------------------------------------------------------------- EXTNAME - SPECTRUM Name of this BINTABLE TELESCOP - ASCA Mission/Satellite name INSTRUME - SIS1 Instrument/Detector FILTER - NONE Instrument filter in use EXPOSURE - 7479.3 Integration time (in secs) of PHA data AREASCAL - 1.0000 Area scaling factor BACKSCAL - 0.10410 Background scaling factor BACKFILE - NONE Associated background file CORRSCAL - 1.0000 Correlation scaling factor CORRFILE - none Associated correlation file RESPFILE - NONE Associated redistribution matrix file ANCRFILE - none Associated ancillary response file XFLT0001 - none XSPEC selection filter POISSERR - TRUE Whether Poissonian errors apply CHANTYPE - PI Whether channels have been corrected TLMIN1 - 0 First legal Detector channel DETCHANS - 512 No. of legal detector channels NCHAN - 512 No. of detector channels in dataset PHAVERSN - 1.1.0 OGIP FITS version number STAT_ERR - FALSE Statistical Error SYS_ERR - TRUE Fractional Systematic Error QUALITY - TRUE Quality Flag GROUPING - FALSE Grouping Flag -------------------------------------------------------------------- -------------------------------------------------------------------- ... ... -------- ... GROUPING ... -------- ... --------------------------------------------- ... Channel Grouping (Channel-Channel) : ... 0 - 16 of undefined grouping (Channel quality=bad) ... 17 - 31 are grouped by a factor 15 ... 32 - 52 are grouped by a factor 7 ... 53 - 61 are grouped by a factor 9 ... 62 - 76 are grouped by a factor 15 ... 77 - 104 are grouped by a factor 28 ... 105 - 140 are grouped by a factor 36 ... 141 - 223 are grouped by a factor 83 ... 224 - 371 are grouped by a factor 148 ... 372 - 475 are grouped by a factor 104 ... 476 - 511 of undefined grouping (Channel quality=bad) ... --------------------------------------------- ... ...... exiting, changes written to file : ad55014000s110102_0.pi ** grppha 2.8.1 completed successfully-> Source occupies chip(s) 1
Sisrmg Version 1.1, Configured 04/97 This version resolves *all* known keyword incompatibilities with other FTOOLS tasks. If you have previously fudged *any* keywords in the PHA file to compensate, incorrect results will follow. Setting 1st PHA channel to 0 Making v1.1 1180x512 S1C1 Bright PI RMF Calibration data files: ecd = ./sis1c1p40_290296.fits cti = ./sisph2pi_110397.fits echo = ./sisechos_290296.fits rdd = ./sisrddis_290296.fits Please stand by... ...Done.-> Generating ad55014000s110102_0.arf with point=no
ASCAARF vers 2.81 28 Aug 1998.
Input WMAP array has size 52 by 53 bins
expanded to 52 by 53 bins
First WMAP bin is at detector pixel 656 664
8 detector pixels per WMAP bin
WMAP bin size is 0.21600 mm
0.21216 arcmin
Selected region size is 7.4973 arcmin^2
Optical axis is detector pixel 618.28 773.83
1180 energies from RMF file
Effective area fudge applied
Arf filter applied
Total counts in region = 5.01000E+02
Weighted mean angle from optical axis = 7.483 arcmin
-> Standard Output From STOOL group_event_files:1 ad55014000s100112m.evt 546 1 ad55014000s100412h.evt 546-> SIS1_NOTCHIP0.1 already present in current directory
ad55014000s100112m.evt ad55014000s100412h.evt-> Grouping ad55014000s110212_0.pi to 40 counts/bin
------------------------- MANDATORY KEYWORDS/VALUES ------------------------- -------------------------------------------------------------------- -------------------------------------------------------------------- EXTNAME - SPECTRUM Name of this BINTABLE TELESCOP - ASCA Mission/Satellite name INSTRUME - SIS1 Instrument/Detector FILTER - NONE Instrument filter in use EXPOSURE - 7479.3 Integration time (in secs) of PHA data AREASCAL - 1.0000 Area scaling factor BACKSCAL - 0.10410 Background scaling factor BACKFILE - NONE Associated background file CORRSCAL - 1.0000 Correlation scaling factor CORRFILE - none Associated correlation file RESPFILE - NONE Associated redistribution matrix file ANCRFILE - none Associated ancillary response file XFLT0001 - none XSPEC selection filter POISSERR - TRUE Whether Poissonian errors apply CHANTYPE - PI Whether channels have been corrected TLMIN1 - 0 First legal Detector channel DETCHANS - 1024 No. of legal detector channels NCHAN - 1024 No. of detector channels in dataset PHAVERSN - 1.1.0 OGIP FITS version number STAT_ERR - FALSE Statistical Error SYS_ERR - TRUE Fractional Systematic Error QUALITY - TRUE Quality Flag GROUPING - FALSE Grouping Flag -------------------------------------------------------------------- -------------------------------------------------------------------- ... ... -------- ... GROUPING ... -------- ... --------------------------------------------- ... Channel Grouping (Channel-Channel) : ... 0 - 32 of undefined grouping (Channel quality=bad) ... 33 - 62 are grouped by a factor 30 ... 63 - 104 are grouped by a factor 14 ... 105 - 120 are grouped by a factor 16 ... 121 - 149 are grouped by a factor 29 ... 150 - 200 are grouped by a factor 51 ... 201 - 268 are grouped by a factor 68 ... 269 - 431 are grouped by a factor 163 ... 432 - 678 are grouped by a factor 247 ... 679 - 928 are grouped by a factor 250 ... 929 - 1023 are grouped by a factor 95 ... --------------------------------------------- ... ...... exiting, changes written to file : ad55014000s110212_0.pi ** grppha 2.8.1 completed successfully-> Source occupies chip(s) 1
Sisrmg Version 1.1, Configured 04/97 This version resolves *all* known keyword incompatibilities with other FTOOLS tasks. If you have previously fudged *any* keywords in the PHA file to compensate, incorrect results will follow. Setting 1st PHA channel to 0 Making v1.1 1180x1024 S1C1 Bright2 PI RMF Calibration data files: ecd = ./sis1c1p40_290296.fits cti = ./sisph2pi_110397.fits echo = ./sisechos_290296.fits rdd = ./sisrddis_290296.fits Please stand by... ...Done.-> Generating ad55014000s110212_0.arf with point=no
ASCAARF vers 2.81 28 Aug 1998.
Input WMAP array has size 52 by 53 bins
expanded to 52 by 53 bins
First WMAP bin is at detector pixel 656 664
8 detector pixels per WMAP bin
WMAP bin size is 0.21600 mm
0.21216 arcmin
Selected region size is 7.4973 arcmin^2
Optical axis is detector pixel 618.28 773.83
1180 energies from RMF file
Effective area fudge applied
Arf filter applied
Total counts in region = 5.30000E+02
Weighted mean angle from optical axis = 7.406 arcmin
-> Standard Output From STOOL group_event_files:1 ad55014000g200170m.evt 3439 1 ad55014000g200270l.evt 3439 1 ad55014000g200370h.evt 3439-> GIS2_REGION256.4 already present in current directory
ad55014000g200170m.evt ad55014000g200270l.evt ad55014000g200370h.evt-> Deleting ad55014000g210170_1.pi since it has 424 events
1 ad55014000g300170m.evt 3652 1 ad55014000g300270l.evt 3652 1 ad55014000g300370h.evt 3652-> GIS3_REGION256.4 already present in current directory
ad55014000g300170m.evt ad55014000g300270l.evt ad55014000g300370h.evt-> Deleting ad55014000g310170_1.pi since it has 434 events
XSPEC 9.01 13:37:16 29-Dec-99
Plot device not set, use "cpd" to set it
Type "help" or "?" for further information
!XSPEC> data ad55014000s110102_0.pi
Net count rate (cts/s) for file 1 6.7519E-02+/- 3.1299E-03
1 data set is in use
!XSPEC> setplot energy
!XSPEC> ignore bad
!XSPEC> iplot
!PLT> log y on
!PLT> rescale y
!PLT> hard /ps
!PLT> quit
!XSPEC> exit
!Do you really want to exit (y) y
XSPEC: quit
-> Plotting ad55014000s110212_0_pi.ps from ad55014000s110212_0.pi
XSPEC 9.01 13:37:31 29-Dec-99
Plot device not set, use "cpd" to set it
Type "help" or "?" for further information
!XSPEC> data ad55014000s110212_0.pi
Net count rate (cts/s) for file 1 7.1263E-02+/- 3.1696E-03
1 data set is in use
!XSPEC> setplot energy
!XSPEC> ignore bad
!XSPEC> iplot
!PLT> log y on
!PLT> rescale y
!PLT> hard /ps
!PLT> quit
!XSPEC> exit
!Do you really want to exit (y) y
XSPEC: quit
Type "help" for information
[1]xronos> Current User Interface is ; command driven
[2]xronos> Enter up to 50 input filenames and options for series 1 (or rtn)
Ser. A filename 1 +options[.rbf]=> ad55014000s100002_0.lc
Selected FITS extensions: 1 - RATE TABLE;
Source ............ RIDGE_EDGE5 Start Time (d) .... 10760 21:21:46.419
FITS Extension .... 1 - `RATE ` Stop Time (d) ..... 10761 03:50:34.212
No. of Rows ....... 10 Bin Time (s) ...... 726.1
Right Ascension ... 2.9645E+02 Internal time sys.. Converted to TJD
Declination ....... 2.4663E+01 Experiment ........ ASCA SIS1
Filter ............ NONE
Corrections applied: Vignetting - No ; Deadtime - No ; Bkgd - No ; Clock - No
Selected Columns: 1 - Time; 2 - Y-axis; 3 - Y-error;
File contains binned data.
Ser. A filename 2 +options[.rbf]=>
Enter up to 50 input filenames and options for series 2 (or rtn)
Ser. B filename 1 +options[.rbf]=>
Enter up to 50 input filenames and options for series 3 (or rtn)
Ser. C filename 1 +options[.rbf]=>
[3]xronos>
Maximum of 1 Intvs. with 33 Newbins of 726.148 (s)
Intv 1 Start10760 21:27:49
Ser.1 Avg 0.6764E-01 Chisq 8.731 Var 0.9791E-04 Newbs. 10
Min 0.4916E-01 Max 0.8092E-01expVar 0.1121E-03 Bins 10
Results from Statistical Analysis
Newbin Integration Time (s).. 726.15
Interval Duration (s)........ 18880.
No. of Newbins .............. 10
Average (c/s) ............... 0.67636E-01 +/- 0.35E-02
Standard Deviation (c/s)..... 0.98948E-02
Minimum (c/s)................ 0.49160E-01
Maximum (c/s)................ 0.80922E-01
Variance ((c/s)**2).......... 0.97908E-04 +/- 0.46E-04
Expected Variance ((c/s)**2). 0.11213E-03 +/- 0.53E-04
Third Moment ((c/s)**3)......-0.37582E-06
Average Deviation (c/s)...... 0.86798E-02
Skewness.....................-0.38794 +/- 0.77
Kurtosis..................... -1.0441 +/- 1.5
RMS fractional variation....< 0.22900 (3 sigma)
Chi-Square................... 8.7315 dof 9
Chi-Square Prob of constancy. 0.46235 (0 means < 1.e-38)
Kolm.-Smir. Prob of constancy 0.27464 (0 means < 1.e-38)
[4]xronos> [5]xronos>
Maximum of 1 Intvs. with 33 Newbins of 726.148 (s)
Intv 1 Start10760 21:27:49
Ser.1 Avg 0.6764E-01 Chisq 8.731 Var 0.9791E-04 Newbs. 10
Min 0.4916E-01 Max 0.8092E-01expVar 0.1121E-03 Bins 10
Light curve ready !
Frme 1 Written to output file : xronos.qlc1
PLT> LA File ad55014000s100002_0.lc
PLT> hard /ps
PLT> [6]xronos>
-> TIMEDEL=5.0000000000E-01 for ad55014000g200170m.evtad55014000g200170m.evt[2] ad55014000g200270l.evt[2] ad55014000g200370h.evt[2]-> Making L1 light curve of ft971108_2038_0350G2HK.fits with irate=HIGH
ghkcurve: ALLGTI found in input HK file, will be applied to data. ghkcurve: 4120 output records from 4123 good input G2_L1 records.-> Making L1 light curve of ft971108_2038_0350G2HK.fits with irate=HI+MED
ghkcurve: ALLGTI found in input HK file, will be applied to data. ghkcurve: 8851 output records from 10964 good input G2_L1 records.-> Merging GTIs from the following files:
ad55014000g300170m.evt[2] ad55014000g300270l.evt[2] ad55014000g300370h.evt[2]-> Making L1 light curve of ft971108_2038_0350G3HK.fits with irate=HIGH
ghkcurve: ALLGTI found in input HK file, will be applied to data. ghkcurve: 4002 output records from 4005 good input G3_L1 records.-> Making L1 light curve of ft971108_2038_0350G3HK.fits with irate=HI+MED
ghkcurve: ALLGTI found in input HK file, will be applied to data. ghkcurve: 8741 output records from 10795 good input G3_L1 records.
*** tlmFrm Version 1.1 (1997-08-25) ***
total number of superframes: 3214
frame data: 153175526.417752 ---> 153175670.417308
S1, C2, 4 ccd mode; Output File = fr971108_2038.0350_s1c2m4a.fits
frame data: 153175690.417246 ---> 153175834.416803
S1, C3, 4 ccd mode; Output File = fr971108_2038.0350_s1c3m4a.fits
frame data: 153175854.416741 ---> 153175998.416295
S1, C0, 4 ccd mode; Output File = fr971108_2038.0350_s1c0m4a.fits
frame data: 153176018.416234 ---> 153176162.415788
S1, C1, 4 ccd mode; Output File = fr971108_2038.0350_s1c1m4a.fits
frame data: 153181546.399081 ---> 153181690.398631
S0, C3, 2 ccd mode; Output File = fr971108_2038.0350_s0c3m2a.fits
frame data: 153181710.398569 ---> 153181854.398117
S0, C0, 2 ccd mode; Output File = fr971108_2038.0350_s0c0m2a.fits
frame data: 153181874.398054 ---> 153182018.397602
S0, C3, 2 ccd mode; Output File = fr971108_2038.0350_s0c3m2b.fits
frame data: 153182038.397539 ---> 153182182.397085
S0, C0, 2 ccd mode; Output File = fr971108_2038.0350_s0c0m2b.fits
Total of 8 sets of frame data are extracted.
-> Processing fr971108_2038.0350_s0c0m2a.fitsDark upper (ADU) : 40 Dark lower (ADU) : -40 Input frame data : fr971108_2038.0350_s0c0m2a.fits Output zero level image : rdd.tmp Bias level = 339-> Adding keywords to header of fr971108_2038.0350_s0c0m2a.fits
Dark upper (ADU) : 40 Dark lower (ADU) : -40 Input frame data : fr971108_2038.0350_s0c0m2b.fits Output zero level image : rdd.tmp Bias level = 339-> Adding keywords to header of fr971108_2038.0350_s0c0m2b.fits
Dark upper (ADU) : 40 Dark lower (ADU) : -40 Input frame data : fr971108_2038.0350_s0c3m2a.fits Output zero level image : rdd.tmp Bias level = 316-> Adding keywords to header of fr971108_2038.0350_s0c3m2a.fits
Dark upper (ADU) : 40 Dark lower (ADU) : -40 Input frame data : fr971108_2038.0350_s0c3m2b.fits Output zero level image : rdd.tmp Bias level = 316-> Adding keywords to header of fr971108_2038.0350_s0c3m2b.fits
Dark upper (ADU) : 40 Dark lower (ADU) : -40 Input frame data : fr971108_2038.0350_s1c0m4a.fits Output zero level image : rdd.tmp Bias level = 226-> Adding keywords to header of fr971108_2038.0350_s1c0m4a.fits
Dark upper (ADU) : 40 Dark lower (ADU) : -40 Input frame data : fr971108_2038.0350_s1c1m4a.fits Output zero level image : rdd.tmp Bias level = 194-> Adding keywords to header of fr971108_2038.0350_s1c1m4a.fits
Dark upper (ADU) : 40 Dark lower (ADU) : -40 Input frame data : fr971108_2038.0350_s1c2m4a.fits Output zero level image : rdd.tmp Bias level = 185-> Adding keywords to header of fr971108_2038.0350_s1c2m4a.fits
Dark upper (ADU) : 40 Dark lower (ADU) : -40 Input frame data : fr971108_2038.0350_s1c3m4a.fits Output zero level image : rdd.tmp Bias level = 221-> Adding keywords to header of fr971108_2038.0350_s1c3m4a.fits
SUNSHINE==0 && T_DY_NT>64 && T_SAA>64 && SAA==0 && COR>6 && (ELV>10 || ELV<10 )-> Extracting GTIs from ft971108_2038_0350.mkf
1 ad55014000g200170m.unf 15395 1 ad55014000g200270l.unf 15395 1 ad55014000g200370h.unf 15395-> Fetching GIS2_CALSRC256.2
XSPEC 9.01 13:56:01 29-Dec-99
Plot device not set, use "cpd" to set it
Type "help" or "?" for further information
!XSPEC> query yes
Querying disabled - assuming answer is yes
!XSPEC> data ad55014000g220170.cal
Net count rate (cts/s) for file 1 0.1469 +/- 2.7916E-03
1 data set is in use
!XSPEC> ignore bad
!XSPEC> ignore **-4.0
!XSPEC> ignore 8.0-**
!XSPEC> model const/b + gauss/b + gauss/b
Background components must be from the additive model list
mo = constant[1] ) + gaussian/b[2] + gaussian/b[3]
Input parameter value, delta, min, bot, top, and max values for ...
Mod parameter 1 of component 1 constant factor
1.000 1.0000E-02 0. 0. 1.0000E+10 1.0000E+10
!
Mod parameter 2 of component 2 gaussian LineE
6.500 5.0000E-02 0. 0. 1.0000E+06 1.0000E+06
! 5.9
Mod parameter 3 of component 2 gaussian Sigma
0.1000 5.0000E-02 0. 0. 10.00 20.00
! 0.0
Mod parameter 4 of component 2 gaussian norm
1.000 1.0000E-02 0. 0. 1.0000E+24 1.0000E+24
!
Mod parameter 5 of component 3 gaussian LineE
6.500 5.0000E-02 0. 0. 1.0000E+06 1.0000E+06
! 6.5
Mod parameter 6 of component 3 gaussian Sigma
0.1000 5.0000E-02 0. 0. 10.00 20.00
! 0.0
Mod parameter 7 of component 3 gaussian norm
1.000 1.0000E-02 0. 0. 1.0000E+24 1.0000E+24
!
---------------------------------------------------------------------------
---------------------------------------------------------------------------
mo = constant[1] ) + gaussian/b[2] + gaussian/b[3]
Model Fit Model Component Parameter Value
par par comp
1 1 1 constant factor 1.00000 +/- 0.
2 2 2 gaussian/b LineE 5.90000 +/- 0.
3 3 2 gaussian/b Sigma 0. +/- 0.
4 4 2 gaussian/b norm 1.00000 +/- 0.
5 5 3 gaussian/b LineE 6.50000 +/- 0.
6 6 3 gaussian/b Sigma 0. +/- 0.
7 7 3 gaussian/b norm 1.00000 +/- 0.
---------------------------------------------------------------------------
---------------------------------------------------------------------------
7 variable fit parameters
Chi-Squared = 8.9302E+05 using 84 PHA bins.
Reduced chi-squared = 1.1598E+04
!XSPEC> newpar 5 = 2 1.101005
6 variable fit parameters
Chi-Squared = 8.8591E+05 using 84 PHA bins.
Reduced chi-squared = 1.1358E+04
!XSPEC> newpar 6 = 3 1.049288
5 variable fit parameters
Chi-Squared = 8.8591E+05 using 84 PHA bins.
Reduced chi-squared = 1.1214E+04
!XSPEC> renorm
Chi-Squared = 739.9 using 84 PHA bins.
Reduced chi-squared = 9.366
!XSPEC> fit
Chi-Squared Lvl Fit param # 1 2 3 4
5
Due to zero model norms
fit parameter 1 is temporarily frozen
600.97 0 1.000 5.893 9.3428E-02 4.2179E-02
3.7495E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
306.75 0 1.000 5.870 0.1443 6.0062E-02
3.3113E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
171.75 -1 1.000 5.923 0.1642 8.2442E-02
2.2766E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
144.70 -2 1.000 5.976 0.1922 9.5151E-02
1.4470E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
144.27 -3 1.000 5.969 0.1863 9.4101E-02
1.5509E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
144.25 -4 1.000 5.970 0.1867 9.4364E-02
1.5247E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
144.25 -5 1.000 5.970 0.1864 9.4301E-02
1.5310E-02
---------------------------------------------------------------------------
---------------------------------------------------------------------------
mo = constant[1] ) + gaussian/b[2] + gaussian/b[3]
Model Fit Model Component Parameter Value
par par comp
1 1 1 constant factor 1.00000 +/- -1.0000
2 2 2 gaussian/b LineE 5.96974 +/- 0.11083E-01
3 3 2 gaussian/b Sigma 0.186378 +/- 0.12151E-01
4 4 2 gaussian/b norm 9.430070E-02 +/- 0.28200E-02
5 2 3 gaussian/b LineE 6.57271 = par 2 * 1.1010
6 3 3 gaussian/b Sigma 0.195564 = par 3 * 1.0493
7 5 3 gaussian/b norm 1.531015E-02 +/- 0.19142E-02
---------------------------------------------------------------------------
---------------------------------------------------------------------------
Chi-Squared = 144.2 using 84 PHA bins.
Reduced chi-squared = 1.826
!XSPEC> setplot energy
!XSPEC> iplot data
!PLT> label top GIS2 Calibration Source, should peak near 5.9 keV
!PLT> log x off
!PLT> rescale x 4 8
!PLT> hard /ps
!PLT> quit
!XSPEC> exit
!Do you really want to exit (y) y
XSPEC: quit
-> Calibration source ad55014000g220170.cal peaks at 5.96974 +/- 0.011083 keV1 ad55014000g300170m.unf 14174 1 ad55014000g300270l.unf 14174 1 ad55014000g300370h.unf 14174-> Fetching GIS3_CALSRC256.2
XSPEC 9.01 13:56:52 29-Dec-99
Plot device not set, use "cpd" to set it
Type "help" or "?" for further information
!XSPEC> query yes
Querying disabled - assuming answer is yes
!XSPEC> data ad55014000g320170.cal
Net count rate (cts/s) for file 1 0.1294 +/- 2.6277E-03
1 data set is in use
!XSPEC> ignore bad
!XSPEC> ignore **-4.0
!XSPEC> ignore 8.0-**
!XSPEC> model const/b + gauss/b + gauss/b
Background components must be from the additive model list
mo = constant[1] ) + gaussian/b[2] + gaussian/b[3]
Input parameter value, delta, min, bot, top, and max values for ...
Mod parameter 1 of component 1 constant factor
1.000 1.0000E-02 0. 0. 1.0000E+10 1.0000E+10
!
Mod parameter 2 of component 2 gaussian LineE
6.500 5.0000E-02 0. 0. 1.0000E+06 1.0000E+06
! 5.9
Mod parameter 3 of component 2 gaussian Sigma
0.1000 5.0000E-02 0. 0. 10.00 20.00
! 0.0
Mod parameter 4 of component 2 gaussian norm
1.000 1.0000E-02 0. 0. 1.0000E+24 1.0000E+24
!
Mod parameter 5 of component 3 gaussian LineE
6.500 5.0000E-02 0. 0. 1.0000E+06 1.0000E+06
! 6.5
Mod parameter 6 of component 3 gaussian Sigma
0.1000 5.0000E-02 0. 0. 10.00 20.00
! 0.0
Mod parameter 7 of component 3 gaussian norm
1.000 1.0000E-02 0. 0. 1.0000E+24 1.0000E+24
!
---------------------------------------------------------------------------
---------------------------------------------------------------------------
mo = constant[1] ) + gaussian/b[2] + gaussian/b[3]
Model Fit Model Component Parameter Value
par par comp
1 1 1 constant factor 1.00000 +/- 0.
2 2 2 gaussian/b LineE 5.90000 +/- 0.
3 3 2 gaussian/b Sigma 0. +/- 0.
4 4 2 gaussian/b norm 1.00000 +/- 0.
5 5 3 gaussian/b LineE 6.50000 +/- 0.
6 6 3 gaussian/b Sigma 0. +/- 0.
7 7 3 gaussian/b norm 1.00000 +/- 0.
---------------------------------------------------------------------------
---------------------------------------------------------------------------
7 variable fit parameters
Chi-Squared = 1.0937E+06 using 84 PHA bins.
Reduced chi-squared = 1.4204E+04
!XSPEC> newpar 5 = 2 1.101005
6 variable fit parameters
Chi-Squared = 1.0860E+06 using 84 PHA bins.
Reduced chi-squared = 1.3924E+04
!XSPEC> newpar 6 = 3 1.049288
5 variable fit parameters
Chi-Squared = 1.0860E+06 using 84 PHA bins.
Reduced chi-squared = 1.3747E+04
!XSPEC> renorm
Chi-Squared = 818.2 using 84 PHA bins.
Reduced chi-squared = 10.36
!XSPEC> fit
Chi-Squared Lvl Fit param # 1 2 3 4
5
Due to zero model norms
fit parameter 1 is temporarily frozen
653.60 0 1.000 5.893 0.1002 3.6192E-02
3.0907E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
256.78 0 1.000 5.863 0.1440 5.8124E-02
2.6605E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
100.78 -1 1.000 5.911 0.1505 8.3306E-02
1.7012E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
93.219 -2 1.000 5.929 0.1588 8.9830E-02
1.3470E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
93.014 -3 1.000 5.926 0.1548 8.9332E-02
1.3976E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
93.013 -1 1.000 5.926 0.1551 8.9406E-02
1.3901E-02
---------------------------------------------------------------------------
---------------------------------------------------------------------------
mo = constant[1] ) + gaussian/b[2] + gaussian/b[3]
Model Fit Model Component Parameter Value
par par comp
1 1 1 constant factor 1.00000 +/- -1.0000
2 2 2 gaussian/b LineE 5.92601 +/- 0.96316E-02
3 3 2 gaussian/b Sigma 0.155092 +/- 0.11506E-01
4 4 2 gaussian/b norm 8.940628E-02 +/- 0.25933E-02
5 2 3 gaussian/b LineE 6.52456 = par 2 * 1.1010
6 3 3 gaussian/b Sigma 0.162736 = par 3 * 1.0493
7 5 3 gaussian/b norm 1.390121E-02 +/- 0.16182E-02
---------------------------------------------------------------------------
---------------------------------------------------------------------------
Chi-Squared = 93.01 using 84 PHA bins.
Reduced chi-squared = 1.177
!XSPEC> setplot energy
!XSPEC> iplot data
!PLT> label top GIS3 Calibration Source, should peak near 5.9 keV
!PLT> log x off
!PLT> rescale x 4 8
!PLT> hard /ps
!PLT> quit
!XSPEC> exit
!Do you really want to exit (y) y
XSPEC: quit
-> Calibration source ad55014000g320170.cal peaks at 5.92601 +/- 0.0096316 keV
CLEANSIS_V1.6
allocating image arrays...
PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS.
* Anomalous pixels may consist of at least two populations.
1. Persistent HOT pixels are removed by comparing to the chip mean.
2. Flickering WARM pixels are removed by comparing to the cell mean.
3. In faint areas (zero bgd), flickering pixels are removed with a
cutoff threshold.
Hints:
Choose cell size and thresholds based on the expected background and the PSF.
Use the DIRTYSIS option to examine the anomalous pixel spectra.
Try a multiple pass clean:
Choose a PHA cut to optimize the S/N of the flickering pixels,
then a broad band clean.
Be suspicious of extended source cleans.
For very bright sources you may need to turn off the iteration option.
See the help page for further info (fhelp cleansis)
Poisson clean cell size : 5
Poisson probability threshold : 0.575E-05
Zero Bgd Cutoff threshold (>) : 3
Iterate : F
Dirtysis : F
Minimum PHA value (inclusive) : 0
Maximum PHA value (inclusive) : 4095
open output file: ad55014000s000102m.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 63
copy bad pix array...
cleaning chip # 0
cleaning chip # 1
Hot pixels & counts : 2 48
Flickering pixels iter, pixels & cnts : 1 1 3
cleaning chip # 2
cleaning chip # 3
Number of pixels rejected : 3
Number of (internal) image counts : 63
Number of image cts rejected (N, %) : 5180.95
By chip : 0 1 2 3
Pixels rejected : 0 3 0 0
Image counts : 0 63 0 0
Image cts rejected: 0 51 0 0
Image cts rej (%) : 0.00 80.95 0.00 0.00
filtering data...
Total counts : 0 63 0 0
Total cts rejected: 0 51 0 0
Total cts rej (%) : 0.00 80.95 0.00 0.00
Number of clean counts accepted : 12
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 3
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad55014000s000112m.unf
CLEANSIS_V1.6
allocating image arrays...
PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS.
* Anomalous pixels may consist of at least two populations.
1. Persistent HOT pixels are removed by comparing to the chip mean.
2. Flickering WARM pixels are removed by comparing to the cell mean.
3. In faint areas (zero bgd), flickering pixels are removed with a
cutoff threshold.
Hints:
Choose cell size and thresholds based on the expected background and the PSF.
Use the DIRTYSIS option to examine the anomalous pixel spectra.
Try a multiple pass clean:
Choose a PHA cut to optimize the S/N of the flickering pixels,
then a broad band clean.
Be suspicious of extended source cleans.
For very bright sources you may need to turn off the iteration option.
See the help page for further info (fhelp cleansis)
Poisson clean cell size : 5
Poisson probability threshold : 0.575E-05
Zero Bgd Cutoff threshold (>) : 3
Iterate : F
Dirtysis : F
Minimum PHA value (inclusive) : 0
Maximum PHA value (inclusive) : 4095
open output file: ad55014000s000112m.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 68
copy bad pix array...
cleaning chip # 0
cleaning chip # 1
Hot pixels & counts : 2 48
Flickering pixels iter, pixels & cnts : 1 1 3
cleaning chip # 2
cleaning chip # 3
Number of pixels rejected : 3
Number of (internal) image counts : 68
Number of image cts rejected (N, %) : 5175.00
By chip : 0 1 2 3
Pixels rejected : 0 3 0 0
Image counts : 0 68 0 0
Image cts rejected: 0 51 0 0
Image cts rej (%) : 0.00 75.00 0.00 0.00
filtering data...
Total counts : 0 68 0 0
Total cts rejected: 0 51 0 0
Total cts rej (%) : 0.00 75.00 0.00 0.00
Number of clean counts accepted : 17
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 3
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad55014000s000202l.unf
CLEANSIS_V1.6
allocating image arrays...
PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS.
* Anomalous pixels may consist of at least two populations.
1. Persistent HOT pixels are removed by comparing to the chip mean.
2. Flickering WARM pixels are removed by comparing to the cell mean.
3. In faint areas (zero bgd), flickering pixels are removed with a
cutoff threshold.
Hints:
Choose cell size and thresholds based on the expected background and the PSF.
Use the DIRTYSIS option to examine the anomalous pixel spectra.
Try a multiple pass clean:
Choose a PHA cut to optimize the S/N of the flickering pixels,
then a broad band clean.
Be suspicious of extended source cleans.
For very bright sources you may need to turn off the iteration option.
See the help page for further info (fhelp cleansis)
Poisson clean cell size : 5
Poisson probability threshold : 0.575E-05
Zero Bgd Cutoff threshold (>) : 3
Iterate : F
Dirtysis : F
Minimum PHA value (inclusive) : 0
Maximum PHA value (inclusive) : 4095
open output file: ad55014000s000202l.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 3191
copy bad pix array...
cleaning chip # 0
cleaning chip # 1
Hot pixels & counts : 6 2806
Flickering pixels iter, pixels & cnts : 1 7 48
cleaning chip # 2
cleaning chip # 3
Number of pixels rejected : 13
Number of (internal) image counts : 3191
Number of image cts rejected (N, %) : 285489.44
By chip : 0 1 2 3
Pixels rejected : 0 13 0 0
Image counts : 0 3191 0 0
Image cts rejected: 0 2854 0 0
Image cts rej (%) : 0.00 89.44 0.00 0.00
filtering data...
Total counts : 0 3191 0 0
Total cts rejected: 0 2854 0 0
Total cts rej (%) : 0.00 89.44 0.00 0.00
Number of clean counts accepted : 337
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 13
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad55014000s000212l.unf
CLEANSIS_V1.6
allocating image arrays...
PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS.
* Anomalous pixels may consist of at least two populations.
1. Persistent HOT pixels are removed by comparing to the chip mean.
2. Flickering WARM pixels are removed by comparing to the cell mean.
3. In faint areas (zero bgd), flickering pixels are removed with a
cutoff threshold.
Hints:
Choose cell size and thresholds based on the expected background and the PSF.
Use the DIRTYSIS option to examine the anomalous pixel spectra.
Try a multiple pass clean:
Choose a PHA cut to optimize the S/N of the flickering pixels,
then a broad band clean.
Be suspicious of extended source cleans.
For very bright sources you may need to turn off the iteration option.
See the help page for further info (fhelp cleansis)
Poisson clean cell size : 5
Poisson probability threshold : 0.575E-05
Zero Bgd Cutoff threshold (>) : 3
Iterate : F
Dirtysis : F
Minimum PHA value (inclusive) : 0
Maximum PHA value (inclusive) : 4095
open output file: ad55014000s000212l.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 3255
copy bad pix array...
cleaning chip # 0
cleaning chip # 1
Hot pixels & counts : 6 2806
Flickering pixels iter, pixels & cnts : 1 7 48
cleaning chip # 2
cleaning chip # 3
Number of pixels rejected : 13
Number of (internal) image counts : 3255
Number of image cts rejected (N, %) : 285487.68
By chip : 0 1 2 3
Pixels rejected : 0 13 0 0
Image counts : 0 3255 0 0
Image cts rejected: 0 2854 0 0
Image cts rej (%) : 0.00 87.68 0.00 0.00
filtering data...
Total counts : 0 3255 0 0
Total cts rejected: 0 2854 0 0
Total cts rej (%) : 0.00 87.68 0.00 0.00
Number of clean counts accepted : 401
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 13
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad55014000s000302h.unf
CLEANSIS_V1.6
allocating image arrays...
PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS.
* Anomalous pixels may consist of at least two populations.
1. Persistent HOT pixels are removed by comparing to the chip mean.
2. Flickering WARM pixels are removed by comparing to the cell mean.
3. In faint areas (zero bgd), flickering pixels are removed with a
cutoff threshold.
Hints:
Choose cell size and thresholds based on the expected background and the PSF.
Use the DIRTYSIS option to examine the anomalous pixel spectra.
Try a multiple pass clean:
Choose a PHA cut to optimize the S/N of the flickering pixels,
then a broad band clean.
Be suspicious of extended source cleans.
For very bright sources you may need to turn off the iteration option.
See the help page for further info (fhelp cleansis)
Poisson clean cell size : 5
Poisson probability threshold : 0.575E-05
Zero Bgd Cutoff threshold (>) : 3
Iterate : F
Dirtysis : F
Minimum PHA value (inclusive) : 0
Maximum PHA value (inclusive) : 4095
open output file: ad55014000s000302h.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 273
copy bad pix array...
cleaning chip # 0
cleaning chip # 1
Hot pixels & counts : 5 243
Flickering pixels iter, pixels & cnts : 1 1 6
cleaning chip # 2
cleaning chip # 3
Number of pixels rejected : 6
Number of (internal) image counts : 273
Number of image cts rejected (N, %) : 24991.21
By chip : 0 1 2 3
Pixels rejected : 0 6 0 0
Image counts : 0 273 0 0
Image cts rejected: 0 249 0 0
Image cts rej (%) : 0.00 91.21 0.00 0.00
filtering data...
Total counts : 0 273 0 0
Total cts rejected: 0 249 0 0
Total cts rej (%) : 0.00 91.21 0.00 0.00
Number of clean counts accepted : 24
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 6
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad55014000s000312h.unf
CLEANSIS_V1.6
allocating image arrays...
PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS.
* Anomalous pixels may consist of at least two populations.
1. Persistent HOT pixels are removed by comparing to the chip mean.
2. Flickering WARM pixels are removed by comparing to the cell mean.
3. In faint areas (zero bgd), flickering pixels are removed with a
cutoff threshold.
Hints:
Choose cell size and thresholds based on the expected background and the PSF.
Use the DIRTYSIS option to examine the anomalous pixel spectra.
Try a multiple pass clean:
Choose a PHA cut to optimize the S/N of the flickering pixels,
then a broad band clean.
Be suspicious of extended source cleans.
For very bright sources you may need to turn off the iteration option.
See the help page for further info (fhelp cleansis)
Poisson clean cell size : 5
Poisson probability threshold : 0.575E-05
Zero Bgd Cutoff threshold (>) : 3
Iterate : F
Dirtysis : F
Minimum PHA value (inclusive) : 0
Maximum PHA value (inclusive) : 4095
open output file: ad55014000s000312h.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 279
copy bad pix array...
cleaning chip # 0
cleaning chip # 1
Hot pixels & counts : 6 249
cleaning chip # 2
cleaning chip # 3
Number of pixels rejected : 6
Number of (internal) image counts : 279
Number of image cts rejected (N, %) : 24989.25
By chip : 0 1 2 3
Pixels rejected : 0 6 0 0
Image counts : 0 279 0 0
Image cts rejected: 0 249 0 0
Image cts rej (%) : 0.00 89.25 0.00 0.00
filtering data...
Total counts : 0 279 0 0
Total cts rejected: 0 249 0 0
Total cts rej (%) : 0.00 89.25 0.00 0.00
Number of clean counts accepted : 30
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 6
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad55014000s000402h.unf
CLEANSIS_V1.6
allocating image arrays...
PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS.
* Anomalous pixels may consist of at least two populations.
1. Persistent HOT pixels are removed by comparing to the chip mean.
2. Flickering WARM pixels are removed by comparing to the cell mean.
3. In faint areas (zero bgd), flickering pixels are removed with a
cutoff threshold.
Hints:
Choose cell size and thresholds based on the expected background and the PSF.
Use the DIRTYSIS option to examine the anomalous pixel spectra.
Try a multiple pass clean:
Choose a PHA cut to optimize the S/N of the flickering pixels,
then a broad band clean.
Be suspicious of extended source cleans.
For very bright sources you may need to turn off the iteration option.
See the help page for further info (fhelp cleansis)
Poisson clean cell size : 5
Poisson probability threshold : 0.575E-05
Zero Bgd Cutoff threshold (>) : 3
Iterate : F
Dirtysis : F
Minimum PHA value (inclusive) : 0
Maximum PHA value (inclusive) : 4095
open output file: ad55014000s000402h.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 3234
copy bad pix array...
cleaning chip # 0
Hot pixels & counts : 62 1775
Flickering pixels iter, pixels & cnts : 1 29 238
cleaning chip # 1
cleaning chip # 2
cleaning chip # 3
Hot pixels & counts : 36 895
Flickering pixels iter, pixels & cnts : 1 15 91
Number of pixels rejected : 142
Number of (internal) image counts : 3234
Number of image cts rejected (N, %) : 299992.73
By chip : 0 1 2 3
Pixels rejected : 91 0 0 51
Image counts : 2200 0 0 1034
Image cts rejected: 2013 0 0 986
Image cts rej (%) : 91.50 0.00 0.00 95.36
filtering data...
Total counts : 2200 0 0 1034
Total cts rejected: 2013 0 0 986
Total cts rej (%) : 91.50 0.00 0.00 95.36
Number of clean counts accepted : 235
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 142
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad55014000s000412h.unf
CLEANSIS_V1.6
allocating image arrays...
PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS.
* Anomalous pixels may consist of at least two populations.
1. Persistent HOT pixels are removed by comparing to the chip mean.
2. Flickering WARM pixels are removed by comparing to the cell mean.
3. In faint areas (zero bgd), flickering pixels are removed with a
cutoff threshold.
Hints:
Choose cell size and thresholds based on the expected background and the PSF.
Use the DIRTYSIS option to examine the anomalous pixel spectra.
Try a multiple pass clean:
Choose a PHA cut to optimize the S/N of the flickering pixels,
then a broad band clean.
Be suspicious of extended source cleans.
For very bright sources you may need to turn off the iteration option.
See the help page for further info (fhelp cleansis)
Poisson clean cell size : 5
Poisson probability threshold : 0.575E-05
Zero Bgd Cutoff threshold (>) : 3
Iterate : F
Dirtysis : F
Minimum PHA value (inclusive) : 0
Maximum PHA value (inclusive) : 4095
open output file: ad55014000s000412h.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 3262
copy bad pix array...
cleaning chip # 0
Hot pixels & counts : 61 1761
Flickering pixels iter, pixels & cnts : 1 30 253
cleaning chip # 1
cleaning chip # 2
cleaning chip # 3
Hot pixels & counts : 34 875
Flickering pixels iter, pixels & cnts : 1 17 111
Number of pixels rejected : 142
Number of (internal) image counts : 3262
Number of image cts rejected (N, %) : 300091.97
By chip : 0 1 2 3
Pixels rejected : 91 0 0 51
Image counts : 2219 0 0 1043
Image cts rejected: 2014 0 0 986
Image cts rej (%) : 90.76 0.00 0.00 94.53
filtering data...
Total counts : 2219 0 0 1043
Total cts rejected: 2014 0 0 986
Total cts rej (%) : 90.76 0.00 0.00 94.53
Number of clean counts accepted : 262
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 142
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad55014000s100102m.unf
CLEANSIS_V1.6
allocating image arrays...
PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS.
* Anomalous pixels may consist of at least two populations.
1. Persistent HOT pixels are removed by comparing to the chip mean.
2. Flickering WARM pixels are removed by comparing to the cell mean.
3. In faint areas (zero bgd), flickering pixels are removed with a
cutoff threshold.
Hints:
Choose cell size and thresholds based on the expected background and the PSF.
Use the DIRTYSIS option to examine the anomalous pixel spectra.
Try a multiple pass clean:
Choose a PHA cut to optimize the S/N of the flickering pixels,
then a broad band clean.
Be suspicious of extended source cleans.
For very bright sources you may need to turn off the iteration option.
See the help page for further info (fhelp cleansis)
Poisson clean cell size : 5
Poisson probability threshold : 0.575E-05
Zero Bgd Cutoff threshold (>) : 3
Iterate : F
Dirtysis : F
Minimum PHA value (inclusive) : 0
Maximum PHA value (inclusive) : 4095
open output file: ad55014000s100102m.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 227
copy bad pix array...
cleaning chip # 0
cleaning chip # 1
Hot pixels & counts : 10 206
Flickering pixels iter, pixels & cnts : 1 1 4
cleaning chip # 2
cleaning chip # 3
Number of pixels rejected : 11
Number of (internal) image counts : 227
Number of image cts rejected (N, %) : 21092.51
By chip : 0 1 2 3
Pixels rejected : 0 11 0 0
Image counts : 0 227 0 0
Image cts rejected: 0 210 0 0
Image cts rej (%) : 0.00 92.51 0.00 0.00
filtering data...
Total counts : 0 227 0 0
Total cts rejected: 0 210 0 0
Total cts rej (%) : 0.00 92.51 0.00 0.00
Number of clean counts accepted : 17
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 11
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad55014000s100112m.unf
CLEANSIS_V1.6
allocating image arrays...
PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS.
* Anomalous pixels may consist of at least two populations.
1. Persistent HOT pixels are removed by comparing to the chip mean.
2. Flickering WARM pixels are removed by comparing to the cell mean.
3. In faint areas (zero bgd), flickering pixels are removed with a
cutoff threshold.
Hints:
Choose cell size and thresholds based on the expected background and the PSF.
Use the DIRTYSIS option to examine the anomalous pixel spectra.
Try a multiple pass clean:
Choose a PHA cut to optimize the S/N of the flickering pixels,
then a broad band clean.
Be suspicious of extended source cleans.
For very bright sources you may need to turn off the iteration option.
See the help page for further info (fhelp cleansis)
Poisson clean cell size : 5
Poisson probability threshold : 0.575E-05
Zero Bgd Cutoff threshold (>) : 3
Iterate : F
Dirtysis : F
Minimum PHA value (inclusive) : 0
Maximum PHA value (inclusive) : 4095
open output file: ad55014000s100112m.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 232
copy bad pix array...
cleaning chip # 0
cleaning chip # 1
Hot pixels & counts : 10 206
Flickering pixels iter, pixels & cnts : 1 1 4
cleaning chip # 2
cleaning chip # 3
Number of pixels rejected : 11
Number of (internal) image counts : 232
Number of image cts rejected (N, %) : 21090.52
By chip : 0 1 2 3
Pixels rejected : 0 11 0 0
Image counts : 0 232 0 0
Image cts rejected: 0 210 0 0
Image cts rej (%) : 0.00 90.52 0.00 0.00
filtering data...
Total counts : 0 232 0 0
Total cts rejected: 0 210 0 0
Total cts rej (%) : 0.00 90.52 0.00 0.00
Number of clean counts accepted : 22
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 11
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad55014000s100202h.unf
CLEANSIS_V1.6
allocating image arrays...
PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS.
* Anomalous pixels may consist of at least two populations.
1. Persistent HOT pixels are removed by comparing to the chip mean.
2. Flickering WARM pixels are removed by comparing to the cell mean.
3. In faint areas (zero bgd), flickering pixels are removed with a
cutoff threshold.
Hints:
Choose cell size and thresholds based on the expected background and the PSF.
Use the DIRTYSIS option to examine the anomalous pixel spectra.
Try a multiple pass clean:
Choose a PHA cut to optimize the S/N of the flickering pixels,
then a broad band clean.
Be suspicious of extended source cleans.
For very bright sources you may need to turn off the iteration option.
See the help page for further info (fhelp cleansis)
Poisson clean cell size : 5
Poisson probability threshold : 0.575E-05
Zero Bgd Cutoff threshold (>) : 3
Iterate : F
Dirtysis : F
Minimum PHA value (inclusive) : 0
Maximum PHA value (inclusive) : 4095
open output file: ad55014000s100202h.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 10773
copy bad pix array...
cleaning chip # 0
Hot pixels & counts : 0 0
Flickering pixels iter, pixels & cnts : 1 316 2402
cleaning chip # 1
Hot pixels & counts : 0 0
Flickering pixels iter, pixels & cnts : 1 310 2346
cleaning chip # 2
Hot pixels & counts : 0 0
Flickering pixels iter, pixels & cnts : 1 314 2379
cleaning chip # 3
Hot pixels & counts : 0 0
Flickering pixels iter, pixels & cnts : 1 307 2028
Number of pixels rejected : 1247
Number of (internal) image counts : 10773
Number of image cts rejected (N, %) : 915584.98
By chip : 0 1 2 3
Pixels rejected : 316 310 314 307
Image counts : 2807 2780 2755 2431
Image cts rejected: 2402 2346 2379 2028
Image cts rej (%) : 85.57 84.39 86.35 83.42
filtering data...
Total counts : 2807 2780 2755 2431
Total cts rejected: 2402 2346 2379 2028
Total cts rej (%) : 85.57 84.39 86.35 83.42
Number of clean counts accepted : 1618
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 1247
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad55014000s100212h.unf
CLEANSIS_V1.6
allocating image arrays...
PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS.
* Anomalous pixels may consist of at least two populations.
1. Persistent HOT pixels are removed by comparing to the chip mean.
2. Flickering WARM pixels are removed by comparing to the cell mean.
3. In faint areas (zero bgd), flickering pixels are removed with a
cutoff threshold.
Hints:
Choose cell size and thresholds based on the expected background and the PSF.
Use the DIRTYSIS option to examine the anomalous pixel spectra.
Try a multiple pass clean:
Choose a PHA cut to optimize the S/N of the flickering pixels,
then a broad band clean.
Be suspicious of extended source cleans.
For very bright sources you may need to turn off the iteration option.
See the help page for further info (fhelp cleansis)
Poisson clean cell size : 5
Poisson probability threshold : 0.575E-05
Zero Bgd Cutoff threshold (>) : 3
Iterate : F
Dirtysis : F
Minimum PHA value (inclusive) : 0
Maximum PHA value (inclusive) : 4095
open output file: ad55014000s100212h.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 12152
copy bad pix array...
cleaning chip # 0
Hot pixels & counts : 0 0
Flickering pixels iter, pixels & cnts : 1 354 2765
cleaning chip # 1
Hot pixels & counts : 0 0
Flickering pixels iter, pixels & cnts : 1 349 2769
cleaning chip # 2
Hot pixels & counts : 0 0
Flickering pixels iter, pixels & cnts : 1 335 2596
cleaning chip # 3
Hot pixels & counts : 0 0
Flickering pixels iter, pixels & cnts : 1 331 2296
Number of pixels rejected : 1369
Number of (internal) image counts : 12152
Number of image cts rejected (N, %) : 1042685.80
By chip : 0 1 2 3
Pixels rejected : 354 349 335 331
Image counts : 3181 3210 2983 2778
Image cts rejected: 2765 2769 2596 2296
Image cts rej (%) : 86.92 86.26 87.03 82.65
filtering data...
Total counts : 3181 3210 2983 2778
Total cts rejected: 2765 2769 2596 2296
Total cts rej (%) : 86.92 86.26 87.03 82.65
Number of clean counts accepted : 1726
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 1369
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad55014000s100302l.unf
CLEANSIS_V1.6
allocating image arrays...
PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS.
* Anomalous pixels may consist of at least two populations.
1. Persistent HOT pixels are removed by comparing to the chip mean.
2. Flickering WARM pixels are removed by comparing to the cell mean.
3. In faint areas (zero bgd), flickering pixels are removed with a
cutoff threshold.
Hints:
Choose cell size and thresholds based on the expected background and the PSF.
Use the DIRTYSIS option to examine the anomalous pixel spectra.
Try a multiple pass clean:
Choose a PHA cut to optimize the S/N of the flickering pixels,
then a broad band clean.
Be suspicious of extended source cleans.
For very bright sources you may need to turn off the iteration option.
See the help page for further info (fhelp cleansis)
Poisson clean cell size : 5
Poisson probability threshold : 0.575E-05
Zero Bgd Cutoff threshold (>) : 3
Iterate : F
Dirtysis : F
Minimum PHA value (inclusive) : 0
Maximum PHA value (inclusive) : 4095
open output file: ad55014000s100302l.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 8276
copy bad pix array...
cleaning chip # 0
cleaning chip # 1
Hot pixels & counts : 12 8030
Flickering pixels iter, pixels & cnts : 1 8 97
cleaning chip # 2
cleaning chip # 3
Number of pixels rejected : 20
Number of (internal) image counts : 8276
Number of image cts rejected (N, %) : 812798.20
By chip : 0 1 2 3
Pixels rejected : 0 20 0 0
Image counts : 0 8276 0 0
Image cts rejected: 0 8127 0 0
Image cts rej (%) : 0.00 98.20 0.00 0.00
filtering data...
Total counts : 0 8276 0 0
Total cts rejected: 0 8127 0 0
Total cts rej (%) : 0.00 98.20 0.00 0.00
Number of clean counts accepted : 149
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 20
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad55014000s100312l.unf
CLEANSIS_V1.6
allocating image arrays...
PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS.
* Anomalous pixels may consist of at least two populations.
1. Persistent HOT pixels are removed by comparing to the chip mean.
2. Flickering WARM pixels are removed by comparing to the cell mean.
3. In faint areas (zero bgd), flickering pixels are removed with a
cutoff threshold.
Hints:
Choose cell size and thresholds based on the expected background and the PSF.
Use the DIRTYSIS option to examine the anomalous pixel spectra.
Try a multiple pass clean:
Choose a PHA cut to optimize the S/N of the flickering pixels,
then a broad band clean.
Be suspicious of extended source cleans.
For very bright sources you may need to turn off the iteration option.
See the help page for further info (fhelp cleansis)
Poisson clean cell size : 5
Poisson probability threshold : 0.575E-05
Zero Bgd Cutoff threshold (>) : 3
Iterate : F
Dirtysis : F
Minimum PHA value (inclusive) : 0
Maximum PHA value (inclusive) : 4095
open output file: ad55014000s100312l.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 8294
copy bad pix array...
cleaning chip # 0
cleaning chip # 1
Hot pixels & counts : 12 8030
Flickering pixels iter, pixels & cnts : 1 8 97
cleaning chip # 2
cleaning chip # 3
Number of pixels rejected : 20
Number of (internal) image counts : 8294
Number of image cts rejected (N, %) : 812797.99
By chip : 0 1 2 3
Pixels rejected : 0 20 0 0
Image counts : 0 8294 0 0
Image cts rejected: 0 8127 0 0
Image cts rej (%) : 0.00 97.99 0.00 0.00
filtering data...
Total counts : 0 8294 0 0
Total cts rejected: 0 8127 0 0
Total cts rej (%) : 0.00 97.99 0.00 0.00
Number of clean counts accepted : 167
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 20
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad55014000s100402h.unf
CLEANSIS_V1.6
allocating image arrays...
PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS.
* Anomalous pixels may consist of at least two populations.
1. Persistent HOT pixels are removed by comparing to the chip mean.
2. Flickering WARM pixels are removed by comparing to the cell mean.
3. In faint areas (zero bgd), flickering pixels are removed with a
cutoff threshold.
Hints:
Choose cell size and thresholds based on the expected background and the PSF.
Use the DIRTYSIS option to examine the anomalous pixel spectra.
Try a multiple pass clean:
Choose a PHA cut to optimize the S/N of the flickering pixels,
then a broad band clean.
Be suspicious of extended source cleans.
For very bright sources you may need to turn off the iteration option.
See the help page for further info (fhelp cleansis)
Poisson clean cell size : 5
Poisson probability threshold : 0.575E-05
Zero Bgd Cutoff threshold (>) : 3
Iterate : F
Dirtysis : F
Minimum PHA value (inclusive) : 0
Maximum PHA value (inclusive) : 4095
open output file: ad55014000s100402h.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 1136
copy bad pix array...
cleaning chip # 0
cleaning chip # 1
Hot pixels & counts : 11 1073
Flickering pixels iter, pixels & cnts : 1 3 16
cleaning chip # 2
cleaning chip # 3
Number of pixels rejected : 14
Number of (internal) image counts : 1136
Number of image cts rejected (N, %) : 108995.86
By chip : 0 1 2 3
Pixels rejected : 0 14 0 0
Image counts : 0 1136 0 0
Image cts rejected: 0 1089 0 0
Image cts rej (%) : 0.00 95.86 0.00 0.00
filtering data...
Total counts : 0 1136 0 0
Total cts rejected: 0 1089 0 0
Total cts rej (%) : 0.00 95.86 0.00 0.00
Number of clean counts accepted : 47
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 14
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad55014000s100412h.unf
CLEANSIS_V1.6
allocating image arrays...
PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS.
* Anomalous pixels may consist of at least two populations.
1. Persistent HOT pixels are removed by comparing to the chip mean.
2. Flickering WARM pixels are removed by comparing to the cell mean.
3. In faint areas (zero bgd), flickering pixels are removed with a
cutoff threshold.
Hints:
Choose cell size and thresholds based on the expected background and the PSF.
Use the DIRTYSIS option to examine the anomalous pixel spectra.
Try a multiple pass clean:
Choose a PHA cut to optimize the S/N of the flickering pixels,
then a broad band clean.
Be suspicious of extended source cleans.
For very bright sources you may need to turn off the iteration option.
See the help page for further info (fhelp cleansis)
Poisson clean cell size : 5
Poisson probability threshold : 0.575E-05
Zero Bgd Cutoff threshold (>) : 3
Iterate : F
Dirtysis : F
Minimum PHA value (inclusive) : 0
Maximum PHA value (inclusive) : 4095
open output file: ad55014000s100412h.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 1144
copy bad pix array...
cleaning chip # 0
cleaning chip # 1
Hot pixels & counts : 11 1073
Flickering pixels iter, pixels & cnts : 1 3 16
cleaning chip # 2
cleaning chip # 3
Number of pixels rejected : 14
Number of (internal) image counts : 1144
Number of image cts rejected (N, %) : 108995.19
By chip : 0 1 2 3
Pixels rejected : 0 14 0 0
Image counts : 0 1144 0 0
Image cts rejected: 0 1089 0 0
Image cts rej (%) : 0.00 95.19 0.00 0.00
filtering data...
Total counts : 0 1144 0 0
Total cts rejected: 0 1089 0 0
Total cts rej (%) : 0.00 95.19 0.00 0.00
Number of clean counts accepted : 55
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 14
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad55014000g200170m.unfOffset of 213408004.000000 from 1993-01-01 00:00:00 is date and time (including leapseconds) = 1999-10-07 00:00:00.00000 Modified Julian Day = 51458.000000000000000-> leapsec.fits already present in current directory
Offset of 197078404.000000 from 1993-01-01 00:00:00 is date and time (including leapseconds) = 1999-04-01 00:00:00.00000 Modified Julian Day = 51269.000000000000000-> leapsec.fits already present in current directory
Offset of 150000000.000000 from 1993-01-01 00:00:00 is date and time (including leapseconds) = 1997-10-03 02:39:56.00000 Modified Julian Day = 50724.111064814816928
ad55014000s000302h.unf|S0CCDPOW|0100|Which S0 CCDs are in use(0123): 0=OFF 1=ON ad55014000s000402h.unf|S0CCDPOW|1001|Which S0 CCDs are in use(0123): 0=OFF 1=ON ad55014000s000302h.unf|S0CCDMOD|1|How many S0 CCDs are in use: 1, 2, or 4 ad55014000s000402h.unf|S0CCDMOD|2|How many S0 CCDs are in use: 1, 2, or 4 ad55014000s000302h.unf|S0CCDLST|1 1 1 1|S0 CCD readout order ad55014000s000402h.unf|S0CCDLST|3 0 3 0|S0 CCD readout order-> listing ad55014000s000302h.unf
ad55014000s000312h.unf|S0CCDPOW|0100|Which S0 CCDs are in use(0123): 0=OFF 1=ON ad55014000s000412h.unf|S0CCDPOW|1001|Which S0 CCDs are in use(0123): 0=OFF 1=ON ad55014000s000312h.unf|S0CCDMOD|1|How many S0 CCDs are in use: 1, 2, or 4 ad55014000s000412h.unf|S0CCDMOD|2|How many S0 CCDs are in use: 1, 2, or 4 ad55014000s000312h.unf|S0CCDLST|1 1 1 1|S0 CCD readout order ad55014000s000412h.unf|S0CCDLST|3 0 3 0|S0 CCD readout order-> listing ad55014000s000312h.unf
ad55014000s000301h.unf|S0CCDPOW|0100|Which S0 CCDs are in use(0123): 0=OFF 1=ON ad55014000s000401h.unf|S0CCDPOW|1001|Which S0 CCDs are in use(0123): 0=OFF 1=ON ad55014000s000301h.unf|S0CCDMOD|1|How many S0 CCDs are in use: 1, 2, or 4 ad55014000s000401h.unf|S0CCDMOD|2|How many S0 CCDs are in use: 1, 2, or 4 ad55014000s000301h.unf|S0CCDLST|1 1 1 1|S0 CCD readout order ad55014000s000401h.unf|S0CCDLST|3 0 3 0|S0 CCD readout order-> listing ad55014000s000301h.unf
ad55014000s100202h.unf|S1CCDPOW|1111|Which S1 CCDs are in use(0123): 0=OFF 1=ON ad55014000s100402h.unf|S1CCDPOW|0100|Which S1 CCDs are in use(0123): 0=OFF 1=ON ad55014000s100202h.unf|S1CCDMOD|4|How many S1 CCDs are in use: 1, 2, or 4 ad55014000s100402h.unf|S1CCDMOD|1|How many S1 CCDs are in use: 1, 2, or 4 ad55014000s100202h.unf|S1CCDLST|2 3 0 1|S1 CCD readout order ad55014000s100402h.unf|S1CCDLST|1 1 1 1|S1 CCD readout order-> listing ad55014000s100202h.unf
ad55014000s100212h.unf|S1CCDPOW|1111|Which S1 CCDs are in use(0123): 0=OFF 1=ON ad55014000s100412h.unf|S1CCDPOW|0100|Which S1 CCDs are in use(0123): 0=OFF 1=ON ad55014000s100212h.unf|S1CCDMOD|4|How many S1 CCDs are in use: 1, 2, or 4 ad55014000s100412h.unf|S1CCDMOD|1|How many S1 CCDs are in use: 1, 2, or 4 ad55014000s100212h.unf|S1CCDLST|2 3 0 1|S1 CCD readout order ad55014000s100412h.unf|S1CCDLST|1 1 1 1|S1 CCD readout order-> listing ad55014000s100212h.unf
ad55014000s100201h.unf|S1CCDPOW|1111|Which S1 CCDs are in use(0123): 0=OFF 1=ON ad55014000s100401h.unf|S1CCDPOW|0100|Which S1 CCDs are in use(0123): 0=OFF 1=ON ad55014000s100201h.unf|S1CCDMOD|4|How many S1 CCDs are in use: 1, 2, or 4 ad55014000s100401h.unf|S1CCDMOD|1|How many S1 CCDs are in use: 1, 2, or 4 ad55014000s100201h.unf|S1CCDLST|2 3 0 1|S1 CCD readout order ad55014000s100401h.unf|S1CCDLST|1 1 1 1|S1 CCD readout order-> listing ad55014000s100201h.unf
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