DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 229
No. |
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
observation_id
|
exposure
|
awarded_exposure
|
xis0_exposure
|
xis1_exposure
|
xis2_exposure
|
xis3_exposure
|
xis0_observation_mode
|
xis1_observation_mode
|
xis2_observation_mode
|
xis3_observation_mode
|
hxd_observation_mode
|
hxd_coarse_clock_rate_exposure
|
hxd_first_clock_rate_exposure
|
hxd_normal_clock_rate_exposure
|
hxd_all_clock_rate_exposure
|
hxd_wam_exposure
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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1 | Crab Nebula | 83.6449 | 22.0152 | 82.892626 | 21.982571 | 84.11016 | -1.295832 | 184.56274906 | -5.77473152 | 84.9987 | 53614.1083449074 | 2005-09-01 02:36:01 | 53614.1771759259 | 2005-09-01 04:15:08 | 100015030 | 2.1 | 5 | 2.1 | 2.1 | 2.1 | 2.1 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 2.3074 | 2.3074 | 5.9439 | 0 | PROCESSED | 57527.235150463 | 2016-05-19 05:38:37 | 54247 | 2007-05-27 00:00:00 | 54109.3966782407 | 2007-01-09 09:31:13 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000015 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | HXD boresight check with Crab | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100015030/ | |||||
2 | E0102-72 | 15.9884 | -72.0403 | 15.58329 | -72.308299 | 314.593543 | -65.036118 | 301.56673438 | -45.05476105 | 119.5512 | 53595.2489236111 | 2005-08-13 05:58:27 | 53595.4618518518 | 2005-08-13 11:05:04 | 100001020 | 4.1598 | 10 | 4.1598 | 4.1598 | 4.1598 | 4.1598 | 1 | 1 | 1 | 2 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | PROCESSED | 57520.6779861111 | 2016-05-12 16:16:18 | 54247 | 2007-05-27 00:00:00 | 54035.6312731482 | 2006-10-27 15:09:02 | 3.0.22.43 | 5 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000001 | XIS door open with a SMC SNR E0102-72 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | XIS door open | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100001020/ | Quick Look | |||
3 | N132D | 81.2751 | -69.6506 | 81.377584 | -69.69262 | 312.405312 | -85.522517 | 280.31335191 | -32.77744994 | 53.3312 | 53598.2402777778 | 2005-08-16 05:46:00 | 53598.5140046296 | 2005-08-16 12:20:10 | 100002060 | 5.9635 | 7 | 5.9635 | 5.9635 | 5.9635 | 5.9635 | 1 | 1 | 1 | 1 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | PROCESSED | 57520.6925115741 | 2016-05-12 16:37:13 | 54247 | 2007-05-27 00:00:00 | 54038.4700810185 | 2006-10-30 11:16:55 | 3.0.22.43 | 6 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000002 | HXD HV ON WITH N132D, and 5 pointings with XIS | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | HXD HV ON WITH N132D | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100002060/ | Quick Look | |||
4 | DEM_L71/N23 | 76.4474 | -67.958 | 76.476582 | -68.023213 | 338.826937 | -84.59461 | 278.75859594 | -34.83581885 | 70.5849 | 53598.5206365741 | 2005-08-16 12:29:43 | 53599.6042592593 | 2005-08-17 14:30:08 | 100003010 | 5.7897 | 40 | 5.7897 | 5.7897 | 5.7897 | 5.7897 | 2 | 2 | 2 | 2 | 0 | 0 | 0 | 0 | 0 | 93.6061 | 0 | PROCESSED | 57520.7098611111 | 2016-05-12 17:02:12 | 54247 | 2007-05-27 00:00:00 | 54035.7018171296 | 2006-10-27 16:50:37 | 3.0.22.43 | 5 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000003 | LMC SNRs L71/N23 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | LMC SNRs | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100003010/ | Quick Look | |||
5 | A 2052 | 229.2779 | 6.8766 | 228.662841 | 7.059342 | 224.77082 | 24.150691 | 9.31339919 | 49.96215441 | 281.2328 | 53602.4238078704 | 2005-08-20 10:10:17 | 53602.743287037 | 2005-08-20 17:50:20 | 100006010 | 13.9021 | 20 | 13.9021 | 13.9021 | 13.9021 | 13.9021 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 13.4163 | 13.4163 | 27.5839 | 0 | PROCESSED | 57520.7207407407 | 2016-05-12 17:17:52 | 53705 | 2005-12-01 00:00:00 | 53905.4607523148 | 2006-06-19 11:03:29 | 3.0.22.43 | 11 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000006 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Outer region of A 2052 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100006010/ | Quick Look | ||||
6 | A 2052 | 229.3237 | 7.1059 | 228.709513 | 7.288472 | 224.747048 | 24.38343 | 9.64711471 | 50.05514889 | 281.2373 | 53602.7440393518 | 2005-08-20 17:51:25 | 53603.3406944445 | 2005-08-21 08:10:36 | 100006020 | 25.7431 | 20 | 25.7431 | 25.7431 | 25.7431 | 25.7431 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 21.0642 | 21.0642 | 51.5199 | 0 | PROCESSED | 57520.7246527778 | 2016-05-12 17:23:30 | 53705 | 2005-12-01 00:00:00 | 53905.4610300926 | 2006-06-19 11:03:53 | 3.0.22.43 | 5 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000006 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Outer region of A 2052 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100006020/ | Quick Look | ||||
7 | A 2052 | 229.0933 | 7.1516 | 228.479191 | 7.335016 | 224.492199 | 24.361996 | 9.50335527 | 50.26933049 | 281.2093 | 53603.3412615741 | 2005-08-21 08:11:25 | 53603.6114351852 | 2005-08-21 14:40:28 | 100006030 | 12.969 | 20 | 12.969 | 12.969 | 12.969 | 12.969 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 13.1413 | 13.1413 | 23.3279 | 0 | PROCESSED | 57520.7271527778 | 2016-05-12 17:27:06 | 53705 | 2005-12-01 00:00:00 | 53905.4613310185 | 2006-06-19 11:04:19 | 3.0.22.43 | 9 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000006 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Outer region of A 2052 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100006030/ | Quick Look | ||||
8 | A 2052 | 229.3311 | 7.2632 | 228.717502 | 7.445744 | 224.705557 | 24.536292 | 9.85579143 | 50.13807877 | 91.2371 | 53762.482650463 | 2006-01-27 11:35:01 | 53762.9209953704 | 2006-01-27 22:06:14 | 100006050 | 22.366 | 20 | 22.366 | 22.366 | 22.366 | 22.366 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 20.388 | 20.388 | 37.8659 | 0 | PROCESSED | 57532.800162037 | 2016-05-24 19:12:14 | 54247 | 2007-05-27 00:00:00 | 54040.5318634259 | 2006-11-01 12:45:53 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000006 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Outer region of A 2052 | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100006050/ | Quick Look | |||
9 | NGC 4945 | 196.3681 | -49.4152 | 195.638243 | -49.147517 | 216.98939 | -38.593586 | 305.27752827 | 13.39262005 | 96.1296 | 53750.3365625 | 2006-01-15 08:04:39 | 53752.9655092593 | 2006-01-17 23:10:20 | 100008030 | 95.0663 | 10 | 95.0817 | 95.1297 | 95.0663 | 95.1063 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 84.9813 | 84.9813 | 227.1157 | 2 | PROCESSED | 57532.7353240741 | 2016-05-24 17:38:52 | 54247 | 2007-05-27 00:00:00 | 54040.3587615741 | 2006-11-01 08:36:37 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000008 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | NGC 4945 | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100008030/ | Quick Look | |||
10 | PSR1509-58 | 228.4798 | -59.0943 | 227.494741 | -58.907902 | 243.862404 | -39.360151 | 320.34145971 | -1.12587132 | 287.6342 | 53605.36 | 2005-08-23 08:38:24 | 53606.8597569444 | 2005-08-24 20:38:03 | 100009010 | 65.1618 | 60 | 65.1618 | 65.3227 | 65.2427 | 65.2427 | 3 | 3 | 3 | 3 | 1 | 0 | 0 | 49.7357 | 49.7357 | 129.5298 | 4 | PROCESSED | 57526.9045486111 | 2016-05-18 21:42:33 | 53705 | 2005-12-01 00:00:00 | 53905.4622337963 | 2006-06-19 11:05:37 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000009 | HXD spectrum and timing check | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | PSR1509-58 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100009010/ | Quick Look | |||
11 | Crab Nebula | 83.6267 | 22.0751 | 82.874095 | 22.042383 | 84.095945 | -1.235244 | 184.50282132 | -5.75691305 | 86.8655 | 53607.0070833333 | 2005-08-25 00:10:12 | 53607.1389814815 | 2005-08-25 03:20:08 | 100010010 | 2.9379 | 5 | 2.9379 | 2.9379 | 2.9379 | 2.9379 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 3.4387 | 3.4387 | 11.3819 | 0 | PROCESSED | 57526.8678703704 | 2016-05-18 20:49:44 | 54247 | 2007-05-27 00:00:00 | 54118.9886689815 | 2007-01-18 23:43:41 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000010 | Crab nebula multi pointings | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab Offset 1 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010010/ | Quick Look | |||
12 | Crab nebula | 83.6336 | 21.9568 | 82.881657 | 21.924117 | 84.097114 | -1.353715 | 184.60669551 | -5.81484075 | 86.8687 | 53607.1394560185 | 2005-08-25 03:20:49 | 53607.2779282407 | 2005-08-25 06:40:13 | 100010020 | 3.6533 | 5 | 3.6533 | 3.6533 | 3.6533 | 3.6533 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 3.8067 | 3.8067 | 11.934 | 0 | PROCESSED | 57526.8772337963 | 2016-05-18 21:03:13 | 54247 | 2007-05-27 00:00:00 | 54118.9337615741 | 2007-01-18 22:24:37 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000010 | Crab nebula multi pointings | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab Offset 1 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010020/ | Quick Look | |||
13 | Crab nebula | 83.6511 | 21.6763 | 82.900722 | 21.643705 | 84.100986 | -1.634666 | 184.85366771 | -5.95118505 | 86.8795 | 53607.5153125 | 2005-08-25 12:22:03 | 53607.7153472222 | 2005-08-25 17:10:06 | 100010040 | 9.5806 | 5 | 9.5806 | 9.5806 | 9.5806 | 9.5806 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 8.1783 | 8.1783 | 17.248 | 0 | PROCESSED | 57526.8981828704 | 2016-05-18 21:33:23 | 54247 | 2007-05-27 00:00:00 | 54118.943125 | 2007-01-18 22:38:06 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000010 | Crab nebula multi pointings | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab Offset 1 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010040/ | Quick Look | |||
14 | Crab nebula | 83.5677 | 22.0135 | 82.815455 | 21.980499 | 84.038563 | -1.294359 | 184.52566905 | -5.83608695 | 86.8444 | 53607.9175810185 | 2005-08-25 22:01:19 | 53608.0695023148 | 2005-08-26 01:40:05 | 100010060 | 4.8779 | 5 | 4.8779 | 4.8779 | 4.8779 | 4.8779 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 5.0217 | 5.0217 | 13.076 | 0 | PROCESSED | 57526.9066087963 | 2016-05-18 21:45:31 | 54247 | 2007-05-27 00:00:00 | 54122.4195486111 | 2007-01-22 10:04:09 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000010 | Crab nebula multi pointings | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab Offset 1 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010060/ | Quick Look | |||
15 | Crab nebula | 83.6922 | 22.0221 | 82.939876 | 21.989699 | 84.154283 | -1.290862 | 184.58047361 | -5.73399538 | 86.8671 | 53608.0699768518 | 2005-08-26 01:40:46 | 53608.2084027778 | 2005-08-26 05:00:06 | 100010070 | 4.0899 | 5 | 4.0899 | 4.0899 | 4.0899 | 4.0899 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 4.2283 | 4.2283 | 11.9259 | 0 | PROCESSED | 57526.9072222222 | 2016-05-18 21:46:24 | 54247 | 2007-05-27 00:00:00 | 54119.0149074074 | 2007-01-19 00:21:28 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000010 | Crab nebula multi pointings | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab Offset 1 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010070/ | Quick Look | |||
16 | Crab nebula | 83.5807 | 22.8483 | 82.82374 | 22.81535 | 84.087744 | -0.460898 | 183.82410841 | -5.37832099 | 86.8677 | 53608.3175810185 | 2005-08-26 07:37:19 | 53608.5139583333 | 2005-08-26 12:20:06 | 100010090 | 6.716 | 5 | 6.716 | 6.716 | 6.716 | 6.716 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 6.3768 | 6.3768 | 16.9501 | 0 | PROCESSED | 57526.9164699074 | 2016-05-18 21:59:43 | 54247 | 2007-05-27 00:00:00 | 54119.0235648148 | 2007-01-19 00:33:56 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000010 | Crab nebula multi pointings | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab Offset 1 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010090/ | Quick Look | |||
17 | Crab nebula | 83.5122 | 24.0135 | 82.748583 | 23.980205 | 84.077056 | 0.70598 | 182.80375415 | -4.80497322 | 86.8675 | 53608.7179976852 | 2005-08-26 17:13:55 | 53608.930625 | 2005-08-26 22:20:06 | 100010110 | 9.4805 | 5 | 9.4805 | 9.4805 | 9.4805 | 9.4805 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 7.363 | 7.363 | 18.336 | 0 | PROCESSED | 57526.9265162037 | 2016-05-18 22:14:11 | 54247 | 2007-05-27 00:00:00 | 54118.98625 | 2007-01-18 23:40:12 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000010 | Crab nebula multi pointings | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab Offset 1 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010110/ | Quick Look | |||
18 | Crab nebula | 83.6374 | 21.9009 | 82.885769 | 21.868236 | 84.09817 | -1.409717 | 184.65605757 | -5.84178049 | 86.8664 | 53608.9333217593 | 2005-08-26 22:23:59 | 53609.069525463 | 2005-08-27 01:40:07 | 100010120 | 4.7456 | 5 | 4.7456 | 4.7456 | 4.7456 | 4.7456 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 5.1787 | 5.1787 | 11.7579 | 1 | PROCESSED | 57526.9343287037 | 2016-05-18 22:25:26 | 54247 | 2007-05-27 00:00:00 | 54118.9946180556 | 2007-01-18 23:52:15 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000010 | Crab nebula multi pointings | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab Offset 1 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010120/ | Quick Look | |||
19 | Crab nebula | 83.5044 | 22.0116 | 82.752181 | 21.978293 | 83.979835 | -1.293628 | 184.49566519 | -5.88665136 | 86.8658 | 53609.0701388889 | 2005-08-27 01:41:00 | 53609.2014583333 | 2005-08-27 04:50:06 | 100010130 | 4.222 | 5 | 4.222 | 4.222 | 4.222 | 4.222 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 4.3724 | 4.3724 | 11.3359 | 0 | PROCESSED | 57526.9346180556 | 2016-05-18 22:25:51 | 54247 | 2007-05-27 00:00:00 | 54119.0454282407 | 2007-01-19 01:05:25 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000010 | Crab nebula multi pointings | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab Offset 1 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010130/ | Quick Look | |||
20 | Galactic bulge | 236.4313 | -31.7013 | 235.648361 | -31.545749 | 241.296308 | -11.543137 | 340.99994533 | 17.99808229 | 283.5446 | 53609.4365856482 | 2005-08-27 10:28:41 | 53611.060625 | 2005-08-29 01:27:18 | 100011010 | 61.133 | 70 | 61.133 | 61.133 | 61.133 | 61.133 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 47.9834 | 47.9834 | 140.282 | 2 | PROCESSED | 57526.962037037 | 2016-05-18 23:05:20 | 54247 | 2007-05-27 00:00:00 | 54034.8288310185 | 2006-10-26 19:53:31 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000011 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Galactic bulge | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100011010/ | Quick Look | ||||
21 | Eta Carinae | 161.281 | -59.6845 | 160.794333 | -59.421136 | 202.162077 | -58.916082 | 287.6040589 | -0.62575348 | 343.8621 | 53611.0750347222 | 2005-08-29 01:48:03 | 53612.0627546296 | 2005-08-30 01:30:22 | 100012010 | 49.782 | 40 | 49.79 | 49.782 | 49.782 | 49.798 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 55.9607 | 55.9607 | 85.2529 | 0 | PROCESSED | 57526.9773032407 | 2016-05-18 23:27:19 | 53705 | 2005-12-01 00:00:00 | 53905.4648842593 | 2006-06-19 11:09:26 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000012 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Eta Carinae | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100012010/ | Quick Look | ||||
22 | N103B | 77.2315 | -68.7507 | 77.290508 | -68.812132 | 329.838884 | -84.691105 | 279.61119012 | -34.36730962 | 73.8586 | 53612.0740162037 | 2005-08-30 01:46:35 | 53613.0626273148 | 2005-08-31 01:30:11 | 100013010 | 33.0646 | 40 | 33.0646 | 33.0646 | 33.0646 | 33.0646 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 37.2814 | 37.2814 | 85.4059 | 1 | PROCESSED | 57526.9730324074 | 2016-05-18 23:21:10 | 54247 | 2007-05-27 00:00:00 | 54034.8733449074 | 2006-10-26 20:57:37 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000013 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | N103B | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100013010/ | Quick Look | ||||
23 | E0102-72 | 15.9813 | -72.0378 | 15.57605 | -72.305808 | 314.596715 | -65.033076 | 301.56958331 | -45.05740554 | 140.1798 | 53613.0710648148 | 2005-08-31 01:42:20 | 53613.7640509259 | 2005-08-31 18:20:14 | 100014010 | 24.3339 | 20 | 24.3339 | 24.3339 | 24.3339 | 24.3339 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 24.5144 | 24.5144 | 59.8639 | 2 | PROCESSED | 57511.5174884259 | 2016-05-03 12:25:11 | 53705 | 2005-12-01 00:00:00 | 53905.4615740741 | 2006-06-19 11:04:40 | 3.0.22.43 | 13 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000014 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | XIS monitor with E0102-72 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100014010/ | Quick Look | ||||
24 | Crab Nebula | 83.6296 | 22.1792 | 82.876409 | 22.146495 | 84.103227 | -1.131361 | 184.41590928 | -5.69889955 | 84.9998 | 53613.9762152778 | 2005-08-31 23:25:45 | 53614.1077314815 | 2005-09-01 02:35:08 | 100015020 | 4.95 | 5 | 4.95 | 4.95 | 4.95 | 4.95 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 5.1178 | 5.1178 | 11.3599 | 0 | PROCESSED | 57527.2276388889 | 2016-05-19 05:27:48 | 54247 | 2007-05-27 00:00:00 | 54109.1090972222 | 2007-01-09 02:37:06 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000015 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | HXD boresight check with Crab | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100015020/ | Quick Look | ||||
25 | SN1006 SW BG | 224.655 | -42.4005 | 223.837497 | -42.201017 | 234.783022 | -24.341132 | 326.632731 | 14.54333558 | 310.4886 | 53624.9999189815 | 2005-09-11 23:59:53 | 53626.0071643518 | 2005-09-13 00:10:19 | 100019040 | 32.3334 | 50 | 32.3334 | 32.3494 | 32.3414 | 32.3414 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 24.6736 | 24.6736 | 87.0159 | 5 | PROCESSED | 57527.3647453704 | 2016-05-19 08:45:14 | 54247 | 2007-05-27 00:00:00 | 54035.4482638889 | 2006-10-27 10:45:30 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000019 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | SN1006 observation with XIS and HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100019040/ | Quick Look | ||||
26 | SN1006 SW BG | 224.6468 | -42.4025 | 223.829311 | -42.202989 | 234.777387 | -24.344913 | 326.62625739 | 14.54451897 | 100.3489 | 53761.7199652778 | 2006-01-26 17:16:45 | 53762.4752777778 | 2006-01-27 11:24:24 | 100019060 | 27.9813 | 50 | 27.9813 | 27.9893 | 27.9973 | 27.9973 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 29.5504 | 29.5504 | 65.2499 | 2 | PROCESSED | 57532.7989814815 | 2016-05-24 19:10:32 | 54247 | 2007-05-27 00:00:00 | 54040.5663541667 | 2006-11-01 13:35:33 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000019 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | SN1006 observation with XIS and HXD | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100019060/ | Quick Look | |||
27 | Fornax Cluster | 54.6395 | -35.4918 | 54.160816 | -35.653913 | 38.755932 | -52.830853 | 236.7850293 | -53.61976834 | 103.5002 | 53626.0756018518 | 2005-09-13 01:48:52 | 53627.5002662037 | 2005-09-14 12:00:23 | 100020010 | 76.0782 | 100 | 76.0782 | 76.0782 | 76.0782 | 76.0782 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 71.1128 | 71.1128 | 123.0639 | 3 | PROCESSED | 57527.3377430556 | 2016-05-19 08:06:21 | 54247 | 2007-05-27 00:00:00 | 54035.4442013889 | 2006-10-27 10:39:39 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000020 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Fornax Cluster | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100020010/ | Quick Look | ||||
28 | Crab Nebula | 82.7325 | 21.9883 | 81.980613 | 21.951274 | 83.263643 | -1.282782 | 184.12771921 | -6.50224239 | 88.0978 | 53628.3006828704 | 2005-09-15 07:12:59 | 53628.5835416667 | 2005-09-15 14:00:18 | 100022020 | 10.9198 | 10 | 10.9198 | 10.9198 | 10.9198 | 10.9198 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 6.3401 | 6.3401 | 24.4 | 2 | PROCESSED | 57527.3262615741 | 2016-05-19 07:49:49 | 54247 | 2007-05-27 00:00:00 | 54109.1486342593 | 2007-01-09 03:34:02 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000022 | Crab at 50arcmin off from the XIS aimpoint to study stray light. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab at 50 arcmin off | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100022020/ | Quick Look | |||
29 | Crab Nebula | 84.5289 | 22.0469 | 83.776247 | 22.018539 | 84.930453 | -1.297747 | 184.974122 | -5.06424795 | 87.5879 | 53629.0921759259 | 2005-09-16 02:12:44 | 53629.368275463 | 2005-09-16 08:50:19 | 100022030 | 12.8244 | 10 | 12.8404 | 12.8324 | 12.8244 | 12.8484 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 10.3518 | 10.3518 | 23.824 | 1 | PROCESSED | 57527.3478009259 | 2016-05-19 08:20:50 | 54247 | 2007-05-27 00:00:00 | 54109.1621527778 | 2007-01-09 03:53:30 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000022 | Crab at 50arcmin off from the XIS aimpoint to study stray light. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab at 50 arcmin off | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100022030/ | Quick Look | |||
30 | Crab Nebula | 83.6282 | 22.0761 | 82.875589 | 22.04339 | 84.097378 | -1.234306 | 184.5027205 | -5.75520363 | 87.79 | 53628.5852199074 | 2005-09-15 14:02:43 | 53628.8265393518 | 2005-09-15 19:50:13 | 100023010 | 11.9978 | 10 | 11.9978 | 11.9978 | 11.9978 | 11.9978 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 10.5132 | 10.5132 | 20.8239 | 0 | PROCESSED | 57527.3355902778 | 2016-05-19 08:03:15 | 54247 | 2007-05-27 00:00:00 | 54109.2268287037 | 2007-01-09 05:26:38 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000023 | Calibration of detector response at both of XIS/HXD nominal positions, together with an absolute flux confirmation with differnt hit-pattern widths. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab at nominal positions | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100023010/ | Quick Look | |||
31 | BD +30 3639 | 293.6887 | 30.5051 | 293.198078 | 30.394341 | 303.540216 | 51.224252 | 64.77556877 | 5.01383279 | 277.8713 | 53634.3814930556 | 2005-09-21 09:09:21 | 53635.2473842593 | 2005-09-22 05:56:14 | 100025010 | 35.2146 | 40 | 35.2306 | 35.2306 | 35.2146 | 35.2226 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 33.3728 | 33.3728 | 74.8039 | 1 | PROCESSED | 57527.3931597222 | 2016-05-19 09:26:09 | 54247 | 2007-05-27 00:00:00 | 54035.4664583333 | 2006-10-27 11:11:42 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000025 | The proposed target, BD +30 3639, is a prototypical planetary nebula which emit diffuse X-rays; planetary nebulae represent the final evolutionary stage of low mass stars, and contain very rich information on the stellar nucleosynthesis. The Chandra ACIS spectrum of BD +30 3639 bears an amazingly strong Ne-K line, most certainly because the X-ray emitting material directly reflect the "onion-like structure" of elements insied evolved stars. However, the ACIS was not able to resolve C, N, O lines, which are of vital importance. The XMM RGS and Chandra LETG could do, but we need very long exposure. Using the Suzaku XIS-BI with the excellent low-energy performance, we can for the first time measure the C/N/O/Mg abundance ratios of this important object in a short time. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Observation of planetary nebula BD +30 3639 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100025010/ | Quick Look | |||
32 | RXJ1713-3946-BKGD2 | 257.2742 | -41.0338 | 256.397744 | -40.970376 | 259.926088 | -18.035902 | 345.80577047 | -0.54060643 | 270.0033 | 53641.2980671296 | 2005-09-28 07:09:13 | 53642.1843055556 | 2005-09-29 04:25:24 | 100026030 | 37.5132 | 40 | 37.5372 | 37.5292 | 37.5132 | 37.5132 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 31.8982 | 31.8982 | 76.5659 | 0 | PROCESSED | 57527.4461574074 | 2016-05-19 10:42:28 | 54247 | 2007-05-27 00:00:00 | 54035.6187268518 | 2006-10-27 14:50:58 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000026 | RXJ1713 is very important sources in which we can study particle accelerator in the universe. X-ray synchrotron spectrum suggest the existence of distribution of high energy electron. Very similar TeV and ASCA morphologies show close connection between these energy bands. The interaction with molecular cloud suggests that proton accelerator resides in this object. The photon index of RXJ1713 seems to be difficult in the frame work of standard diffusive shock scenario. To obtain precise spectrum in the hard X-ray region is therefore very important to determine the energy cut off and to study the mechanism that produce such high energy electrons. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Observation of RXJ1713.7-3946 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100026030/ | Quick Look | |||
33 | M82-Wind | 148.8893 | 69.7655 | 147.850184 | 70.002482 | 118.869306 | 52.161633 | 141.33880284 | 40.49464345 | 137.7608 | 53647.5072800926 | 2005-10-04 12:10:29 | 53648.1418287037 | 2005-10-05 03:24:14 | 100033010 | 32.3274 | 100 | 32.3274 | 32.3274 | 32.3274 | 32.3274 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 30.2224 | 30.2224 | 54.8021 | 0 | PROCESSED | 57527.5155092593 | 2016-05-19 12:22:20 | 54247 | 2007-05-27 00:00:00 | 54037.0057175926 | 2006-10-29 00:08:14 | 3.0.22.43 | 5 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000033 | We propose to observe the largely extened emission with the size of about 12kpc around M82 with Suzaku for 100ksec. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Largely Extended Emission (~12kpc) around M82 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100033010/ | Quick Look | |||
34 | Sgr_A_west | 266.3057 | -29.1697 | 265.509983 | -29.149828 | 266.748763 | -5.770252 | 359.75546849 | -0.04768885 | 264.9601 | 53637.5953356482 | 2005-09-24 14:17:17 | 53638.7273032407 | 2005-09-25 17:27:19 | 100027020 | 42.8148 | 50 | 42.8148 | 42.8148 | 42.8148 | 42.8148 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 36.091 | 36.091 | 97.8 | 0 | PROCESSED | 57527.4293865741 | 2016-05-19 10:18:19 | 54247 | 2007-05-27 00:00:00 | 54035.5135532407 | 2006-10-27 12:19:31 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000027 | We propose to obtain high quality spectra from 6 positions near the GC. The objective is to resolve 6.4 , 6.7 and 6.9 keV line and determine the high energy tail from each positions and/or from the sub-structures in each position. Combining all the results, we can see which sub-sub-structure is X-ray reflection from Sgr A* ( 6.4 keV line+ 7.1 keV edge + high energy tail), thermal plasma (6.7+6.9 keV lines, with no hard X-ray tail), non thermal emission (e.g. line but hard X-ray tail). Unexpected spectral feature could be also found, depending on the real origin. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Suzaku Observation of Galactic Center Region | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100027020/ | Quick Look | |||
35 | E0102-72 | 16.139 | -72.1205 | 15.73725 | -72.388297 | 314.467235 | -65.111919 | 301.50933431 | -44.97149935 | 119.4064 | 53593.3086458333 | 2005-08-11 07:24:27 | 53595.2485069444 | 2005-08-13 05:57:51 | 100001010 | 2.4068 | 70 | 2.4068 | 2.4068 | 2.4068 | 2.4068 | 1 | 1 | 1 | 1 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | PROCESSED | 57520.6843287037 | 2016-05-12 16:25:26 | 54247 | 2007-05-27 00:00:00 | 54035.5925115741 | 2006-10-27 14:13:13 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000001 | XIS door open with a SMC SNR E0102-72 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | XIS door open | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100001010/ | Quick Look | |||
36 | 1E1743.1-2843(GC_BGD_3) | 266.592 | -28.6516 | 265.799503 | -28.633124 | 266.987582 | -5.246121 | 0.32828705 | 0.00813221 | 264.88 | 53638.7286111111 | 2005-09-25 17:29:12 | 53638.793275463 | 2005-09-25 19:02:19 | 100027050 | 1.9846 | 5 | 1.9846 | 1.9846 | 1.9846 | 1.9846 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 1.7934 | 1.7934 | 5.5679 | 0 | PROCESSED | 57527.4093055556 | 2016-05-19 09:49:24 | 54247 | 2007-05-27 00:00:00 | 53905.6343055556 | 2006-06-19 15:13:24 | 3.0.22.43 | 5 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000027 | We propose to obtain high quality spectra from 6 positions near the GC. The objective is to resolve 6.4 , 6.7 and 6.9 keV line and determine the high energy tail from each positions and/or from the sub-structures in each position. Combining all the results, we can see which sub-sub-structure is X-ray reflection from Sgr A* ( 6.4 keV line+ 7.1 keV edge + high energy tail), thermal plasma (6.7+6.9 keV lines, with no hard X-ray tail), non thermal emission (e.g. line but hard X-ray tail). Unexpected spectral feature could be also found, depending on the real origin. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Suzaku Observation of Galactic Center Region | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100027050/ | Quick Look | |||
37 | HESS J1616-508 | 244.1248 | -50.8971 | 243.177731 | -50.773494 | 251.629905 | -29.09136 | 332.40352084 | -0.15000913 | 282.8476 | 53632.5000231482 | 2005-09-19 12:00:02 | 53633.8183333333 | 2005-09-20 19:38:24 | 100028010 | 41.352 | 50 | 41.352 | 41.376 | 41.352 | 41.368 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 35.3731 | 35.3731 | 113.8899 | 0 | PROCESSED | 57527.3838194444 | 2016-05-19 09:12:42 | 54247 | 2007-05-27 00:00:00 | 54035.4361111111 | 2006-10-27 10:28:00 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000028 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | New HESS sources and the Galactic ridge Background | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100028010/ | Quick Look | ||||
38 | HESS J1616-508_BGD1 | 243.666 | -51.1742 | 242.717138 | -51.048595 | 251.369654 | -29.420684 | 332.00349288 | -0.15039556 | 283.0062 | 53631.9497222222 | 2005-09-18 22:47:36 | 53632.4990856482 | 2005-09-19 11:58:41 | 100028020 | 19.3277 | 25 | 19.3277 | 20.63 | 19.36 | 19.6323 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 16.6426 | 16.6426 | 47.4479 | 0 | PROCESSED | 57527.3573148148 | 2016-05-19 08:34:32 | 54247 | 2007-05-27 00:00:00 | 54035.1692476852 | 2006-10-27 04:03:43 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000028 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | New HESS sources and the Galactic ridge Background | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100028020/ | Quick Look | ||||
39 | GRO J1655-40 | 253.5027 | -39.8455 | 252.639975 | -39.764411 | 256.800671 | -17.156383 | 344.98315976 | 2.45489032 | 268.0237 | 53635.3140625 | 2005-09-22 07:32:15 | 53636.2968055556 | 2005-09-23 07:07:24 | 100029010 | 35.2228 | 40 | 0 | 35.2336 | 35.2228 | 35.2308 | 0 | 1 | 2 | 2 | 1 | 0 | 0 | 28.7315 | 28.7315 | 84.9019 | 1 | PROCESSED | 57527.3997337963 | 2016-05-19 09:35:37 | 54247 | 2007-05-27 00:00:00 | 54035.4940625 | 2006-10-27 11:51:27 | 3.0.22.43 | 5 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000029 | We propose to observe GRO J1655-40, a transient galactic black hole candidate. With M=~7 Msolar and distinct radio lobes, GRO J1655-40 has been classified as a microquasar. It was highly variable during the first few years after its discovery while showing irregular flaring and a wide range of continuum states. Discrete Fe K absorption structure was observed with ASCA. In the summer of 1997 it entered an extended quiescence that lasted for ~8 years. In March 2005 it became active again and XMM & Chandra have observed it since. Only Suzaku can provide the broadband sensitivity required to map the Fe K structure and the continuum as they change. GRO J1655-40 is rapidly declining and must be observed soon before it reenters quiescence. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | GRO J1655-40 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100029010/ | Quick Look | |||
40 | NGC3516 | 166.7299 | 72.5779 | 165.877553 | 72.848305 | 123.367172 | 57.997458 | 133.2179652 | 42.40001774 | 148.9366 | 53655.5813541667 | 2005-10-12 13:57:09 | 53658.3801388889 | 2005-10-15 09:07:24 | 100031010 | 134.4696 | 150 | 134.5096 | 134.5956 | 134.5096 | 134.4696 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 122.818 | 122.818 | 241.6848 | 0 | PROCESSED | 57527.6243634259 | 2016-05-19 14:59:05 | 54247 | 2007-05-27 00:00:00 | 54036.4704976852 | 2006-10-28 11:17:31 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000031 | NGC 3516 is one of the brightest Seyfert 1s seen in BAT currently visible to Suzaku. Recent BAT and RXTE observations show that this source is ~2-3 mCrb in the 2-10 keV band and ~4-5 mCrb in 15-100 keV. NGC 3516 is currently much brighter than when XMM observed it in 2000 (e.g., it has since returned to "typical" flux). This source's Fe K line and Compton reflection hump are both quite strong (e.g., as seen with SAX; R is ~1.8 in SAX data). | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | NGC 3516 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100031010/ | Quick Look | |||
41 | M82-Wind | 148.894 | 69.7643 | 147.854963 | 70.001295 | 118.872596 | 52.161537 | 141.33883884 | 40.49666381 | 146.246 | 53662.0401273148 | 2005-10-19 00:57:47 | 53662.9390393518 | 2005-10-19 22:32:13 | 100033020 | 40.3586 | 100 | 40.3586 | 40.3826 | 40.3586 | 40.3666 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 38.3533 | 38.3533 | 77.658 | 0 | PROCESSED | 57527.6127546296 | 2016-05-19 14:42:22 | 54247 | 2007-05-27 00:00:00 | 54036.4196296296 | 2006-10-28 10:04:16 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000033 | We propose to observe the largely extened emission with the size of about 12kpc around M82 with Suzaku for 100ksec. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Largely Extended Emission (~12kpc) around M82 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100033020/ | Quick Look | |||
42 | M82-Wind | 148.8885 | 69.7652 | 147.849381 | 70.00218 | 118.869202 | 52.16123 | 141.33933547 | 40.4945935 | 137.7608 | 53670.4681134259 | 2005-10-27 11:14:05 | 53671.1002199074 | 2005-10-28 02:24:19 | 100033030 | 28.3638 | 100 | 28.3798 | 28.3798 | 28.3718 | 28.3638 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 25.8121 | 25.8121 | 54.604 | 1 | PROCESSED | 57527.6784606482 | 2016-05-19 16:16:59 | 54247 | 2007-05-27 00:00:00 | 54036.8639467593 | 2006-10-28 20:44:05 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000033 | We propose to observe the largely extened emission with the size of about 12kpc around M82 with Suzaku for 100ksec. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Largely Extended Emission (~12kpc) around M82 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100033030/ | Quick Look | |||
43 | Her X-1 | 254.465 | 35.3306 | 254.01442 | 35.406187 | 246.002276 | 57.482156 | 58.13562438 | 37.51514805 | 249.5714 | 53648.6450462963 | 2005-10-05 15:28:52 | 53649.4341898148 | 2005-10-06 10:25:14 | 100035010 | 36.1235 | 40 | 36.9235 | 36.1235 | 36.9235 | 36.9235 | 2 | 1 | 2 | 2 | 1 | 0 | 0 | 33.3229 | 33.3229 | 68.178 | 0 | PROCESSED | 57527.5593518518 | 2016-05-19 13:25:28 | 54247 | 2007-05-27 00:00:00 | 54036.0084375 | 2006-10-28 00:12:09 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000035 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | HXD Performance Verification using Her X-1 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100035010/ | Quick Look | ||||
44 | Sgr_A_west | 266.3063 | -29.1685 | 265.51059 | -29.148631 | 266.749258 | -5.769039 | 359.75676556 | -0.04750971 | 264.9604 | 53642.1914467593 | 2005-09-29 04:35:41 | 53643.187025463 | 2005-09-30 04:29:19 | 100037010 | 43.7412 | 50 | 43.7412 | 43.7492 | 43.7492 | 43.7492 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 39.3941 | 39.3941 | 86.0139 | 0 | PROCESSED | 57527.4581828704 | 2016-05-19 10:59:47 | 54247 | 2007-05-27 00:00:00 | 54035.6663310185 | 2006-10-27 15:59:31 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000037 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Suzaku Obseration of Galactic Center region 2 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100037010/ | Quick Look | ||||
45 | GRS1915+105 | 288.8014 | 10.9368 | 288.21144 | 10.848425 | 292.141211 | 32.943669 | 45.35928754 | -0.22611181 | 260.5762 | 53659.6951967593 | 2005-10-16 16:41:05 | 53661.9724305556 | 2005-10-18 23:20:18 | 100039010 | 84.7777 | 80 | 85.0631 | 86.4305 | 85.0711 | 84.7777 | 3 | 3 | 3 | 3 | 1 | 0 | 0 | 68.8623 | 68.8623 | 196.7338 | 2 | PROCESSED | 57527.9188541667 | 2016-05-19 22:03:09 | 54247 | 2007-05-27 00:00:00 | 54043.8117476852 | 2006-11-04 19:28:55 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000039 | This observation will be performed as a part of the big multiwavelength campain including Suzaku, VLA, Integral, RXTE, and Spitzer. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Campaign of coordinated observation of GRS 1915+105 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100039010/ | Quick Look | |||
46 | RXJ1856.5-3754 | 284.1433 | -37.91 | 283.291633 | -37.976029 | 281.504649 | -15.032837 | 358.59722216 | -17.21146697 | 84.0127 | 53817.9388078704 | 2006-03-23 22:31:53 | 53819.4433217593 | 2006-03-25 10:38:23 | 100041020 | 79.169 | 80 | 79.177 | 79.169 | 79.177 | 79.177 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 53.2099 | 53.2099 | 129.9759 | 1 | PROCESSED | 57533.3325231482 | 2016-05-25 07:58:50 | 54247 | 2007-05-27 00:00:00 | 54042.2967824074 | 2006-11-03 07:07:22 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000041 | We propose Suzaku observation of a nearby isolated neuron star RXJ1856.5-3754 for the low energy QE calibration of the XIS. Our main purpose is, however, using this source as a soft X-ray QE calibrator on the sky. We hope this source will be observed again in future to check possible contamination on the filter surface etc. Note that the calibration is not only for the BI-CCD(XIS1), but also for FI-CCDs or relative QE among them. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | LOW ENERGY QE CALIBRATION OF XIS | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100041020/ | Quick Look | ||
47 | Crab nebula | 83.6399 | 21.8519 | 82.888543 | 21.819249 | 84.098328 | -1.458773 | 184.69891686 | -5.86604099 | 86.8683 | 53604.3898263889 | 2005-08-22 09:21:21 | 53604.4890972222 | 2005-08-22 11:44:18 | 100007030 | 2.7861 | 5 | 2.7861 | 2.7861 | 2.7901 | 2.7861 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 2.1927 | 2.1927 | 8.5541 | 0 | PROCESSED | 57520.7416203704 | 2016-05-12 17:47:56 | 54247 | 2007-05-27 00:00:00 | 54105.2865393518 | 2007-01-05 06:52:37 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000007 | Crab nebula multi pointings | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab Nebula | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100007030/ | Quick Look | |||
48 | E0102-72 | 15.9926 | -72.0236 | 15.587314 | -72.291594 | 314.630688 | -65.030221 | 301.56327722 | -45.07133229 | 226.8326 | 53720.0716203704 | 2005-12-16 01:43:08 | 53723.4377199074 | 2005-12-19 10:30:19 | 100044010 | 59.731 | 20 | 59.735 | 125.9195 | 59.731 | 59.737 | 3 | 3 | 3 | 3 | 1 | 0 | 0 | 115.3302 | 115.3302 | 290.8037 | 1 | PROCESSED | 57532.5803935185 | 2016-05-24 13:55:46 | 54247 | 2007-05-27 00:00:00 | 54119.7612615741 | 2007-01-19 18:16:13 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001097 | We propose the calibration observations for XIS: E0102-72 ... Gain and QE in the low energy band Cas A ... Gain and QE in the high energy band Eta Carinae ... Contamination of the BI chip | CALIBRATION | 1 | A | HIRONORI MATSUMOTO | JAP | 0 | SWG | XIS FLIGHT CAIBRATION PLAN | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100044010/ | Quick Look | |||
49 | CYGNUS LOOP | 314.0345 | 31.9311 | 313.518544 | 31.738505 | 329.353732 | 46.719144 | 75.67403832 | -8.61676541 | 64.2261 | 53884.1556018518 | 2006-05-29 03:44:04 | 53884.3793865741 | 2006-05-29 09:06:19 | 100049010 | 8.3805 | 10 | 8.3805 | 8.3805 | 8.3805 | 8.3805 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 6.0211 | 6.0211 | 19.304 | 0 | PROCESSED | 57534.4628240741 | 2016-05-26 11:06:28 | 54258 | 2007-06-07 00:00:00 | 54059.411099537 | 2006-11-20 09:51:59 | 3.0.22.43 | 5 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 015007 | Here is the list of the calibration sources in the AO-1 round: 1) E0102.2-7219 20ks x 2 2) PKS2155-304 30ks (simultaneous observation with CXO and XMM) 3) Galactic Center Plasma 50ks 4) Cygnus Loop 40ks (=10ks x 4), and 5) RXJ1856.5-3754 40ks | CALIBRATION | 1 | A | HIRONORI MATSUMOTO | JAP | 1 | SWG | XIS FLIGHT CALIBRATION PLAN | SPE | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100049010/ | Quick Look | ||
50 | CYGNUS LOOP | 314.0785 | 32.0438 | 313.563 | 31.85105 | 329.470002 | 46.807189 | 75.78588033 | -8.57358243 | 64.2263 | 53884.3796759259 | 2006-05-29 09:06:44 | 53884.6086342593 | 2006-05-29 14:36:26 | 100049020 | 7.8928 | 10 | 7.8928 | 7.8928 | 7.8928 | 7.8928 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 7.452 | 7.452 | 19.7699 | 0 | PROCESSED | 57534.4674884259 | 2016-05-26 11:13:11 | 54258 | 2007-06-07 00:00:00 | 54088.8429513889 | 2006-12-19 20:13:51 | 3.0.22.43 | 5 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 015007 | Here is the list of the calibration sources in the AO-1 round: 1) E0102.2-7219 20ks x 2 2) PKS2155-304 30ks (simultaneous observation with CXO and XMM) 3) Galactic Center Plasma 50ks 4) Cygnus Loop 40ks (=10ks x 4), and 5) RXJ1856.5-3754 40ks | CALIBRATION | 1 | A | HIRONORI MATSUMOTO | JAP | 1 | SWG | XIS FLIGHT CALIBRATION PLAN | SPE | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100049020/ | Quick Look | ||
51 | CYGNUS LOOP | 313.9494 | 32.0818 | 313.434356 | 31.889502 | 329.346118 | 46.886158 | 75.74490282 | -8.46508453 | 64.2292 | 53884.6089236111 | 2006-05-29 14:36:51 | 53884.8377777778 | 2006-05-29 20:06:24 | 100049030 | 11.6971 | 10 | 11.7051 | 11.6971 | 11.7051 | 11.7051 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 12.2688 | 12.2688 | 19.772 | 0 | PROCESSED | 57534.4722800926 | 2016-05-26 11:20:05 | 54258 | 2007-06-07 00:00:00 | 54052.4915046296 | 2006-11-13 11:47:46 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 015007 | Here is the list of the calibration sources in the AO-1 round: 1) E0102.2-7219 20ks x 2 2) PKS2155-304 30ks (simultaneous observation with CXO and XMM) 3) Galactic Center Plasma 50ks 4) Cygnus Loop 40ks (=10ks x 4), and 5) RXJ1856.5-3754 40ks | CALIBRATION | 1 | A | HIRONORI MATSUMOTO | JAP | 1 | SWG | XIS FLIGHT CALIBRATION PLAN | SPE | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100049030/ | Quick Look | ||
52 | Crab nebula | 83.9887 | 22.0345 | 83.236236 | 22.00353 | 84.429494 | -1.290207 | 184.71743044 | -5.49499441 | 86.8666 | 53608.5155902778 | 2005-08-26 12:22:27 | 53608.7153472222 | 2005-08-26 17:10:06 | 100010100 | 9.694 | 5 | 9.694 | 9.694 | 9.694 | 9.694 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 7.5812 | 7.5812 | 17.2479 | 0 | PROCESSED | 57526.9259606482 | 2016-05-18 22:13:23 | 54247 | 2007-05-27 00:00:00 | 54122.4242939815 | 2007-01-22 10:10:59 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000010 | Crab nebula multi pointings | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab Offset 1 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010100/ | Quick Look | |||
53 | Vega | 279.2264 | 38.7699 | 278.806278 | 38.72626 | 285.283614 | 61.72204 | 67.43212753 | 19.23869014 | 301.7896 | 53615.367349537 | 2005-09-02 08:48:59 | 53615.603587963 | 2005-09-02 14:29:10 | 100017010 | 11.3985 | 10 | 11.4065 | 11.4065 | 11.4065 | 11.3985 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 11.5751 | 11.5751 | 20.4039 | 0 | PROCESSED | 57527.2607407407 | 2016-05-19 06:15:28 | 54247 | 2007-05-27 00:00:00 | 53906.0764814815 | 2006-06-20 01:50:08 | 3.0.22.43 | 5 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000017 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | XIS OBF check with Vega | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100017010/ | Quick Look | ||||
54 | A0535+026 | 84.7243 | 26.3189 | 83.946776 | 26.291426 | 85.267864 | 2.964757 | 181.44092218 | -2.64422146 | 83.608 | 53627.5694907407 | 2005-09-14 13:40:04 | 53628.0418865741 | 2005-09-15 01:00:19 | 100021010 | 21.761 | 20 | 21.761 | 21.761 | 21.761 | 21.761 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 21.2572 | 21.2572 | 40.7839 | 1 | PROCESSED | 57527.3122337963 | 2016-05-19 07:29:37 | 54247 | 2007-05-27 00:00:00 | 54035.0644444444 | 2006-10-27 01:32:48 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000021 | We propose to observe the X-ray binary pulsar A0535+26. The main objectives is measuring changes in the cyclotron resonance energy in an outburst decay.It is known from another X-ray pulsar 4U0115+63 that the cyclotron resonance energy increased from 11 keV to 16 keV, as the luminosity decreased across a threshold luminosity of 4x10^37 erg/s. The flare of A0535+26 is a chance to know whether this behavior is the RULE among binary pulsars or an EXCEPTION. A0535+26 is fading down and will reach 30mCrab (5-100keV) on September 17, which is 5x10^36 erg/s. It is better to be observed as soon as possible, before it fades out. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | TOO Observation of A0535+026 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100021010/ | Quick Look | |||
55 | Crab nebula | 83.7552 | 22.0249 | 83.002845 | 21.992803 | 84.212769 | -1.290605 | 184.60948321 | -5.68314749 | 86.8656 | 53609.2022106482 | 2005-08-27 04:51:11 | 53609.3125810185 | 2005-08-27 07:30:07 | 100010140 | 3.419 | 5 | 3.419 | 3.419 | 3.419 | 3.419 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 3.7554 | 3.7554 | 9.5319 | 0 | PROCESSED | 57526.9383217593 | 2016-05-18 22:31:11 | 54247 | 2007-05-27 00:00:00 | 54118.9983796296 | 2007-01-18 23:57:40 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000010 | Crab nebula multi pointings | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab Offset 1 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010140/ | Quick Look | |||
56 | Crab Nebula | 83.6309 | 22.0151 | 82.87863 | 21.982404 | 84.097185 | -1.295359 | 184.55585082 | -5.78574816 | 87.8466 | 53628.8269212963 | 2005-09-15 19:50:46 | 53629.0904976852 | 2005-09-16 02:10:19 | 100023020 | 12.5271 | 10 | 12.5311 | 12.5271 | 12.5364 | 12.5351 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 13.3529 | 13.3529 | 22.764 | 1 | PROCESSED | 57527.3409143518 | 2016-05-19 08:10:55 | 54247 | 2007-05-27 00:00:00 | 54109.193599537 | 2007-01-09 04:38:47 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000023 | Calibration of detector response at both of XIS/HXD nominal positions, together with an absolute flux confirmation with differnt hit-pattern widths. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab at nominal positions | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100023020/ | Quick Look | |||
57 | NGC 2110 | 88.0444 | -7.458 | 87.440268 | -7.468978 | 87.743148 | -30.884192 | 212.92660512 | -16.54877043 | 103.4188 | 53629.3796296296 | 2005-09-16 09:06:40 | 53631.8308333333 | 2005-09-18 19:56:24 | 100024010 | 101.7487 | 100 | 101.9265 | 103.7601 | 101.7487 | 102.1483 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 86.0433 | 86.0433 | 211.7558 | 4 | PROCESSED | 57527.4030324074 | 2016-05-19 09:40:22 | 54247 | 2007-05-27 00:00:00 | 54035.4624189815 | 2006-10-27 11:05:53 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000024 | The Narrow Emission Line Galaxy NGC 2110 was the brightest AGN in the initial BAT survey release (BAT flux of 2.1E-10 erg/cm2/sec) visible to Suzaku during Sept./Oct., and is still currently bright in BAT. A 2003 RXTE observation yielded F_2-10 keV = 4E-11 erg/cm2/sec. The source is currently almost 3 times brighter than during the SAX observations. The main goals are to measure the high energy cutoff and to place a strong limit on the presence of reflection. The Compton reflection hump is weak in SAX data (suggesting that the Fe K line originates in Compton-thin material). Determining the strength of the reflection component is critical for constraining the geometry of the accreting material. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Narrow Emission Line Galaxy NGC 2110 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100024010/ | Quick Look | |||
58 | GX 349+2 | 256.427 | -36.366 | 255.587548 | -36.298664 | 258.786235 | -13.451096 | 349.14511841 | 2.78820606 | 85.6584 | 53808.5453240741 | 2006-03-14 13:05:16 | 53809.2216782407 | 2006-03-15 05:19:13 | 400003010 | 25.2308 | 50 | 25.2308 | 25.2332 | 25.2308 | 25.2308 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 20.0507 | 20.0507 | 58.434 | 2 | PROCESSED | 57533.2006365741 | 2016-05-25 04:48:55 | 54247 | 2007-05-27 00:00:00 | 54041.9132060185 | 2006-11-02 21:55:01 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001026 | We propose Suzaku observations of two luminous low-mass X-ray binaries (Z sources), GX 349+2 and Cyg X-2, to investigate the origin of the hard tails of Z sources, of which the spectral photon indices are reported to become occasionally less than unity. With the high sensitivity of the HXD, we detect the spectral shape up to several 100 keV and reveal existence of particle acceleration caused by high radiation pressure. | GALACTIC POINT SOURCES | 4 | A | HIROMITSU TAKAHASHI | JAP | 0 | SWG | SUZAKU OBSERVATIONS OF THE HARD TAILS OF LUMINOUS LOW-MASS X-RAY BINARIES (Z SOURCES) | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/400003010/ | Quick Look | ||
59 | SS CYG | 325.6789 | 43.5736 | 325.187819 | 43.344381 | 350.451149 | 52.649921 | 90.55119171 | -7.12024619 | 276.5788 | 53676.0503703704 | 2005-11-02 01:12:32 | 53676.9856944444 | 2005-11-02 23:39:24 | 400006010 | 39.4512 | 40 | 39.4512 | 39.4512 | 39.4512 | 39.4512 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 32.0472 | 32.0472 | 80.81 | 1 | PROCESSED | 57527.7175925926 | 2016-05-19 17:13:20 | 54247 | 2007-05-27 00:00:00 | 54036.9898148148 | 2006-10-28 23:45:20 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001043 | Although the boundary layer that is formed between the rapidly rotating inner accretion disk and the white dwarf surface has been known as a hard-X-ray emitter, its geometry and structure has not been well understood yet. We aim to investigate the boundary layer structure with SS Cyg, the brightest dwarf nova, by means of a soft X-ray component with the BI CCD, a fluorescent Fe K-alpha line with the FI CCDs, and a continuum reflection by the white dwarf surface with the HXD PIN. It is of great use to observe states of a different mass accretion rate, and hence we propose to observe both in quiescence and in outburst. | GALACTIC POINT SOURCES | 4 | A | MANABU ISHIDA | JAP | 0 | SWG | SS CYG OBSERVATION IN QUIESCENCE | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/400006010/ | Quick Look | |||
60 | X1630-472 | 248.4706 | -47.343 | 247.550146 | -47.238721 | 254.054156 | -25.085181 | 336.93140696 | 0.30212129 | 69.0657 | 53781.9791087963 | 2006-02-15 23:29:55 | 53782.5474305556 | 2006-02-16 13:08:18 | 400010020 | 21.429 | 200 | 21.429 | 21.485 | 21.429 | 21.429 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 17.0223 | 17.0223 | 49.1019 | 0 | PROCESSED | 57533.0117592593 | 2016-05-25 00:16:56 | 54247 | 2007-05-27 00:00:00 | 54041.4892013889 | 2006-11-02 11:44:27 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001058 | We propose to monitor a transient black hole binary in outburst through a series of 20 ks observations. Our goal is to map the physical conditions in the accretion disk as the source evolves through the various continuum states using the spectral diagnostics available in the Fe K fluorescence emission. Measurements of the Fe K emission will allow us to quantify the thermal, kinematic, and geometric conditions in both the disk and the surrounding material. Correlating the Fe K diagnostics with sensitive measurements of the direct and reprocessed continuum emission will allow us to map the evolving conditions and constrain models of the dynamic accretion processes in black hole binaries. We will monitor 7 targets with the RXTE. This observation will be triggered when one becomes active. | GALACTIC POINT SOURCES | 4 | A | JEAN COTTAM | JAP | 0 | SWG-TOO | FE K SPECTROSCOPY OF TRANSIENT BLACK HOLE BINARIES | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/400010020/ | Quick Look | ||
61 | NGC 4051 | 180.8556 | 44.5807 | 180.217538 | 44.859022 | 159.275193 | 40.404023 | 148.68917976 | 70.06918189 | 135.3482 | 53684.8015509259 | 2005-11-10 19:14:14 | 53687.4315277778 | 2005-11-13 10:21:24 | 700004010 | 119.578 | 150 | 119.61 | 119.61 | 119.586 | 119.578 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 120.0047 | 120.0047 | 227.1918 | 3 | PROCESSED | 57528.0225810185 | 2016-05-20 00:32:31 | 54247 | 2007-05-27 00:00:00 | 54037.5713078704 | 2006-10-29 13:42:41 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001012 | We propose to obtain a broad band spectrum of the narrow-line Seyfert 1 (NLS1) NGC 4051. NLS1s are often presumed that they host a relatively small black hole with a very high accretion rate. Such a class would have played an important role in the growth of black holes in a cosmological context. We will measure the intrinsic photon index, amount of reflection, and high energy cutoff for the first time to investigate an accretion disk under a high accretion rate and compare them with conventional broad-line Seyferts. | EXTRAGALACTIC COMPACT SOURCES | 7 | A | YUICHI TERASHIMA | JAP | 0 | SWG | THE ACCRETION IN THE NARROW-LINE SEYFERT 1 NGC 4051 PROBED BY A BROAD BAND SPECTRUM | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/700004010/ | Quick Look | ||
62 | SN1006 SW-Rim | 225.5051 | -42.0698 | 224.686984 | -41.873221 | 235.327536 | -23.832864 | 327.36692545 | 14.52303039 | 297.2712 | 53623.5862962963 | 2005-09-10 14:04:16 | 53624.993287037 | 2005-09-11 23:50:20 | 100019030 | 28.5245 | 50 | 28.5325 | 28.5245 | 28.5409 | 28.5405 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 27.0082 | 27.0082 | 121.5519 | 5 | PROCESSED | 57527.3126967593 | 2016-05-19 07:30:17 | 54247 | 2007-05-27 00:00:00 | 54034.9697453704 | 2006-10-26 23:16:26 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000019 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | SN1006 observation with XIS and HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100019030/ | Quick Look | ||||
63 | BD +30 3639 | 293.6993 | 30.5065 | 293.208675 | 30.395694 | 303.554886 | 51.223276 | 64.78119899 | 5.00649051 | 237.7342 | 53676.9934837963 | 2005-11-02 23:50:37 | 53677.8230324074 | 2005-11-03 19:45:10 | 100025020 | 31.1384 | 40 | 31.1384 | 31.1624 | 31.1464 | 31.1544 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 27.1258 | 27.1258 | 71.638 | 1 | PROCESSED | 57527.9315509259 | 2016-05-19 22:21:26 | 54247 | 2007-05-27 00:00:00 | 54037.1080902778 | 2006-10-29 02:35:39 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000025 | The proposed target, BD +30 3639, is a prototypical planetary nebula which emit diffuse X-rays; planetary nebulae represent the final evolutionary stage of low mass stars, and contain very rich information on the stellar nucleosynthesis. The Chandra ACIS spectrum of BD +30 3639 bears an amazingly strong Ne-K line, most certainly because the X-ray emitting material directly reflect the "onion-like structure" of elements insied evolved stars. However, the ACIS was not able to resolve C, N, O lines, which are of vital importance. The XMM RGS and Chandra LETG could do, but we need very long exposure. Using the Suzaku XIS-BI with the excellent low-energy performance, we can for the first time measure the C/N/O/Mg abundance ratios of this important object in a short time. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Observation of planetary nebula BD +30 3639 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100025020/ | Quick Look | |||
64 | KS1741-293(GC_BGD_2) | 266.2069 | -29.3515 | 265.410046 | -29.331146 | 266.666918 | -5.954235 | 359.55541243 | -0.06909433 | 265.0174 | 53637.5288541667 | 2005-09-24 12:41:33 | 53637.5946296296 | 2005-09-24 14:16:16 | 100027040 | 1.937 | 5 | 1.937 | 1.937 | 1.937 | 1.937 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 1.7637 | 1.7637 | 5.68 | 0 | PROCESSED | 57527.404525463 | 2016-05-19 09:42:31 | 54247 | 2007-05-27 00:00:00 | 53907.393275463 | 2006-06-21 09:26:19 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000027 | We propose to obtain high quality spectra from 6 positions near the GC. The objective is to resolve 6.4 , 6.7 and 6.9 keV line and determine the high energy tail from each positions and/or from the sub-structures in each position. Combining all the results, we can see which sub-sub-structure is X-ray reflection from Sgr A* ( 6.4 keV line+ 7.1 keV edge + high energy tail), thermal plasma (6.7+6.9 keV lines, with no hard X-ray tail), non thermal emission (e.g. line but hard X-ray tail). Unexpected spectral feature could be also found, depending on the real origin. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Suzaku Observation of Galactic Center Region | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100027040/ | Quick Look | |||
65 | HESS J1616-508_BGD2 | 244.4656 | -50.6883 | 243.5199 | -50.566183 | 251.824242 | -28.844194 | 332.70353325 | -0.14997577 | 283.1793 | 53633.8196412037 | 2005-09-20 19:40:17 | 53634.3120833333 | 2005-09-21 07:29:24 | 100028030 | 21.8735 | 25 | 21.8895 | 21.8895 | 21.8815 | 21.8735 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 18.2063 | 18.2063 | 42.5359 | 0 | PROCESSED | 57527.3722800926 | 2016-05-19 08:56:05 | 54247 | 2007-05-27 00:00:00 | 54035.4698842593 | 2006-10-27 11:16:38 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000028 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | New HESS sources and the Galactic ridge Background | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100028030/ | Quick Look | ||||
66 | ULXs in NGC 1313 | 49.5245 | -66.5352 | 49.373425 | -66.716272 | 341.380796 | -74.178462 | 283.41323765 | -44.63106544 | 172.6337 | 53658.556400463 | 2005-10-15 13:21:13 | 53659.6252777778 | 2005-10-16 15:00:24 | 100032010 | 32.878 | 40 | 32.878 | 32.878 | 32.878 | 32.878 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 30.38 | 30.38 | 92.3439 | 1 | PROCESSED | 57527.587349537 | 2016-05-19 14:05:47 | 54247 | 2007-05-27 00:00:00 | 54036.1929398148 | 2006-10-28 04:37:50 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000032 | We propose Suzaku observation of a nearby (4.5 Mpc) galaxy NGC 1313 hosting two prototypical ULXs. These ASCA specta of many ULXs were described with a "high temperature diskbb" model, spectra obtained with XMM (and Chandra) prefer a "power-law plus low-temperature disk" modeling. The superior 5-10 keV sensitivity of Suzaku allows us to examine whether the spectra of luminous ULXs indeed exhibit a turn-over around 5 keV or extend up to 10 keV. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | ULXs in NGC 1313 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100032010/ | Quick Look | |||
67 | A 3376 | 90.5561 | -39.9584 | 90.148808 | -39.956705 | 90.960808 | -63.398292 | 246.50686261 | -25.98989573 | 107.6124 | 53649.6153703704 | 2005-10-06 14:46:08 | 53653.4495833333 | 2005-10-10 10:47:24 | 100034010 | 118.7792 | 150 | 118.7792 | 121.7373 | 118.8498 | 119.3357 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 100.5401 | 100.5401 | 331.2537 | 3 | PROCESSED | 57527.6218171296 | 2016-05-19 14:55:25 | 54247 | 2007-05-27 00:00:00 | 54109.6396990741 | 2007-01-09 15:21:10 | 3.0.22.43 | 5 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000034 | Abell 3376 (z=0.046) is a merging cluster with a T=4 keV (*3) hosting a pair of strong radio halos (see figure). It is one of the few clusters from which BeppoSAX positively detected excess hard X-rays (Nevalainen et al. ApJ 608, 166, 2004). Because of the relatively low temperature, the HXD-PIN energy band is expected to be relatively free from thermal emission, making this object ideal to the search for non-thermal signals. We expect the non-thermal flux to be 4-5% of the PIN background at 20 keV, and a 150 ksec on-source exposure would be needed to securely detect this. To know the current background over the full COR range, an off-source exposure for one day or a ~40 ksec exposure onto a very soft source, would be required immediately before or after the on-source data acquisition. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Diffuse Hard X-rays from Clusters | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100034010/ | Quick Look | |||
68 | 1E1743.1-2843 GCBGD3 | 266.5944 | -28.6526 | 265.801896 | -28.634135 | 266.98972 | -5.247071 | 0.32852719 | 0.00581314 | 264.8798 | 53644.2657523148 | 2005-10-01 06:22:41 | 53644.3162268518 | 2005-10-01 07:35:22 | 100037050 | 2.4 | 5 | 2.4 | 2.4 | 2.4 | 2.4 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 2.2329 | 2.2329 | 4.3539 | 0 | PROCESSED | 57527.4530902778 | 2016-05-19 10:52:27 | 54247 | 2007-05-27 00:00:00 | 54056.1970833333 | 2006-11-17 04:43:48 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000037 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Suzaku Obseration of Galactic Center region 2 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100037050/ | Quick Look | ||||
69 | NORTH POLAR SPUR | 260.5905 | 4.7489 | 259.972652 | 4.795886 | 259.371969 | 27.842624 | 26.83412197 | 21.95376599 | 264.1143 | 53646.4785763889 | 2005-10-03 11:29:09 | 53647.4515277778 | 2005-10-04 10:50:12 | 100038010 | 43.0689 | 50 | 43.1489 | 44.2129 | 43.0689 | 43.2929 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 40.7715 | 40.7715 | 84.0019 | 0 | PROCESSED | 57527.5342824074 | 2016-05-19 12:49:22 | 54247 | 2007-05-27 00:00:00 | 54035.8928009259 | 2006-10-27 21:25:38 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000038 | We propose to observe the North Polar Spur for 100 ksec. The main objectives are below (1) Search for emission lines of N and C that originates from low kT emission (2) Precisely determine the abundance of the NPS The measurement of N and C lines will be the first for XIS. This is also the first for extended sources. The first trial to measure the emission from the C-band (below 0.3keV) by using BI. This will be a guide line how to use the C-band data. Since the C-band intensity is already known, this will be the first calibration of the BI at low energy. The scientific objectives are already given in the mail distributed in the swg. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | North Polar Spur | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100038010/ | Quick Look | |||
70 | CAS A | 350.8761 | 58.8091 | 350.310124 | 58.534509 | 27.390357 | 54.841399 | 111.74552355 | -2.13963884 | 214.5537 | 53783.6003472222 | 2006-02-17 14:24:30 | 53783.9218055556 | 2006-02-17 22:07:24 | 100043020 | 14.155 | 10 | 14.155 | 14.155 | 14.155 | 14.155 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 17.3713 | 17.3713 | 27.768 | 0 | PROCESSED | 57533.0311805556 | 2016-05-25 00:44:54 | 54247 | 2007-05-27 00:00:00 | 54041.4627893518 | 2006-11-02 11:06:25 | 3.0.22.43 | 5 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001097 | We propose the calibration observations for XIS: E0102-72 ... Gain and QE in the low energy band Cas A ... Gain and QE in the high energy band Eta Carinae ... Contamination of the BI chip | CALIBRATION | 1 | A | HIRONORI MATSUMOTO | JAP | 0 | SWG | XIS FLIGHT CAIBRATION PLAN | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100043020/ | Quick Look | ||
71 | Crab Nebula | 83.6372 | 22.097 | 82.884469 | 22.064333 | 84.106634 | -1.213794 | 184.48946706 | -5.73697 | 84.9994 | 53613.8323032407 | 2005-08-31 19:58:31 | 53613.975787037 | 2005-08-31 23:25:08 | 100015010 | 5.6587 | 5 | 5.6587 | 5.6587 | 5.6587 | 5.6587 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 5.7907 | 5.7907 | 12.3879 | 0 | PROCESSED | 57527.2296412037 | 2016-05-19 05:30:41 | 54247 | 2007-05-27 00:00:00 | 54109.1053240741 | 2007-01-09 02:31:40 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000015 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | HXD boresight check with Crab | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100015010/ | Quick Look | ||||
72 | Crab nebula | 83.6105 | 22.3483 | 82.856361 | 22.315501 | 84.093042 | -0.96164 | 184.26290563 | -5.62323625 | 86.8596 | 53607.2790509259 | 2005-08-25 06:41:50 | 53607.5139583333 | 2005-08-25 12:20:06 | 100010030 | 8.1129 | 5 | 8.1129 | 8.1129 | 8.1129 | 8.1129 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 7.8359 | 7.8359 | 20.264 | 1 | PROCESSED | 57526.8876388889 | 2016-05-18 21:18:12 | 54247 | 2007-05-27 00:00:00 | 54118.9698958333 | 2007-01-18 23:16:39 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000010 | Crab nebula multi pointings | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab Offset 1 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010030/ | Quick Look | |||
73 | N132D | 81.2794 | -69.6524 | 81.381964 | -69.694399 | 312.375338 | -85.522525 | 280.31514531 | -32.77566051 | 53.3291 | 53595.4703125 | 2005-08-13 11:17:15 | 53597.5313541667 | 2005-08-15 12:45:09 | 100002010 | 7.4066 | 80 | 7.4066 | 7.4066 | 7.4066 | 7.4066 | 2 | 2 | 2 | 2 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | PROCESSED | 57520.7109606482 | 2016-05-12 17:03:47 | 54247 | 2007-05-27 00:00:00 | 54038.5875925926 | 2006-10-30 14:06:08 | 3.0.22.43 | 6 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000002 | HXD HV ON WITH N132D, and 5 pointings with XIS | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | HXD HV ON WITH N132D | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100002010/ | Quick Look | |||
74 | TYCHO SNR HXD BKGD | 9.2173 | 64.3076 | 8.488109 | 64.032592 | 44.61366 | 53.051862 | 121.35322514 | 1.48051733 | 84.2005 | 53915.6541782407 | 2006-06-29 15:42:01 | 53916.7606944444 | 2006-06-30 18:15:24 | 500025010 | 51.0088 | 50 | 51.0088 | 51.0088 | 51.0088 | 51.0088 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 48.7224 | 48.7224 | 95.5939 | 2 | PROCESSED | 57534.8010300926 | 2016-05-26 19:13:29 | 54302 | 2007-07-21 00:00:00 | 54052.5940509259 | 2006-11-13 14:15:26 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001099 | We propose to observe Tycho's Supernova Remnant with Suzaku. The proposal has two main goals: (1) to measure the energy spectrum of the entire remnant above 10 keV with the HXD, and (2) to study the 0.5-10 keV band spectrum as a function of position with the XIS. | GALACTIC DIFFUSE EMISSION | 5 | A | JOHN HUGHES | JAP | 0 | SWG | SUZAKU STUDY OF TYCHO'S SUPERNOVA REMNANT | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500025010/ | Quick Look | ||
75 | Crab nebula | 83.6222 | 22.1365 | 82.869251 | 22.10376 | 84.094492 | -1.173718 | 184.44846107 | -5.72755512 | 86.8666 | 53608.2089236111 | 2005-08-26 05:00:51 | 53608.316087963 | 2005-08-26 07:35:10 | 100010080 | 3.382 | 5 | 3.382 | 3.382 | 3.382 | 3.382 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 3.7003 | 3.7003 | 9.2539 | 0 | PROCESSED | 57526.9140856482 | 2016-05-18 21:56:17 | 54247 | 2007-05-27 00:00:00 | 54119.0056134259 | 2007-01-19 00:08:05 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000010 | Crab nebula multi pointings | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab Offset 1 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010080/ | Quick Look | |||
76 | BULGE 2 | 270.6176 | -29.5847 | 269.818763 | -29.585758 | 270.530563 | -6.144879 | 1.30042786 | -3.49803376 | 83.2679 | 53801.7493981482 | 2006-03-07 17:59:08 | 53802.0689699074 | 2006-03-08 01:39:19 | 500002010 | 13.028 | 10 | 13.052 | 13.044 | 13.036 | 13.028 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 10.6741 | 10.6741 | 27.5999 | 1 | PROCESSED | 57533.1394444444 | 2016-05-25 03:20:48 | 54247 | 2007-05-27 00:00:00 | 54041.664525463 | 2006-11-02 15:56:55 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001014 | Leading . | GALACTIC DIFFUSE EMISSION | 5 | A | DAN MCCAMMON | JAP | 0 | SWG | THE SOFT GALACTIC BULGE | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500002010/ | Quick Look | ||
77 | CYGNUS LOOP | 313.9037 | 31.9696 | 313.388205 | 31.777464 | 329.228113 | 46.799115 | 75.63250703 | -8.50670526 | 64.2245 | 53884.8380671296 | 2006-05-29 20:06:49 | 53885.0891666667 | 2006-05-30 02:08:24 | 100049040 | 11.7656 | 10 | 11.7816 | 11.7816 | 11.7736 | 11.7656 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 9.788 | 9.788 | 21.6879 | 0 | PROCESSED | 57534.4771296296 | 2016-05-26 11:27:04 | 54258 | 2007-06-07 00:00:00 | 54052.5201157407 | 2006-11-13 12:28:58 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 015007 | Here is the list of the calibration sources in the AO-1 round: 1) E0102.2-7219 20ks x 2 2) PKS2155-304 30ks (simultaneous observation with CXO and XMM) 3) Galactic Center Plasma 50ks 4) Cygnus Loop 40ks (=10ks x 4), and 5) RXJ1856.5-3754 40ks | CALIBRATION | 1 | A | HIRONORI MATSUMOTO | JAP | 1 | SWG | XIS FLIGHT CALIBRATION PLAN | SPE | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100049040/ | Quick Look | ||
78 | A3376 WEST RELIC | 90.0363 | -39.9917 | 89.629297 | -39.992531 | 90.071049 | -63.433501 | 246.43145562 | -26.38385089 | 126.3601 | 54034.3950231482 | 2006-10-26 09:28:50 | 54035.9176388889 | 2006-10-27 22:01:24 | 800011020 | 62.2648 | 60 | 62.2648 | 62.2648 | 62.2648 | 62.2648 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 55.5629 | 55.5629 | 131.5378 | 2 | PROCESSED | 57535.9705902778 | 2016-05-27 23:17:39 | 54694 | 2008-08-16 00:00:00 | 54090.2671643518 | 2006-12-21 06:24:43 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001039 | We propose a 150 ks observation of the giant radio relic in the west of the A3376 cluster. A3376 is a low temperature (4.5 keV) cluster with possible excess hard X-ray emission in 2.7 sigma significance by Beppo-SAX, and also with a pair of giant radio relics. This target is best suited for cluster hard excess survey with HXD. Following the first observation planned around October 2005 located near the east relic, the observation of the west relic 23 arcmin away can bring us the first spacial information on cluster excess hard X-rays. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | KAZUHIRO NAKAZAWA | JAP | 0 | SWG | SEARCH FOR EXCESS HARD X-RAY EMISSION FROM ABELL 3376 | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/800011020/ | Quick Look | ||
79 | GRB060105 | 297.6095 | 46.3384 | 297.227077 | 46.210211 | 319.460988 | 65.110067 | 80.2506255 | 9.98748628 | 191.1906 | 53740.5089351852 | 2006-01-05 12:12:52 | 53741.5002083333 | 2006-01-06 12:00:18 | 900001010 | 42.2208 | 40 | 42.2208 | 42.2208 | 42.2208 | 42.2208 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 37.718 | 37.718 | 85.6419 | 2 | PROCESSED | 57532.6415856482 | 2016-05-24 15:23:53 | 54247 | 2007-05-27 00:00:00 | 54039.776712963 | 2006-10-31 18:38:28 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001008 | (i) Early break in lightcurve of X-ray afterglows using HXD. Recent Swift/XRT observations reveal that early X-ray afterglows of GRB has flat portion with very shallow decay. It may suggest continuous energy input from the central engine. The transition from its phase to general afterglow may display hard-to-soft evolution reflecting the cooling frequency. Thus multi wavelength observation will provide a key to the physics of central engine activity. (ii) Emission lines in the afterglows. The confirmation of line existence should be a matter of great importance because there remains unanswered questions. Some data may indicate a prominent iron line but others seem to suggest significant lower energy lines instead without iron lines. | EXTRAGALACTIC COMPACT SOURCES | 9 | A | TOSHIO MURAKAMI | JAP | 0 | SWG-TOO | TOO OBSERVATIONS OF GAMMA-RAY BURSTS | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/900001010/ | Quick Look | ||
80 | A2218_offset | 244.4769 | 65.4468 | 244.387309 | 65.566901 | 174.329918 | 79.629039 | 97.72059475 | 40.11912915 | 237.1965 | 53645.3474537037 | 2005-10-02 08:20:20 | 53646.32375 | 2005-10-03 07:46:12 | 100030020 | 44.8592 | 50 | 44.8592 | 46.1907 | 44.9141 | 45.3747 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 42.5366 | 42.5366 | 84.3439 | 0 | PROCESSED | 57527.5203125 | 2016-05-19 12:29:15 | 54247 | 2007-05-27 00:00:00 | 54036.969224537 | 2006-10-28 23:15:41 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000030 | Search of redshifted (z=0.171) OVII emission line from warm-hot intergalactic matter around a cluster which shows a merger feature in the line of sight, with no central cool component. The depth of the structure can be ~20 Mpc, and the redshift allows a clear separation of the lines from the Galactic hot gas. The low background and the superior resolution of XIS in the soft X-ray energy range will allow the best measurement of the WHIM emission so far. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | A2218 and its offset observation | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100030020/ | Quick Look | |||
81 | ABELL 1795 Far North | 207.223 | 26.9995 | 206.646903 | 27.247656 | 193.71055 | 35.352954 | 35.63943573 | 77.21561208 | 130.4264 | 53715.3208796296 | 2005-12-11 07:42:04 | 53715.9730092593 | 2005-12-11 23:21:08 | 800012030 | 30.6406 | 30 | 30.6486 | 30.6406 | 30.6639 | 30.6566 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 27.8833 | 27.8833 | 56.3379 | 1 | PROCESSED | 57532.4195833333 | 2016-05-24 10:04:12 | 54247 | 2007-05-27 00:00:00 | 54039.1003703704 | 2006-10-31 02:24:32 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001056 | We propose a 120 ks Suzaku observation of Abell 1795. Five overlapping XIS pointings will: i) map the temperature to the virial radius for the first time; ii) check for the presence of soft excess emission and, if found, possibly determine whether the excess is associated with the cluster or our Galaxy; and iii) determine the run of abundance with radius in detail at r< 500. This observation will demonstrate the scientific value of the low-background and good spectral resolution of the Suzaku XIS in cluster studies. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | MARK BAUTZ | JAP | 0 | SWG | TEMPERATURE, MASS AND SOFT-EXCESS MAPS TO THE VIRIAL RADIUS IN ABELL 1795 | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/800012030/ | Quick Look | ||
82 | SN 1006 SW-Rim | 225.4961 | -42.0706 | 224.678007 | -41.87399 | 235.320846 | -23.835662 | 327.36052248 | 14.52564865 | 117.2713 | 53761.0914930556 | 2006-01-26 02:11:45 | 53761.7155555556 | 2006-01-26 17:10:24 | 100019050 | 28.4186 | 50 | 28.4186 | 28.4186 | 28.4186 | 28.4186 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 24.7444 | 24.7444 | 53.91 | 0 | PROCESSED | 57532.7834375 | 2016-05-24 18:48:09 | 54247 | 2007-05-27 00:00:00 | 54040.4586689815 | 2006-11-01 11:00:29 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000019 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | SN1006 observation with XIS and HXD | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100019050/ | Quick Look | |||
83 | BULGE 3 | 274.7046 | -31.4846 | 273.893726 | -31.505472 | 274.041648 | -8.109784 | 1.3002625 | -7.49777303 | 80.4025 | 53800.3437962963 | 2006-03-06 08:15:04 | 53801.7474421296 | 2006-03-07 17:56:19 | 500001010 | 51.8468 | 50 | 51.8548 | 51.8548 | 51.8548 | 51.8468 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 45.0783 | 45.0783 | 121.2459 | 0 | PROCESSED | 57533.1540972222 | 2016-05-25 03:41:54 | 54247 | 2007-05-27 00:00:00 | 54041.7128703704 | 2006-11-02 17:06:32 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001014 | Leading . | GALACTIC DIFFUSE EMISSION | 5 | A | DAN MCCAMMON | JAP | 0 | SWG | THE SOFT GALACTIC BULGE | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500001010/ | Quick Look | ||
84 | SN1006 NW | 225.6364 | -41.8003 | 224.819551 | -41.604176 | 235.339658 | -23.546444 | 327.59294648 | 14.70833496 | 115.0008 | 53766.4881365741 | 2006-01-31 11:42:55 | 53767.55375 | 2006-02-01 13:17:24 | 500017010 | 53.0194 | 50 | 53.0194 | 53.0277 | 53.0273 | 53.0273 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 60.4123 | 60.4123 | 92.0679 | 0 | PROCESSED | 57532.8347685185 | 2016-05-24 20:02:04 | 54247 | 2007-05-27 00:00:00 | 54040.7669675926 | 2006-11-01 18:24:26 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001062 | We propose two Suzaku pointings of the Galactic supernova remnant (SNR) that exploded as a supernova in 1006. The main goal of the project is to use the XIS measure the abundances of low-Z elements in the ejecta. | GALACTIC DIFFUSE EMISSION | 5 | A | JOHN HUGHES | JAP | 0 | SWG | THE EJECTA IN SN1006 | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500017010/ | Quick Look | ||
85 | A 2218 OFFSETB | 249.9091 | 65.2119 | 249.835523 | 65.307656 | 180.044789 | 81.713752 | 96.37864193 | 38.09205953 | 233.3309 | 53670.1916319444 | 2005-10-27 04:35:57 | 53670.4620833333 | 2005-10-27 11:05:24 | 800020010 | 14.9215 | 15 | 14.9375 | 14.9335 | 14.9215 | 14.9415 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 14.1931 | 14.1931 | 23.3561 | 0 | PROCESSED | 57527.6596180556 | 2016-05-19 15:49:51 | 54247 | 2007-05-27 00:00:00 | 54036.8343981482 | 2006-10-28 20:01:32 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001096 | To confirm the presence of redshifted oxygen lines from the WHIM surrounding A2218, we propose observations of 2 positions. One is a 35 ksec pointing on A2218 to raise the photon statistics of the oxygen feature, and the other is a 15 ksec pointing at about 1 degree west of the cluster to know the amplitude of the intensity variation of the Galactic oxygen lines. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | TAKAYA OHASHI | JAP | 0 | SWG | SEARCH FOR OXYGEN LINES FROM WARM IGM | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/800020010/ | Quick Look | |||
86 | CAS A | 350.8729 | 58.8094 | 350.30695 | 58.534812 | 27.388607 | 54.842749 | 111.74406014 | -2.13880346 | 214.7372 | 53768.5363657407 | 2006-02-02 12:52:22 | 53768.833599537 | 2006-02-02 20:00:23 | 100043010 | 0 | 10 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 1 | 0 | 0 | 10.3268 | 10.3268 | 25.6739 | 1 | PROCESSED | 57532.8451736111 | 2016-05-24 20:17:03 | 54247 | 2007-05-27 00:00:00 | 54040.7488888889 | 2006-11-01 17:58:24 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001097 | We propose the calibration observations for XIS: E0102-72 ... Gain and QE in the low energy band Cas A ... Gain and QE in the high energy band Eta Carinae ... Contamination of the BI chip | CALIBRATION | 1 | A | HIRONORI MATSUMOTO | JAP | 0 | SWG | XIS FLIGHT CAIBRATION PLAN | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100043010/ | Quick Look | ||
87 | A 2218 CENTER | 249.0052 | 66.205 | 248.955095 | 66.304813 | 172.75657 | 81.615548 | 97.72589248 | 38.11630228 | 233.3294 | 53669.4904050926 | 2005-10-26 11:46:11 | 53670.1905555556 | 2005-10-27 04:34:24 | 800019010 | 31.9354 | 35 | 31.9434 | 31.9434 | 31.9354 | 31.9434 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 28.9371 | 28.9371 | 60.4879 | 1 | PROCESSED | 57527.6471990741 | 2016-05-19 15:31:58 | 54247 | 2007-05-27 00:00:00 | 54036.9596990741 | 2006-10-28 23:01:58 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001096 | To confirm the presence of redshifted oxygen lines from the WHIM surrounding A2218, we propose observations of 2 positions. One is a 35 ksec pointing on A2218 to raise the photon statistics of the oxygen feature, and the other is a 15 ksec pointing at about 1 degree west of the cluster to know the amplitude of the intensity variation of the Galactic oxygen lines. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | TAKAYA OHASHI | JAP | 0 | SWG | SEARCH FOR OXYGEN LINES FROM WARM IGM | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/800019010/ | Quick Look | |||
88 | A 2052 | 229.0471 | 6.9211 | 228.432118 | 7.104686 | 224.516271 | 24.128025 | 9.16646689 | 50.17566284 | 281.2031 | 53603.6121875 | 2005-08-21 14:41:33 | 53603.9938425926 | 2005-08-21 23:51:08 | 100006040 | 16.7443 | 20 | 16.7443 | 16.7443 | 16.7443 | 16.7443 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 12.8395 | 12.8395 | 32.9519 | 0 | PROCESSED | 57520.7325810185 | 2016-05-12 17:34:55 | 53705 | 2005-12-01 00:00:00 | 53905.4634143518 | 2006-06-19 11:07:19 | 3.0.22.43 | 5 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000006 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Outer region of A 2052 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100006040/ | Quick Look | ||||
89 | Crab Nebula | 83.5484 | 22.0881 | 82.795741 | 22.055005 | 84.024019 | -1.219032 | 184.45272098 | -5.81121698 | 85.0004 | 53614.9103009259 | 2005-09-01 21:50:50 | 53615.0418518518 | 2005-09-02 01:00:16 | 100015050 | 5.3447 | 5 | 5.3447 | 5.3447 | 5.3447 | 5.3447 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 5.4859 | 5.4859 | 11.356 | 0 | PROCESSED | 57527.2511342593 | 2016-05-19 06:01:38 | 54247 | 2007-05-27 00:00:00 | 54109.1357986111 | 2007-01-09 03:15:33 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000015 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | HXD boresight check with Crab | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100015050/ | Quick Look | ||||
90 | NGC 2992 | 146.4207 | -14.2696 | 145.81924 | -14.038457 | 154.003817 | -26.061971 | 249.65504756 | 28.81616071 | 88.7924 | 53693.8781597222 | 2005-11-19 21:04:33 | 53694.9759722222 | 2005-11-20 23:25:24 | 700005020 | 37.4935 | 120 | 37.6565 | 39.6915 | 37.4935 | 37.8205 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 33.8991 | 33.8991 | 94.8479 | 1 | PROCESSED | 57528.0334490741 | 2016-05-20 00:48:10 | 54247 | 2007-05-27 00:00:00 | 54037.7316087963 | 2006-10-29 17:33:31 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001013 | NGC 2992 is a nearby Seyfert 1.9 galaxy showing long-term (20 yrs) large amplitude (factor of 20) variability. This object showed switching between Compton-thick and -thin. Recent RXTE monitoring has shown that this object is highly variable on shorter time scales (2 weeks). We propose three Suzaku observations to monitor the variability of absorption column, broad band continuum shape, and Fe line intensity to understand the cause of the remarkable variability. | EXTRAGALACTIC COMPACT SOURCES | 7 | A | YUICHI TERASHIMA | JAP | 0 | SWG | THE SPECTRAL VARIABILITY IN NGC 2992: FE-LINE, REFLECTION, AND COMPTON-THIN/THICK SWITCHING | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/700005020/ | Quick Look | ||
91 | Cas A | 350.8254 | 58.8156 | 350.259841 | 58.54105 | 27.364711 | 54.864063 | 111.72292809 | -2.12474901 | 12.9937 | 53614.2486458333 | 2005-09-01 05:58:03 | 53614.7640509259 | 2005-09-01 18:20:14 | 100016010 | 27.965 | 20 | 27.973 | 27.973 | 27.973 | 27.965 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 24.13 | 24.13 | 44.4959 | 2 | PROCESSED | 57527.2832175926 | 2016-05-19 06:47:50 | 53705 | 2005-12-01 00:00:00 | 53905.4659606482 | 2006-06-19 11:10:59 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000016 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Cas A | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100016010/ | Quick Look | ||||
92 | NEP | 272.7884 | 65.9814 | 272.771336 | 65.967881 | 333.879188 | 88.742697 | 95.75202722 | 28.67554678 | 290.9299 | 53615.6136921296 | 2005-09-02 14:43:43 | 53617.625162037 | 2005-09-04 15:00:14 | 100018010 | 106.2015 | 100 | 106.2015 | 106.2175 | 106.2495 | 106.2255 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 106.125 | 106.125 | 173.5718 | 3 | PROCESSED | 57527.2880092593 | 2016-05-19 06:54:44 | 53705 | 2005-12-01 00:00:00 | 53905.4636921296 | 2006-06-19 11:07:43 | 3.0.22.43 | 6 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000018 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | HXD background at North Ecliptic Pole | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100018010/ | Quick Look | ||||
93 | A3376 WEST RELIC | 90.0415 | -39.9946 | 89.634521 | -39.995405 | 90.079962 | -63.436398 | 246.43569548 | -26.38071178 | 132.0018 | 53681.5938078704 | 2005-11-07 14:15:05 | 53684.7883912037 | 2005-11-10 18:55:17 | 800011010 | 126.9969 | 150 | 126.9969 | 127.1809 | 127.0769 | 127.0289 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 112.9113 | 112.9113 | 230.9397 | 3 | PROCESSED | 57528.0013541667 | 2016-05-20 00:01:57 | 54247 | 2007-05-27 00:00:00 | 54037.6050231482 | 2006-10-29 14:31:14 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001039 | We propose a 150 ks observation of the giant radio relic in the west of the A3376 cluster. A3376 is a low temperature (4.5 keV) cluster with possible excess hard X-ray emission in 2.7 sigma significance by Beppo-SAX, and also with a pair of giant radio relics. This target is best suited for cluster hard excess survey with HXD. Following the first observation planned around October 2005 located near the east relic, the observation of the west relic 23 arcmin away can bring us the first spacial information on cluster excess hard X-rays. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | KAZUHIRO NAKAZAWA | JAP | 0 | SWG | SEARCH FOR EXCESS HARD X-RAY EMISSION FROM ABELL 3376 | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/800011010/ | Quick Look | ||
94 | Crab Nebula | 83.6274 | 22.0192 | 82.875108 | 21.986487 | 84.094124 | -1.29112 | 184.55062413 | -5.78629385 | 86.8663 | 53604.1571412037 | 2005-08-22 03:46:17 | 53604.2501273148 | 2005-08-22 06:00:11 | 100007010 | 1.7229 | 5 | 1.7229 | 1.7229 | 1.7229 | 1.7229 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 1.808 | 1.808 | 8.034 | 0 | PROCESSED | 57520.7330324074 | 2016-05-12 17:35:34 | 54247 | 2007-05-27 00:00:00 | 54105.2758912037 | 2007-01-05 06:37:17 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000007 | Crab nebula multi pointings | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab Nebula | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100007010/ | Quick Look | |||
95 | Crab nebula | 83.6201 | 22.1854 | 82.866876 | 22.152649 | 84.094711 | -1.124779 | 184.40591259 | -5.70300776 | 86.8631 | 53604.2507175926 | 2005-08-22 06:01:02 | 53604.3889351852 | 2005-08-22 09:20:04 | 100007020 | 3.0531 | 5 | 3.0571 | 3.0531 | 3.0531 | 3.0531 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 3.1343 | 3.1343 | 11.94 | 1 | PROCESSED | 57520.7416782407 | 2016-05-12 17:48:01 | 54247 | 2007-05-27 00:00:00 | 54105.2987268518 | 2007-01-05 07:10:10 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000007 | Crab nebula multi pointings | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab Nebula | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100007020/ | Quick Look | |||
96 | Crab nebula | 83.4512 | 22.0082 | 82.699013 | 21.974637 | 83.930395 | -1.294795 | 184.47195778 | -5.93010486 | 86.7989 | 53604.489849537 | 2005-08-22 11:45:23 | 53604.5835416667 | 2005-08-22 14:00:18 | 100007040 | 4.2682 | 5 | 4.2682 | 4.2682 | 4.2682 | 4.2682 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 4.1392 | 4.1392 | 8.056 | 0 | PROCESSED | 57520.7454513889 | 2016-05-12 17:53:27 | 54247 | 2007-05-27 00:00:00 | 54105.3073726852 | 2007-01-05 07:22:37 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000007 | Crab nebula multi pointings | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Crab Nebula | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100007040/ | Quick Look | |||
97 | NGC 4945 | 196.3733 | -49.4666 | 195.643253 | -49.198924 | 217.025297 | -38.636782 | 305.27803835 | 13.34111135 | 313.9078 | 53605.101087963 | 2005-08-23 02:25:34 | 53605.1034490741 | 2005-08-23 02:28:58 | 100008020 | 0.1776 | 10 | 0.1815 | 0.1815 | 0.1796 | 0.1776 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 0.2001 | 0.2001 | 0.202 | 0 | PROCESSED | 57526.8486574074 | 2016-05-18 20:22:04 | 54247 | 2007-05-27 00:00:00 | 54034.6891435185 | 2006-10-26 16:32:22 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000008 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | NGC 4945 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100008020/ | Quick Look | ||||
98 | CYG X-1 | 299.5907 | 35.1892 | 299.120596 | 35.052727 | 313.656273 | 54.237702 | 71.32454904 | 3.06010347 | 276.9898 | 53648.2025347222 | 2005-10-05 04:51:39 | 53648.6335532407 | 2005-10-05 15:12:19 | 100036010 | 18.213 | 20 | 18.213 | 18.213 | 18.213 | 18.213 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 18.1457 | 18.1457 | 37.2299 | 0 | PROCESSED | 57527.5598726852 | 2016-05-19 13:26:13 | 54247 | 2007-05-27 00:00:00 | 54037.7278819444 | 2006-10-29 17:28:09 | 3.0.22.43 | 5 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000036 | We propose to probe the geometry of optically-thick accretion disks which should exist around a BH even in the hard state and to verify the HXD performance to thermal cut-off in hard X-rays expected from AGN. The 1st may be done by measuring the cool disk emission with the XIS-BI, resolving the fluorescent Fe-K line with the XIS-FI and detecting the reflection continuum with the HXD. Since these features are thought to come from the optically-thick disk a simultaneous measurement will for the 1st time allow for self-consistent constraining of the disk geometry in the hard state. Cyg X-1 is the best & most secure object for this stufy and is now in the low/hard state. A 20 ks Suzaku obs. is sufficient to get a fine spectrum up to 300 keV & to determine the cutoff with a high significance. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Cyg X-1 in the low state | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100036010/ | Quick Look | |||
99 | Sgr_B2 | 266.8775 | -28.4435 | 266.086257 | -28.426412 | 267.234561 | -5.032377 | 0.63628385 | -0.09835114 | 265.3727 | 53653.5194560185 | 2005-10-10 12:28:01 | 53655.2954050926 | 2005-10-12 07:05:23 | 100037060 | 76.5966 | 100 | 76.6286 | 76.6446 | 76.5966 | 76.6286 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 70.8192 | 70.8192 | 153.4319 | 0 | PROCESSED | 57527.5776041667 | 2016-05-19 13:51:45 | 54247 | 2007-05-27 00:00:00 | 54036.2262731482 | 2006-10-28 05:25:50 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000037 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Suzaku Obseration of Galactic Center region 2 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100037060/ | Quick Look | ||||
100 | Sgr_B2_BGD | 267.0943 | -28.1356 | 266.304946 | -28.119568 | 267.419629 | -4.720546 | 0.99854005 | -0.10262599 | 269.0208 | 53655.2988888889 | 2005-10-12 07:10:24 | 53655.4620833333 | 2005-10-12 11:05:24 | 100037070 | 9.1612 | 10 | 9.1612 | 9.1643 | 9.1643 | 9.1632 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 9.5364 | 9.5364 | 14.092 | 0 | PROCESSED | 57527.5688078704 | 2016-05-19 13:39:05 | 54247 | 2007-05-27 00:00:00 | 54036.0749884259 | 2006-10-28 01:47:59 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000037 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Suzaku Obseration of Galactic Center region 2 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100037070/ | Quick Look | ||||
101 | MKN 3 | 93.8839 | 71.0477 | 92.433649 | 71.063052 | 91.875357 | 47.63268 | 143.2836301 | 22.71631463 | 71.8326 | 53665.0848263889 | 2005-10-22 02:02:09 | 53667.2682175926 | 2005-10-24 06:26:14 | 100040010 | 95.0265 | 100 | 95.0265 | 95.0772 | 95.0452 | 95.0345 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 91.3441 | 91.3441 | 188.6299 | 0 | PROCESSED | 57527.6643055556 | 2016-05-19 15:56:36 | 54247 | 2007-05-27 00:00:00 | 53906.4896759259 | 2006-06-20 11:45:08 | 3.0.22.43 | 5 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000040 | Mkn 3 is the second brightest Compton-thick Sy 2 currently visible with Suzaku. The broadband spectrum of Mkn 3, as probed by previous SAX and Chandra observations, is dominated by a reflection component (Compton hump strength R is near 1), but there is also evidence for a strongly absorbed hard X-ray power law that may be direct emission from the obscured nucleus, filtering through Compton-thick material (such as the molecular torus). | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | MKN 3 | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100040010/ | Quick Look | ||
102 | RXJ1856.5-3754 | 284.1498 | -37.9103 | 283.298136 | -37.976359 | 281.509901 | -15.033652 | 358.59888263 | -17.21635309 | 269.4259 | 53667.2829976852 | 2005-10-24 06:47:31 | 53669.4793287037 | 2005-10-26 11:30:14 | 100041010 | 76.2548 | 80 | 0 | 76.2548 | 0 | 0 | 0 | 2 | 0 | 0 | 1 | 0 | 0 | 62.6217 | 62.6217 | 189.72 | 3 | PROCESSED | 57527.6811111111 | 2016-05-19 16:20:48 | 54247 | 2007-05-27 00:00:00 | 54037.2294791667 | 2006-10-29 05:30:27 | 3.0.22.43 | 5 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000041 | We propose Suzaku observation of a nearby isolated neuron star RXJ1856.5-3754 for the low energy QE calibration of the XIS. Our main purpose is, however, using this source as a soft X-ray QE calibrator on the sky. We hope this source will be observed again in future to check possible contamination on the filter surface etc. Note that the calibration is not only for the BI-CCD(XIS1), but also for FI-CCDs or relative QE among them. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | LOW ENERGY QE CALIBRATION OF XIS | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100041010/ | Quick Look | ||
103 | E0102-72 | 16.027 | -72.0223 | 15.622199 | -72.290248 | 314.64413 | -65.039289 | 301.54815221 | -45.07189388 | 294.0751 | 53768.8467592593 | 2006-02-02 20:19:20 | 53769.4065393518 | 2006-02-03 09:45:25 | 100044030 | 20.8277 | 20 | 20.8357 | 20.8437 | 20.8437 | 20.8277 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 20.2688 | 20.2688 | 48.36 | 1 | PROCESSED | 57532.8615740741 | 2016-05-24 20:40:40 | 54247 | 2007-05-27 00:00:00 | 53905.6764351852 | 2006-06-19 16:14:04 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001097 | We propose the calibration observations for XIS: E0102-72 ... Gain and QE in the low energy band Cas A ... Gain and QE in the high energy band Eta Carinae ... Contamination of the BI chip | CALIBRATION | 1 | A | HIRONORI MATSUMOTO | JAP | 0 | SWG | XIS FLIGHT CAIBRATION PLAN | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100044030/ | Quick Look | ||
104 | ETA CARINAE | 161.248 | -59.6859 | 160.761598 | -59.422588 | 202.142 | -58.929196 | 287.58997588 | -0.63475906 | 156.124 | 53769.4163194444 | 2006-02-03 09:59:30 | 53769.9481944444 | 2006-02-03 22:45:24 | 100045010 | 21.3678 | 20 | 21.3678 | 21.3678 | 21.3678 | 21.3678 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 18.1458 | 18.1458 | 45.9459 | 1 | PROCESSED | 57532.9369907407 | 2016-05-24 22:29:16 | 54247 | 2007-05-27 00:00:00 | 54040.9846643518 | 2006-11-01 23:37:55 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001097 | We propose the calibration observations for XIS: E0102-72 ... Gain and QE in the low energy band Cas A ... Gain and QE in the high energy band Eta Carinae ... Contamination of the BI chip | CALIBRATION | 1 | A | HIRONORI MATSUMOTO | JAP | 0 | SWG | XIS FLIGHT CAIBRATION PLAN | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100045010/ | Quick Look | ||
105 | BULGE 6 | 282.6839 | -33.8925 | 281.860158 | -33.951684 | 280.687841 | -10.9215 | 1.99857856 | -14.59644221 | 88.3467 | 53802.7373032407 | 2006-03-08 17:41:43 | 53803.0466087963 | 2006-03-09 01:07:07 | 500003010 | 14.2617 | 10 | 14.2617 | 14.2617 | 14.2617 | 14.2617 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 11.414 | 11.414 | 26.7159 | 1 | PROCESSED | 57533.1570833333 | 2016-05-25 03:46:12 | 54247 | 2007-05-27 00:00:00 | 54041.7424305556 | 2006-11-02 17:49:06 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001014 | Leading . | GALACTIC DIFFUSE EMISSION | 5 | A | DAN MCCAMMON | JAP | 0 | SWG | THE SOFT GALACTIC BULGE | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500003010/ | Quick Look | ||
106 | X1630-472 | 248.4772 | -47.3405 | 247.556757 | -47.236251 | 254.058584 | -25.081993 | 336.93627828 | 0.30053306 | 75.5959 | 53794.9708333333 | 2006-02-28 23:18:00 | 53795.6968055556 | 2006-03-01 16:43:24 | 400010030 | 21.5216 | 200 | 21.5216 | 21.5216 | 21.5216 | 21.5216 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 19.0328 | 19.0328 | 62.718 | 0 | PROCESSED | 57533.1079050926 | 2016-05-25 02:35:23 | 54247 | 2007-05-27 00:00:00 | 54041.5956018518 | 2006-11-02 14:17:40 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001058 | We propose to monitor a transient black hole binary in outburst through a series of 20 ks observations. Our goal is to map the physical conditions in the accretion disk as the source evolves through the various continuum states using the spectral diagnostics available in the Fe K fluorescence emission. Measurements of the Fe K emission will allow us to quantify the thermal, kinematic, and geometric conditions in both the disk and the surrounding material. Correlating the Fe K diagnostics with sensitive measurements of the direct and reprocessed continuum emission will allow us to map the evolving conditions and constrain models of the dynamic accretion processes in black hole binaries. We will monitor 7 targets with the RXTE. This observation will be triggered when one becomes active. | GALACTIC POINT SOURCES | 4 | A | JEAN COTTAM | JAP | 0 | SWG-TOO | FE K SPECTROSCOPY OF TRANSIENT BLACK HOLE BINARIES | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/400010030/ | Quick Look | ||
107 | LOCKMANHOLE | 163.4063 | 57.6108 | 162.636897 | 57.876997 | 137.149157 | 45.549363 | 148.98193179 | 53.14624927 | 119.611 | 53688.2372337963 | 2005-11-14 05:41:37 | 53689.8300694444 | 2005-11-15 19:55:18 | 100046010 | 76.9806 | 100 | 76.9806 | 77.0446 | 77.0126 | 77.0206 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 94.5107 | 94.5107 | 137.6079 | 3 | PROCESSED | 57528.0048148148 | 2016-05-20 00:06:56 | 54247 | 2007-05-27 00:00:00 | 54037.5889814815 | 2006-10-29 14:08:08 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001098 | We propose a 100 ks observation of LockmanHole with Suzaku. The main purpose is to obtain a template dataset of HXD background. | CALIBRATION | 1 | A | MOTOHIDE KOKUBUN | JAP | 0 | SWG | BACKGROUND ESTABLISHMENT OF HXD | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100046010/ | Quick Look | ||
108 | AE AQUARII | 310.0612 | -0.931 | 309.416636 | -1.108991 | 312.236832 | 16.82972 | 45.23545862 | -24.46836188 | 250.6241 | 54033.2319907407 | 2006-10-25 05:34:04 | 54034.3829282407 | 2006-10-26 09:11:25 | 400001020 | 47.9743 | 50 | 47.9743 | 48.5956 | 48.1316 | 48.3103 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 45.5384 | 45.5384 | 99.4239 | 1 | PROCESSED | 57526.8238773148 | 2016-05-18 19:46:23 | 54526 | 2008-03-01 00:00:00 | 54109.7083449074 | 2007-01-09 17:00:01 | 3.0.22.43 | 9 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001004 | We have a new idea that a magnetized white dwarf can be a particle-acceleration cite to emit non thermal emission. In order to understand the particle acceleration process in rotation-powered objects, it is important to measure the hard X-ray emission from magnetized white dwarfs, in addition to that from well-known neutron stars. Here, we propose a 100ksec observation of a magnetic cataclysmic valiable, AE Aqurii. It is difficult for INTEGRAL mission, and is challenging even for the HXD, but it will be a ``first detection'' of the non-thermal emission in the hard X-ray band from a white dwarf with Suzaku. | GALACTIC POINT SOURCES | 4 | A | YUKIKATSU TERADA | JAP | 0 | SWG | SEARCH FOR THE NON-THERMAL EMISSION FROM MAGNETIZED WHITE DWARF WITH SUZAKU | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/400001020/ | Quick Look | ||
109 | GX 349+2 | 256.4194 | -36.3657 | 255.579957 | -36.298328 | 258.779942 | -13.451385 | 349.14166441 | 2.79326977 | 78.9359 | 53813.9267708333 | 2006-03-19 22:14:33 | 53814.6043402778 | 2006-03-20 14:30:15 | 400003020 | 28.1177 | 50 | 28.1177 | 28.1317 | 28.1204 | 28.1204 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 25.6573 | 25.6573 | 58.538 | 0 | PROCESSED | 57533.2767939815 | 2016-05-25 06:38:35 | 54247 | 2007-05-27 00:00:00 | 54042.1657407407 | 2006-11-03 03:58:40 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001026 | We propose Suzaku observations of two luminous low-mass X-ray binaries (Z sources), GX 349+2 and Cyg X-2, to investigate the origin of the hard tails of Z sources, of which the spectral photon indices are reported to become occasionally less than unity. With the high sensitivity of the HXD, we detect the spectral shape up to several 100 keV and reveal existence of particle acceleration caused by high radiation pressure. | GALACTIC POINT SOURCES | 4 | A | HIROMITSU TAKAHASHI | JAP | 0 | SWG | SUZAKU OBSERVATIONS OF THE HARD TAILS OF LUMINOUS LOW-MASS X-RAY BINARIES (Z SOURCES) | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/400003020/ | Quick Look | ||
110 | SN1006 NE BG | 226.7036 | -41.3998 | 225.886024 | -41.207391 | 236.037501 | -22.925171 | 328.51405135 | 14.65073262 | 293.6503 | 53617.7018865741 | 2005-09-04 16:50:43 | 53622.1668287037 | 2005-09-09 04:00:14 | 100019010 | 44.7503 | 50 | 44.7543 | 44.7543 | 44.7543 | 44.7503 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 37.3883 | 37.3883 | 385.6018 | 5 | PROCESSED | 57527.2923148148 | 2016-05-19 07:00:56 | 54247 | 2007-05-27 00:00:00 | 54035.4224768518 | 2006-10-27 10:08:22 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000019 | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | SN1006 observation with XIS and HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100019010/ | Quick Look | ||||
111 | X1630-472 | 248.4828 | -47.3401 | 247.56235 | -47.235876 | 254.062648 | -25.080987 | 336.93914719 | 0.29801709 | 78.3341 | 53774.6318981482 | 2006-02-08 15:09:56 | 53775.1390972222 | 2006-02-09 03:20:18 | 400010010 | 22.1902 | 200 | 22.1902 | 22.1902 | 22.1902 | 22.1902 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 22.247 | 22.247 | 43.816 | 0 | PROCESSED | 57532.9380787037 | 2016-05-24 22:30:50 | 54247 | 2007-05-27 00:00:00 | 54040.9540856482 | 2006-11-01 22:53:53 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001058 | We propose to monitor a transient black hole binary in outburst through a series of 20 ks observations. Our goal is to map the physical conditions in the accretion disk as the source evolves through the various continuum states using the spectral diagnostics available in the Fe K fluorescence emission. Measurements of the Fe K emission will allow us to quantify the thermal, kinematic, and geometric conditions in both the disk and the surrounding material. Correlating the Fe K diagnostics with sensitive measurements of the direct and reprocessed continuum emission will allow us to map the evolving conditions and constrain models of the dynamic accretion processes in black hole binaries. We will monitor 7 targets with the RXTE. This observation will be triggered when one becomes active. | GALACTIC POINT SOURCES | 4 | A | JEAN COTTAM | JAP | 0 | SWG-TOO | FE K SPECTROSCOPY OF TRANSIENT BLACK HOLE BINARIES | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/400010010/ | Quick Look | ||
112 | 73P/SW3 | 279.6627 | 33.4734 | 279.203358 | 33.427762 | 284.650097 | 56.423756 | 62.35168426 | 17.03145652 | 46.5564 | 53862.4804282407 | 2006-05-07 11:31:49 | 53862.5419444444 | 2006-05-07 13:00:24 | 500012020 | 3.248 | 5 | 3.248 | 3.248 | 3.248 | 3.248 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 2.1119 | 2.1119 | 5.2799 | 0 | PROCESSED | 57533.7332407407 | 2016-05-25 17:35:52 | 54256 | 2007-06-05 00:00:00 | 54042.2282175926 | 2006-11-03 05:28:38 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001050 | Cometary X-ray emission is likely the result of charge exchange interactions between the highly charged solar wind and neutral material ablated from the nucleus. Recent measurements using Chandra coupled with precise laboratory measurements at EBIT lend support for this hypothesis. In fact we have successfully deconvolved the Chandra/ACIS observation of comet C/Linear using direct observations of charge exchanging plasmas at EBIT using a flight spare XRS detector system. Here, we propose to observe a magnitude 1 comet, 73P/SW 3, the brightest comet of the decade during May 2006 within only 0.08 AU of the earth using the XIS1 (BI) instrument on Suzaku. The exceptional low energy response of the XIS will allow us to unambiguously identify the x-ray emission mechanism in comets. | GALACTIC DIFFUSE EMISSION | 5 | A | FREDERICK PORTER | JAP | 0 | SWG | AN XIS OBSERVATION OF THE BRIGHTEST COMET OF THE DECADE: 73P/SCHWASSMANN-WACHMANN 3 | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500012020/ | Quick Look | ||
113 | 73P/SW3 | 316.717 | 24.6807 | 316.164001 | 24.478965 | 328.484877 | 39.12074 | 71.53645371 | -15.07849931 | 72.7087 | 53868.1752314815 | 2006-05-13 04:12:20 | 53868.2085532407 | 2006-05-13 05:00:19 | 500013010 | 2.353 | 20 | 2.353 | 2.353 | 2.353 | 2.353 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 2.595 | 2.595 | 2.8719 | 0 | PROCESSED | 57534.2831597222 | 2016-05-26 06:47:45 | 54256 | 2007-06-05 00:00:00 | 54042.2312268518 | 2006-11-03 05:32:58 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001050 | Cometary X-ray emission is likely the result of charge exchange interactions between the highly charged solar wind and neutral material ablated from the nucleus. Recent measurements using Chandra coupled with precise laboratory measurements at EBIT lend support for this hypothesis. In fact we have successfully deconvolved the Chandra/ACIS observation of comet C/Linear using direct observations of charge exchanging plasmas at EBIT using a flight spare XRS detector system. Here, we propose to observe a magnitude 1 comet, 73P/SW 3, the brightest comet of the decade during May 2006 within only 0.08 AU of the earth using the XIS1 (BI) instrument on Suzaku. The exceptional low energy response of the XIS will allow us to unambiguously identify the x-ray emission mechanism in comets. | GALACTIC DIFFUSE EMISSION | 5 | A | FREDERICK PORTER | JAP | 0 | SWG | AN XIS OBSERVATION OF THE BRIGHTEST COMET OF THE DECADE: 73P/SCHWASSMANN-WACHMANN 3 | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500013010/ | Quick Look | ||
114 | 73P/SW3 | 317.1042 | <