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 1
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 | 4U1626-67 | 248.0601 | -67.4675 | 246.801189 | -67.3606 | 258.324109 | -44.911512 | 321.78071552 | -13.09322804 | 103.0359 | 53803.0543518518 | 2006-03-09 01:18:16 | 53805.818275463 | 2006-03-11 19:38:19 | 400015010 | 102.6392 | 100 | 102.654 | 102.6392 | 102.6472 | 102.654 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 93.3932 | 93.3932 | 238.7819 | 3 | PROCESSED | 57533.2349652778 | 2016-05-25 05:38:21 | 54247 | 2007-05-27 00:00:00 | 54042.4663657407 | 2006-11-03 11:11:34 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001081 | The X-ray spectrum of the 7 second LMXRB pulsar 4U1626-67 is dominated by low energy line emission with little evedence of iron K line in the pulse phase resolved spectra. It showd also cyclotron line at 37 keV that departs from the correlation of energy cutoff cyclotron energy observed in many other X-ray pulsars. This Suzaku observation allow to characterize the overall continuum, the low energy, the iron K alpha and cyclotron lines as function of the pulse phase, | GALACTIC POINT SOURCES | 4 | A | LORELLA ANGELINI | JAP | 0 | SWG | 4U1626-67: PHASE RESOLVED SPECTRA AND CYCLOTRON LINE | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/400015010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '400015010'
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