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 | GRO J1008-57 | 152.4324 | -58.2988 | 152.000949 | -58.052431 | 193.900762 | -61.316578 | 282.99756699 | -1.83025918 | 104.6149 | 54434.481087963 | 2007-11-30 11:32:46 | 54435.8023032407 | 2007-12-01 19:15:19 | 902003010 | 47.746 | 40 | 47.746 | 47.7654 | 0 | 47.7814 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 42.3701 | 42.3701 | 114.146 | 1 | PROCESSED | 57540.795462963 | 2016-06-01 19:05:28 | 54434 | 2007-11-30 00:00:00 | 54441.1193171296 | 2007-12-07 02:51:49 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 027003 | The cyclotron resonance is a direct method to know the surface magnetic field of X-ray binary pulsars. It was measured from a little more than ten X-ray pulsars. The flares of the Be transient pulsars are rare occasions that we can measure it. For this X-ray binary pulsar GRO J1008-57, Suzaku HXD GSO is the only useful detector. The inferred resonance energy of 90 keV will be the highest resonance energy. It locates at the higher end of the resonance energy distribution. Considering the span of the flares, this will be the first and the last chance for Suzaku to observe GRO J1008-57, and generally speaking, a feature at ~100keV. | GALACTIC POINT SOURCES | 9 | A | SWG | JAP | 2 | TOO | SUZAKU TOO PROPOSAL OF GRO J1008-57 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/902003010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '902003010'
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