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
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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