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 GX 339-4 255.7095 -48.7885 254.761689 -48.717523 259.577896 -25.861992 338.94163546 -4.32765826 281.8009 54733.942650463 2008-09-24 22:37:25 54736.0968055556 2008-09-27 02:19:24 403067010 104.994 100 105.018 104.994 0 104.994 2 2 0 2 1 0 0 114.7759 114.7759 186.0917 2 PROCESSED 57544.0505092593 2016-06-05 01:12:44 55148 2009-11-13 00:00:00 54780.5803935185 2008-11-10 13:55:46 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 031174 Understanding black hole systems in their canonical hard state is a major goal of high energy astrophysics. This state features a hard X-ray spectrum, a high level of timing noise, and emission from a steady jet at radio, IR, and perhaps higher frequencies. Along with our multi-wavelength, radio to X-ray, program, Suzaku observations can constrain theoretical models by answering the following questions: Does the inner edge of the accretion disk recede in the hard state? How is the location of the disk's inner edge related to the presence of a jet? Here, we propose to extend X-ray and radio studies of the hard state to low flux levels in order to answer these questions. GALACTIC POINT SOURCES 4 A JOHN TOMSICK USA 3 AO3-TOO CONSTRAINING MODELS FOR BLACK HOLE ACCRETION IN THE HARD STATE XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/403067010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '403067010'

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