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 | ANTICENTER | 113.3357 | -19.5305 | 112.785719 | -19.421448 | 119.46206 | -40.613154 | 234.9976882 | 0.00424804 | 280.7829 | 54212.8606481482 | 2007-04-22 20:39:20 | 54215.4197222222 | 2007-04-25 10:04:24 | 502021010 | 89.5429 | 80 | 89.5509 | 89.5589 | 0 | 89.5429 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 78.9887 | 78.9887 | 221.0508 | 3 | PROCESSED | 57538.5236689815 | 2016-05-30 12:34:05 | 54744 | 2008-10-05 00:00:00 | 54223.2040046296 | 2007-05-03 04:53:46 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 020032 | We propose to observe diffuse radiation from the Galactic plane in the general direction of the anticenter. Absolute measurement of the O VII and O VIII line fluxes will help establish the origin of this mysterious component of the diffuse background. This will allow a search for spectral signatures of non-thermal emission, i.e. charge- exchange emission, in the 3/4 keV band and the determination of abundances in hot gas thermal emission without risk of confusion by emission from hot gas in the Galactic Bulge. | GALACTIC DIFFUSE EMISSION | 5 | B | KENSUKE MASUI | JAP | 2 | AO2 | SOFT X-RAY DIFFUSE EMISSION FROM THE GALACTIC DISK | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/502021010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '502021010'
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