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 | SWIFT J0911.2+4533 | 137.9062 | 45.5305 | 137.073312 | 45.735684 | 126.030873 | 27.898314 | 174.70874001 | 43.11152809 | 111.3983 | 54764.185787037 | 2008-10-25 04:27:32 | 54766.2105787037 | 2008-10-27 05:03:14 | 703008010 | 93.879 | 80 | 93.879 | 93.879 | 0 | 93.895 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 80.2256 | 80.2256 | 174.9298 | 4 | PROCESSED | 57544.2883564815 | 2016-06-05 06:55:14 | 55148 | 2009-11-13 00:00:00 | 54782.4040625 | 2008-11-12 09:41:51 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 030034 | The hard X-ray survey with Swift BAT have been finding various types of AGNs. Many buried AGNs with very low scattered X-rays have been discovered, for example. We propose to obtain broad band spectra of Compton-thin buried AGNs in the Swift sample. The data will be used to measure the amount of absoption in the direct and reflected emission and to constrain the structure of the obscuring matter around the AGN. | EXTRAGALACTIC COMPACT SOURCES | 7 | A | YUICHI TERASHIMA | JAP | 3 | AO3 | THE STRUCTURE OF BURIED COMPTON-THIN AGNS DISCOVERED BY SWIFT | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/703008010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '703008010'
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