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 | UGC 03142 | 70.9469 | 28.9681 | 70.161272 | 28.87543 | 73.291585 | 6.626144 | 172.09277202 | -10.99747628 | 264.8107 | 56335.692349537 | 2013-02-12 16:36:59 | 56336.9946296296 | 2013-02-13 23:52:16 | 707032010 | 51.2847 | 50 | 51.2847 | 51.2927 | 0 | 51.3007 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 47.5632 | 47.5632 | 112.51 | 1 | PROCESSED | 57610.6216898148 | 2016-08-10 14:55:14 | 56721 | 2014-03-05 00:00:00 | 56349.5963541667 | 2013-02-26 14:18:45 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 071424 | A hard X-ray-selected (BAT) AGN sample shows a remarkable 70% of the local population of type 1 AGN to have extreme hard excesses above 20 keV, likely caused by Compton-thick gas in the line-of-sight, covering at least 50% of the source. We request six snapshot observations to complete a Suzaku survey of a BAT-flux-limited sample and make a complete and unbiased measurement of the incidence. Analysis of the new sources will be performed in conjunction with existing exposures, providing exciting new insight into the previously unknown structures in hard X-ray selected AGN. | EXTRAGALACTIC COMPACT SOURCES | 7 | C | TRACEY TURNER | USA | 7 | AO7 | INVESTIGATING COMPTON-THICK ABSORBERS IN TYPE 1 AGN: OVERHAULING THE AGN PARADIGM | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/707032010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '707032010'
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