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 IGR J12391-1612 189.807 -16.1292 189.153193 -15.854578 195.389743 -10.939243 298.65896251 46.64122293 122.9437 54818.9051273148 2008-12-18 21:43:23 54822.2910648148 2008-12-22 06:59:08 703007010 130.274 120 130.274 130.274 0 130.274 2 2 0 2 1 0 0 111.0893 111.0893 292.4838 2 PROCESSED 57545.0634953704 2016-06-06 01:31:26 55206 2010-01-10 00:00:00 54840.5288425926 2009-01-09 12:41:32 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 030012 We propose a Suzaku observation of a Compton thick candidate, IGR J12391-1612. This source is a bright Seyfert 2 galaxy in the INTEGRAL AGN catalog by Beckman et al. 2006. By a follow-up observation in the optical band, this source was classified as an X-ray luminous type 2 Seyfert galaxy. A Chandra follow-up observation was also performed, but the shape of the X-ray spectrum was not well determined due to a short exposure of 3.5ks. Thank to the wide-band spectroscopy of Suzaku, we can obtain an X-ray spectrum in the 0.5-100 keV band. We will reveal the nature of this Compton thick Seyfert in a spectral analysis. EXTRAGALACTIC COMPACT SOURCES 7 A HISAMITSU AWAKI JAP 3 AO3 X-RAY OBSERVATION OF A COMPTON THICK CANDIDATE, IGR J12391-1612 HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/703007010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '703007010'

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