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 | ARK 347 | 181.0952 | 20.2476 | 180.45595 | 20.52594 | 172.634722 | 18.942585 | 243.01628342 | 77.22827936 | 294.4295 | 55377.99625 | 2010-06-30 23:54:36 | 55378.8668171296 | 2010-07-01 20:48:13 | 705002010 | 38.9726 | 40 | 38.9886 | 38.9726 | 0 | 38.9886 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 35.9876 | 35.9876 | 75.2099 | 0 | PROCESSED | 57552.4401851852 | 2016-06-13 10:33:52 | 55772 | 2011-07-30 00:00:00 | 55404.2387268518 | 2010-07-27 05:43:46 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 050003 | We propose to observe two Swift/BAT selected obscured AGNs with significant scattered emission, Mrk 18 and Ark 347. Hard X-ray selected AGNs show some peculiar characteristics compared to optically selected ones such as weak scattering emission from the opening part of the putative torus and weak plasma emission in the soft X-ray band. The targets are Swift/BAT selected AND show significant scattered emission, which are poorly explored with Suzaku so far. Our aims are to constrain the geometrical structure of the obscuring matter based on broad-band X-ray spectra and compare them with other hard X-ray or optically selected obscured AGNs. | EXTRAGALACTIC COMPACT SOURCES | 7 | B | YUICHI TERASHIMA | JAP | 5 | AO5 | THE STRUCTURE OF COMPTON-THIN AGNS WITH SIGNIFICANT SCATTERED EMISSION SELECTED BY SWIFT/BAT | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/705002010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '705002010'
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