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 SWIFT J0350.1-5019 57.5315 -50.3337 57.174394 -50.483946 28.735241 -67.001155 259.74491819 -49.02538792 320.5309 53838.5046875 2006-04-13 12:06:45 53838.6752199074 2006-04-13 16:12:19 701017010 2.6998 20 2.7158 2.7158 2.6998 2.7078 2 2 2 2 1 0 0 1.1771 1.1771 9.165 0 PROCESSED 57533.4464930556 2016-05-25 10:42:57 54750 2008-10-11 00:00:00 53905.4679398148 2006-06-19 11:13:50 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010133 Swift/BAT extragalactic survey above E>15 keV has provided us with the first truely unbiased AGN sample in the local universe. The second BAT catalog contains about 80 sources, where a significant fraction is "new" AGNs without measurement of spectra below 15 keV. Here we propose to observe 6 new (non type-1) AGNs with Suzaku to make the BAT sample complete. Many are expected to be Compton-thick AGNs and hence the HXD data are crucial. This will lead us to the first direct measurement of the fraction of Compton thick AGNs and column density distribution, which are key parameters in the population synthesis of the X-ray background. This proposal is complementary to our separate proposal tntitled "broad band spectra of new Swift/BAT AGNs and the origin of the X-ray background". EXTRAGALACTIC COMPACT SOURCES 7 A YOSHIHIRO UEDA JAP 1 AO1 DIRECT DETERMINATION OF THE FRACTION OF COMPTON THICK AGNS IN THE LOCAL UNIVERSE HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701017010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '701017010'

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