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 ESO 119-G008 72.2547 -57.6544 72.033322 -57.73981 38.878903 -77.915205 266.66680471 -38.87724734 324.43 56411.0111458333 2013-04-29 00:16:03 56413.2355787037 2013-05-01 05:39:14 708004010 100.5873 100 100.5953 100.5953 0 100.5873 2 2 0 2 1 0 0 103.7614 103.7614 192.1719 3 PROCESSED 57611.2384375 2016-08-11 05:43:21 56837 2014-06-29 00:00:00 56475.7648611111 2013-07-02 18:21:24 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 080027 At faint fluxes, the Swift/BAT AGN survey is uncovering sources with very hard photon indices (Gamma) above 10 keV. The origin of a low Gamma in the hard band is ill-understood, but may include high/atypical obscuration, non-thermal X-rays without radio jets, or electron coronae with high temperatures or optical depths. In AO7, we observed two such Seyfert 2s and discovered Compton-thick obscuration in one source, and a buried AGN spectrum with no reflection or high-energy cutoff in the other. The hard BAT Gamma values thus have a variety of origins, and our strategy is very effective in selecting objects with interesting spectra. Here, we propose to observe two hardest sources (Gamma<~1) with no prior X-ray observations below 10 keV in order to shed light on the nature of this population. EXTRAGALACTIC COMPACT SOURCES 7 A POSHAK GANDHI JAP 8 AO8 THE VARIED NATURE OF SWIFT/BAT HARD-SPECTRUM SEYFERT 2S XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/708004010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '708004010'

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