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 | 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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