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 NGC 3431 162.8114 -17.015 162.196181 -16.749458 171.110311 -22.386386 266.03803779 37.10135134 298.5009 56089.5660648148 2012-06-11 13:35:08 56091.5571412037 2012-06-13 13:22:17 707012010 65.6756 70 65.6756 65.6756 0 65.6756 2 2 0 2 1 0 0 59.8819 59.8819 171.9959 2 PROCESSED 57605.6909259259 2016-08-05 16:34:56 56473 2013-06-30 00:00:00 56106.3662384259 2012-06-28 08:47:23 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 070067 The nature of the hard X-ray emission of many AGN remains ill-understood. Using the latest 70 month Swift/BAT sky survey, we have selected optically-classified Seyfert 2s with a very hard BAT photon index (Gamma<1.4). The BAT energy range is not strongly affected by obscuration unless the column is Compton-thick. The selected sources are radio-quiet, arguing against jet-dominated non-thermal spectra. The cause of a low Gamma is unknown, but may include high or atypical obscuration, non-thermal X-ray emission without associated radio/optical jets or the presence of electron coronae with temperatures or optical depths higher than average. Our aim is to observe two of the hardest Seyfert 2s (neither of which has prior pointed observations below 10 keV) with Suzaku to elucidate their nature. EXTRAGALACTIC COMPACT SOURCES 7 A POSHAK GANDHI JAP 7 AO7 WHAT IS THE NATURE OF SWIFT/BAT HARD-SPECTRUM SEYFERT 2S? XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/707012010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '707012010'

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