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 565-G019 | 143.6802 | -21.9346 | 143.106087 | -21.711094 | 154.563677 | -34.141633 | 253.87283017 | 21.67453181 | 298.0016 | 56067.8709259259 | 2012-05-20 20:54:08 | 56069.9022222222 | 2012-05-22 21:39:12 | 707013010 | 78.9239 | 80 | 78.9239 | 78.9319 | 0 | 78.9319 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 71.1211 | 71.1211 | 175.4878 | 2 | PROCESSED | 57605.5328935185 | 2016-08-05 12:47:22 | 56448 | 2013-06-05 00:00:00 | 56079.3396643518 | 2012-06-01 08:09:07 | 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/ver3.0/707013010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '707013010'
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