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 | IRAS 00397-1312 | 10.5707 | -12.9503 | 9.941553 | -13.224287 | 4.464578 | -16.066781 | 113.89016485 | -75.66108211 | 246.4295 | 55558.1361342593 | 2010-12-28 03:16:02 | 55560.2501388889 | 2010-12-30 06:00:12 | 705046010 | 83.7928 | 90 | 83.7928 | 83.7928 | 0 | 83.7928 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 71.9314 | 71.9314 | 182.6317 | 1 | PROCESSED | 57632.5965856482 | 2016-09-01 14:19:05 | 56040 | 2012-04-23 00:00:00 | 55670.3615046296 | 2011-04-19 08:40:34 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 051441 | We propose two Suzaku-HXD observations of two ULIRGs hosting a deeply buried AGN. These two objects are expected to host a powerful AGN in the luminosity range of quasars, based on solid evidence from mid-IR Spitzer spectroscopy. However, these sources are completely buried behind a screen of dust with column density in excess of 10^24 cm^-2, so not only the primary emission below 10 keV is obscured, but the reflected emission, usually ascribed to a circumnuclear "torus", is also absent. This suggests a complete spherical coverage of the X-ray source along all directions. The unique capabilities of Suzaku at high energies will allow to confirm the existence of these objects, representing the most extreme examples of buried AGNs, both in terms of obscuration and of intrinsic luminosity. | EXTRAGALACTIC COMPACT SOURCES | 7 | C | GUIDO RISALITI | USA | 5 | AO5 | BURIED QUASAR 2S INSIDE ULIRGS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/705046010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '705046010'
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