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 323-G032 | 193.3499 | -41.5832 | 192.653913 | -41.311875 | 210.129179 | -32.696187 | 303.32560645 | 21.28704922 | 104.5857 | 54456.5856481482 | 2007-12-22 14:03:20 | 54458.1459953704 | 2007-12-24 03:30:14 | 702119010 | 79.2494 | 80 | 80.8178 | 79.2494 | 0 | 80.8014 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 86.8967 | 86.8967 | 134.7778 | 1 | PROCESSED | 57540.9568055556 | 2016-06-01 22:57:48 | 54854 | 2009-01-23 00:00:00 | 54483.1116203704 | 2008-01-18 02:40:44 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 022033 | The high-energy detectors onboard Swift and INTEGRAL are mapping the hard (>10 keV) X-ray sky. Although limited to bright X-ray fluxes (~1e-11 erg/cm2/s), the large area surveyed so far has allowed to build up sizable samples of hard X-ray selected AGN almost unbiased against X-ray absorption. On the basis of a careful analysis of the available X-ray observations below 10 keV, we identified a sample of relatively bright AGN which are likely to be obscured by Compton-thick (logN_H >24) cold gas. Two of them were observed in EAO-1 and the results confirmed our predictions. We propose further Suzaku observations of 3 bright objects (F(20-40 keV) ~ 0.7-1.4 x 1e-11 erg/cm2/s) which will allow us to unveil previously unknown nearby heavily obscured AGN. | EXTRAGALACTIC COMPACT SOURCES | 7 | A | ANDREA COMASTRI | EUR | 2 | AO2 | BRIGHT COMPTON-THICK GALAXIES IN THE BACKYARD - PART II | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702119010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '702119010'
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