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 ESO 263-G013 152.4256 -42.8603 151.905124 -42.614062 176.412344 -49.376708 273.99206854 10.74227458 292.0779 54252.4568287037 2007-06-01 10:57:50 54253.5946064815 2007-06-02 14:16:14 702120010 45.2947 40 45.3027 45.3027 0 45.2947 2 2 0 2 1 0 0 40.1035 40.1035 98.2999 2 PROCESSED 57538.8009143518 2016-05-30 19:13:19 54745 2008-10-06 00:00:00 54258.5006134259 2007-06-07 12:00:53 3.0.22.43 3 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 B ANDREA COMASTRI EUR 2 AO2 BRIGHT COMPTON-THICK GALAXIES IN THE BACKYARD - PART II HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702120010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '702120010'

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