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 4992 197.2442 11.5776 196.620329 11.84391 191.275652 17.435393 318.61367169 73.91298788 297.9177 53904.2287615741 2006-06-18 05:29:25 53905.2112615741 2006-06-19 05:04:13 701080010 38.7886 40 38.7886 38.7886 38.7886 38.7886 2 2 2 2 1 0 0 33.6179 33.6179 84.8819 1 PROCESSED 57534.7313657407 2016-05-26 17:33:10 54422 2007-11-18 00:00:00 53926.1865856482 2006-07-10 04:28:41 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 012016 The high-energy detectors onboard Swift and INTEGRAL have started to survey the hard X-ray sky above 10 keV. Although limited to bright X-ray fluxes (~10^-11 cgs), the large area surveyed so far has allowed to build up sizable sa mples of hard X-ray selected AGN almost unbiased against X-ray absorption. The AGN content of these surveys is dominated by obscured AGN. We have identified 3 objects which are most likely obscured by Compton-thick matter and very bright above 10 keV. We propose to observe them with Suzaku for 40 ks each to study their broad-band X-ray spectra and unveil previously unknown nearby heavily obscured AGN, with important consequences for the study of the AGN evolution and the synthesis of the X-ray background. EXTRAGALACTIC COMPACT SOURCES 7 A ANDREA COMASTRI EUR 1 AO1 BRIGHT COMPTON THICK GALAXIES IN THE BACKYARD HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701080010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '701080010'

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