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 MRK 520 330.1768 10.545 329.561779 10.304216 336.215385 21.249415 69.38972894 -34.038497 250.5002 56258.8186458333 2012-11-27 19:38:51 56260.6571412037 2012-11-29 15:46:17 407014010 79.7795 80 79.7795 79.7875 0 79.7955 2 2 0 2 1 0 0 77.641 77.641 158.8258 1 PROCESSED 57608.1523263889 2016-08-08 03:39:21 56644 2013-12-18 00:00:00 56275.7255555556 2012-12-14 17:24:48 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 070028 Compton-thick AGNs contribute to the hard X-ray background and are key objects for investigating the cosmological evolution of AGNs. But heavy obscuration under 10 keV, and source misidentification mean that very few sources have been studied in detail. We have developed new infrared and hard X-ray diagnostics of AGN identification, based on which we select one candidate, Mrk 520, which must be very highly obscured and likely Compton-thick. With Suzaku, we will characterize all emission components, not only thermal and scattering components under 10 keV, but also the heavily obscured continuum over 10 keV, and reflection components. GALACTIC POINT SOURCES 4 C KEIKO MATSUTA JAP 7 AO7 MRK 520 : A NEW COMPTON-THICK AGN? XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/407014010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '407014010'

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