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 | 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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