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 SWIFT J2248.8+1725 342.1903 17.444 341.576565 17.179413 350.711211 23.025613 85.72592105 -36.41328844 248.2402 56997.6938888889 2014-12-06 16:39:12 56999.668287037 2014-12-08 16:02:20 709004010 78.0938 80 78.0938 78.0938 0 78.0938 2 2 0 2 1 0 0 68.8266 68.8266 170.56 1 PROCESSED 57617.5240046296 2016-08-17 12:34:34 57460 2016-03-13 00:00:00 57092.3224652778 2015-03-11 07:44:21 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 090018 We propose to observe two hard X-ray bright Seyfert galaxies with a highly accreting small BH. This class of objects is of importance in studying accretion processes under a large mass accretion rate and therefore mass growth of black holes. Our aims are (1) to measure a continuum shape such as spectral slope and high energy cutoff, (2) to compare them with other classes of AGNs, and (3) to search for highly ionized outflows with a large column density. All of these will be fundamental pieces of information to better understand accretion physics and ``feedback'' processes in galaxies. EXTRAGALACTIC COMPACT SOURCES 7 C YUICHI TERASHIMA JAP 9 AO9 ACCRETION AND OUTFLOW IN THE HARD X-RAY SELECTED LOW-MASS SEYFERTS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/709004010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '709004010'

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