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 PKS 1345+12 206.9131 12.3498 206.299989 12.598696 200.201065 21.844458 347.38894416 70.20282736 113.9421 54472.3082407407 2008-01-07 07:23:52 54473.6799768518 2008-01-08 16:19:10 702053010 52.9844 50 52.9844 52.9844 0 52.9844 2 2 0 2 1 0 0 45.2034 45.2034 118.5038 4 PROCESSED 57541.3141782407 2016-06-02 07:32:25 54854 2009-01-23 00:00:00 54483.4984375 2008-01-18 11:57:45 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021341 We wish to take advantage of the sensitivity of Suzaku above 10 keV to constrain the energy source -- starburst or black-hole driven activity -- in three of the brightest warm transitional ultraluminous infrared galaxies, PKS 1345+12, Mrk 463, and 3C 273. These objects are arguably the best local laboratories to study the basic physical processes involved in creating massive early type hosts on the one hand, and feeding embedded supermassive black holes on the other hand, in major galaxy mergers. The Suzaku data will be used to search for the high-energy signature of deeply buried active black holes and to look for short time scale variability, another signature of black-hole driven activity. These data will be combined with our A01 spectra and be part of S. Teng's PhD thesis at UMD. EXTRAGALACTIC COMPACT SOURCES 7 C SYLVAIN VEILLEUX USA 2 AO2 SPECTRA OF THE BRIGHTEST WARM ULTRALUMINOUS INFRARED GALAXIES HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702053010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '702053010'

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