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 LMC X -3 84.7048 -64.0785 84.635001 -64.10439 45.912813 -86.683865 273.57060216 -32.09537201 185.5067 54822.3015856482 2008-12-22 07:14:17 54823.8675694444 2008-12-23 20:49:18 403020010 73.9738 60 73.9738 73.9818 0 73.9875 2 2 0 2 1 0 0 70.0505 70.0505 135.2838 1 PROCESSED 57545.0347800926 2016-06-06 00:50:05 55206 2010-01-10 00:00:00 54840.5013310185 2009-01-09 12:01:55 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 030102 Ionized iron K absorption lines are commonly observed from high state black hole binaries. Thus the highly ionized plasma are thought to be generally associated with optically thick accretion disks. Huge outflow by the plasma has been confirmed by some of these objects, and thus such plasma is thought to have an important role on accretion flow. In order to establish generality of the plasma by detecting the absorption lines, and to distinguish whether creation mechanism of the plasma is determined by X-ray luminosity or there is another key parameter, we propose Suzaku observation of luminous persistent black hole binary LMC X-3, with exposure of 60ks. This observation will enable us to find critical parameters which determine the creation of the accretion disk wind. GALACTIC POINT SOURCES 4 C AYA KUBOTA JAP 3 AO3 SEARCH FOR IRON K ABSORPTION LINES FROM LMC X-3 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/403020010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '403020010'

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