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 | 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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