DARTS Astro

total 1

No. target_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 proposal_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 hxd_burst_num processing_status processing_end_time_mjd processing_end_time public_date_mjd public_date distribute_start_date_mjd distribute_start_date processing_version processing_quantity processing_software proposal_id proposal_abstract proposal_category proposal_category_code proposal_priority pi_name co_pi_name proposal_affiliated_country proposal_cycle_count observation_type proposal_title main_detector xis_injection_flag 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://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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