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 KS1741-293(GC_BGD_2) 266.2069 -29.3515 265.410046 -29.331146 266.666918 -5.954235 359.55541243 -0.06909433 265.0174 53637.5288541667 2005-09-24 12:41:33 53637.5946296296 2005-09-24 14:16:16 100027040 1.937 5 1.937 1.937 1.937 1.937 1 1 1 1 1 0 0 1.7637 1.7637 5.68 0 PROCESSED 57527.404525463 2016-05-19 09:42:31 54247 2007-05-27 00:00:00 53907.393275463 2006-06-21 09:26:19 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000027 We propose to obtain high quality spectra from 6 positions near the GC. The objective is to resolve 6.4 , 6.7 and 6.9 keV line and determine the high energy tail from each positions and/or from the sub-structures in each position. Combining all the results, we can see which sub-sub-structure is X-ray reflection from Sgr A* ( 6.4 keV line+ 7.1 keV edge + high energy tail), thermal plasma (6.7+6.9 keV lines, with no hard X-ray tail), non thermal emission (e.g. line but hard X-ray tail). Unexpected spectral feature could be also found, depending on the real origin. CALIBRATION 1 A SWG JAP 0 SWG Suzaku Observation of Galactic Center Region N https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/100027040/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '100027040'

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