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 AB DOR 82.2881 -65.4658 82.252574 -65.503277 15.679222 -86.688003 275.31538375 -33.00189818 204.2849 54108.0647569444 2007-01-08 01:33:15 54109.4724421296 2007-01-09 11:20:19 401031020 49.0965 45 49.0965 49.0965 0 49.0965 2 2 0 2 1 0 0 44.9611 44.9611 121.6199 2 PROCESSED 57536.5000578704 2016-05-28 12:00:05 54502 2008-02-06 00:00:00 54133.0127083333 2007-02-02 00:18:18 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 011021 We propose to observe the rapidly rotating star AB Doradus for 80 ks with Suzaku Our main goals are to detect non-thermal hard X-rays and fluorescent Fe at 6.4 keV with the HXD and the XIS during a stellar flare. Such a spectral feature can be induced by non-thermal electrons in the impulsive flare phase, or by X-rays of the very hot flare plasma. The hard X-ray detectors will be used to detect non-thermal bremsstrahlung expected when a beam of non-thermal electrons (typically observed in the radio) impacts the dense chromosphere. We will also study the coronal element composition and its temporal evolution during the flare. Finally, we will attempt coordination with the Australian Telescope to monitor the non-thermal electron population, without any timing constraint for Suzaku. GALACTIC POINT SOURCES 4 B MARC AUDARD USA 1 AO1 NON-THERMAL HARD X-RAYS AND FLUORESCENT FE IN STELLAR FLARES HXD N https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/401031020/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '401031020'

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