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 EV LAC 341.7127 44.3232 341.158134 44.059332 6.045133 46.919235 100.60502245 -13.08073089 256.1601 54432.9692013889 2007-11-28 23:15:39 54434.4655208333 2007-11-30 11:10:21 402032010 68.9493 100 68.9493 69.1333 0 69.1275 2 1 0 2 1 0 0 65.0113 65.0113 129.2328 2 PROCESSED 57540.7939236111 2016-06-01 19:03:15 54808 2008-12-08 00:00:00 54441.0876851852 2007-12-07 02:06:16 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021013 We propose a 100 ks Suzaku XIS observation of the dMe flare star EV Lac to measure coronal element abundances during quiescence and flares of different sizes. EV Lac undergoes frequent small flares, and is known to have undergone a very large flare at ~300 times the quiescent count rate in 2000. Coronal abundance changes shed light on the process of chromospheric evaporation under conditions different to those on the Sun. Depending on the size and spectrum of the flare, we may also be able to detect a hard burst of emission that would serve as a time marker for particle acceleration during the flare. GALACTIC POINT SOURCES 4 C UNA HWANG USA 2 AO2 FLARE AND QUIESENT CONORAL ELEMENT ABUNDANCES IN EV LAC XIS Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/402032010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '402032010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏