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 RXJ1713-3946-BKGD2 257.2742 -41.0338 256.397744 -40.970376 259.926088 -18.035902 345.80577047 -0.54060643 270.0033 53641.2980671296 2005-09-28 07:09:13 53642.1843055556 2005-09-29 04:25:24 100026030 37.5132 40 37.5372 37.5292 37.5132 37.5132 2 2 2 2 1 0 0 31.8982 31.8982 76.5659 0 PROCESSED 57527.4461574074 2016-05-19 10:42:28 54247 2007-05-27 00:00:00 54035.6187268518 2006-10-27 14:50:58 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000026 RXJ1713 is very important sources in which we can study particle accelerator in the universe. X-ray synchrotron spectrum suggest the existence of distribution of high energy electron. Very similar TeV and ASCA morphologies show close connection between these energy bands. The interaction with molecular cloud suggests that proton accelerator resides in this object. The photon index of RXJ1713 seems to be difficult in the frame work of standard diffusive shock scenario. To obtain precise spectrum in the hard X-ray region is therefore very important to determine the energy cut off and to study the mechanism that produce such high energy electrons. CALIBRATION 1 A SWG JAP 0 SWG Observation of RXJ1713.7-3946 N https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/100026030/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '100026030'

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