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 HESS J1731-347 263.0179 -34.7706 262.185573 -34.73474 264.142481 -11.47104 353.53173388 -0.68198005 79.8005 54154.7807060185 2007-02-23 18:44:13 54155.7432291667 2007-02-24 17:50:15 401099010 40.6189 38 40.6269 40.6189 0 40.6269 2 2 0 2 1 0 0 34.6479 34.6479 83.1559 0 PROCESSED 57537.4739351852 2016-05-29 11:22:28 54528 2008-03-03 00:00:00 54160.3931944444 2007-03-01 09:26:12 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 012042 The hard (Gamma=2.0) TeV source HESS J1731-347 discovered in the H.E.S.S. Galactic plane survey has an intriguing possible counterpart seen in ROSAT survey data. The X-ray data show an unidentified, extended nebular structure with a hard spectrum, in close coincidence to the TeV source. It is plausible to assume that the same energetic particle population is responsible for the emission in both bands. Suzaku is optimally suited to establish the likely non-thermal nature of the X-ray spectrum and to search for the high-energy end of the emitting particle spectrum, which is likely visible in the HXD domain. The observations will help to clarify the nature of HESS J1731-347, which may be a new type of Galactic particle accelerator. GALACTIC POINT SOURCES 4 A GERD PUEHLHOFER EUR 1 AO1 THE HIGH ENERGY PARTICLE SPECTRUM OF THE TEV/X-RAY NEBULA HESS J1731-347 XIS N https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/401099010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '401099010'

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