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 LS I+61 303_3 40.2018 61.1949 39.239095 60.980826 59.865781 42.86376 135.72005286 1.06843757 246.2753 54872.1842592593 2009-02-10 04:25:20 54873.7252199074 2009-02-11 17:24:19 403017010 68.6273 60 68.6273 68.6273 0 68.6273 2 2 0 2 1 0 0 65.0685 65.0685 133.1218 1 PROCESSED 57545.5290856482 2016-06-06 12:41:53 55330 2010-05-14 00:00:00 54893.4210300926 2009-03-03 10:06:17 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 030077 We propose to observe a gamma-ray binary LS I+61 303 simultaneously with the GeV/TeV gamma-ray (GLAST/VERITAS), radio, and optical, in order to ob tain the orbital-phase dependent multi-wavelength spectra (SED) in the early 2009. This observation will give us information of the relation between the binary geometry and the emission to understand the gamma-ray emissio n mechanism. Suzaku data also will enable us to probe the material distribution in the binary system by searching the Fe-K emission or absorption line, edge, an d so on. This observation will open a new window to study gamma-ray binaries, which are expected to be found with GLAST. GALACTIC POINT SOURCES 4 A YASUSHI FUKAZAWA JAP 3 AO3 X-RAY SPECTRAL VARIABILITY OF THE GAMMA-RAY BINARY LS I+61 303 HXD Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/403017010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '403017010'

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