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 1E 1048.1-5937 162.5452 -59.8394 162.049535 -59.57411 203.219635 -58.558248 288.24102095 -0.47209541 101.4368 54800.9597337963 2008-11-30 23:02:01 54802.5927083333 2008-12-02 14:13:30 403005010 100.4231 100 100.443 100.4231 0 100.4231 2 2 0 2 1 0 0 68.1049 68.1049 141.0819 0 PROCESSED 57544.6078472222 2016-06-05 14:35:18 55178 2009-12-13 00:00:00 54812.0471875 2008-12-12 01:07:57 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 030013 Observations in soft X-ray through hard X-ray bands are key to understand the emission processes in the magnetosphere of Anomalous X-ray Pulsars (AXPs). We propose to observe the two AXPs, 1E 2259+586 and 1E 1048.1-5937, with SUZAKU. Although no detections of the hard X-ray emissions have been reported, the results of the simulation using XSPEC for HXD indicate that SUZAKU detects the hard X-ray emissions above 20~keV from both AXPs for the first time with a quite high probability. The time resolution of HXD is able to provide the pulse profiles and the phase-resolved spectra in hard X-rays emissions. With these results of the observations, SUZAKU will provide a crucial information to study the emission processes in the magnetosphere of AXPs. GALACTIC POINT SOURCES 4 C JUMPEI TAKATA JAP 3 AO3 X-RAY OBSERVATIONS OF ANOMALOUS X-RAY PULSARS WITH SUZAKU HXD Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/403005010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '403005010'

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