DARTS Astro
total 1
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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 |
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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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