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 V1223 SGR 283.7445 -31.105 282.940068 -31.169256 281.851865 -8.228404 5.0082738 -14.31987205 79.9528 54203.4803240741 2007-04-13 11:31:40 54204.9418055556 2007-04-14 22:36:12 402002010 60.706 60 60.706 60.706 0 60.706 2 2 0 2 1 0 0 46.2861 46.2861 126.2719 2 PROCESSED 57538.1822800926 2016-05-30 04:22:29 54744 2008-10-05 00:00:00 54210.6596875 2007-04-20 15:49:57 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 020008 The standard theory of the post-shock plasma in intermediate polars predicts that the shock height is negligibly small compared with the radius of the white dwarf under normal accretion state. Some recent observational results, however, seem to contradict this prediction, and suggest that the shock height may be of the same order as the white dwarf radius. The shock height is an important quantity for the post-shock plasma in that it is deeply related to the mass accretion rate, heating and cooling mechanism of the post-shock plasma and so on. We therefore propose to observe two of the brightest intermediate polars EX Hya and V1223 Sgr to measure their shock height directly in terms of the reflection spectrum from the HXD-PIN and the iron K-shell structure from the XIS. GALACTIC POINT SOURCES 4 A MANABU ISHIDA JAP 2 AO2 MEASUREMENT OF THE SHOCK HEIGHT IN INTERMEDIATE POLARS HXD Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/402002010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '402002010'

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