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 4U 1700+24 256.6316 23.9071 256.110961 23.972677 252.098688 46.519124 45.07419011 32.98144858 280.149 54334.7787615741 2007-08-22 18:41:25 54335.875162037 2007-08-23 21:00:14 402023010 50.2445 50 50.2525 50.2605 0 50.2445 2 2 0 2 1 0 0 45.3268 45.3268 94.7158 2 PROCESSED 57539.6636226852 2016-05-31 15:55:37 54723 2008-09-14 00:00:00 54350.4606481482 2007-09-07 11:03:20 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 020105 We propose the observation of Neutron Star Low Mass X-ray Binary (LMXB) system 4U 1700+24.This system would be Advection Dominant Accretion Flow (ADAF) and we research the hard-tail in hard X-ray region. Though the X-ray intensity in a Low Hard state is very faint, $sim$10$^{33}$ erg/s we can obtain the energy spectrum of 10-100keV for the first time using Suzaku 50ksec observation because it is the nearest LMXB. If we know the extension of hard-tail in low luminosity state, we can understand the physical state of electron in the accretion disk and/or compact object. Suzaku is the best satellite to research the faint emission around 100keV. GALACTIC POINT SOURCES 4 B OSAMU NAGAE JAP 2 AO2 STUDY OF MASS ACCRETION FLOW IN ADAF FOR LOW LUMINOUS X-RAY BINARY 4U 1700+24 HXD Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/402023010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '402023010'

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