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 1822-37 276.4461 -37.1042 275.595774 -37.133404 275.279951 -13.781506 356.85149319 -11.29112534 258.4537 54010.4563888889 2006-10-02 10:57:12 54011.5189699074 2006-10-03 12:27:19 401051010 37.7434 40 37.7682 37.7682 37.7434 37.7434 2 2 2 2 1 0 0 33.1785 33.1785 91.8059 0 PROCESSED 57535.7615393518 2016-05-27 18:16:37 54695 2008-08-17 00:00:00 54024.6539814815 2006-10-16 15:41:44 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 011121 We propose a 40 ks observation of the accretion disk corona source 4U 1822-37. Despite repeated observations over the years and even excellent high-resolution data from the Chandra Observatory, the nature and origin of the corona and even the source of the Fe K fluorescence emission remains controversial. The spectral resolution of the XIS and the broad-band coverage provided by the combined XIS and HXD instruments make Suzaku uniquely suited to a definitive measurement. Determining the physical conditions in this source is particularly interesting. Because of its geometry 4U 1822-37 is a link between x-ray binaries and AGN, and an therefore serve as a laboratory for studying accretion processes throughout the universe. GALACTIC POINT SOURCES 4 B JEAN COTTAM USA 1 AO1 ACCRETION PHYSICS IN THE ADC SOURCE 4U 1822-37 XIS Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/401051010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '401051010'

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