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 GX 301-2 186.689 -62.7212 185.98909 -62.444416 221.478022 -52.575765 300.10817936 0.01514837 109.0098 54836.4396296296 2009-01-05 10:33:04 54838.0419328704 2009-01-07 01:00:23 403044020 61.8136 50 61.8136 61.8136 0 61.8136 2 2 0 2 1 0 0 54.9922 54.9922 138.3981 2 PROCESSED 57545.1371064815 2016-06-06 03:17:26 55328 2010-05-12 00:00:00 54851.4303125 2009-01-20 10:19:39 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 031152 We propose the first observation of the bright neutron star GX 301-2 with Suzaku. The aim of the proposed 60 ks observation is a study of the broadband spectrum of the source in unprecedented detail and quality. This will allow us to analyze the structure (including density and clumpiness) of the intense wind of the optical companion and the gas stream flowing from Wray 977 to the neutron star. Spectral data will be used to study the evolution of nH and the iron line with very high time resolution. Furthermore, we will perform phase resolved spectroscopy to study the spectral variation of the cyclotron line with pulse phase. GALACTIC POINT SOURCES 4 A RICHARD ROTHSCHILD USA 3 AO3 BROAD-BAND STUDY OF GX 301-2 HXD Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/403044020/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '403044020'

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