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 340+0 251.4463 -45.6133 250.537018 -45.522593 255.990327 -23.069192 339.58535361 -0.07953483 81.21 54892.2765740741 2009-03-02 06:38:16 54894.8168287037 2009-03-04 19:36:14 403060010 107.3127 100 107.3145 107.3127 0 107.3145 2 2 0 2 1 0 0 86.104 86.104 219.4467 1 PROCESSED 57545.7913541667 2016-06-06 18:59:33 55329 2010-05-13 00:00:00 54908.7293055556 2009-03-18 17:30:12 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 031164 In this proposal we request to observe accreting neutron stars sources GX 340+0, GX 3+1 and GX 13+1. The observational goal of the observations is to collect high-spectral resolution data in the region of K$_alpha$ iron line. Our scientific motivation is to put the origin of the line emission under additional theoretical scrutiny. We wish to compare the performance of the wind-reprocessing model to relativistic model in as many sources as possible. This proposal is a part of our broader effort to investigate the origin of iron emission line in Galactic X-ray binaries, which includes a parallel proposal to observe WD binaries. GALACTIC POINT SOURCES 4 B NIKOLAI SHAPOSHNIKOV USA 3 AO3 IRON KALPHA EMISSION LINE DIAGNOSTICS IN ACCRETING NEUTRON STARS XIS Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/403060010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '403060010'

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