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 1608-52 243.2309 -52.3757 242.269732 -52.248184 251.350346 -30.651804 330.98178647 -0.83761569 125.7606 55273.9986689815 2010-03-18 23:58:05 55274.9154166667 2010-03-19 21:58:12 404044030 31.7568 30 31.7568 31.7568 0 31.7568 2 2 0 2 1 0 0 15.3094 15.3094 79.1938 0 PROCESSED 57550.9191898148 2016-06-11 22:03:38 55652 2011-04-01 00:00:00 55286.259849537 2010-03-31 06:14:11 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 041223 The true nature of X-ray emission from neutron star X-ray binaries (NSXRBs) has not been clear for sometime and there are many possibilities for the spectral model. Recent progress has been made, but relies on RXTE data which lacks the low energy sensitivity where disk emission is most prominent. Using Suzaku we propose four 30 ksec observations of the transient 4U 1608-52 throughout an outburst. We will test how spectral parameters change with luminosity, allowing us to untangle the correct model. An essential part of this proposal is the unique ability of Suzaku to detect asymmetric broad iron emission lines in NSXRBs. We will study how the iron line varies throughout the outburst, which combined with the spectral fits will test the interaction between the accretion disk and corona. GALACTIC POINT SOURCES 4 A EDWARD CACKETT USA 4 AO4-TOO ACCRETION DISK EVOLUTION THROUGHOUT A NEUTRON STAR LMXB OUTBURST HXD Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/404044030/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '404044030'

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