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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 XB 1916-053 289.7027 -5.2415 289.037629 -5.333849 290.520863 16.806325 31.35614078 -8.46800846 250.2538 54047.242974537 2006-11-08 05:49:53 54048.1119791667 2006-11-09 02:41:15 401095010 38.4647 40 39.0967 39.0887 38.4647 39.0967 2 2 2 2 1 0 0 37.4857 37.4857 75.082 2 PROCESSED 57536.0684259259 2016-05-28 01:38:32 54735 2008-09-26 00:00:00 54088.866087963 2006-12-19 20:47:10 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 012038 We propose Suzaku observations of the dipping low mass X-ray binaries XB1916-053, XB1323-619, EXO0748-676 and X 1624-490. The changes in both the continuum and the He- and H- like Fe K absorption features during dips have been recently demonstrated to be consistent with a change in the properties of the photoionized absorbers present in these systems. We will use the XIS to characterise the photoionised absorbers and reliably determine the values of the ionization parameter for each source, and the simultaneous spectra of HXD to uniquely determine the underlying continuum shapes including any contributions due to reflection components and to extend the photoionized absorber fits to higher energies. This will test the validity of the ionized absorber model also >10 keV. GALACTIC POINT SOURCES 4 A MARIA DIAZ TRIGO EUR 1 AO1 BROAD-BAND OBSERVATIONS OF HIGHLY-IONIZED ABSORBERS IN DIPPING LMXBS XIS Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/401095010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '401095010'

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