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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 X1630-472 248.5239 -47.3401 247.603368 -47.236061 254.092996 -25.076506 336.95804041 0.27755382 107.6616 53809.226412037 2006-03-15 05:26:02 53809.743912037 2006-03-15 17:51:14 400010050 23.1671 200 23.1751 23.1769 23.1768 23.1671 2 1 2 2 1 0 0 18.8605 18.8605 44.706 0 PROCESSED 57533.2189930556 2016-05-25 05:15:21 54247 2007-05-27 00:00:00 54041.9302662037 2006-11-02 22:19:35 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001058 We propose to monitor a transient black hole binary in outburst through a series of 20 ks observations. Our goal is to map the physical conditions in the accretion disk as the source evolves through the various continuum states using the spectral diagnostics available in the Fe K fluorescence emission. Measurements of the Fe K emission will allow us to quantify the thermal, kinematic, and geometric conditions in both the disk and the surrounding material. Correlating the Fe K diagnostics with sensitive measurements of the direct and reprocessed continuum emission will allow us to map the evolving conditions and constrain models of the dynamic accretion processes in black hole binaries. We will monitor 7 targets with the RXTE. This observation will be triggered when one becomes active. GALACTIC POINT SOURCES 4 A JEAN COTTAM JAP 0 SWG-TOO FE K SPECTROSCOPY OF TRANSIENT BLACK HOLE BINARIES HXD N https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/400010050/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '400010050'

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