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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 SWIFT J1753.5-0127 268.3714 -1.4588 267.723576 -1.449322 268.234398 21.971701 24.89300861 12.1795145 261.3846 54362.8585185185 2007-09-19 20:36:16 54365.4377777778 2007-09-22 10:30:24 402088010 94.6005 93 94.6085 94.6165 0 94.6005 2 2 0 2 1 0 0 81.739 81.739 222.836 3 PROCESSED 57540.1123842593 2016-06-01 02:41:50 54743 2008-10-04 00:00:00 54371.6366319444 2007-09-28 15:16:45 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021147 While the spectrally hard state represents the most common mode of accretion in black hole X-ray binaries, the nature of its accretion flow is poorly understood. We recently discovered cool accretion disks extending close to the innermost stable circular orbit in the hard states of two black hole transients. Such disks could give rise to strong reflection features, but instead these are weak or not detected. We propose a 70 ks Suzaku observation of Swift J1753.5-0127 (one of the two transients), which is currently in a prolonged hard state. Our goal is to put tight constraints on the strength of the reflection features and increase our understanding of the geometry of the spectrally hard component. Understanding accretion onto compact objects is fundamental to NASA's "SEU" theme. GALACTIC POINT SOURCES 4 A JEROEN HOMAN USA 2 AO2 CONSTRAINING REFLECTION FEATURES IN THE HARD STATE OF BLACK HOLE X-RAY BINARIES XIS Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/402088010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '402088010'

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