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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 CYGNUS X-1 299.5964 35.2723 299.126812 35.135802 313.711652 54.314398 71.39800953 3.09942804 95.8123 54924.0537384259 2009-04-03 01:17:23 54924.5654282407 2009-04-03 13:34:13 404075010 15.3091 300 15.3091 15.3188 0 15.3108 2 1 0 2 1 0 0 15.5374 15.5374 44.2039 1 PROCESSED 57546.0113425926 2016-06-07 00:16:20 54922 2009-04-01 00:00:00 54949.4917824074 2009-04-28 11:48:10 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 044131 In both stellar-mass and supermassive black holes, connections between X-ray flux and radio flux hint at disk-jet connections expected theoretically. The next step in this work is to move beyond fluxes, and tie the physical parameters of the disk to radio jet emission. Cygnus X-1 is bright and highly variable in both X-rays and radio bands; moreover, it is the only black hole that always permits two measurements of the disk (through disk continuum and broad Fe K disk line/reflection). We propose to observe Cygnus X-1 on 20 occasions for 15 ksec (each) during AO-4, simultaneously with the updated Ryle radio telescope. This will form a modest Large Program with public data access, and an important legacy dataset for Suzaku. This project addresses NASA Beyond Einstein science goals. GALACTIC POINT SOURCES 4 A JON MILLER SHIN YAMADA USJ 4 AO4 A STRONG TEST OF DISK-JET CONNECTIONS IN AN ACCRETING BLACK HOLE HXD Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/404075010/ Quick Look

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SELECT * FROM suzaku_master_data WHERE observation_id = '404075010'

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