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 CYGNUS X-1 299.6653 35.165 299.194917 35.028212 313.740573 54.19441 71.33570459 2.99545336 212.8004 55182.0619328704 2009-12-17 01:29:11 55182.5508564815 2009-12-17 13:13:14 404075070 22.1019 300 22.1019 22.1099 0 23.664 1 1 0 1 1 0 0 3.4607 3.4607 42.236 0 PROCESSED 57549.8755671296 2016-06-10 21:00:49 54922 2009-04-01 00:00:00 55200.4490046296 2010-01-04 10:46:34 3.0.22.43 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 N https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/404075070/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '404075070'

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