DARTS Astro
total 1
Show the used SQL Download WgetScript
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 |
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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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