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 SS 433 287.9527 4.99 287.334904 4.905608 290.182673 27.181461 39.69879316 -2.23786427 78.6446 53833.4611458333 2006-04-08 11:04:03 53834.4579166667 2006-04-09 10:59:24 401004010 40.1976 40 40.2216 40.1976 40.2296 40.2136 2 2 2 2 1 0 0 30.4749 30.4749 86.11 2 PROCESSED 57533.4357638889 2016-05-25 10:27:30 54400 2007-10-27 00:00:00 53906.5501736111 2006-06-20 13:12:15 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010031 SS433 is the most intensively studied jet source, however the nature of the object and the jet-formation mechanism remain unknown. We propose to examine the fundamental system parameters; the jet's mass-outflow rate and the total X-ray luminosity. The ionized or blue-shifted iron absorption edge recently discovered with XMM-Newton indicates either the absorber is photo-ionized by a hidden X-ray as luminous as 1E39 erg/s, or is moving along with the jet. SS433 may be an ultra-luminous source if seen face-on, or an unobserved cool component may coexist in the X-ray jet. The spectral continuum over 10 keV to be obtained with the HXD and the absorption edge by the XIS will reveal the nature of the absorber. GALACTIC POINT SOURCES 4 A NOBUYUKI KAWAI JAP 1 AO1 SS 433 OBSERVATIONS OF THE HARD X-RAY CONTINUUM AND THE IRON ABSORPTION EDGE XIS N https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/401004010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '401004010'

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