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-3 308.2593 40.981 307.808438 40.809488 328.80084 56.880196 79.93230299 0.62160244 252.424 54052.0902893518 2006-11-13 02:10:01 54054.3676388889 2006-11-15 08:49:24 401011010 99.7445 100 99.7462 99.7462 0 99.7445 2 2 0 2 1 0 0 95.3893 95.3893 196.745 1 PROCESSED 57536.1520717593 2016-05-28 03:38:59 54456 2007-12-22 00:00:00 54088.9545023148 2006-12-19 22:54:29 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010058 We propose an observation of the unusual X-ray binary Cygnus X-3. Cyg X-3 is a final stage of the massive binary stars consisting of a WR(N) star and a compact star. However the nature of the compact star is not well understood. We have fore scientific objective. (A)Determine the Doppler modulation of iron K lines and discuss the binary nature. (2) Determine the iron abundance in the WR wind. (3) Search for the high energy cut off about 100keV of the power law component. (4) Search for the X-ray emission from radio knots. For these four sciences, we propose 100ksec observation of Cyg X-3. GALACTIC POINT SOURCES 4 C SHUNJI KITAMOTO JAP 1 AO1 WIDE BAND OBSERVATION OF CYGNUS X-3 WITH SUZAKU SPE Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/401011010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '401011010'

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