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 GX 9+9 262.9404 -16.8929 262.215892 -16.856936 263.194726 6.381396 8.57505694 9.06920034 97.5329 55271.6738773148 2010-03-16 16:10:23 55273.9918981482 2010-03-18 23:48:20 404071010 85.1871 75 85.2087 85.2031 0 85.1871 2 1 0 2 1 0 0 61.6942 61.6942 200.2639 0 PROCESSED 57550.9767476852 2016-06-11 23:26:31 55652 2011-04-01 00:00:00 55285.4179513889 2010-03-30 10:01:51 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 042011 We propose two 75 ks Suzaku observations of the bright neutron star low mass X-ray binary (LMXB) GX9+9, spread over six months. We will investigate the presence of X-ray narrow absorption features in the Suzaku spectra, which are a signature of a disk wind. Such features, identified with ions such as Fe XXV and Fe XXVI, have been observed in a number of LMXBs and give us information about the mass outflow rate and the launching mechanism of the wind. We will study the connection of the disk wind to the presence of radio jet emission with simultaneous radio observations. Finally, we will determine if the broad Fe emission line indicated by the XMM-Newton spectrum is relativistically broadened. Variability will be studied as a function of accretion rate in the two proposed observations. GALACTIC POINT SOURCES 4 B MARIA DIAZ TRIGO EUR 4 AO4 A STUDY OF THE DISK WIND-JET CONNECTION IN GX9+9 WITH MULTIWAVELENGTH OBSERVATIONS HXD Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/404071010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '404071010'

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