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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 4U1700-37 255.9894 -37.8441 255.139416 -37.774677 258.577099 -14.956185 347.75582102 2.17172645 269.6945 53991.447662037 2006-09-13 10:44:38 53992.918912037 2006-09-14 22:03:14 401058010 81.4425 80 81.4569 81.4704 81.4425 81.4544 3 3 3 3 1 0 0 82.1093 82.1093 127.109 1 PROCESSED 57535.6097916667 2016-05-27 14:38:06 54526 2008-03-01 00:00:00 54053.5428240741 2006-11-14 13:01:40 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 011135 The compact object in the massive X-ray binary 4U1700-37/HD153919 has been inferred to be a neutron star based on its spectral shape, but no pulsations have been observed. One possible explanation for the absence of observed pulsations is that the pulsed signal is beamed in directions other than our line of sight. This can be tested using Suzaku by searching for pulsations in the iron K line. This line is formed efficiently under almost all conditions of ionization and temperature, and so represents an X-ray bolometer which should respond to pulsed X-rays no matter where they are pointed. We plan to make such a search, and to probe the other properties of the wind and compact object in this system by observing with Suzaku for 80 ks away from eclipse. GALACTIC POINT SOURCES 4 A TIMOTHY KALLMAN USA 1 AO1 IRON LINE VARIABILITY IN 4U1700-37 XIS N https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/401058010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '401058010'

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