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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 SERPENS X-1 279.9934 5.0285 279.376671 4.981655 281.288405 28.078275 36.11311789 4.83561165 256.1423 54032.2853819444 2006-10-24 06:50:57 54033.2259143518 2006-10-25 05:25:19 401048010 37.1578 37 37.1578 37.2698 37.2058 37.1658 2 1 2 2 1 0 0 31.0695 31.0695 81.2399 2 PROCESSED 57535.9734722222 2016-05-27 23:21:48 54526 2008-03-01 00:00:00 54056.4719328704 2006-11-17 11:19:35 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 011113 The potential well around low-magnetic field neutron stars is very similar to that around Schwarzschild black holes. Doppler shifts expected at the inner disk around such neutron stars should be very similar, and should produce relativistic FeK-alpha emission lines like those observed in some black hole systems. To date, however, relativistically broadened FeK-alpha emission lines have not been clearly detected in neutron star systems, in part because their lines are generally weaker than those found in black hole systems. We propose to observe the neutron star binaries 4U 1820-30, Cygnus X-2, and Serpens X-1 for 37 ksec each in Suzaku Cycle 1, to confirm possible evidence of relativistic broadening. Relativistic phenomena and accretion studies are central to NASA's ``SEU'' theme. GALACTIC POINT SOURCES 4 B JON MILLER USA 1 AO1 A SUZAKU STUDY OF BROAD IRON LINES IN NEUTRON STAR BINARIES XIS N https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/401048010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '401048010'

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