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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 1RXSJ165256.3-264503 253.236 -26.7533 252.46137 -26.671186 255.025143 -4.179065 355.1420085 10.81079439 277.5876 54337.0024421296 2007-08-25 00:03:31 54338.0419444444 2007-08-26 01:00:24 402004010 49.5822 40 49.5822 49.5822 0 49.5822 2 2 0 2 1 0 0 46.6581 46.6581 89.7779 2 PROCESSED 57539.6777083333 2016-05-31 16:15:54 54723 2008-09-14 00:00:00 54350.4155092593 2007-09-07 09:58:20 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 020015 We propose to study wide-band X-ray properties of 5 unidentified sources with luminosities of ~10^35 erg/s, which were detected in the ROSAT All Sky Survey. These sources are a part of the complete X-ray sample in the luminosity range > 10^34 erg/s in the Galactic bulge constructed by Mori (2005). Our goal is to obtain, for the first time, a clear picture about X-ray populations in the bulge, by utilizing the Suzaku fine spectra together with optical identifications. This is a new step toward understanding the formation history of the bulge. Furthermore, because the luminosity range we observe corresponds to a "missing link" region ever studied for a neutron star or black-hole X-ray binary, our results are also unique to test acrretion disk theories at intermediate mass accretion rates. GALACTIC POINT SOURCES 4 C HIDEYUKI MORI JAP 2 AO2 SPECTRAL STUDIES OF UNIDENTIFIED X-RAY SOURCES IN THE GALACTIC BULGE XIS Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/402004010/ Quick Look

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SELECT * FROM suzaku_master_data WHERE observation_id = '402004010'

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