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 GK PER 52.8202 43.8404 51.968435 43.670553 61.500851 24.010688 151.00566373 -10.1477205 257.5144 54875.4415277778 2009-02-13 10:35:48 54876.0899884259 2009-02-14 02:09:35 403081010 30.3888 30 30.3888 30.3888 0 30.3888 2 2 0 2 1 0 0 27.3999 27.3999 55.9979 2 PROCESSED 57545.5260648148 2016-06-06 12:37:32 55330 2010-05-14 00:00:00 54893.4257407407 2009-03-03 10:13:04 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 033107 We propose observations of 5 Intermediate Polars, a subcategory of magnetic CVs, as the first step toward establishment of an averaged hard X-ray spectrum of IPs that exist near the Solar system.The averaged spectrum should be compared with that of the Galactic Diffese X-ray Emssion (GDXE), to investigate the claimed spectral resemblance between them in energies above 10 keV. If the averaged IP spectrum shows any discrepancy with that of the GDXE, the "point-source origin" explanation for the GDXE would face a lack of appropriate hard X-ray source populations. This in turn is expected to strengthen the competing "truly diffuse origin"explanation, which attributes the GDXE hard X-rays to non thermal emission from electrons being accelerated in the interstellar space. GALACTIC POINT SOURCES 4 C TAKAYUKI YUASA THOMAS HARRISON JUS 3 AO3 SURVEY OBSERVATION OF INTERMEDIATE POLARS HXD Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/403081010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '403081010'

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