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 1RXS J070407.9+26250 106.0316 26.4199 105.25762 26.494968 104.352906 3.774212 190.26714041 14.29962915 96.1437 54749.1266319444 2008-10-10 03:02:21 54750.3682175926 2008-10-11 08:50:14 403003010 53.5519 50 53.5519 53.5519 0 53.5519 2 2 0 2 1 0 0 41.1405 41.1405 107.2319 0 PROCESSED 57544.1456944445 2016-06-05 03:29:48 55148 2009-11-13 00:00:00 54780.5445949074 2008-11-10 13:04:13 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 030009 Soft Intermediate Polar (IP) is a group of IPs whose X-ray spectra are extremely soft compared with general IPs. Recent observations reveal that some soft IPs have a soft blackbody emission component like polars, yet its nature is not fully understood. Systematic study of the soft IP blackbody emission is important in the sense that it may provide a clue to understand comprehensively the emission characteristics of polars and IPs in the soft X-ray band, and to follow possible evolutionary link from IPs to polars, etc. We propose to observe five soft IPs, each for 50ksec, in order to search for the blackbody component and to measure its temperature and flux systematically. GALACTIC POINT SOURCES 4 B MANABU ISHIDA JAP 3 AO3 OBSERVATIONS OF SOFT INTERMEDIATE POLARS XIS Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/403003010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '403003010'

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