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 106.0341 26.4126 105.260164 26.487679 104.355942 3.767203 190.27497025 14.29877104 282.0717 54548.4868865741 2008-03-23 11:41:07 54549.9862384259 2008-03-24 23:40:11 402008010 58.3157 50 58.3237 58.3157 0 58.3237 1 1 0 1 1 0 0 49.4766 49.4766 129.5278 0 PROCESSED 57541.9808912037 2016-06-02 23:32:29 54933 2009-04-12 00:00:00 54566.326712963 2008-04-10 07:50:28 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 020029 Soft Intermediate Polar (IP) is a small group of IPs whose X-ray spectrum is extremely soft compared with general IPs. Recent observations reveal that some soft IPs harbor a soft blackbody 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 possible evolutionary link from IPs to polars, the origin of the soft excess in polars, etc. We propose to observe five soft IPs, each for 50ksec, in order to search for the blackbody component and to measure their temperature and flux systematically. GALACTIC POINT SOURCES 4 C MANABU ISHIDA JAP 2 AO2 OBSERVATIONS OF SOFT INTERMEDIATE POLARS XIS Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/402008010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '402008010'

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