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 ALGOL 47.0831 40.8965 46.267674 40.705521 56.181748 22.363141 149.0355551 -14.93487401 244.4771 54167.6197222222 2007-03-08 14:52:24 54169.6132986111 2007-03-10 14:43:09 401093010 102.1642 105 102.1642 102.1642 0 102.1642 2 2 0 2 1 0 0 102.4729 102.4729 172.1928 1 PROCESSED 57537.6825810185 2016-05-29 16:22:55 54736 2008-09-27 00:00:00 54186.3983564815 2007-03-27 09:33:38 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 012024 Stellar and solar coronae reveal high-energy phenomena including the presence of accelerated electrons, explosive dissipation of magnetic energy, and heating to extreme temperatures. Many of these processes are likely to be physically related. We propose to use Suzaku's suite of instruments to observe the interplay between thermal and non-thermal high-energy processes in the active, eclipsing binary Algol. Our prime objective is the observation of hard X-rays above 10 keV, but also the appearance of an Fe fluorescence line that could be induced either by irradiation from flaring plasma or by electron beams. These models can be distinguished by correlating the emission with nonthermal hard X-rays as possibly detected by the HXD. GALACTIC POINT SOURCES 4 C MANUEL GUEDEL EUR 1 AO1 A SYNOPTIC VIEW OF HIGH-ENERGY PHENOMENA IN THE CORONA OF ALGOL HXD Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/401093010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '401093010'

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