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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 SIGMA^2 CRB 243.6552 33.7881 243.181435 33.91264 231.394365 53.752123 54.56402364 46.14689859 281.1207 53969.4764467593 2006-08-22 11:26:05 53972.1925231482 2006-08-25 04:37:14 401034010 109.1604 110 109.1904 109.1604 109.1684 109.1764 2 2 2 2 1 0 0 98.8376 98.8376 234.6539 3 PROCESSED 57535.3877777778 2016-05-27 09:18:24 54526 2008-03-01 00:00:00 54021.2578587963 2006-10-13 06:11:19 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 011025 Suzaku is a powerful instrument for studying the hot (>100 MK) coronal quiescent and flare emission from RS CVn binaries. We propose to obtain 110 ksec (3 day elapsed time) observations of the RS CVn systems Sigma^2 CrB (F6V + G0V) and Sigma Gem (K0III +?). Our goals are i) to better characterize their hard (> 10 keV) emission, ii) to understand the origin of coronal thermal and nonthermal plasma by studying the evolution of the coronal thermal structure, and iii) to investigate the persistent and flaring nonthermal electron population using a combination of X-ray and radio cm+mm continuum data. Such studies require the long duty cycle of Suzaku observations and its high sensitivity, particularly the greatly enhanced capability in the 10-25 keV region provided by HXD. GALACTIC POINT SOURCES 4 B ALEXANDER BROWN USA 1 AO1 SUZAKU OBSERVATIONS OF THERMAL AND NONTHERMAL CORONAL EMISSION ON THE RS CVN BINARIES SIGMA^2 CRB AND SIGMA GEM HXD N https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/401034010/ Quick Look

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SELECT * FROM suzaku_master_data WHERE observation_id = '401034010'

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