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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 HD432 2.3072 59.1394 1.650501 58.861236 35.115755 51.206006 117.5327944 -3.28915956 247.7181 54469.7038310185 2008-01-04 16:53:31 54470.5154513889 2008-01-05 12:22:15 402034010 38.2406 40 38.2486 38.2406 0 38.2486 2 2 0 2 1 0 0 35.0503 35.0503 70.12 1 PROCESSED 57540.9911574074 2016-06-01 23:47:16 54908 2009-03-18 00:00:00 54483.4635532407 2008-01-18 11:07:31 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021016 Suzaku XIS spectra of three "X-ray deficient" Hertzsprung gap giants will explore why they display anomalous coronal behavior compared with cooler giants only slightly further advanced in their evolution. The apparent sharp transition in coronal properties on the way to helium flash might be caused by disruption of a "fossil" magnetosphere by a newly born solar-like dynamo. A key discriminator is the coronal energy distribution, especially enhanced and sporadic hard emission associated with flaring. The proposed targets are the brightest not previously observed in X-rays at CCD resolution; all three have supporting high resolution UV spectra. Expanding the sample of high quality, high energy information on this key class of objects is essential for probing their odd behavior. GALACTIC POINT SOURCES 4 C THOMAS AYRES USA 2 AO2 ANOMALOUS CORONAE OF HERTZSPRUNG GAP GIANTS XIS Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/402034010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '402034010'

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