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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 MARS-P10 103.2518 25.125 102.483772 25.186994 101.989505 2.233931 190.42954859 11.48582895 298.135 54560.0767708333 2008-04-04 01:50:33 54560.16 2008-04-04 03:50:24 403006100 3.7716 100 3.7956 3.7716 0 3.796 1 1 0 1 1 0 0 4.0014 4.0014 7.1839 0 PROCESSED 57542.0546527778 2016-06-03 01:18:42 54953 2009-05-02 00:00:00 54577.1537847222 2008-04-21 03:41:27 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 030015 We propose Suzaku XIS observation of Mars. With XMM-Newton RGS, X-rays from Mars are suggested to have two components: one due to fluorescent scattering of solar X-rays in its atmosphere and the other due to the solar wind charge exchange in its exosphere. X-rays thus can be a new probe to study the puzzling Martian exosphere that holds key information about how the Martian air has been lost. With XIS, we can detect the emission lines with the highest photon statistics ever. For the first time, we will observe the solar wind near the Mars simultaneously with Mars Express and extract information about the exosphere. This will be the first X-ray observation of Mars at solar minimum when the exosphere is expected to be dense and X-rays from the exosphere will largely increase. GALACTIC POINT SOURCES 4 A YUICHIRO EZOE JAP 3 AO3 SUZAKU OBSERVATION OF X-RAY EMISSION LINES FROM THE MARTIAN EXOSPHERE INDUCED BY THE SOLAR WIND CHARGE EXCHANGE XIS Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/403006100/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '403006100'

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