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 JUPITER 226.6349 -16.1983 225.936085 -16.00589 228.727521 1.247844 344.01962259 35.67652355 118.4908 53793.86 2006-02-27 20:38:24 53794.9585532407 2006-02-28 23:00:19 401001040 42.2558 36 42.2638 42.2638 42.2638 42.2558 2 2 2 2 1 0 0 35.7067 35.7067 94.9059 2 PROCESSED 57533.1103819444 2016-05-25 02:38:57 54401 2007-10-28 00:00:00 53906.5712615741 2006-06-20 13:42:37 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 011003 We propose XIS observations of Jupiter with an exposure time of 144 ks (4 planetary rotations). Our goals are: 1) to obtain and study the highest resolution x-ray CCD spectra of Jupiter's planetary x-ray emission, including separation into auroral and low-latitude components; and 2) to fully characterize the high energy (>1 keV) auroral component recently discovered in 2003 XMM-Newton data. These spectral studies will provide greater understanding of the physical properties of, and physical processes occurring in, the planet's magnetosphere. This research supports the National and NASA objectives of exploring the Solar System, in particular the Jupiter system, and the universe, and of understanding their structure, in particular Jupiter's magnetospheric and atmospheric structure. GALACTIC POINT SOURCES 4 C RONALD ELSNER USA 1 AO1 JUPITER OBSERVATIONS WITH THE XIS: THE X-RAY SPECTRUM XIS N https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/401001040/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '401001040'

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