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 EUVE J0317-85.5 48.9864 -85.5003 51.11405 -85.679196 278.533864 -69.749958 299.84736337 -30.72881529 65.46 55028.6017476852 2009-07-16 14:26:31 55030.1460185185 2009-07-18 03:30:16 404019010 63.0843 60 63.0843 63.0843 0 63.0843 2 2 0 2 1 0 0 56.8965 56.8965 133.4138 1 PROCESSED 57547.8712847222 2016-06-08 20:54:39 55406 2010-07-29 00:00:00 55040.2674305556 2009-07-28 06:25:06 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 040083 Where is the particle acceleration site in the universe? The Cosmic-ray origin is the long standing mystery for near 100 years. The first discovery of "the white dwarf pulsar" in the AE Aquarii system with Suzaku is one of the most important step in this study, because Suzaku demonstrated the possibility of particle acceleration in white dwarfs. The next important step is to search for the sign of non-thermal emission from a NORMAL white dwarf. Here, we propose the Suzaku observation of an isolated white dwarf EUVE J0317-85.5, which has very high magnetic field strength of 450 MG and very fast rotation period 725 sec among this type of objects. GALACTIC POINT SOURCES 4 B ATSUSHI HARAYAMA JAP 4 AO4 FIRST SEARCH FOR NON THERMAL EMISSION FROM AN ISOLATED MAGNETIZED WHITE DWARF HXD Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/404019010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '404019010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏