DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
No. |
object_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
|
awarded_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
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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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://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/404019010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '404019010'
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