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 | JUPITER | 28.9811 | 10.6021 | 28.315769 | 10.357786 | 30.678261 | -1.183373 | 147.5984875 | -49.15640747 | 249.1843 | 55937.2038773148 | 2012-01-11 04:53:35 | 55938.208599537 | 2012-01-12 05:00:23 | 506006030 | 34.8942 | 160 | 34.9022 | 34.9102 | 0 | 34.8942 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 32.2081 | 32.2081 | 86.7918 | 2 | PROCESSED | 57604.3101273148 | 2016-08-04 07:26:35 | 56319 | 2013-01-27 00:00:00 | 55952.170787037 | 2012-01-26 04:05:56 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 060017 | Suzaku observation of Jupiter in early 2006 detected diffuse hard X-ray emission, with spatial size 6 times the Jovian diameter and elongation along the inner radiation belt. This indicates that electrons are accelerated up to several tens of MeV and confined in a very large region. We propose to observe Jupiter again in a different epoch. Comparison with the previous spectra and image will reveal how Jovian magnetosphere interacts with the solar wind and will give us clues about how electrons are accelerated in such a large region around Jupiter. | GALACTIC DIFFUSE EMISSION | 5 | B | KUMI ISHIKAWA | JAP | 6 | AO6 | STUDY OF DIFFUSE X-RAY EMISSION FROM JOVIAN MAGNETOSPHERE | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/506006030/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '506006030'
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