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
1 JUPITER 28.7092 10.4688 28.044402 10.223855 30.381154 -1.215152 147.29554938 -49.38035583 249.1847 55930.8245717593 2012-01-04 19:47:23 55931.8508564815 2012-01-05 20:25:14 506006020 35.518 160 35.522 35.518 0 35.526 2 2 0 2 1 0 0 34.367 34.367 88.6599 0 PROCESSED 57604.3110185185 2016-08-04 07:27:52 56316 2013-01-24 00:00:00 55946.2294097222 2012-01-20 05:30:21 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/ver3.0/506006020/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '506006020'

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