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 RABBIT 214.6544 -60.9713 213.733054 -60.740946 236.398817 -43.82174 313.31134091 0.131367 105.7763 54876.850787037 2009-02-14 20:25:08 54877.5224421296 2009-02-15 12:32:19 503071010 21.274 20 21.282 21.274 0 21.29 1 1 0 1 1 0 0 18.0126 18.0126 57.984 0 PROCESSED 57545.5405439815 2016-06-06 12:58:23 55330 2010-05-14 00:00:00 54892.945162037 2009-03-02 22:41:02 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 030076 K3/PSR J1420-6048 is one of the TeV gamma-ray pulsar wind nebulae detected by HESS, which are thought to be main particle accelerators to the Galactic Cosmic rays. It was also detected by EGRET and its X-ray spectrum is very hard. In order to reveal the radiation mechanism, we propose to observe the extended source for 50 ksec on HXD nominal position and contamination source for 20 ksec on XIS nominal position. The main purpose of this observation is to obtain the hard X-ray spectrum up to about 40 keV. GALACTIC DIFFUSE EMISSION 5 C TETSUICHI KISHISHITA JAP 3 AO3 SUZAKU OBSERVATION OF TEV GAMMA-RAY PWN K3/PSR J1420-6048 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/503071010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '503071010'

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