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 | K3/PSR J1420-6048 | 215.0274 | -60.7627 | 214.105774 | -60.533369 | 236.492647 | -43.553641 | 313.55205119 | 0.26755801 | 90.771 | 54842.5598263889 | 2009-01-11 13:26:09 | 54843.8801388889 | 2009-01-12 21:07:24 | 503110010 | 50.269 | 50 | 50.269 | 50.269 | 0 | 50.269 | 1 | 1 | 0 | 1 | 1 | 0 | 0 | 50.0618 | 50.0618 | 114.0639 | 2 | PROCESSED | 57545.1792013889 | 2016-06-06 04:18:03 | 55328 | 2010-05-12 00:00:00 | 54854.3728703704 | 2009-01-23 08:56:56 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 033076 | 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 | ROGER ROMANI | JUS | 3 | AO3 | SUZAKU OBSERVATION OF TEV GAMMA-RAY PWN K3/PSR J1420-6048 | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/503110010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '503110010'
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