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 | WESTERLUND 2 | 155.9878 | -57.7462 | 155.527496 | -57.492284 | 195.71117 | -59.569482 | 284.25564056 | -0.32444098 | 166.5036 | 54866.5949189815 | 2009-02-04 14:16:41 | 54867.1669444444 | 2009-02-05 04:00:24 | 503053020 | 33.4924 | 30 | 33.5004 | 33.4924 | 0 | 33.5004 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 32.073 | 32.073 | 49.4159 | 1 | PROCESSED | 57545.4584606482 | 2016-06-06 11:00:11 | 55329 | 2010-05-13 00:00:00 | 54880.5574189815 | 2009-02-18 13:22:41 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 030059 | Although young open clusters with many massive stars have been recognized as gamma-ray sources, the emission mechanism of the gamma-ray is hardly known. We propose a Suzaku observation of an open cluster Westerlund 2 (RCW 49), from which gamma-ray emission has been detected with H.E.S.S. We observe this cluster to detect X-ray nonthermal emission from open clusters with TeV gamma-ray emission for the first time. We try to find out whether the emission comes from electrons or protons, and discuss the particle acceleration in open clusters. | GALACTIC DIFFUSE EMISSION | 5 | A | YUTAKA FUJITA | JAP | 3 | AO3 | NONTHERMAL EMISSION FROM AN OPEN CLUSTER WESTERLUND 2 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/503053020/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '503053020'
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