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 WESTERLUND 2 156.0088 -57.7448 155.54834 -57.490842 195.724597 -59.560466 284.2643696 -0.3172737 343.7602 54687.6527199074 2008-08-09 15:39:55 54689.327962963 2008-08-11 07:52:16 503053010 73.67 100 73.67 73.67 0 73.67 2 2 0 2 1 0 0 86.5776 86.5776 144.7298 0 PROCESSED 57543.2480555556 2016-06-04 05:57:12 55252 2010-02-25 00:00:00 54706.476412037 2008-08-28 11:26:02 3.0.22.43 2 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/ver3.0/503053010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '503053010'

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