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 A2319CENTER 290.3341 43.878 289.944223 43.782148 306.012819 64.798086 75.63759851 13.45022652 251.6652 54035.9326041667 2006-10-27 22:22:57 54038.1466898148 2006-10-30 03:31:14 801040010 99.5332 100 99.5492 99.5412 99.5332 99.5492 2 2 2 2 1 0 0 93.9548 93.9548 191.268 2 PROCESSED 57535.9905555556 2016-05-27 23:46:24 54735 2008-09-26 00:00:00 54063.5741666667 2006-11-24 13:46:48 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010085 We propose the observations of the A2319 cluster with the Suzaku HXD and XIS to investigate particle acceleration processes in the intracluster medium(ICM). A2319 is a nearby massive merging cluster whose collision axis is nearly along the line of sight, and has diffuse non-thermal radio emission. We will detect non-thermal hard X-ray with HXD, and determine the velocity difference between the two subclusters with XIS. With these results, we will determine dynamical status of the ICM and get implications on the particle acceleration processes. We will compare the results with theoretical models, numerical simulations, and radio and optical observations to get an overall picture of particle acceleration in clusters. EXTRAGALACTIC DIFFUSE SOURCES 8 B MOTOKAZU TAKIZAWA JAP 1 AO1 PARTICLE ACCELERATION IN THE A2319 CLUSTER HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801040010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '801040010'

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