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 ABELL 115 13.9939 26.3802 13.320825 26.109701 23.360956 18.75409 124.19588168 -36.48041221 44.0022 55401.606087963 2010-07-24 14:32:46 55403.0529398148 2010-07-26 01:16:14 805077010 66.1556 65 66.1629 66.1556 0 66.1829 2 2 0 2 1 0 0 61.8298 61.8298 124.968 2 PROCESSED 57552.6853472222 2016-06-13 16:26:54 55780 2011-08-07 00:00:00 55414.1298148148 2010-08-06 03:06:56 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 051521 We propose central and offset pointed observations of the strongly merging ``double'' cluster A115 to study the properties of the intracluster gas at the virial radius. Ultimately, the results can be compared with results from both relaxed and other merging systems to determine the effects of mergers on the extended gas halos of clusters (e.g., departures from hydrostatic equilibrium, and the level of non-thermal pressure support). Additionally, we will verify the presence of hard X-ray emission between the subclusters, marginally detected in Chandra observations, accurately measure its temperature, and determine its origin by confirming it as hot thermal (shock heated gas) or non-thermal (shock or turbulent accelerated particles) emission. EXTRAGALACTIC DIFFUSE SOURCES 8 B SCOTT RANDALL USA 5 AO5 THE EXTENDED ATMOSPHERES OF STRONGLY MERGING GALAXY CLUSTERS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805077010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '805077010'

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