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 A2744_NE 3.7189 -30.3078 3.087931 -30.585769 350.157324 -29.032997 9.14048559 -81.37985976 233.5002 56616.3325694445 2013-11-20 07:58:54 56618.5994791667 2013-11-22 14:23:15 808008010 82.773 80 82.781 82.781 0 82.773 2 2 0 2 1 0 0 71.7365 71.7365 195.8377 2 PROCESSED 57613.443900463 2016-08-13 10:39:13 56995 2014-12-04 00:00:00 56629.7456481482 2013-12-03 17:53:44 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 080005 We propose an additional 80ks pointing to complete our mapping of A2744 out to large radii and constrain the thermodynamical history of the cluster growth. A2744 is a multiple merger, nicknamed Pandora's cluster. Our analysis of existing Suzaku data suggest that this cluster has an anisotropic temperature structure near the virial radius and there is not a simple correlation between temperature and surface mass density of member galaxies. With proposed observations, we can determine, for the first time, the temperature and entropy profiles near the radio relic in the northeast and further test a scenario of gas heating and shock propagation in the cluster outskirts. Suzaku is most suited for this study because of the lowest background and excellent sensitivity. EXTRAGALACTIC DIFFUSE SOURCES 8 B NAOMI OTA JAP 8 AO8 REVEALING THE THERMODYNAMICAL EVOLUTION IN THE PANDORA'S CLUSTER XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808008010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '808008010'

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