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 HYDRA A FAR SE 139.7 -12.375 139.09881 -12.163612 146.431142 -26.609663 243.28582967 25.05625041 300 56082.6736342593 2012-06-04 16:10:02 56083.9368981482 2012-06-05 22:29:08 807088010 40.939 40 40.947 40.939 0 40.947 2 2 0 2 1 0 0 37.9143 37.9143 109.1358 0 PROCESSED 57605.5894444444 2016-08-05 14:08:48 56464 2013-06-21 00:00:00 56096.2405208333 2012-06-18 05:46:21 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 072020 Galaxy cluster outskirts are the regions where structure formation occurs through the accretion of smaller structures along large-scale filaments. Thanks to its low background, Suzaku has allowed for the first time to measure the thermodynamical properties of the ICM out to the virial radius. Recently, we used archival ROSAT observations to detect cluster emission out to large radii and quantify the deviations from spherical symmetry. Based on this work, we propose to map the outskirts of Hydra A, which was found to have the highest azimuthal scatter. This will allow us to measure the temperature profiles out to the virial radius and infer the bias on the mean thermodynamical properties and the mass reconstruction when clusters are observed along preferential directions. EXTRAGALACTIC DIFFUSE SOURCES 8 B DOMINIQUE ECKERT EUR 7 AO7 MAPPING THE OUTSKIRTS OF HYDRA A WITH SUZAKU XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/807088010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '807088010'

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