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 2204 248.0963 5.6404 247.481247 5.74563 245.314616 27.222606 21.10023438 33.35451369 261.3606 53995.3098958333 2006-09-17 07:26:15 53996.5098958333 2006-09-18 12:14:15 801091010 49.1113 55 49.1113 49.1113 49.1113 49.1113 2 2 2 2 1 0 0 51.9372 51.9372 103.6439 1 PROCESSED 57535.6038194444 2016-05-27 14:29:30 54526 2008-03-01 00:00:00 54020.8840277778 2006-10-12 21:13:00 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 012018 Measurements of the intracluster gas temperatures out to large radii, where most of the cluster mass resides, are of the utmost importance for the use of clusters in precision cosmology and for studies of cluster physics. Previous attempts to measure temperatures at the cluster virial radius have failed. Here we show that such measurements appear feasible now for the first time with the Suzaku X-ray CCDs. Furthermore, we show that A2204 and A2163 are optimal targets for such an investigation. We, therefore, propose to observe A2204 for 55 ks and A2163 for 100 ks to measure the gas temperature to 10% and 15% accuracy (1-sigma), respectively, out to the cluster virial radii. EXTRAGALACTIC DIFFUSE SOURCES 8 B THOMAS REIPRICH EUR 1 AO1 A2204 AND A2163: GALAXY CLUSTER GAS TEMPERATURE MEASUREMENT UP TO THE VIRIAL RADIUS SPE N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801091010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '801091010'

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