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 A383_FIELD_2 41.9447 -3.4083 41.315431 -3.616408 38.400744 -18.662791 177.53047769 -53.46482162 60.9996 55389.1380208333 2010-07-12 03:18:45 55390.062662037 2010-07-13 01:30:14 805063010 43.3415 40 43.3575 43.3415 0 43.3575 2 2 0 2 1 0 0 39.2589 39.2589 79.8749 0 PROCESSED 57552.6168055556 2016-06-13 14:48:12 55287 2010-04-01 00:00:00 55411.2445601852 2010-08-03 05:52:10 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 051115 We propose observations of 5 clusters of galaxies to probe the cluster environment out to r200 in order to (1) determine the temperature and density profiles for a representative sample of clusters, including those apparently discrepant with numerical simulations; (2) search for azimuthal variations at these scales which may be indicative of the ongoing cluster accretion process; (3) construct the largest sample to date of clusters with accurate X-ray mass determination out to r200; and (4) provide a fiducial data set for detailed comparison with high resolution numerical simulations. These targets capitalize on our large sample of clusters surveyed with XMM and will provide a large enough data set to truly sample the properties of clusters at large radii. EXTRAGALACTIC DIFFUSE SOURCES 8 A ERIC MILLER USA 5 AO5 THE OUTER LIMITS OF RICH CLUSTERS: SUZAKU OBSERVATIONS TO R200 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805063010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '805063010'

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