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 SHAPLEY OFF-FILAMENT 201.0894 -30.5701 200.390777 -30.309695 211.196223 -20.080758 311.26734846 31.76827748 298.8248 54666.4273958333 2008-07-19 10:15:27 54670.1905439815 2008-07-23 04:34:23 803068010 143.4669 140 143.4749 143.4749 0 143.4669 2 2 0 2 1 0 0 110.8111 110.8111 325.0858 2 PROCESSED 57543.1803240741 2016-06-04 04:19:40 55073 2009-08-30 00:00:00 54707.3575694444 2008-08-29 08:34:54 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 031451 It is, in principle, possible to search for the signature of the Warm-Hot Intergalactic Medium (WHIM) in regions between clusters, where WHIM filaments are expected. However, the complexity of the filament network and the distance between clusters makes this approach very difficult (if not impossible), except in few cases where several clusters are sufficiently close together, such as within a supercluster. We propose an investigation using Suzaku of a region within the Shapley Supercluster where, following the cluster network, a filament is expected and a ROSAT PSPC investigation has found excess emission. Suzaku s characteristics will allow a clear detection and characterization of the filament. A second observation in an empty region nearby will be used as control field. EXTRAGALACTIC DIFFUSE SOURCES 8 B MASSIMILIANO GALEAZZI USA 3 AO3 FILAMENTARY X-RAY STRUCTURE IN THE SHAPLEY SUPERCLUSTER XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/803068010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '803068010'

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