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
|
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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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