This HTML5 document contains 30 embedded RDF statements represented using HTML+Microdata notation.

The embedded RDF content will be recognized by any processor of HTML5 Microdata.

Namespace Prefixes

PrefixIRI
dctermshttp://purl.org/dc/terms/
dbohttp://dbpedia.org/ontology/
foafhttp://xmlns.com/foaf/0.1/
n11https://global.dbpedia.org/id/
dbthttp://dbpedia.org/resource/Template:
rdfshttp://www.w3.org/2000/01/rdf-schema#
rdfhttp://www.w3.org/1999/02/22-rdf-syntax-ns#
owlhttp://www.w3.org/2002/07/owl#
wikipedia-enhttp://en.wikipedia.org/wiki/
dbchttp://dbpedia.org/resource/Category:
provhttp://www.w3.org/ns/prov#
dbphttp://dbpedia.org/property/
xsdhhttp://www.w3.org/2001/XMLSchema#
wikidatahttp://www.wikidata.org/entity/
dbrhttp://dbpedia.org/resource/

Statements

Subject Item
dbr:Widefield_ASKAP_L-Band_Legacy_All-Sky_Blind_Survey
rdfs:label
Widefield ASKAP L-Band Legacy All-Sky Blind Survey
rdfs:comment
The Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY) is a next-generation survey of the 21 cm radio emission from neutral hydrogen (HI) in the Local Universe. It is hosted by the Australian Square Kilometer Array Pathfinder (ASKAP) telescope, WALLABY will survey three-quarters of the sky over a Declination range −90° to +30° to a redshift of 0.26. It will have a angular resolution of 30 arcsec and a sensitivity of 1.6 mJy/beam in each 4 km/s channel. WALLABY is expected to detect about 500,000 galaxies with a mean redshift of 0.05, at a mean distance of about 200 Mpc. The scientific goals of WALLABY include:
dcterms:subject
dbc:Science_and_technology_in_Australia dbc:Science_experiments dbc:Hydrogen
dbo:wikiPageID
65561121
dbo:wikiPageRevisionID
1085502431
dbo:wikiPageWikiLink
dbc:Hydrogen dbr:Arcsec_(angle_unit) dbr:Norma_(constellation) dbc:Science_and_technology_in_Australia dbr:Galaxy dbr:Angular_resolution dbr:Australian_Square_Kilometre_Array_Pathfinder dbr:Bärbel_Koribalski dbr:Hydra_(constellation) dbr:Declination dbr:Redshift dbr:Megaparsec dbc:Science_experiments dbr:NGC 4636 dbr:Hydrogen_line dbr:Universe
owl:sameAs
wikidata:Q104862852 n11:FeyTC
dbp:wikiPageUsesTemplate
dbt:Citation_needed
dbo:abstract
The Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY) is a next-generation survey of the 21 cm radio emission from neutral hydrogen (HI) in the Local Universe. It is hosted by the Australian Square Kilometer Array Pathfinder (ASKAP) telescope, WALLABY will survey three-quarters of the sky over a Declination range −90° to +30° to a redshift of 0.26. It will have a angular resolution of 30 arcsec and a sensitivity of 1.6 mJy/beam in each 4 km/s channel. WALLABY is expected to detect about 500,000 galaxies with a mean redshift of 0.05, at a mean distance of about 200 Mpc. The scientific goals of WALLABY include: * a census of gas-rich galaxies in the vicinity of the Local Group; * a study of the HI properties of galaxies, groups and clusters, including the influence of the environment on galaxy evolution;
prov:wasDerivedFrom
wikipedia-en:Widefield_ASKAP_L-Band_Legacy_All-Sky_Blind_Survey?oldid=1085502431&ns=0
dbo:wikiPageLength
6812
foaf:isPrimaryTopicOf
wikipedia-en:Widefield_ASKAP_L-Band_Legacy_All-Sky_Blind_Survey