This HTML5 document contains 34 embedded RDF statements represented using HTML+Microdata notation.

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

PrefixNamespace IRI
vivohttp://vivoweb.org/ontology/core#
marcrelhttp://id.loc.gov/vocabulary/relators/
dctermshttp://purl.org/dc/terms/
n15http://hub.abes.fr/edp/periodical/articletype/
n13http://hub.abes.fr/edp/periodical/aa/2015/volume_582/issue_2015/aa25497-14/m/
n17http://orcid.org/0000-0002-3073-5871#
n14http://hub.abes.fr/edp/periodical/aa/
n16http://hub.abes.fr/edp/periodical/aa/2015/volume_582/issue_2015/
bibohttp://purl.org/ontology/bibo/
rdachttp://rdaregistry.info/Elements/c/
hubhttp://hub.abes.fr/namespace/
rdfhttp://www.w3.org/1999/02/22-rdf-syntax-ns#
n4http://hub.abes.fr/referentiel/edparticlecategories/subject/
n5http://hub.abes.fr/edp/periodical/aa/2015/volume_582/issue_2015/aa25497-14/subject/
n7http://hub.abes.fr/edp/periodical/aa/2015/volume_582/issue_2015/aa25497-14/authorship/
rdawhttp://rdaregistry.info/Elements/w/
n2http://hub.abes.fr/edp/periodical/aa/2015/volume_582/issue_2015/aa25497-14/
xsdhhttp://www.w3.org/2001/XMLSchema#
Subject Item
n2:w
rdf:type
bibo:Article rdac:C10001
dcterms:isPartOf
n16:w
dcterms:subject
n4:extragalacticastronomy n5:galaxiesevolution n5:galaxieshighredshift n5:infraredgalaxies
dcterms:title
The spectral energy distribution of galaxies at z > 2.5: Implications from the Herschel/SPIRE color-color diagram
dcterms:date
2015-01-01
rdaw:P10072
n13:print n13:web
vivo:relatedBy
n7:1 n7:3 n7:6 n7:8 n7:5 n7:7 n7:2 n7:4
marcrel:aut
n2:buatveronique n2:heinissebastien n2:shaozhengyi n2:fangtingyuan n2:houjinliang n2:burgarelladenis n2:cieslalaure n17:person
dcterms:abstract
We use the Herschel SPIRE color-color diagram to study the spectral energy distribution (SED) and the redshift estimation of high- z galaxies. We compiled a sample of 57 galaxies with spectroscopically confirmed redshifts and SPIRE detections in all three bands at z = 2.5 -6.4, and compared their average SPIRE colors with SED templates from local and high- z libraries. We find that local SEDs are inconsistent with high- z observations. The local calibrations of the parameters need to be adjusted to describe the average colors of high- z galaxies. For high- z libraries, the templates with an evolution from z = 0 to 3 can well describe the average colors of the observations at high redshift. Using these templates, we defined color cuts to divide the SPIRE color-color diagram into different regions with different mean redshifts. We tested this method and two other color cut methods using a large sample of 783 Herschel-selected galaxies, and find that although these methods can separate the sample into populations with different mean redshifts, the dispersion of redshifts in each population is considerably large. Additional information is needed for better sampling.
hub:articleType
n15:researcharticle
hub:publisher-id
aa25497-14
dcterms:dateCopyrighted
2015-01-01
dcterms:rights
© ESO, 2015
dcterms:rightsHolder
ESO
hub:isPartOfThisJournal
n14:w