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dc.contributor.authorFerreras, I.
dc.contributor.authorLisker, T.
dc.contributor.authorPasquali, A.
dc.contributor.authorKaviraj, S.
dc.date.accessioned2013-10-31T14:01:09Z
dc.date.available2013-10-31T14:01:09Z
dc.date.issued2009-05-01
dc.identifier.citationFerreras , I , Lisker , T , Pasquali , A & Kaviraj , S 2009 , ' Exploring the formation of spheroidal galaxies out to z ∼ 1.5 in GOODS ' , Monthly Notices of the Royal Astronomical Society , vol. 395 , no. 1 , pp. 554-566 . https://doi.org/10.1111/j.1365-2966.2009.14573.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 2067881
dc.identifier.otherPURE UUID: c1f51144-c40e-4c32-8cbb-a64a579f78eb
dc.identifier.otherScopus: 64549117397
dc.identifier.otherORCID: /0000-0002-5601-575X/work/77850229
dc.identifier.urihttp://hdl.handle.net/2299/11952
dc.description.abstractThe formation of massive spheroidal galaxies is studied on a visually classified sample extracted from the Advanced Camera for Surveys/Hubble Space Telescope (ACS/HST) images of the Great Observatories Origins Deep Survey north and south fields, covering a total area of 360 arcmin . The sample size (910 galaxies brighter than i = 24) allows us to explore in detail the evolution over a wide range of redshifts (0.4 <z <1.5; median redshift 0.68). Three key observables are considered: comoving number density, internal colour distribution and the Kormendy relation. The comoving number density of the most massive galaxies is found not to change significantly with redshift. Extrapolation of our sample to z = 0 gives an increase in the comoving number density of M > 10 M galaxies by a factor of 2 between z = 1 and 0, in contrast with a factor of ∼50 for lower mass galaxies (10 <M / M <10 ). One-quarter of the whole sample of early types are photometrically classified as blue galaxies. On a volume-limited sample out to z <0.7, the average stellar mass of the blue ellipticals is 5 × 10 M compared to 4 × 10 M for red ellipticals. On a volume-limited subsample out to z = 1.4 probing the brightest galaxies (M <-21), we find the median redshift of blue and red early types: 1.10 and 0.85, respectively. Blue early types only amount to 4 per cent of this sample (compared to 26 per cent in the full sample). The intrinsic colour distribution correlates overall bluer colours with blue cores (positive radial gradients of colour), suggesting an inside-out process of formation. The redshift evolution of the observed colour gradients is incompatible with a significant variation in stellar age within each galaxy. The slope of the Kormendy relation in the subsample of massive galaxies does not change over 0.4 <z <1.4 and is compatible with z = 0 values. The 'zero-point' of the Kormendy relation (i.e. the surface brightness at a fixed half-light radius) is 1 mag fainter (in the B band) for the subsample of low-mass (M <3.5 × 10 M ) early types.en
dc.format.extent13
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleExploring the formation of spheroidal galaxies out to z ∼ 1.5 in GOODSen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=64549117397&partnerID=8YFLogxK
rioxxterms.versionSMUR
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2009.14573.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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