Matches in SemOpenAlex for { <https://semopenalex.org/work/W3124085116> ?p ?o ?g. }
- W3124085116 endingPage "42" @default.
- W3124085116 startingPage "30" @default.
- W3124085116 abstract "We have analysed five-epoch Great Observatories Origins Deep Survey (GOODS) HST–ACS B, V, I775 and z data sets (v. 1.0 release), in conjunction with existing VLT–ISAAC imaging in the J, H and Ks bands, to derive estimated redshifts for the sample of 198 extremely red galaxies (ERGs) with Ks < 22 (Vega) and (I775−Ks) > 3.92 selected by Roche, Dunlop & Almaini (2003) from 50.4 arcmin2 of the GOODS/Chandra Deep Field South. We find that, at this depth, the ERG population spans the redshift range 0.5 < zphot < 4.75 and over two decades in mass (∼3 × 109 M⊙ to ∼3 × 1011 M⊙). Our results show that the dust-corrected red envelope of galaxy evolution is well modelled by a starburst at redshift zf= 5 followed thereafter by passive evolution. We explore the evolution of the ERG luminosity function (LF) from redshifts 〈zphot〉= 1.0 to 〈zphot〉= 2.5 and compare it with the global Ks-band LF at redshifts 1 < zphot < 2. We find that the bright end of the ERG LF does not decrease from redshifts 〈zphot〉= 2.0 to 〈zphot〉= 2.5 and we connect this fact with the presence of progenitors of the local L > L* population at redshifts zphot > 2. We determine lower limits of ρc= (6.1 ± 1.9) × 10−5 Mpc−3 and ρc= (2.1 ± 1.1) × 10−5 Mpc−3 on the comoving densities of progenitors of local massive galaxies already assembled at redshifts 〈zphot〉= 2.5 and 〈zphot〉= 3.5, respectively. We have investigated the existence of high-redshift Lyman-break galaxies massive enough to be included in this ERG sample. Out of an initial list of 12 potential very high redshift candidates, we have identified two ERGs which have a high probability of lying at zphot > 4. We discuss the advantages of multicolour to single-colour selection techniques in obtaining reliable lists of very high redshift candidate sources, and present revised lower redshift estimates for sources previously claimed as potential z > 5 dropouts in recent studies." @default.
- W3124085116 created "2021-02-01" @default.
- W3124085116 creator A5007647078 @default.
- W3124085116 creator A5039140400 @default.
- W3124085116 creator A5049150471 @default.
- W3124085116 creator A5057206732 @default.
- W3124085116 date "2004-09-01" @default.
- W3124085116 modified "2023-09-24" @default.
- W3124085116 title "A deeper view of extremely red galaxies: the redshift distribution in the GOODS/CDFS ISAAC field" @default.
- W3124085116 cites W1666786580 @default.
- W3124085116 cites W1850418687 @default.
- W3124085116 cites W1969514664 @default.
- W3124085116 cites W1994671833 @default.
- W3124085116 cites W2014651197 @default.
- W3124085116 cites W2019273625 @default.
- W3124085116 cites W2020547167 @default.
- W3124085116 cites W2025802512 @default.
- W3124085116 cites W2026287317 @default.
- W3124085116 cites W2027904987 @default.
- W3124085116 cites W2029438261 @default.
- W3124085116 cites W2034892354 @default.
- W3124085116 cites W2037932817 @default.
- W3124085116 cites W2043533977 @default.
- W3124085116 cites W2045895958 @default.
- W3124085116 cites W2057984445 @default.
- W3124085116 cites W2091685842 @default.
- W3124085116 cites W2094602492 @default.
- W3124085116 cites W2098914923 @default.
- W3124085116 cites W2120875714 @default.
- W3124085116 cites W2121890276 @default.
- W3124085116 cites W2142238829 @default.
- W3124085116 cites W2142517620 @default.
- W3124085116 cites W2151062050 @default.
- W3124085116 cites W2160848381 @default.
- W3124085116 cites W2164231706 @default.
- W3124085116 cites W2165856394 @default.
- W3124085116 cites W2170847761 @default.
- W3124085116 cites W2591864124 @default.
- W3124085116 cites W3098654965 @default.
- W3124085116 cites W3101531479 @default.
- W3124085116 cites W3101884712 @default.
- W3124085116 cites W3103271964 @default.
- W3124085116 cites W3103273827 @default.
- W3124085116 cites W3103551981 @default.
- W3124085116 cites W3103963708 @default.
- W3124085116 cites W3103966746 @default.
- W3124085116 cites W3104906035 @default.
- W3124085116 cites W3123261968 @default.
- W3124085116 cites W4302443186 @default.
- W3124085116 doi "https://doi.org/10.1111/j.1365-2966.2004.08044.x" @default.
- W3124085116 hasPublicationYear "2004" @default.
- W3124085116 type Work @default.
- W3124085116 sameAs 3124085116 @default.
- W3124085116 citedByCount "25" @default.
- W3124085116 countsByYear W31240851162012 @default.
- W3124085116 countsByYear W31240851162015 @default.
- W3124085116 countsByYear W31240851162016 @default.
- W3124085116 crossrefType "journal-article" @default.
- W3124085116 hasAuthorship W3124085116A5007647078 @default.
- W3124085116 hasAuthorship W3124085116A5039140400 @default.
- W3124085116 hasAuthorship W3124085116A5049150471 @default.
- W3124085116 hasAuthorship W3124085116A5057206732 @default.
- W3124085116 hasBestOaLocation W31240851161 @default.
- W3124085116 hasConcept C121332964 @default.
- W3124085116 hasConcept C12287442 @default.
- W3124085116 hasConcept C125857072 @default.
- W3124085116 hasConcept C1276947 @default.
- W3124085116 hasConcept C144024400 @default.
- W3124085116 hasConcept C149923435 @default.
- W3124085116 hasConcept C168589115 @default.
- W3124085116 hasConcept C174802034 @default.
- W3124085116 hasConcept C17959413 @default.
- W3124085116 hasConcept C2908647359 @default.
- W3124085116 hasConcept C33024259 @default.
- W3124085116 hasConcept C44870925 @default.
- W3124085116 hasConcept C98444146 @default.
- W3124085116 hasConceptScore W3124085116C121332964 @default.
- W3124085116 hasConceptScore W3124085116C12287442 @default.
- W3124085116 hasConceptScore W3124085116C125857072 @default.
- W3124085116 hasConceptScore W3124085116C1276947 @default.
- W3124085116 hasConceptScore W3124085116C144024400 @default.
- W3124085116 hasConceptScore W3124085116C149923435 @default.
- W3124085116 hasConceptScore W3124085116C168589115 @default.
- W3124085116 hasConceptScore W3124085116C174802034 @default.
- W3124085116 hasConceptScore W3124085116C17959413 @default.
- W3124085116 hasConceptScore W3124085116C2908647359 @default.
- W3124085116 hasConceptScore W3124085116C33024259 @default.
- W3124085116 hasConceptScore W3124085116C44870925 @default.
- W3124085116 hasConceptScore W3124085116C98444146 @default.
- W3124085116 hasIssue "1" @default.
- W3124085116 hasLocation W31240851161 @default.
- W3124085116 hasLocation W31240851162 @default.
- W3124085116 hasLocation W31240851163 @default.
- W3124085116 hasOpenAccess W3124085116 @default.
- W3124085116 hasPrimaryLocation W31240851161 @default.
- W3124085116 hasRelatedWork W1647088338 @default.
- W3124085116 hasRelatedWork W2047108234 @default.
- W3124085116 hasRelatedWork W2060449082 @default.