2005
DOI: 10.1111/j.1365-2966.2005.09191.x
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The Las Campanas Infrared Survey -- V. Keck spectroscopy of a large sample of extremely red objects

Abstract: We present deep Keck spectroscopy, using the Deep Imaging Multi‐Object Spectrograph and the Low‐Resolution Imaging Spectrometer spectrographs, of a large and representative sample of 67 extremely red objects (EROs) to H= 20.5 in three fields (SSA22, Chandra Deep Field South and NTT Deep Field) drawn from the Las Campanas Infrared Survey (LCIRS). Using the colour cut (I−H) > 3.0 (Vega magnitudes) adopted in earlier papers in this series, we verify the efficiency of this selection for locating and studying dista… Show more

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Cited by 53 publications
(59 citation statements)
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“…The ERO galaxy population follows a bimodal distribution and consists of both passively evolving ellipticals and dusty starforming galaxies in the redshift interval 1 z 2 (Doherty et al 2005;Fontanot & Monaco 2010;Gonzalez-Perez et al 2011). The ratio of both populations is still a matter of debate (see Conselice et al 2008;Gonzalez-Perez et al 2009;Kong et al 2009;Fontanot & Monaco 2010).…”
Section: Selecting Host Galaxy Candidatesmentioning
confidence: 99%
“…The ERO galaxy population follows a bimodal distribution and consists of both passively evolving ellipticals and dusty starforming galaxies in the redshift interval 1 z 2 (Doherty et al 2005;Fontanot & Monaco 2010;Gonzalez-Perez et al 2011). The ratio of both populations is still a matter of debate (see Conselice et al 2008;Gonzalez-Perez et al 2009;Kong et al 2009;Fontanot & Monaco 2010).…”
Section: Selecting Host Galaxy Candidatesmentioning
confidence: 99%
“…We have compared our photometric redshifts against objects with a known spectroscopic redshift that is taken from the literature (Vanzella et al 2005(Vanzella et al , 2006(Vanzella et al , 2008Mignoli et al 2005;Szokoly et al 2004;Le Fèvre et al 2004;Doherty et al 2005;Wolf et al 2004;Daddi et al 2005;Cristiani et al 2000;Strolger et al 2004;van der Wel et al 2005;Roche et al 2006;Ravikumar et al 2007;Teplitz et al 2007;Xu et al 2007;Gronwall et al 2007;Nilsson et al 2007;Hathi et al 2008;Finkelstein et al 2008;Yang et al 2008;Popesso et al 2009). …”
Section: Redshift Selectionmentioning
confidence: 99%
“…Our first galaxy sample contains 2422 galaxies with secure spectroscopic redshifts (z spec ) from the ESO public compilation in the Chandra Deep Field South (CDFS; Cristiani et al 2000;Croom et al 2001;Bunker et al 2003;Dickinson et al 2004;Stanway et al 2004aStanway et al , 2004bStrolger et al 2004;Szokoly et al 2004;van der Wel et al 2004;Doherty et al 2005;Le Fèvre et al 2005;Mignoli et al 2005;Ravikumar et al 2007;Popesso et al 2009;Balestra et al 2010;Silverman et al 2010;Kurk et al 2013;Vanzella et al 2014) and from Morris et al (2015). In order to obtain multiwavelength photometry for these galaxies, we cross-matched this sample with the public Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS; Grogin et al 2011;Koekemoer et al 2011) catalog for the Great Observatory Origins Deep Survey South field (GOODS-S) obtained by Guo et al (2013).…”
Section: Samplementioning
confidence: 99%