English
Related papers

Related papers: Dusty ERO Search behind Two Massive Clusters

200 papers

We measure the angular clustering of 33 415 extremely red objects (EROs) in the Elais-N1 field covering 5.33 deg$^{2}$, which cover the redshift range $z=0.8$ to $2$. This sample was made by merging the UKIDSS Deep eXtragalactic Survey…

We use deep ground-based imaging in the near-IR to search for counterparts to the luminous submm sources in the catalog of Smail et al (1998). For the majority of the submm sources the near-IR imaging supports the counterparts originally…

Wide field near-infrared (IR) surveys have revealed a population of galaxies with very red optical$-$IR colors, which have been termed ``Extremely Red Objects'' (EROs). Modeling suggests that such red colors (R-K > 5) could be produced by…

Astrophysics · Physics 2009-11-07 Leonidas A. Moustakas , Rachel S. Somerville

The addition of deep near infrared images to the database provided by the HDF-S WFPC2 is essential to monitor the SEDs of the objects on a wide baseline and address a number of key issues including the total stellar content of baryonic…

Astrophysics · Physics 2009-11-07 S. Cristiani , S. Arnouts , A. Fontana , P. Saracco , E. Vanzella

We present near-infrared spectroscopy and Hubble Space Telescope (HST) imaging of EROJ003707+0909.5, the brightest of three gravitationally-lensed images of an Extremely Red Object (ERO) at z=1.6, in the field of the massive cluster A68…

Astrophysics · Physics 2009-11-07 Graham P. Smith , Ian Smail , J. -P. Kneib , C. J. Davis , M. Takamiya , H. Ebeling , O. Czoske

Deep, wide, near-infrared imaging surveys provide an opportunity to study the clustering of various galaxy populations at high redshift on the largest physical scales. We have selected $1<z<2$ extremely red objects (EROs) and $1<z<3$…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 J. -W. Kim , A. C. Edge , D. A. Wake , J. P. Stott

We present a study of the classification of z ~1 extremely red objects (EROs), using a combination of HST/ACS, Spitzer/IRAC, and ground-based images of the COSMOS field. Our sample includes about 5300 EROs with i-Ks>2.45 (AB, equivalently…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 Xu Kong , Guanwen Fang , Nobuo Arimoto , Min Wang

We present optical and near-IR photometry of 96 dusty, far-IR luminous galaxies. We have precise spectroscopic redshifts for all these galaxies yielding a median redshift of z=2.2. The majority, 78, are submm-detected galaxies lying at…

Astrophysics · Physics 2015-06-24 Ian Smail , S. C. Chapman , A. W. Blain , R. J. Ivison

Spatially compact objects with extremely red color in the rest-frame optical to near-infrared (0.4--1 ${\rm \mu m}$) and blue color in the rest-frame ultraviolet (UV; 0.2--0.4 ${\rm \mu m}$) have been discovered at $5 < z < 9$ using the…

Astrophysics of Galaxies · Physics 2023-12-06 Akatoki Noboriguchi , Akio K. Inoue , Tohru Nagao , Yoshiki Toba , Toru Misawa

We present a quantitative study of the morphology of 41 Extremely Red Objects (EROs). The analysis is based on deep otical and near-infrared images from the Hubble Space Telescope public archive, and performed by fitting to each galaxy…

Astrophysics · Physics 2007-05-23 G. Moriondo , A. Cimatti , E. Daddi

We report the discovery of a rich component of dusty star-forming galaxies contaminating the red-sequence in the supercluster system comprising Abell 901a, 901b and A902 at redshift ~0.17. These galaxies do not fit into the colour-density…

Astrophysics · Physics 2010-12-02 C. Wolf , M. E. Gray , K. Meisenheimer

In this paper we present a quantitative study of the classification of Extremely Red Objects (EROs). The analysis is based on the multi-band spatial- and ground-based observations (HST/ACS-$BViz$, HST/NICMOS-$JH$, VLT-$JHK$) in the Hubble…

Cosmology and Nongalactic Astrophysics · Physics 2009-11-13 Guan-Wen Fang , Xu Kong , Min Wang

We explore the evolved galaxy population in the proto-clusters around four high-z radio galaxies at 2<~z<~3 based on wide-field near-infrared imaging. Three of the four fields are known proto-clusters as demonstrated by overdensities of…

Astrophysics · Physics 2008-11-26 T. Kodama , I. Tanaka , M. Kajisawa , J. Kurk , B. Venemans , C. De Breuck , J. Vernet , C. Lidman

We discuss the submillimeter properties of Extremely Red Objects (EROs) in the two Canada-UK Deep Submillimeter Survey (CUDSS) Fields. We measure the mean submillimeter flux of the ERO population (to K < 20.7) and find 0.4 +/- 0.07 mJy for…

Astrophysics · Physics 2009-11-10 Tracy Webb , Mark Brodwin , Steve Eales , Simon Lilly

We present further observations of the extremely red object ERO J094258+4659.2, identified by \citet{iye00} as ERO R1 in their deep images of the cluster A851. We estimate its redshift independently by eight-band photometric redshift…

Aims. We present a determination of the intrinsic colors and ages of galaxies at very high redshift, in particular old galaxies (OGs) within extremely red objects (EROs). To date, the definition of EROs has been restricted to objects with…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 N. Castro-Rodriguez , M. Lopez-Corredoira

We construct a sample of extremely red objects (EROs) within the UKIDSS Ultra Deep Survey by combining the Early Data Release with optical data from the Subaru/XMM-Newton Deep Field. We find a total of 3715 objects over 2013 sq. arcmin with…

We have obtained new deep optical and near-infrared images of the field of the radio-loud quasar 1335.8+2834 at $z=1.086$ where an excess in the surface number density of galaxies was reported by Hutchings et al. [AJ, 106, 1324] from…

Astrophysics · Physics 2009-10-30 T. Yamada , I. Tanaka , A. Aragón-Salamanca , T. Kodama , K. Ohta , N. Arimoto

We report the first detection of the lowest CO transition in a sub-millimetre bright galaxy and extremely red object (ERO) at z = 1.44 using the Very Large Array. The total J = 1 - 0 line luminosity of ERO J164502+4626.4 is (7+-1) x 10^{10}…

Astrophysics · Physics 2009-11-10 T. R. Greve , R. J. Ivison , P. P. Papadopoulos