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Related papers: Structure of Protocluster Galaxies: Accelerated St…

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We study the environments of 6 radio galaxies at 2.2 < z < 2.6 using wide-field near-infrared images. We use colour cuts to identify galaxies in this redshift range, and find that three of the radio galaxies are surrounded by significant…

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 present results from a narrow-band survey of the field around the high redshift radio galaxy MRC 2104-242. We have selected Halpha emitters in a 7sq.arcmin field and compared the measured number density with that of a field sample at…

Astrophysics of Galaxies · Physics 2015-06-19 E. A. Cooke , N. A. Hatch , S. I. Muldrew , E. E. Rigby , J. D. Kurk

We present a multiwavelength study of galaxies around D4UD01, a spectroscopically confirmed protocluster at z = 3.24 to investigate environmental trends. 450 galaxies are selected based on Ks band detection with photometric redshifts…

Astrophysics of Galaxies · Physics 2021-04-21 Ke Shi , Jun Toshikawa , Kyoung-Soo Lee , Tao Wang , Zheng Cai , Taotao Fang

We present new constraints on the evolution of the early-type galaxy color-magnitude relation (CMR) based on deep near-infrared imaging of a galaxy protocluster at z=2.16 obtained using NICMOS on-board the Hubble Space Telescope. This field…

We present a study of protoclusters associated with high redshift radio galaxies. We imaged MRC1017-220 (z=1.77) and MRC0156-252 (z=2.02) using the near-infrared wide-field (7.5'x7.5') imager VLT/HAWK-I in the Y, H and Ks bands. We present…

We have discovered a highly significant over-density of galaxies at z=2.300+/-0.015 in the course of a redshift survey designed to select star-forming galaxies in the redshift range z=2.3+/-0.4 in the field of the bright z=2.72 QSO…

We present a deep image of the radio galaxy MRC 1138-262 taken with the Hubble Space Telescope (HST) at a redshift of z = 2.2. The galaxy is known to have properties of a cD galaxy progenitor and be surrounded by a 3 Mpc-sized structure,…

The redshift range z=2-4 marks a critical transition in large scale structure formation, where the dynamically unrelaxed progenitors of local massive clusters undergo rapid stellar mass assembly. We report the discovery and physical…

Astrophysics of Galaxies · Physics 2026-05-18 Shuaiyi Li , Zheng Cai , Yunjing Wu , Fujiang Yu , Xiaojing Lin , Jingyang Men , Xiaoyang Wei

We discuss the structural and morphological properties of galaxies in a z=1.62 proto-cluster using near-IR imaging data from Hubble Space Telescope Wide Field Camera 3 data of the Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey…

We report a discovery of proto-cluster candidates around high redshift radio galaxies at z~2.5 on the basis of clear statistical excess of colour-selected galaxies around them seen in the deep near-infrared imaging data obtained with CISCO…

Astrophysics · Physics 2009-11-11 Masaru Kajisawa , Tadayuki Kodama , Ichi Tanaka , Toru Yamada , Richard Bower

Radio galaxies are among the most massive galaxies in the high redshift universe and are known to often lie in protocluster environments. We have studied the fields of seven z = 2.2 radio galaxies with HAWK-I narrow-band and broad-band…

Astrophysics of Galaxies · Physics 2016-08-17 Kate Husband , Malcolm N. Bremer , John P. Stott , David N. A. Murphy

We present a panoramic narrow-band study of H-alpha emitters in the field of the z=2.16 proto-cluster around PKS1138-262 using MOIRCS on the Subaru Telescope. We find 83 H-alpha emitters down to a SFR(Ha)~10Msun/yr across a ~7'x7' region…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 Yusei Koyama , Tadayuki Kodama , Ken-ichi Tadaki , Masao Hayashi , Masayuki Tanaka , Ian Smail , Ichi Tanaka , Jaron Kurk

We study the stellar mass assembly of the Spiderweb Galaxy (MRC 1138-262), a massive z = 2.2 radio galaxy in a protocluster and the probable progenitor of a brightest cluster galaxy. Nearby protocluster galaxies are identified and their…

Cosmology and Nongalactic Astrophysics · Physics 2009-11-13 N. A. Hatch , R. A. Overzier , J. D. Kurk , G. K. Miley , H. J. A. Röttgering , A. W. Zirm

This is a study of H-alpha emitters in two dense galaxy proto-clusters surrounding radio galaxies at z~2. We show that the proto-cluster surrounding MRC 1138-262 contains 14+/-2 times more H-alpha candidates than the average field (9 sigma…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 N. A. Hatch , J. D. Kurk , L. Pentericci , B. P. Venemans , E. Kuiper , G. K. Miley , H. J. A. Röttgering

We present a spectroscopic campaign to follow-up red colour-selected candidate massive galaxies in two high redshift proto-clusters surrounding radio galaxies. We observed a total of 57 galaxies in the field of MRC0943-242 (z=2.93) and 33…

We present a large-scale galaxy structure Cl J021734-0513 at z~0.65 discovered in the UKIDSS UDS field, made of ~20 galaxy groups and clusters, spreading over 10 Mpc. We report on a VLT/VIMOS spectroscopic follow-up program that, combined…

We report on the discovery of a z=1.58 mature cluster around the high-redshift radio galaxy 7C1753+6311, first identified in the Clusters Around Radio-Loud AGN survey. Two-thirds of the excess galaxies within the central 1Mpc lie on a red…

In this paper we describe our search for galaxy protocluster candidates at $4.5< z < 10$ and explore the environmental and physical properties of their member galaxies identified through JWST wide-field surveys within the CEERS, JADES, and…

We present a detailed study of Near-IR selected galaxies in a protocluster field at z = 3.13. Protocluster galaxies are selected using the available mutliwavelength data with the photometric redshift (photo-z) at 2.9 < z < 3.3, reaching a…

Cosmology and Nongalactic Astrophysics · Physics 2020-08-26 Ke Shi , Jun Toshikawa , Zheng Cai , Kyoung-Soo Lee , Taotao Fang
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