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19992008
most citedThe First Appearance of the Red Sequence of Galaxies in Proto-Clusters at 2<~z<~3

186 citations · 188 across the 4 of their papers we have counts for

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10 papers · 1 filter

astro-ph20082 cited

A spectroscopic study of a z=1.6 galaxy overdensity with GMASS

Jaron Kurk, Andrea Cimatti, Gianni Zamorani +12

The Galaxy Mass Assembly ultra-deep Spectroscopic Survey samples a part of the CDFS to unprecedented depth. The resulting distribution of 150 z>1.4 redshifts reveals a significant…

astro-ph2007186 cited

The First Appearance of the Red Sequence of Galaxies in Proto-Clusters at 2<~z<~3

T. Kodama, I. Tanaka, M. Kajisawa +5

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…

astro-ph2003

Emission line galaxies at z = 6.5

Jaron Kurk, Andrea Cimatti, Sperello di Serego Alighieri +2

We are carrying out a search for Lyman alpha emitting galaxies at z = 6.5 employing slitless spectroscopy at the VLT. In our 43 square arcminute field we find three isolated single…

astro-ph2002

BRIGHT lights, BIG city: Massive galaxies, giant Ly-a nebulae, and proto--clusters

W. van Breugel, M. Reuland, W. de Vries +10

High redshift radio galaxies are great cosmological tools for pinpointing the most massive objects in the early Universe: massive forming galaxies, active super--massive black hole…

astro-ph2001

A search for high redshift clusters associated with radio galaxies at 2 < z < 4

J. D. Kurk, B. P. Venemans, H. J. A. Roettgering +2

High redshift radio galaxies are amongst the most massive galaxies in the early Universe and have properties expected from central galaxies in forming clusters. We are carrying out…

astro-ph2001

Deep VLT spectroscopy of high redshift radio galaxy MRC 2104-242: Evidence for a metallicity gradient

R. Overzier, H. Rottgering, J. Kurk +1

In this contribution we will present deep VLT spectroscopy observations of the giant emission line halo around the z=2.49 radio galaxy MRC 2104-242. The morphology of the halo is d…