activity
19982005
most citedA multi-wavelength study of the proto-cluster surrounding the z=4.1 radio galaxy TN J1338-1942

58 citations · 58 across the 3 of their papers we have counts for

collaborators

12 papers

astro-ph2005

Radio astronomical probes of cosmic reionization and the first luminous sources: probing the 'twilight zone'

C. L. Carilli

The epoch of reionization (EoR) corresponds to a 'cosmic phase transition', when the neutral intergalactic medium (IGM) becomes ionized by the first stars and/or AGN. While the dis…

astro-ph2004

ALMA: Galaxies and AGN

C. L. Carilli

With the ability to see into optically obscured regions with more than an order of magnitude better sensitivity and spatial resolution relative to current (sub)mm telescopes, ALMA…

astro-ph200458 cited

A multi-wavelength study of the proto-cluster surrounding the z=4.1 radio galaxy TN J1338-1942

Carlos De Breuck, Frank Bertoldi, Chris Carilli +8

We present a 1.2 mm (250 GHz) map obtained with MAMBO on the IRAM 30m telescope of the central 25 arcmin^2 of the proto-cluster surrounding the z=4.1 radio galaxy TN J1338-1942. Th…

astro-ph2000

The Dawn of Galaxies: Deep MAMBO Imaging Surveys

F. Bertoldi, K. M. Menten, E. Kreysa +2

We discuss results from sensitive, wide-field imaging of the millimeter extragalactic background using the Max-Planck Millimeter Bolometer array (MAMBO) at the IRAM 30m telescope.

astro-ph2000

Three high-redshift millimeter sources and their radio and near-infrared identifications

F. Bertoldi, C. L. Carilli, K. M. Menten +11

We present millimeter wavelength detections of three faint sources that are most likely high-redshift starburst galaxies. For one of the sources, which was previously discovered wi…

astro-ph2000

Search for clusters at high redshift - I. Candidate Lya emitters near 1138-262 at z=2.2

J. D. Kurk, H. J. A. Rottgering, L. Pentericci +7

Radio, optical and X-ray observations of the powerful radio galaxy PKS 1138-262 at z=2.156 have suggested that this galaxy is a massive galaxy in the center of a forming cluster. W…