A multi-wavelength study of the forming cluster around the z=2.16 radio galaxy MRC 1138-262

Details A multi-wavelength study of the forming cluster around the z=2.16 radio galaxy MRC 1138-262 A multi-wavelength study of the forming cluster around the z=2.16 radio galaxy MRC 1138-262

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..17..262p&link_type=abstract

Galaxy Evolution: Theory & Observations (Eds. Vladimir Avila-Reese, Claudio Firmani, Carlos S. Frenk & Christine Allen) Revista

Astronomy and Astrophysics

Astronomy

H Ii Regions, Ism: Jets And Outflows, Stars: Pre-Main Sequence, Stars: Mass Loss

Scientific paper

We present multi-wavelength observations of a forming cluster around the z=2.16 radio galaxy MRC 1138-262. We study the populations of Ly alpha and H alpha emitters, extremely red objects and X-ray sources. The field of the radio source MRC 1138-262 has been observed at several wavelengths, including deep imaging through narrow band filters corresponding to Ly alpha and H alpha at z ~ 2.16 (with FORS and ISAAC respectively), several optical and near-IR broad bands (B, R, I, J, H and K), and finally radio and X-ray emission.

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