Gas, dust, and star formation in distant radio galaxies Reuland, M.A.

Using data taken with the Wide-Field Infrared Survey Explorer and Herschel Space Observatory physical properties of 6 dwarf elliptical galaxies (dEs) in the Fornax cluster and 19

Chapter 2: Michiel Reuland, Huub Röttgering, Wil van Breugel, and Carlos De Breuck, Monthly Notices of the Royal Astronomical Society, Vol. Stanford, Arjun Dey, Mark Lacy,

Emergence of cosmic structures around distant radio galaxies and quasars.. Overzier,

This has motivated an extensive program to study the properties of massive galaxy clusters in the early universe, using broad-band imaging with the HST/ACS Wide Field Channel (WFC),

(2001) suggested that high-redshift radio galax- ies and EROs could be identical galaxies seen at different stages of their evolution, based on their findings of ERO-like host

0156–252 is the only source in our sample for which the core is detected with sufficient S/N to carry out a (crude) spectral analysis. The X- ray spectrum is shown in Fig. The

5.6.2.4 Redshift evolution of the overdensity In a subsequent paper, we will compare the number densities, masses, and total SFRs of galaxies in protoclusters observed at a wide

One technique for finding distant galaxy overdensities is based on the empirical evidence that powerful radio galaxies are among the most massive forming galaxies at high