Even magneto-optic effects in a ferromagnetic amorphous alloy

Afonso, C.N.; Briones, F.; Vicent, J. L.

doi:10.1016/0378-4363(77)90094-8

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2004

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“…It has been shown that selection at these wavelengths results in samples of star forming systems that omit a significant fraction of heavily obscured galaxies [11]. There have in addition been suggestions that the most strongly star forming systems suffer the most obscuration [1,8,3,12,7]. Using radio selection to construct a star forming galaxy sample allows the detection of such systems, and the average obscuration in this case is significantly higher than in optically selected samples [1,8].…”

Section: Introductionmentioning

confidence: 99%

Extremely Red Galaxies in the Phoenix Deep Survey

Hopkins

Afonso

Georgakakis

et al. 2004

Multiwavelength Cosmology

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The Phoenix Deep Survey (PDS) is a multiwavelength survey based on deep 1.4 GHz radio observations used to identify a large sample of star forming galaxies to z = 1. Here we present an exploration of the evolutionary constraints on the star-forming population imposed by the 1.4 GHz source counts, followed by an analysis of the average properties of extremely red galaxies in the PDS, by using the "stacking" technique.

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Section: Introductionmentioning

confidence: 99%