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Part of book or chapter of book . 2007 . Peer-reviewed
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Part of book or chapter of book . 1994 . Peer-reviewed
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https://dx.doi.org/10.1007/978...
Other literature type
Data sources: Microsoft Academic Graph
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An infrared search for primeval galaxies

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Other literature type 01 Jan 1994 English Publisher:Springer Berlin Heidelberg
Authors: F. Mannucci; S. V. W. Beckwith; M. J. Mccaughrean;

doi: 10.1007/bfb0102389 , 10.1007/978-94-011-1070-9_149

An infrared search for primeval galaxies

Abstract

We present early results of a near-infrared search for Primeval Galaxies (PGs), i.e., galaxies forming the bulk of their stars at high redshift. These results are compared with some theoretical expectations on the surface density of the PGs.

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Powered by OpenAIRE graph
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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
2
Average
Top 10%
Average
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