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The Astrophysical Journal Supplement Series
Article . 2002 . Peer-reviewed
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Preprint . 2002
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https://dx.doi.org/10.48550/ar...
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Optical and Near‐Infrared Photometry of Distant Galaxy Clusters

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 01 Oct 2002Embargo end date: 01 Jan 2002 Australia English Publisher:American Astronomical SocietyJournal:The Astrophysical Journal Supplement Series, volume 142, pages 153-160 (issn: 0067-0049, eissn: 1538-4365, Copyright policy )
Authors: Spencer A. Stanford; Spencer A. Stanford; Spencer A. Stanford; Roberto De Propris; Bradford P. Holden; Bradford P. Holden; Peter R. Eisenhardt; +3 Authors

doi: 10.1086/340972 , 10.48550/arxiv.astro-ph/0203498

arXiv: http://arxiv.org/abs/astro-ph/0203498

handle: 1885/66638

Optical and Near‐Infrared Photometry of Distant Galaxy Clusters

Abstract

We present optical and near-infrared photometry of 45 clusters of galaxies at 0.1 < z < 1.3. Galaxy catalogs in each cluster were defined at the longest wavelenth available, generally the K-band, down to approximately two magnitudes below M*. We include finding chart images of the band used for catalog definition. The photometry has been used in previously published papers to examine the origin and evolution of galaxies in distant clusters.

Accepted for publication in The Astrophysical Journal Supplement. 232 pages including 43 figures. Tables in ascii format to be electronically available from the ApJ

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Australia
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Keywords

Galaxies: Evolution, Galaxies: Formation, Astrophysics (astro-ph), Galaxies: High-redshift, Galaxies: Photometry, FOS: Physical sciences, Keywords: Galaxies: Clusters: General, Astrophysics

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    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).
    		 31
    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.
    		 Average
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    		 Top 10%
    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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citations
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!
31
Average
Top 10%
Top 10%
Green
gold
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