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Journal ArticleDOI

A search for large low-surface brightness galaxies in deep CCD data

TLDR
In this article, the authors describe a search for very low-surface-brightness features in deep CCD frames, which would not be detected using more typical connected-pixel algorithms.
Abstract
In this paper, we describe a search for very low-surface-brightness features in deep CCD frames. We show how cross-correlation with templates can be used to detect low-surface-brightness features, which would not be detected using more typical connected-pixel algorithms. The search technique is specifically designed to search for large, low-surface- brightness galaxies like Malin 1. Although we identify 19 potentially interesting, extended, low-surface-brightness objects, we conclude that Malin 1 type objects per se are less prolific than `normal' L^*^ galaxies, and that galaxies with -22 < M_v_ < 19 and μ_0_ ~26 Vmu are at least an order of magnitude less common than their normal-surface- brightness counterparts.

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Journal ArticleDOI

The las campanas distant cluster survey - the catalog

TL;DR: In this article, an optically selected catalog of 1073 galaxy cluster and group candidates at 0.3 z 1.3 was presented, with a false-detection rate of ~30%.
Journal ArticleDOI

The Ursa Major Cluster of Galaxies; 2, Bimodality of the Distribution of Central Surface Brightnesses

TL;DR: The Ursa Major Cluster appears to be unevolved and made up of H I-rich spiral galaxies such as those one finds in the field as discussed by the authors, and the existence of separate high and low surface brightness families suggests that there are discrete radial configurations that are stable.
Journal ArticleDOI

The Ursa Major Cluster of Galaxies. II. Bimodality of the Distribution of Central Surface Brightnesses

TL;DR: In this article, B,R,I,K' photometry has been obtained for 79 galaxies, including 62 in a complete sample with M(B)<-16.5 mag.
Journal ArticleDOI

The Las Campanas Distant Cluster Survey - The Catalog

TL;DR: In this paper, an optically selected catalog of 1073 galaxy cluster and group candidates at 0.3 was presented, with a false-detection rate of 30% at z=0.3, while at z = 0.8 the most massive systems (sigma>1000 km/s).
Journal ArticleDOI

A survey for low surface brightness galaxies around M31. I. The newly discovered dwarf andromeda V

TL;DR: And VI (And VI) was confirmed to be a nearby dSph galaxy when it resolved into stars easily with a short V-band exposure with the 4 m telescope as mentioned in this paper.
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