Document Type
Article
Publication Date
1-2013
Department
Physics and Astronomy
Abstract
Analysis of galaxies with overlapping images offers a direct way to probe the distribution of dust extinction and its effects on the background light. We present a catalog of 1990 such galaxy pairs selected from the Sloan Digital Sky Survey (SDSS) by volunteers of the Galaxy Zoo project. We highlight subsamples which are particularly useful for retrieving such properties of the dust distribution as UV extinction, the extent perpendicular to the disk plane, and extinction in the inner parts of disks. The sample spans wide ranges of morphology and surface brightness, opening up the possibility of using this technique to address systematic changes in dust extinction or distribution with galaxy type. This sample will form the basis for forthcoming work on the ranges of dust distributions in local disk galaxies, both for their astrophysical implications and as the low-redshift part of a study of the evolution of dust properties. Separate lists and figures show deep overlaps, where the inner regions of the foreground galaxy are backlit, and the relatively small number of previously-known overlapping pairs outside the SDSS DR7 sky coverage.
Original Publication Information
Keel, William C., et al. "Galaxy Zoo: A Catalog of Overlapping Galaxy Pairs for Dust Studies." 2013. Publications of the Astronomical Society of the Pacific 125(923): 2-16.
ThinkIR Citation
Keel, William C.; Manning, Anna M.; Holwerda, Benne W.; Mezzoprete, Massimo; Lintott, Chris J.; Schawinski, Kevin; Gay, Pamela; and Masters, Karen L., "Galaxy zoo : a catalog of overlapping galaxy pairs for dust studies." (2013). Faculty and Staff Scholarship. 222.
https://ir.library.louisville.edu/faculty/222
DOI
10.1086/669233
Comments
This is an author-created, un-copyedited version of an article accepted for publication/published in Publications of the Astronomical Society of the Pacific. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it.
The Version of Record is available online at https://doi.org/10.1086/669233