How to Find More Supernovae with Less Work: Object ClassificationTechniques for Difference Imaging

We present the results of applying new object classificationtechniques to difference images in the context of the Nearby SupernovaFactory supernova search. Most current supernova searches subtractreference images from new images, identify objects in these differenceimages, and apply simple threshold...

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Bibliographic Details
Published in:The Astrophysical journal Vol. 665; no. 2
Main Authors: Bailey, Stephen, Aragon, Cecilia, Romano, Raquel, Thomas, RollinC, Weaver, Benjamin A., Wong, Daniel
Format: Journal Article
Language:English
Published: United States 02-05-2007
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Summary:We present the results of applying new object classificationtechniques to difference images in the context of the Nearby SupernovaFactory supernova search. Most current supernova searches subtractreference images from new images, identify objects in these differenceimages, and apply simple threshold cuts on parameters such as statisticalsignificance, shape, and motionto reject objects such as cosmic rays,asteroids, and subtraction artifacts. Although most static objectssubtract cleanly, even a very low false positive detection rate can leadto hundreds of non-supernova candidates which must be vetted by humaninspection before triggering additional followup. In comparison to simplethreshold cuts, more sophisticated methods such as Boosted DecisionTrees, Random Forests, and Support Vector Machines provide dramaticallybetter object discrimination. At the Nearby Supernova Factory, we reducedthe number of non-supernova candidates by a factor of 10 while increasingour supernova identification efficiency. Methods such as these will becrucial for maintaining a reasonable false positive rate in the automatedtransient alert pipelines of upcoming projects such as PanSTARRS andLSST.
Bibliography:DE-AC02-05CH11231; NSF:AST-0407297, 0087344, AND0426879
LBNL-62659
USDOE Director, Office of Science
National ScienceFoundation
ISSN:0004-637X
1538-4357
DOI:10.1086/519832