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Difference image analysis: extension to a spatially varying photometric scale factor and other considerations

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dc.contributor.author Bramich, D. M
dc.contributor.author Horne, Keith
dc.contributor.author Albrow, M. D
dc.contributor.author Tsapras, Y
dc.contributor.author Snodgrass, C
dc.contributor.author Street, R. A
dc.contributor.author Hundertmark, M
dc.contributor.author Kains, N
dc.contributor.author Arellano Ferro, A
dc.contributor.author Figuera Jaimes, R
dc.contributor.author Giridhar, S
dc.date.accessioned 2012-12-11T16:02:22Z
dc.date.available 2012-12-11T16:02:22Z
dc.date.issued 2013-01-21
dc.identifier.citation Monthly Notices of the Royal Astronomical Society, Vol. 428, No. 3, pp. 2275-2289 en
dc.identifier.issn 1365-2966
dc.identifier.uri http://hdl.handle.net/2248/5942
dc.description Restricted Access en
dc.description.abstract We present a general framework for matching the point-spread function (PSF), photometric scaling and sky background between two images, a subject which is commonly referred to as difference image analysis (DIA). We introduce the new concept of a spatially varying photometric scale factor which will be important for DIA applied to wide-field imaging data in order to adapt to transparency and airmass variations across the field-of-view. Furthermore, we demonstrate how to separately control the degree of spatial variation of each kernel basis function, the photometric scale factor and the differential sky background. We discuss the common choices for kernel basis functions within our framework, and we introduce the mixed-resolution delta basis functions to address the problem of the size of the least-squares problem to be solved when using delta basis functions. We validate and demonstrate our algorithm on simulated and real data. We also describe a number of useful optimizations that may be capitalized on during the construction of the least-squares matrix and which have not been reported previously. We pay special attention to presenting a clear notation for the DIA equations which are set out in a way that will hopefully encourage developers to tackle the implementation of DIA software. en
dc.language.iso en en
dc.publisher Oxford University Press on behalf of the Royal Astronomical Society en
dc.relation.uri http://dx.doi.org/10.1093/mnras/sts184 en
dc.relation.uri http://mnras.oxfordjournals.org/content/early/2012/11/09/mnras.sts184 en
dc.rights © Royal Astronomical Society en
dc.subject Methods: statistical en
dc.subject Techniques: image processing en
dc.subject Techniques: photometric en
dc.subject Methods: data analysis en
dc.title Difference image analysis: extension to a spatially varying photometric scale factor and other considerations en
dc.type Article en


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