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Journal ArticleDOI

Optimal Image Subtraction Method: Summary Derivations, Applications, and Publicly Shared Application Using IDL

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TLDR
Computer algorithms for the OIS method were developed, written using the Interactive Data Language (IDL) and applications demonstrating these algorithms are presented, and a complete description of the Gaussian components basis vectors used by Alard & Lupton to construct the convolution kernel is presented.
Abstract
To detect objects that vary in brightness or spatial coordinates over time, C. Alard and R. H. Lupton in 1998 proposed an "optimal image subtraction" (OIS) method that constructs a convolution kernel from a set of matching stars distributed across the two images to be subtracted. Using multivariable least squares, the kernel is derived and can be designed to vary by pixel coordinates across the convolved image. Local effects in the optics, including aberrations or other spatially sensitive perturbations to a perfect image, can be mitigated. This paper presents the specific systems of equations that originate from the OIS method. Also included is a complete description of the Gaussian components basis vectors used by Alard & Lupton to construct the convolution kernel. An alternative set of basis vectors, called the delta function basis, is also described. Important issues are addressed, including the selection of the matching stars, differential background correction, constant photometric flux, contaminated pixel masking, and alignment at the subpixel level. Computer algorithms for the OIS method were developed, written using the Interactive Data Language (IDL), and applications demonstrating these algorithms are presented.

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Citations
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Journal ArticleDOI

Cluster Difference Imaging Photometric Survey. I. Light Curves of Stars in Open Clusters from TESS Sectors 6 & 7

TL;DR: The Cluster Difference Imaging Photometric Survey (CDIPS) as mentioned in this paper uses the TESS images to find giant transiting planets with known ages and to provide light curves suitable for studies in stellar astrophysics.
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Precision Light Curves from TESS Full-Frame Images: A Difference Imaging Approach

TL;DR: A difference image analysis pipeline that achieves the mission specification noise floor of 60~ppm~hr, and is provided as an open-source tool at this https URL in both IDL and PYTHON.
References
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Journal ArticleDOI

A Method for Optimal Image Subtraction

TL;DR: In this paper, a new method was proposed for image subtraction using a simple least-squares analysis using all the pixels of both images, and also showed that it is possible to fit the differential background variation at the same time.
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Image subtraction using a space-varying kernel

TL;DR: In this paper, the authors generalize the theory to the case of space-varying kernels and show that the CPU cost required for this new extension of the method is almost the same as for fitting a constant kernel solution.
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The ALADIN interactive sky atlas - A reference tool for identification of astronomical sources

TL;DR: The Aladin interactive sky atlas as mentioned in this paper provides simultaneous access to digitized images of the sky, astronomical catalogues, and databases, and facilitates direct, visual comparison of observational data at any wavelength with images of optical sky, and with reference catalogues.
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Expanding the Realm of Microlensing Surveys with Difference Image Photometry

TL;DR: In this paper, the authors present a new technique for monitoring microlensing activity even in highly crowded fields, and use this technique to place limits on low-mass MACHOs in the haloes of M31 and the Galaxy.
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