PSFs of coadded images
arXiv:2209.09253 · doi:10.21105/astro.2209.09253
Abstract
We provide a detailed exploration of the connection between choice of coaddition schemes and the point-spread function (PSF) of the resulting coadded images. In particular, we investigate what properties of the coaddition algorithm lead to the final coadded image having a well-defined PSF. The key elements of this discussion are as follows: 1. We provide an illustration of how linear coaddition schemes can produce a coadd that lacks a well-defined PSF even for relatively simple scenarios and choices of weight functions. 2. We provide a more formal demonstration of the fact that a linear coadd only has a well-defined PSF in the case that either (a) each input image has the same PSF or (b) the coadd is produced with weights that are independent of the signal. 3. We discuss some reasons that two plausible nonlinear coaddition algorithms (median and clipped-mean) fail to produce a consistent PSF profile for stars. 4. We demonstrate that all nonlinear coaddition procedures fail to produce a well-defined PSF for extended objects. In the end, we conclude that, for any purpose where a well-defined PSF is desired, one should use a linear coaddition scheme with weights that do not correlate with the signal and are approximately uniform across typical objects of interest.
13 pages, 4 figures; pedagogical article; v2 accepted for publication in the Open Journal of Astrophysics
Cited by in corpus (7)
- A General Framework for Removing Point Spread Function Additive Systematics in Cosmological Weak Lensing Analysis
- Simulating image coaddition with the Nancy Grace Roman Space Telescope: I. Simulation methodology and general results
- A Differentiable Perturbation-based Weak Lensing Shear Estimator
- Dark Energy Survey Year 6 Results: Cell-based Coadds and Metadetection Weak Lensing Shape Catalogue
- Simulating image coaddition with the Nancy Grace Roman Space Telescope: II. Analysis of the simulated images and implications for weak lensing
- Simulating image coaddition with the Nancy Grace Roman Space Telescope: III. Software improvements and new linear algebra strategies
- spike: A tool to drizzle HST, JWST, and Roman PSFs for improved analyses