Edward M. Berman
Efficient Point-spread Function Modeling with ShOpt.jl: A Point-spread Function Benchmarking Study with JWST NIRCam Imaging
Berman, Edward M.; McCleary, Jacqueline E.; Koekemoer, Anton M.; Franco, Maximilien; Drakos, Nicole E.; Liu, Daizhong; Nightingale, James W.; Shuntov, Marko; Scognamiglio, Diana; Massey, Richard; Mahler, Guillaume; McCracken, Henry Joy; Robertson, Brant E.; Faisst, Andreas L.; Casey, Caitlin M.; Kartaltepe, Jeyhan S.
Authors
Jacqueline E. McCleary
Anton M. Koekemoer
Maximilien Franco
Nicole E. Drakos
Daizhong Liu
James W. Nightingale
Marko Shuntov
Diana Scognamiglio
Professor Richard Massey r.j.massey@durham.ac.uk
Professor
Dr Guillaume Mahler guillaume.mahler@durham.ac.uk
Academic Visitor
Henry Joy McCracken
Brant E. Robertson
Andreas L. Faisst
Caitlin M. Casey
Jeyhan S. Kartaltepe
Abstract
With their high angular resolutions of 30–100 mas, large fields of view, and complex optical systems, imagers on next-generation optical/near-infrared space observatories, such as the Near-Infrared Camera (NIRCam) on the James Webb Space Telescope, present new opportunities for science and also new challenges for empirical point-spread function (PSF) characterization. In this context, we introduce ShOpt, a new PSF fitting tool developed in Julia and designed to bridge the advanced features of PSFs in the full field of view (PIFF) with the computational efficiency of PSF Extractor (PSFEx). Along with ShOpt, we propose a suite of nonparametric statistics suitable for evaluating PSF fit quality in space-based imaging. Our study benchmarks ShOpt against the established PSF fitters PSFEx and PIFF using real and simulated COSMOS-Web Survey imaging. We assess their respective PSF model fidelity with our proposed diagnostic statistics and investigate their computational efficiencies, focusing on their processing speed relative to the complexity and size of the PSF models. We find that ShOpt can already achieve PSF model fidelity comparable to PSFEx and PIFF while maintaining competitive processing speeds, constructing PSF models for large NIRCam mosaics within minutes.
Citation
Berman, E. M., McCleary, J. E., Koekemoer, A. M., Franco, M., Drakos, N. E., Liu, D., Nightingale, J. W., Shuntov, M., Scognamiglio, D., Massey, R., Mahler, G., McCracken, H. J., Robertson, B. E., Faisst, A. L., Casey, C. M., & Kartaltepe, J. S. (2024). Efficient Point-spread Function Modeling with ShOpt.jl: A Point-spread Function Benchmarking Study with JWST NIRCam Imaging. Astronomical Journal, 168(4), Article 174. https://doi.org/10.3847/1538-3881/ad6a0f
Journal Article Type | Article |
---|---|
Acceptance Date | Jul 29, 2024 |
Online Publication Date | Sep 24, 2024 |
Publication Date | Oct 1, 2024 |
Deposit Date | Oct 4, 2024 |
Publicly Available Date | Oct 4, 2024 |
Journal | The Astronomical Journal |
Print ISSN | 0004-6256 |
Electronic ISSN | 1538-3881 |
Publisher | IOP Publishing |
Peer Reviewed | Peer Reviewed |
Volume | 168 |
Issue | 4 |
Article Number | 174 |
DOI | https://doi.org/10.3847/1538-3881/ad6a0f |
Keywords | Computational methods, Astronomy data analysis, Astronomy image processing, James Webb Space Telescope |
Public URL | https://durham-repository.worktribe.com/output/2898340 |
Files
Published Journal Article
(6.2 Mb)
PDF
Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/
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