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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.

Efficient Point-spread Function Modeling with ShOpt.jl: A Point-spread Function Benchmarking Study with JWST NIRCam Imaging Thumbnail


Authors

Edward M. Berman

Jacqueline E. McCleary

Anton M. Koekemoer

Maximilien Franco

Nicole E. Drakos

Daizhong Liu

James W. Nightingale

Marko Shuntov

Diana Scognamiglio

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

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