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

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...

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Published in:The Astronomical journal Vol. 168; no. 4; pp. 174 - 202
Main Authors: 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.
Format: Journal Article
Language:English
Published: Madison The American Astronomical Society 01-10-2024
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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.
AbstractList 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.
Author Kartaltepe, Jeyhan S.
Massey, Richard
McCleary, Jacqueline E.
Franco, Maximilien
Nightingale, James W.
Casey, Caitlin M.
Liu, Daizhong
Shuntov, Marko
Faisst, Andreas L.
Koekemoer, Anton M.
Drakos, Nicole E.
McCracken, Henry Joy
Mahler, Guillaume
Robertson, Brant E.
Berman, Edward M.
Scognamiglio, Diana
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  givenname: James W.
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  organization: Durham University Department of Physics, Centre for Extragalactic Astronomy, South Rd., Durham DH1 3LE, UK
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  givenname: Henry Joy
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  surname: McCracken
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  surname: Kartaltepe
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  organization: School of Physics and Astronomy Laboratory for Multiwavelength Astrophysics, Rochester Institute of Technology, 84 Lomb Memorial Dr., Rochester, NY 14623, USA
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Snippet 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...
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SubjectTerms Accuracy
Astronomy data analysis
Astronomy image processing
Benchmarks
Complexity
Computational methods
Imaging
Infrared cameras
Infrared telescopes
James Webb Space Telescope
Nonparametric statistics
Observatories
Point spread functions
Software
Space telescopes
Title Efficient Point-spread Function Modeling with ShOpt.jl: A Point-spread Function Benchmarking Study with JWST NIRCam Imaging
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