A Five-Stage Framework for Slitless Grism Spectra: Demonstrated on Euclid Q1 Strong-Lens Candidates and Ported to CEERS NIRCam
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TL;DR
This paper introduces a five-stage framework for extracting and analyzing slitless grism spectra in complex regimes, demonstrated on Euclid and CEERS data, improving redshift accuracy and portability across instruments.
Contribution
The paper presents a novel five-stage spectral extraction framework that enhances redshift determination in crowded slitless spectroscopy, applicable to multiple space telescopes.
Findings
473 Euclid Q1 lens candidates analyzed with high success rate
Median source redshift uncertainty reduced from 0.43 to 0.18
Portability of spectral analysis demonstrated on CEERS JWST/NIRCam data
Abstract
Wide-field slitless grism spectroscopy is difficult in the co-spatial regime, where multiple sources share one cross-dispersion PSF element and catalogue-level decontamination (aXe/LINEAR/Grizli) does not apply -- the regime of strong lenses, binary AGN, and mergers in HST, JWST, Euclid, and Roman grism data. This paper presents a five-stage framework for per-source 1-D spectra and redshifts: distortion-calibrated extraction, Fourier/Sersic/NNLS deblending, robust-PCA cleaning, weighted friend-of-friend with Hungarian cross-orientation matching, and a Bayesian posterior layer. Of 579 published Euclid Q1 lens candidates, 473 fall in the NISP footprint. A 3" DESI DR1 Iron match gives 57 counterparts (51 ZWARN=0, 46 clean v6d anchors). Extending to 9200 A adds features below 12500 A in 312 source and 324 deflector spectra. Source/deflector features are detected in 467/471 of 473; 371…
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