We release fully reduced spectra obtained with NIRSpec onboard JWST as part of the GLASS-JWST Early Release Science Program and a follow-up Director’s Discretionary Time program 2756. From these 263 spectra of 245 unique sources, acquired with low (R = 30–300) and high dispersion (R ∼ 2700) gratings, we derive redshifts for 200 unique sources in the redshift range z = 0–10. We describe the sample selection and characterize its high completeness as a function of redshift and apparent magnitude. Comparison with independent estimates based on different methods and instruments shows that the redshifts are accurate, with 80% differing less than 0.005. We stack the GLASS-JWST spectra to produce the first high-resolution (R ∼ 2700) JWST spectral template extending in the rest frame wavelength from 2000 Å to 20 000 Å. Catalogs, reduced spectra, and template are made publicly available to the community.
The GLASS-JWST early release science program. IV. Data release of 263 spectra from 245 unique sources / Mascia, S.; Roberts-Borsani, G.; Treu, T.; Pentericci, L.; Chen, W.; Calabrò, A.; Merlin, E.; Paris, D.; Santini, P.; Brammer, G.; Henry, A.; Kelly, P. L.; Mason, C.; Morishita, T.; Nanayakkara, T.; Roy, N.; Wang, X.; Williams, H.; Boyett, K.; Bradac, M.; Castellano, M.; Glazebrook, K.; Jones, T.; Napolitano, L.; Vulcani, B.; Watson, P. J.; Yang, L.. - In: ASTRONOMY & ASTROPHYSICS. - ISSN 1432-0746. - 690:(2024), pp. 1-12. [10.1051/0004-6361/202450493]
The GLASS-JWST early release science program. IV. Data release of 263 spectra from 245 unique sources
L. Napolitano;
2024
Abstract
We release fully reduced spectra obtained with NIRSpec onboard JWST as part of the GLASS-JWST Early Release Science Program and a follow-up Director’s Discretionary Time program 2756. From these 263 spectra of 245 unique sources, acquired with low (R = 30–300) and high dispersion (R ∼ 2700) gratings, we derive redshifts for 200 unique sources in the redshift range z = 0–10. We describe the sample selection and characterize its high completeness as a function of redshift and apparent magnitude. Comparison with independent estimates based on different methods and instruments shows that the redshifts are accurate, with 80% differing less than 0.005. We stack the GLASS-JWST spectra to produce the first high-resolution (R ∼ 2700) JWST spectral template extending in the rest frame wavelength from 2000 Å to 20 000 Å. Catalogs, reduced spectra, and template are made publicly available to the community.File | Dimensione | Formato | |
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