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The GLASS-JWST Early Release Science Program. IV. Data release of 263 spectra from 245 unique sources
by
Glazebrook, K
, Watson, P J
, Bradač, M
, Henry, A
, Jones, T
, Treu, T
, Pentericci, L
, Calabrò, A
, Napolitano, L
, Chen, W
, Brammer, G
, Santini, P
, Morishita, T
, Nanayakkara, T
, Castellano, M
, Yang, L
, Paris, D
, Roberts-Borsani, G
, Roy, N
, Wang, X
, Merlin, E
, Mason, C
, Kelly, P L
, Boyett, K
, Vulcani, B
, Mascia, S
, Williams, H
in
Red shift
/ Spectra
2024
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The GLASS-JWST Early Release Science Program. IV. Data release of 263 spectra from 245 unique sources
by
Glazebrook, K
, Watson, P J
, Bradač, M
, Henry, A
, Jones, T
, Treu, T
, Pentericci, L
, Calabrò, A
, Napolitano, L
, Chen, W
, Brammer, G
, Santini, P
, Morishita, T
, Nanayakkara, T
, Castellano, M
, Yang, L
, Paris, D
, Roberts-Borsani, G
, Roy, N
, Wang, X
, Merlin, E
, Mason, C
, Kelly, P L
, Boyett, K
, Vulcani, B
, Mascia, S
, Williams, H
in
Red shift
/ Spectra
2024
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The GLASS-JWST Early Release Science Program. IV. Data release of 263 spectra from 245 unique sources
by
Glazebrook, K
, Watson, P J
, Bradač, M
, Henry, A
, Jones, T
, Treu, T
, Pentericci, L
, Calabrò, A
, Napolitano, L
, Chen, W
, Brammer, G
, Santini, P
, Morishita, T
, Nanayakkara, T
, Castellano, M
, Yang, L
, Paris, D
, Roberts-Borsani, G
, Roy, N
, Wang, X
, Merlin, E
, Mason, C
, Kelly, P L
, Boyett, K
, Vulcani, B
, Mascia, S
, Williams, H
in
Red shift
/ Spectra
2024
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The GLASS-JWST Early Release Science Program. IV. Data release of 263 spectra from 245 unique sources
Paper
The GLASS-JWST Early Release Science Program. IV. Data release of 263 spectra from 245 unique sources
2024
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Overview
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\\sim2700\\)) 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 \\sim 2700\\)) JWST spectral template extending in the rest frame wavelength from 2000~\\AA\\ to 20, 000~\\AA. Catalogs, reduced spectra, and template are made publicly available to the community.
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