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Closing in on the sources of cosmic reionization: first results from the GLASS-JWST program
by
Glazebrook, K
, Henry, A
, Trenti, M
, Pentericci, L
, Treu, T
, Napolitano, L
, Chen, W
, Brammer, G
, Santini, P
, Morishita, T
, Windhorst, R A
, Nanayakkara, T
, Bradac, M
, Yang, L
, Castellano, M
, Paris, D
, Roberts-Borsani, G
, Roy, N
, Wang, X
, Grillo, C
, Merlin, E
, Calabro', A
, Rosati, P
, Mason, C
, Kelly, P L
, Bergamini, P
, Boyett, K
, Vulcani, B
, Mascia, S
, Williams, H
, Fontana, A
, Koekemoer, A M
in
Galaxies
/ Intergalactic media
/ Ionization
/ Photons
/ Red shift
/ Star & galaxy formation
/ Star formation
2023
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Closing in on the sources of cosmic reionization: first results from the GLASS-JWST program
by
Glazebrook, K
, Henry, A
, Trenti, M
, Pentericci, L
, Treu, T
, Napolitano, L
, Chen, W
, Brammer, G
, Santini, P
, Morishita, T
, Windhorst, R A
, Nanayakkara, T
, Bradac, M
, Yang, L
, Castellano, M
, Paris, D
, Roberts-Borsani, G
, Roy, N
, Wang, X
, Grillo, C
, Merlin, E
, Calabro', A
, Rosati, P
, Mason, C
, Kelly, P L
, Bergamini, P
, Boyett, K
, Vulcani, B
, Mascia, S
, Williams, H
, Fontana, A
, Koekemoer, A M
in
Galaxies
/ Intergalactic media
/ Ionization
/ Photons
/ Red shift
/ Star & galaxy formation
/ Star formation
2023
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Closing in on the sources of cosmic reionization: first results from the GLASS-JWST program
by
Glazebrook, K
, Henry, A
, Trenti, M
, Pentericci, L
, Treu, T
, Napolitano, L
, Chen, W
, Brammer, G
, Santini, P
, Morishita, T
, Windhorst, R A
, Nanayakkara, T
, Bradac, M
, Yang, L
, Castellano, M
, Paris, D
, Roberts-Borsani, G
, Roy, N
, Wang, X
, Grillo, C
, Merlin, E
, Calabro', A
, Rosati, P
, Mason, C
, Kelly, P L
, Bergamini, P
, Boyett, K
, Vulcani, B
, Mascia, S
, Williams, H
, Fontana, A
, Koekemoer, A M
in
Galaxies
/ Intergalactic media
/ Ionization
/ Photons
/ Red shift
/ Star & galaxy formation
/ Star formation
2023
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Closing in on the sources of cosmic reionization: first results from the GLASS-JWST program
Paper
Closing in on the sources of cosmic reionization: first results from the GLASS-JWST program
2023
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Overview
The escape fraction of Lyman-continuum (LyC) photons (\\(f_{esc}\\)) is a key parameter for determining the sources of cosmic reionization at \\(z\\geq 6\\). At these redshifts, owing to the opacity of the intergalactic medium, the LyC emission cannot be measured directly. However, LyC leakers during the epoch of reionization could be identified using indirect indicators that have been extensively tested at low and intermediate redshifts. These include a high [OIII]/[OII] flux ratio, high star-formation surface density, and compact sizes. In this work, we present observations of 29 \\(4.5 \\leq z \\leq 8\\) gravitationally lensed galaxies in the Abell 2744 cluster field. From a combined analysis of JWST-NIRSpec and NIRCam data, we accurately derived their physical and spectroscopic properties: our galaxies have low masses \\((\\log(M_\\star)\\sim 8.5)\\), blue UV spectral slopes (\\(\\beta \\sim -2.1\\)), compact sizes (\\(r_e \\sim 0.3-0.5\\) kpc), and high [OIII]/[OII] flux ratios. We confirm that these properties are similar to those characterizing low-redshift LyC leakers. Indirectly inferring the fraction of escaping ionizing photons, we find that more than 80% of our galaxies have predicted \\(f_{esc}\\) values larger than 0.05, indicating that they would be considered leakers. The average predicted \\(f_{esc}\\) value of our sample is 0.12, suggesting that similar galaxies at \\(z\\geq 6\\) have provided a substantial contribution to cosmic reionization.
Publisher
Cornell University Library, arXiv.org
Subject
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