Standard
Closing in on the sources of cosmic reionization : First results from the GLASS-JWST program. / Mascia, S.; Pentericci, L.; Calabro, A.; Treu, T.; Santini, P.; Yang, L.; Napolitano, L.; Roberts-Borsani, G.; Bergamini, P.; Grillo, C.; Rosati, P.; Vulcani, B.; Castellano, M.; Boyett, K.; Fontana, A.; Glazebrook, K.; Henry, A.; Mason, C.; Merlin, E.; Morishita, T.; Nanayakkara, T.; Paris, D.; Roy, N.; Williams, H.; Wang, X.; Brammer, G.; Bradac, M.; Chen, W.; Kelly, P. L.; Koekemoer, A. M.; Trenti, M.; Windhorst, R. A.
In:
Astronomy & Astrophysics, Vol. 672, A155, 14.04.2023.
Research output: Contribution to journal › Journal article › Research › peer-review
Harvard
Mascia, S, Pentericci, L, Calabro, A, Treu, T, Santini, P, Yang, L, Napolitano, L, Roberts-Borsani, G, Bergamini, P, Grillo, C, Rosati, P, Vulcani, B, Castellano, M, Boyett, K, Fontana, A, Glazebrook, K, Henry, A
, Mason, C, Merlin, E, Morishita, T, Nanayakkara, T, Paris, D, Roy, N, Williams, H, Wang, X
, Brammer, G, Bradac, M, Chen, W, Kelly, PL, Koekemoer, AM, Trenti, M & Windhorst, RA 2023, '
Closing in on the sources of cosmic reionization: First results from the GLASS-JWST program',
Astronomy & Astrophysics, vol. 672, A155.
https://doi.org/10.1051/0004-6361/202345866APA
Mascia, S., Pentericci, L., Calabro, A., Treu, T., Santini, P., Yang, L., Napolitano, L., Roberts-Borsani, G., Bergamini, P., Grillo, C., Rosati, P., Vulcani, B., Castellano, M., Boyett, K., Fontana, A., Glazebrook, K., Henry, A.
, Mason, C., Merlin, E., ... Windhorst, R. A. (2023).
Closing in on the sources of cosmic reionization: First results from the GLASS-JWST program.
Astronomy & Astrophysics,
672, [A155].
https://doi.org/10.1051/0004-6361/202345866Vancouver
Mascia S, Pentericci L, Calabro A, Treu T, Santini P, Yang L et al.
Closing in on the sources of cosmic reionization: First results from the GLASS-JWST program.
Astronomy & Astrophysics. 2023 Apr 14;672. A155.
https://doi.org/10.1051/0004-6361/202345866Author
Mascia, S. ; Pentericci, L. ; Calabro, A. ; Treu, T. ; Santini, P. ; Yang, L. ; Napolitano, L. ; Roberts-Borsani, G. ; Bergamini, P. ; Grillo, C. ; Rosati, P. ; Vulcani, B. ; Castellano, M. ; Boyett, K. ; Fontana, A. ; Glazebrook, K. ; Henry, A. ; Mason, C. ; Merlin, E. ; Morishita, T. ; Nanayakkara, T. ; Paris, D. ; Roy, N. ; Williams, H. ; Wang, X. ; Brammer, G. ; Bradac, M. ; Chen, W. ; Kelly, P. L. ; Koekemoer, A. M. ; Trenti, M. ; Windhorst, R. A. / Closing in on the sources of cosmic reionization : First results from the GLASS-JWST program. In: Astronomy & Astrophysics. 2023 ; Vol. 672.
Bibtex
@article{71ff83ff1f5f4d0f8c30b508c5acc454,
title = "Closing in on the sources of cosmic reionization: First results from the GLASS-JWST program",
abstract = "The escape fraction of Lyman-continuum (LyC) photons (f(esc)) is a key parameter for determining the sources of cosmic reionization at z >= 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 = 6 have provided a substantial contribution to cosmic reionization.",
keywords = "galaxies: evolution, galaxies: formation, early Universe, galaxies: clusters: intracluster medium, STAR-FORMING GALAXIES, LYMAN-BREAK GALAXIES, LY-ALPHA EMISSION, HIGH-REDSHIFT GALAXIES, WEBB-SPACE-TELESCOPE, C IV EMISSION, SPECTRAL SIGNATURES, CONTINUUM EMISSION, IONIZING-RADIATION, STELLAR POPULATION",
author = "S. Mascia and L. Pentericci and A. Calabro and T. Treu and P. Santini and L. Yang and L. Napolitano and G. Roberts-Borsani and P. Bergamini and C. Grillo and P. Rosati and B. Vulcani and M. Castellano and K. Boyett and A. Fontana and K. Glazebrook and A. Henry and C. Mason and E. Merlin and T. Morishita and T. Nanayakkara and D. Paris and N. Roy and H. Williams and X. Wang and G. Brammer and M. Bradac and W. Chen and Kelly, {P. L.} and Koekemoer, {A. M.} and M. Trenti and Windhorst, {R. A.}",
year = "2023",
month = apr,
day = "14",
doi = "10.1051/0004-6361/202345866",
language = "English",
volume = "672",
journal = "Astronomy & Astrophysics",
issn = "0004-6361",
publisher = "E D P Sciences",
}
RIS
TY - JOUR
T1 - Closing in on the sources of cosmic reionization
T2 - First results from the GLASS-JWST program
AU - Mascia, S.
AU - Pentericci, L.
AU - Calabro, A.
AU - Treu, T.
AU - Santini, P.
AU - Yang, L.
AU - Napolitano, L.
AU - Roberts-Borsani, G.
AU - Bergamini, P.
AU - Grillo, C.
AU - Rosati, P.
AU - Vulcani, B.
AU - Castellano, M.
AU - Boyett, K.
AU - Fontana, A.
AU - Glazebrook, K.
AU - Henry, A.
AU - Mason, C.
AU - Merlin, E.
AU - Morishita, T.
AU - Nanayakkara, T.
AU - Paris, D.
AU - Roy, N.
AU - Williams, H.
AU - Wang, X.
AU - Brammer, G.
AU - Bradac, M.
AU - Chen, W.
AU - Kelly, P. L.
AU - Koekemoer, A. M.
AU - Trenti, M.
AU - Windhorst, R. A.
PY - 2023/4/14
Y1 - 2023/4/14
N2 - The escape fraction of Lyman-continuum (LyC) photons (f(esc)) is a key parameter for determining the sources of cosmic reionization at z >= 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 = 6 have provided a substantial contribution to cosmic reionization.
AB - The escape fraction of Lyman-continuum (LyC) photons (f(esc)) is a key parameter for determining the sources of cosmic reionization at z >= 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 = 6 have provided a substantial contribution to cosmic reionization.
KW - galaxies: evolution
KW - galaxies: formation
KW - early Universe
KW - galaxies: clusters: intracluster medium
KW - STAR-FORMING GALAXIES
KW - LYMAN-BREAK GALAXIES
KW - LY-ALPHA EMISSION
KW - HIGH-REDSHIFT GALAXIES
KW - WEBB-SPACE-TELESCOPE
KW - C IV EMISSION
KW - SPECTRAL SIGNATURES
KW - CONTINUUM EMISSION
KW - IONIZING-RADIATION
KW - STELLAR POPULATION
U2 - 10.1051/0004-6361/202345866
DO - 10.1051/0004-6361/202345866
M3 - Journal article
VL - 672
JO - Astronomy & Astrophysics
JF - Astronomy & Astrophysics
SN - 0004-6361
M1 - A155
ER -
