Closing in on the sources of cosmic reionization: first results from the GLASS-JWST program

Autor: S. Mascia, L. Pentericci, A. Calabrò, T. Treu, P. Santini, L. Yang, L. Napolitano, G. Roberts-Borsani, P. Bergamini, C. Grillo, P. Rosati, B. Vulcani, M. Castellano, K. Boyett, A. Fontana, K. Glazebrook, A. Henry, C. Mason, E. Merlin, T. Morishita, T. Nanayakkara, D. Paris, N. Roy, H. Williams, X. Wang, G. Brammer, M. Bradač, W. Chen, P. L. Kelly, A. M. Koekemoer, M. Trenti, R. A. Windhorst

Publikováno v: 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 2023, ' Closing in on the sources of cosmic reionization : First results from the GLASS-JWST program ', Astronomy & Astrophysics, vol. 672, A155 . https://doi.org/10.1051/0004-6361/202345866

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 meas

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The prevalence of galaxy overdensities around UV-luminous Lyman 𝛼 emitters in the Epoch of Reionization

Autor: Leonova, E., Oesch, P. A., Qin, Y., Naidu, R. P., Wyithe, J. S. B., de Barros, S., Bouwens, R. J., Ellis, R. S., Endsley, R. M., Hutter, A., Illingworth, G. D., Kerutt, J., Labbe, Nicole, Laporte, N., Magee, D., Mutch, S. J., Roberts-Borsani, G. W., Smit, R., Stark, D. P., Stefanon, M., Tacchella, S., Zitrin, A.

Publikováno v: Leonova, E, Oesch, P A, Qin, Y, Naidu, R P, Wyithe, J S B, de Barros, S, Bouwens, R J, Ellis, R S, Endsley, R M, Hutter, A, Illingworth, G D, Kerutt, J, Labbe, N, Laporte, N, Magee, D, Mutch, S J, Roberts-Borsani, G W, Smit, R, Stark, D P, Stefanon, M, Tacchella, S & Zitrin, A 2022, ' The prevalence of galaxy overdensities around UV-luminous Lyman emitters in the Epoch of Reionization ', Monthly Notices of the Royal Astronomical Society, vol. 515, no. 4, pp. 5790-5801 . https://doi.org/10.1093/mnras/stac1908

Before the end of the Epoch of Reionization, the Hydrogen in the Universe was predominantly neutral. This leads to a strong attenuation of Ly alpha lines of z greater than or similar to 6 galaxies in the intergalactic medium. Nevertheless, Ly alpha h

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https://curis.ku.dk/ws/files/318434333/stac1908.pdf