1. Less and more IGM-transmitted galaxies from z similar to 2.7 to z similar to 6 from VANDELS and VUDS
- Author
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Thomas, R., Pentericci, L., Le Fevre, O., Koekemoer, A. M., Castellano, M., Cimatti, A., Fontanot, F., Gargiulo, A., Garilli, B., Talia, M., Amorin, R., Bardelli, S., Cristiani, S., Cresci, G., Franco, M., Fynbo, J. P. U., Hathi, N. P., Hibon, P., Khusanova, Y., Le Brun, Matthieu, Lemaux, B. C., Mannucci, F., Schaerer, D., Zamorani, G., Zucca, E., Thomas, R., Pentericci, L., Le Fevre, O., Koekemoer, A. M., Castellano, M., Cimatti, A., Fontanot, F., Gargiulo, A., Garilli, B., Talia, M., Amorin, R., Bardelli, S., Cristiani, S., Cresci, G., Franco, M., Fynbo, J. P. U., Hathi, N. P., Hibon, P., Khusanova, Y., Le Brun, Matthieu, Lemaux, B. C., Mannucci, F., Schaerer, D., Zamorani, G., and Zucca, E.
- Abstract
Aims. Our aim is to analyze the variance of the intergalactic medium (IGM) transmission by studying this parameter in the rest-frame UV spectra of a large sample of high-redshift galaxies.Methods. We made use of the VIMOS Ultra Deep Survey and the VANDELS public survey to gain insight into the far UV spectrum of 2.7
- Published
- 2021