Zobrazeno 1 - 10
of 621
pro vyhledávání: '"Marchi, F A"'
Autor:
Talia, M., Schreiber, C., Garilli, B., Pentericci, L., Pozzetti, L., Zamorani, G., Cullen, F., Moresco, M., Calabrò, A., Castellano, M., Fynbo, J. P. U., Guaita, L., Marchi, F., Mascia, S., McLure, R., Mignoli, M., Pompei, E., Vanzella, E., Bongiorno, A., Vietri, G., Amorín, R. O., Bolzonella, M., Carnall, A. C., Cimatti, A., Cresci, G., Cristiani, S., Cucciati, O., Dunlop, J. S., Fontanot, F., Franzetti, P., Gargiulo, A., Hamadouche, M. L., Hathi, N. P., Hibon, P., Iovino, A., Koekemoer, A. M., Mannucci, F., McLeod, D. J., Saldana-Lopez, A.
Publikováno v:
A&A 678, A25 (2023)
VANDELS is a deep spectroscopic survey, performed with the VIMOS instrument at VLT, aimed at studying in detail the physical properties of high-redshift galaxies. VANDELS targeted about 2100 sources at 1
Externí odkaz:
http://arxiv.org/abs/2309.14436
Autor:
Llerena, M., Amorín, R., Cullen, F., Pentericci, L., Calabrò, A., McLure, R., Carnall, A., Pérez-Montero, E., Marchi, F., Bongiorno, A., Castellano, M., Fontana, A., McLeod, D. J., Talia, M., Hathi, N. P., Hibon, P., Mannucci, F., Saxena, A., Schaerer, D., Zamorani, G.
Publikováno v:
A&A 659, A16 (2022)
We study the mean properties of a large representative sample of 217 galaxies showing CIII] emission at $2
Externí odkaz:
http://arxiv.org/abs/2107.00660
Autor:
Ferrari, M., Mularoni, F., Taboni, S., Crosetti, E., Pessina, C., Carobbio, A.L.C., Montalto, N., Marchi, F., Vural, A., Paderno, A., Caprioli, S., Gaudioso, P., Fermi, M., Rigoni, F., Saccardo, T., Contro, G., Ruaro, A., Lo Manto, A., Varago, C., Baldovin, M., Bandolin, L., Filauro, M., Sampieri, C., Missale, F., Ioppi, A., Carta, F., Ramanzin, M., Ravanelli, M., Maiolo, V., Bertotto, I., Del Bon, F., Lancini, D., Mariani, C., Marrosu, V., Tatti, M., Cağlı, S., Yüce, I., Gündoğ, M., Dogan, S., Anile, G., Gottardi, C., Busato, F., Vallin, A., Gennarini, F., Bossi, P., Ghi, M.G., Lionello, M., Zanoletti, E., Marioni, G., Maroldi, R., Mattioli, F., Puxeddu, R., Bertolin, A., Presutti, L., Piazza, C., Succo, G., Peretti, G., Nicolai, P.
Publikováno v:
In Oral Oncology May 2024 152
Autor:
Calabrò, A., Castellano, M., Pentericci, L., Fontanot, F., Menci, N., Cullen, F., McLure, R., Bolzonella, M., Cimatti, A., Marchi, F., Talia, M., Amorín, R., Cresci, G., De Lucia, G., Fynbo, J., Fontana, A., Franco, M., Hathi, N. P., Hibon, P., Hirschmann, M., Mannucci, F., Santini, P., Saxena, A., Schaerer, D., Xie, L., Zamorani, G.
Publikováno v:
A&A 646, A39 (2021)
The estimate of stellar metallicities (Z*) of high-z galaxies are of paramount importance in order to understand the complexity of dust effects and the reciprocal interrelations among stellar mass, dust attenuation, stellar age, and metallicity. Bene
Externí odkaz:
http://arxiv.org/abs/2011.06615
Autor:
Thomas, R., Pentericci, L., Fèvre, O. Le, Zamorani, G., Schaerer, D., Amorin, R., Castellano, M., Carnall, A. C., Cristiani, S., Cullen, F., Finkelstein, S. L., Fontanot, F., Guaita, L., Hibon, P., Hathi, N., Fynbo, J. P. U., Khusanova, Y., Koekemoer, A. M., McLeod, D., McLure, R. J., Marchi, F., Pozzetti, L., Saxena, A., Talia, M., Bolzonella, M.
Publikováno v:
A&A 634, A110 (2020)
Aims. Our aim is to estimate the intergalactic medium transmission towards UV-selected star-forming galaxies at redshift 4 and above and study the effect of the dust attenuation on these measurements. Methods. The ultra-violet spectrum of high redshi
Externí odkaz:
http://arxiv.org/abs/1911.12532
Autor:
Saxena, A., Pentericci, L., Mirabelli, M., Schaerer, D., Schneider, R., Cullen, F., Amorin, R., Bolzonella, M., Bongiorno, A., Carnall, A. C., Castellano, M., Cucciati, O., Fontana, A., Fynbo, J. P. U., Garilli, B., Gargiulo, A., Guaita, L., Hathi, N. P., Hutchison, T. A., Koekemoer, A. M., Marchi, F., McLeod, D. J., McLure, R. J., Papovich, C., Pozzetti, L., Talia, M., Zamorani, G.
Publikováno v:
A&A 636, A47 (2020)
Strong He II emission is produced by low-metallicity stellar populations. Here, we aim to identify and study a sample of He II $\lambda 1640$-emitting galaxies at redshifts of $z \sim 2.5-5$ in the deep VANDELS spectroscopic survey.. We identified a
Externí odkaz:
http://arxiv.org/abs/1911.09999
Autor:
Cullen, F., McLure, R. J., Dunlop, J. S., Khochfar, S., Davé, R., Amorin, R., Bolzonella, M., Carnall, A. C., Castellano, M., Cimatti, A., Cirasuolo, M., Cresci, G., Fynbo, J. P. U., Fontanot, F., Gargiulo, A., Garilli, B., Guaita, L., Hathi, N., Hibon, P., Mannucci, F., Marchi, F., McLeod, D. J., Pentericci, L., Pozzetti, L., Shapley, A. E., Talia, M., Zamorani, G.
We present the results of a study utilising ultra-deep, rest-frame UV, spectroscopy to quantify the relationship between stellar mass and stellar metallicity for 681 star-forming galaxies at $2.5
Externí odkaz:
http://arxiv.org/abs/1903.11081
Autor:
Carnall, A. C., McLure, R. J., Dunlop, J. S., Cullen, F., McLeod, D. J., Wild, V., Johnson, B. D., Appleby, S., Davé, R., Amorin, R., Bolzonella, M., Castellano, M., Cimatti, A., Cucciati, O., Gargiulo, A., Garilli, B., Marchi, F., Pentericci, L., Pozzetti, L., Schreiber, C., Talia, M., Zamorani, G.
We present a Bayesian full-spectral-fitting analysis of 75 massive ($M_* > 10^{10.3} M_\odot$) UVJ-selected galaxies at redshifts of $1.0 < z < 1.3$, combining extremely deep rest-frame ultraviolet spectroscopy from VANDELS with multi-wavelength phot
Externí odkaz:
http://arxiv.org/abs/1903.11082
Autor:
Marchi, F., Pentericci, L., Guaita, L., Talia, M., Castellano, M., Hathi, N., Schaerer, D., Amorin, R., Carnall, A. C., Charlot, S., Chevallard, J., Cullen, F., Finkelstein, S. L., Fontana, A., Fontanot, F., Garilli, B., Hibon, P., Koekemoer, A. M., Maccagni, D., McLure, R. J., Papovich, C., Pozzetti, L., Saxena, A.
Publikováno v:
A&A 631, A19 (2019)
We investigate the physical properties of a sample of 52 Ly{\alpha} emitting galaxies in the VANDELS survey, with particular focus on the role of kinematics and neutral hydrogen column density in the escape and spatial distribution of Ly{\alpha} phot
Externí odkaz:
http://arxiv.org/abs/1903.08593
Autor:
Khusanova, Y., Fèvre, O. Le, Cassata, P., Cucciati, O., Lemaux, B. C., Tasca, L. A. M., Thomas, R., Garilli, B., Brun, V. Le, Maccagni, D., Pentericci, L., Zamorani, G., Amorín, R., Bardelli, S., Castellano, M., Cassarà, L. P., Cimatti, A., Giavalisco, M., Hathi, N. P., Ilbert, O., Koekemoer, A. M., Marchi, F., Pforr, J., Ribeiro, B., Schaerer, D., Tresse, L., Vergani, D., Zucca, E.
Publikováno v:
A&A 634, A97 (2020)
We establish a robust statistical description of the star-forming galaxy population at the end of cosmic HI reionization ($5.0\le{}z\le6.6$) from a large sample of 52 galaxies with spectroscopically confirmed redshifts from the VIMOS UltraDeep Survey
Externí odkaz:
http://arxiv.org/abs/1903.01884