Zobrazeno 1 - 10
of 255
pro vyhledávání: '"Parlanti E."'
Autor:
Marconcini, C., D'Eugenio, F., Maiolino, R., Arribas, S., Bunker, A., Carniani, S., Charlot, S., Perna, M., Del Pino, B. Rodríguez, Übler, H., Pérez-González, P. G., Willott, C. J., Böker, T., Cresci, G., Curti, M., Lamperti, I., Scholtz, J., Parlanti, E., Venturi, G.
We present JWST/NIRSpec integral field spectroscopic (IFS) observations of the \Lyalpha emitter CR7 at z ~ 6.6, observed as part of the GA-NIFS program. Using low-resolution PRISM (R ~ 100) data, we confirm a bright \Lyalpha emitter, and a diffuse \L
Externí odkaz:
http://arxiv.org/abs/2411.08627
Autor:
Scholtz, J., Curti, M., D'Eugenio, F., Übler, H., Maiolino, R., Marconcini, C., Smit, R., Perna, M., Witstok, J., Arribas, S., Böker, T., Bunker, A. J., Carniani, S., Charlot, S., Cresci, G., Pérez-González, P. G., Lamperti, I., Del Pino, B. Rodríguez, Parlanti, E., Venturi, G.
We present deep JWST/NIRSpec integral-field spectroscopy (IFS) and ALMA [CII]$\lambda$158$\mu$m observations of COS-3018, a star-forming galaxy at z$\sim$6.85, as part of the GA-NIFS programme. Both G395H (R$\sim$ 2700) and PRISM (R$\sim$ 100) NIRSpe
Externí odkaz:
http://arxiv.org/abs/2411.07695
Autor:
Venturi, G., Carniani, S., Parlanti, E., Kohandel, M., Curti, M., Pallottini, A., Vallini, L., Arribas, S., Bunker, A. J., Cameron, A. J., Castellano, M., Ferrara, A., Fontana, A., Gallerani, S., Gelli, V., Maiolino, R., Ntormousi, E., Pacifici, C., Pentericci, L., Salvadori, S., Vanzella, E.
Publikováno v:
A&A 691, A19 (2024)
The study of gas-phase metallicity and its spatial distribution at high redshift is crucial to understand the processes that shaped the growth and evolution of galaxies in the early Universe. Here we study the spatially resolved metallicity in three
Externí odkaz:
http://arxiv.org/abs/2403.03977
Autor:
Markov, V., Gallerani, S., Ferrara, A., Pallottini, A., Parlanti, E., Di Mascia, F., Sommovigo, L., Kohandel, M.
A sizable fraction of the heavy elements synthesized by stars in galaxies condenses into sub-micron-sized solid-state particles, known as dust grains. Dust produces a wavelength-dependent attenuation, $A_\lambda$, of the galaxy emission, thereby sign
Externí odkaz:
http://arxiv.org/abs/2402.05996
Autor:
Del Pino, B. Rodríguez, Perna, M., Arribas, S., D'Eugenio, F., Lamperti, I., Pérez-González, P. G., Übler, H., Bunker, A., Carniani, S., Charlot, S., Maiolino, R., Willott, C. J., Böker, T., Chevallard, J., Cresci, G., Curti, M., Jones, G. C., Parlanti, E., Scholtz, J., Venturi, G.
We present NIRSpec IFS observations of a galaxy group around the massive GS_4891 galaxy at z=3.7 in GOODS-South that includes two other two systems, GS_4891_n to the north and GS_28356 to the east. These observations, obtained as part of the GTO GA-N
Externí odkaz:
http://arxiv.org/abs/2309.14431
Autor:
Markov, V., Gallerani, S., Pallottini, A., Sommovigo, L., Carniani, S., Ferrara, A., Parlanti, E., Di Mascia, F.
Publikováno v:
A&A 679, A12 (2023)
Attenuation curves in galaxies depend on dust chemical composition, content, and grain size distribution. Such parameters are related to intrinsic galaxy properties such as metallicity, star formation rate, and stellar age. Due to the lack of observa
Externí odkaz:
http://arxiv.org/abs/2304.11178
Autor:
Parlanti, E., Carniani, S., Pallottini, A., Cignoni, M., Cresci, G., Kohandel, M., Mannucci, F., Marconi, A.
High-redshift galaxies are expected to be more turbulent than local galaxies because of their smaller size and higher star formation and thus stronger feedback from star formation, frequent mergers events, and gravitational instabilities. However, th
Externí odkaz:
http://arxiv.org/abs/2304.00036
Autor:
Morelle, J., Huguet, A., Richard, A., Laverman, A.M., Roose-Amsaleg, C., Parlanti, E., Sourzac, M., Mesnage, V., Lecoq, N., Deloffre, J., Viollier, E., Maire, O., Orvain, F.
Publikováno v:
In Journal of Experimental Marine Biology and Ecology April 2024 573
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Akademický článek
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