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Virgo Filaments: III. The gas content of galaxies in filaments as predicted by the GAEA semi-analytic model.
Published in:
Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202450825
By:
- Zakharova, D.;
- Vulcani, B.;
- De Lucia, G.;
- Finn, R. A.;
- Rudnick, G.;
- Combes, F.;
- Castignani, G.;
- Fontanot, F.;
- Jablonka, P.;
- Xie, L.;
- Hirschmann, M.
Publication type:
Article
Dynamical signature of a stellar bulge in a quasar-host galaxy at z ≃ 6.
Published in:
Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 671, p. 1, doi. 10.1051/0004-6361/202245202
By:
- Tripodi, R.;
- Lelli, F.;
- Feruglio, C.;
- Fiore, F.;
- Fontanot, F.;
- Bischetti, M.;
- Maiolino, R.
Publication type:
Article
The VANDELS survey: the role of ISM and galaxy physical properties in the escape of Lyα emission in z ∼ 3.5 star-forming galaxies.
Published in:
Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 631, p. 1, doi. 10.1051/0004-6361/201935495
By:
- Marchi, F.;
- Pentericci, L.;
- Guaita, L.;
- Talia, M.;
- Castellano, M.;
- Hathi, N.;
- Schaerer, D.;
- Amorin, R.;
- Bolzonella, M.;
- 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.
Publication type:
Article
The contribution of faint AGNs to the ionizing background at z ~4.
Published in:
Astronomy & Astrophysics / Astronomie et Astrophysique, 2018, v. 613, p. 1, doi. 10.1051/0004-6361/201732385
By:
- Grazian, A.;
- Giallongo, E.;
- Boutsia, K.;
- Cristiani, S.;
- Vanzella, E.;
- Scarlata, C.;
- Santini, P.;
- Pentericci, L.;
- Merlin, E.;
- Menci, N.;
- Fontanot, F.;
- Fontana, A.;
- Fiore, F.;
- Civano, F.;
- Castellano, M.;
- Brusa, M.;
- Bonchi, A.;
- Carini, R.;
- Cusano, F.;
- Faccini, M.
Publication type:
Article
Tracing the Evolution of Dust Obscured Star Formation and Accretion Back to the Reionisation Epoch with SPICA.
Published in:
Publications of the Astronomical Society of Australia, 2017, v. 34, p. 1, doi. 10.1017/pasa.2017.49
By:
- Gruppioni, C.;
- Ciesla, L.;
- Hatziminaoglou, E.;
- Pozzi, F.;
- Rodighiero, G.;
- Santini, P.;
- Armus, L.;
- Baes, M.;
- Braine, J.;
- Charmandaris, V.;
- Clements, D. L.;
- Christopher, N.;
- Dannerbauer, H.;
- Efstathiou, A.;
- Egami, E.;
- Fernández-Ontiveros, J. A.;
- Fontanot, F.;
- Franceschini, A.;
- González-Alfonso, E.;
- Griffin, M.
Publication type:
Article
The evolving slope of the stellar mass function at 0.6 ≤ z < 4.5 from deep WFC3 data.
Published in:
Astronomy & Astrophysics / Astronomie et Astrophysique, 2012, v. 538, p. 1, doi. 10.1051/0004-6361/201117513
By:
- Santini, P.;
- Fontana, A.;
- Grazian, A.;
- Salimbeni, S.;
- Fontanot, F.;
- Paris, D.;
- Boutsia, K.;
- Castellano, M.;
- Fiore, F.;
- Gallozzi, S.;
- Giallongo, E.;
- Koekemoer, A. M.;
- Menci, N.;
- Pentericci, L.;
- Somerville, R. S.
Publication type:
Article

Found: 6

Virgo Filaments: III. The gas content of galaxies in filaments as predicted by the GAEA semi-analytic model.

Dynamical signature of a stellar bulge in a quasar-host galaxy at z ≃ 6.

The VANDELS survey: the role of ISM and galaxy physical properties in the escape of Lyα emission in z ∼ 3.5 star-forming galaxies.

The contribution of faint AGNs to the ionizing background at z ~4.

Tracing the Evolution of Dust Obscured Star Formation and Accretion Back to the Reionisation Epoch with SPICA.

The evolving slope of the stellar mass function at 0.6 ≤ z < 4.5 from deep WFC3 data.