Search Results - "Graziani, L."

The assembly of dusty galaxies at z ≥ 4: statistical properties by Graziani, L, Schneider, R, Ginolfi, M, Hunt, L K, Maio, U, Glatzle, M, Ciardi, B

“…ABSTRACT The recent discovery of high-redshift dusty galaxies implies a rapid dust enrichment of their interstellar medium (ISM). To interpret these…”
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Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z > 6.5 Universe by Bouwens, R. J., Smit, R., Schouws, S., Stefanon, M., Bowler, R., Endsley, R., Gonzalez, V., Inami, H., Stark, D., Oesch, P., Hodge, J., Aravena, M., da Cunha, E., Dayal, P., Looze, I. de, Ferrara, A., Fudamoto, Y., Graziani, L., Li, C., Nanayakkara, T., Pallottini, A., Schneider, R., Sommovigo, L., Topping, M., van der Werf, P., Algera, H., Barrufet, L., Hygate, A., Labbé, I., Riechers, D., Witstok, J.

“…Abstract The Reionization Era Bright Emission Line Survey (REBELS) is a cycle-7 ALMA Large Program (LP) that is identifying and performing a first…”
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The ALMA REBELS survey: the dust content of z ∼ 7 Lyman break galaxies by Dayal, P, Ferrara, A, Sommovigo, L, Bouwens, R, Oesch, P A, Smit, R, Gonzalez, V, Schouws, S, Stefanon, M, Kobayashi, C, Bremer, J, Algera, H S B, Aravena, M, Bowler, R A A, da Cunha, E, Fudamoto, Y, Graziani, L, Hodge, J, Inami, H, De Looze, I, Pallottini, A, Riechers, D, Schneider, R, Stark, D, Endsley, R

“…ABSTRACT We include a fully coupled treatment of metal and dust enrichment into the Delphi semi-analytic model of galaxy formation to explain the dust content…”
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The ALMA REBELS Survey: cosmic dust temperature evolution out to z ∼ 7 by Sommovigo, L, Ferrara, A, Pallottini, A, Dayal, P, Bouwens, R J, Smit, R, da Cunha, E, De Looze, I, Bowler, R A A, Hodge, J, Inami, H, Oesch, P, Endsley, R, Gonzalez, V, Schouws, S, Stark, D, Stefanon, M, Aravena, M, Graziani, L, Riechers, D, Schneider, R, van der Werf, P, Algera, H, Barrufet, L, Fudamoto, Y, Hygate, A P S, Labbé, I, Li, Y, Nanayakkara, T, Topping, M

“…ABSTRACT ALMA observations have revealed the presence of dust in the first generations of galaxies in the Universe. However, the dust temperature Td remains…”
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The ALMA REBELS Survey. Epoch of Reionization giants: Properties of dusty galaxies at z ≈ 7 by Ferrara, A, Sommovigo, L, Dayal, P, Pallottini, A, Bouwens, R J, Gonzalez, V, Inami, H, Smit, R, Bowler, R A A, Endsley, R, Oesch, P, Schouws, S, Stark, D, Stefanon, M, Aravena, M, da Cunha, E, De Looze, I, Fudamoto, Y, Graziani, L, Hodge, J, Riechers, D, Schneider, R, Algera, H S B, Barrufet, L, Hygate, A P S, Labbé, I, Li, C, Nanayakkara, T, Topping, M, van der Werf, P

“…ABSTRACT We analyse FIR dust continuum measurements for 14 galaxies (redshift z ≈ 7) in the ALMA Reionization Era Bright Emission Line Survey (REBELS) Large…”
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Full of Orions: a 200-pc mapping of the interstellar medium in the redshift-3 lensed dusty star-forming galaxy SDP.81 by Rybak, Matus, Hodge, J A, Vegetti, S, van der Werf, P, Andreani, P, Graziani, L, McKean, J P

“…ABSTRACT We present a sub-kpc resolved study of the interstellar medium properties in SDP.81, a $z$ = 3.042 strongly gravitationally lensed, dusty star-forming…”
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The ALMA REBELS Survey: The Cosmic H i Gas Mass Density in Galaxies at z ≈ 7 by Heintz, K. E., Oesch, P. A., Aravena, M., Bouwens, R. J., Dayal, P., Ferrara, A., Fudamoto, Y., Graziani, L., Inami, H., Sommovigo, L., Smit, R., Stefanon, M., Topping, M., Pallottini, A., van der Werf, P.

“…Abstract The neutral atomic gas content of individual galaxies at large cosmological distances has until recently been difficult to measure due to the weakness…”
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The assembly of dusty galaxies at z ≥ 4: the build-up of stellar mass and its scaling relations with hints from early JWST data by Di Cesare, C, Graziani, L, Schneider, R, Ginolfi, M, Venditti, A, Santini, P, Hunt, L K

“…ABSTRACT The increasing number of distant galaxies observed with ALMA by the ALPINE and REBELS surveys and the early release observations of the JWST promise…”
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Normal, dust-obscured galaxies in the epoch of reionization by Fudamoto, Y., Oesch, P. A., Schouws, S., Stefanon, M., Smit, R., Bouwens, R. J., Bowler, R. A. A., Endsley, R., Gonzalez, V., Inami, H., Labbe, I., Stark, D., Aravena, M., Barrufet, L., da Cunha, E., Dayal, P., Ferrara, A., Graziani, L., Hodge, J., Hutter, A., Li, Y., De Looze, I., Nanayakkara, T., Pallottini, A., Riechers, D., Schneider, R., Ucci, G., van der Werf, P., White, C.

“…Over the past decades, rest-frame ultraviolet (UV) observations have provided large samples of UV luminous galaxies at redshift ( z ) greater than 6 (refs. 1 –…”
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Where does galactic dust come from? by Ginolfi, M., Graziani, L., Schneider, R., Marassi, S., Valiante, R., Dell'Agli, F., Ventura, P., Hunt, L. K.

“…AbstractHere we investigate the origin of the dust mass (Mdust ) observed in the Milky Way (MW) and of dust scaling relations found in a sample of local…”
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crash3: cosmological radiative transfer through metals by Graziani, L., Maselli, A., Ciardi, B.

“…Here we introduce crash3, the latest release of the 3D radiative transfer code crash. In its current implementation, crash3 integrates into the reference…”
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The history of the dark and luminous side of Milky Way-like progenitors by Graziani, L., de Bennassuti, M., Schneider, R., Kawata, D., Salvadori, S.

“…Abstract Here we investigate the evolution of a Milky Way (MW)-like galaxy with the aim of predicting the properties of its progenitors all the way from z ∼ 20…”
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Cosmic archaeology with massive stellar black hole binaries by Graziani, L, Schneider, R, Marassi, S, Del Pozzo, W, Mapelli, M, Giacobbo, N

“…ABSTRACT The existence of massive stellar black hole binaries (MBHBs), with primary black hole masses $\ge 31 \, \mathrm{ M}_\odot$, was proven by the…”
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Evolution of dwarf galaxies hosting GW150914-like events by Marassi, S, Graziani, L, Ginolfi, M, Schneider, R, Mapelli, M, Spera, M, Alparone, M

“…ABSTRACT Here we present a detailed analysis of the properties and evolution of different dwarf galaxies, candidates to host the coalescence of black hole…”
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Detection of companion galaxies around hot dust-obscured hyper-luminous galaxy W0410-0913 by Ginolfi, M., Piconcelli, E., Zappacosta, L., Jones, G. C., Pentericci, L., Maiolino, R., Travascio, A., Menci, N., Carniani, S., Rizzo, F., Arrigoni Battaia, F., Cantalupo, S., De Breuck, C., Graziani, L., Knudsen, K., Laursen, P., Mainieri, V., Schneider, R., Stanley, F., Valiante, R., Verhamme, A.

“…The phase transition between galaxies and quasars is often identified with the rare population of hyper-luminous, hot dust-obscured galaxies. Galaxy formation…”
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The effect of intergalactic helium on hydrogen reionization: implications for the sources of ionizing photons at z>6 by Ciardi, B., Bolton, J. S., Maselli, A., Graziani, L.

“…We investigate the effect of primordial helium on hydrogen reionization using a hydrodynamical simulation combined with the cosmological radiative transfer…”
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Galaxy formation with radiative and chemical feedback by Graziani, L, Salvadori, S, Schneider, R, Kawata, D, de Bennassuti, M, Maselli, A

“…Here we introduce GAMESH, a novel pipeline that implements self-consistent radiative and chemical feedback in a computational model of galaxy formation. By…”
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The ALMA REBELS Survey: the first infrared luminosity function measurement at z  ∼ 7 by Barrufet, L, Oesch, P A, Bouwens, R, Inami, H, Sommovigo, L, Algera, H, da Cunha, E, Aravena, M, Dayal, P, Ferrara, A, Fudamoto, Y, Gonzalez, V, Graziani, L, Hygate, A P S, de Looze, I, Nanayakkara, T, Pallottini, A, Schneider, R, Stefanon, M, Topping, M, van der Werf, P

“…ABSTRACT We present the first observational infrared luminosity function (IRLF) measurement in the Epoch of Reionization (EoR) based on a ultraviolet…”
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The infrared-luminous progenitors of high- z quasars by Ginolfi, M, Schneider, R, Valiante, R, Pezzulli, E, Graziani, L, Fujimoto, S, Maiolino, R

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The ALMA REBELS Survey: Average [C ii] 158 μm Sizes of Star-forming Galaxies from z ∼ 7 to z ∼ 4 by Fudamoto, Y., Smit, R., Bowler, R. A. A., Oesch, P. A., Bouwens, R., Stefanon, M., Inami, H., Endsley, R., Gonzalez, V., Schouws, S., Stark, D., Algera, H. S. B., Aravena, M., Barrufet, L., da Cunha, E., Dayal, P., Ferrara, A., Graziani, L., Hodge, J. A., Hygate, A. P. S., Inoue, A. K., Nanayakkara, T., Pallottini, A., Pizzati, E., Schneider, R., Sommovigo, L., Sugahara, Y., Topping, M., van der Werf, P., Bethermin, M., Cassata, P., Dessauges-Zavadsky, M., Ibar, E., Faisst, A. L., Fujimoto, S., Ginolfi, M., Hathi, N., Jones, G. C., Pozzi, F., Schaerer, D.

“…Abstract We present the average [C ii ] 158 μ m emission line sizes of UV-bright star-forming galaxies at z ∼ 7. Our results are derived from a stacking…”
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