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20132026
most citedHydrogen reionisation ends by : Lyman- optical depth measured by the XQR-30 sample

302 citations · 6.5k across the 129 of their papers we have counts for

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Showing 2018Show all

7 papers · 1 filter

astro-ph.GA2018★ 13 cited

The interstellar medium of dwarf galaxies: new insights from Machine Learning analysis of emission line spectra

Graziano Ucci, Andrea Ferrara, Simona Gallerani +6

Dwarf galaxies are ideal laboratories to study the physics of the interstellar medium (ISM). Emission lines have been widely used to this aim. Retrieving the full information encod…

astro-ph.GA2018★ 18 cited

Probing the High-Redshift Universe with SPICA: Toward the Epoch of Reionization and Beyond

E. Egami, S. Gallerani, R. Schneider +36

With the recent discovery of a dozen dusty star-forming galaxies and around 30 quasars at z>5 that are hyper-luminous in the infrared ( L, where $μ…

astro-ph.GA2018

Challenges and Techniques for Simulating Line Emission

Karen P. Olsen, Andrea Pallottini, Aida Wofford +9

Modeling emission lines from the millimeter to the UV and producing synthetic spectra is crucial for a good understanding of observations, yet it is an art filled with hazards. Thi…

astro-ph.GA2018★ 54 cited

Witnessing galaxy assembly at the edge of the reionization epoch

V. D'Odorico, C. Feruglio, A. Ferrara +8

We report the discovery of Serenity-18, a galaxy at z=5.939 for which we could measure the content of molecular gas, M(H_2)~ 5 x10^9 M_sun, traced by the CO(6-5) emission, together…

astro-ph.GA2018★ 49 cited

The dense molecular gas in the QSO SDSS J231038.88+185519.7 resolved by ALMA

C. Feruglio, F. Fiore, S. Carniani +13

We present ALMA observations of the CO(6-5) and [CII] emission lines and the sub-millimeter continuum of the quasi-stellar object (QSO) SDSS J231038.88+185519.7. Compared…

astro-ph.GA2018★ 22 cited

GAME: GAlaxy Machine learning for Emission lines

Graziano Ucci, Andrea Ferrara, Andrea Pallottini +1

We present an updated, optimized version of GAME (GAlaxy Machine learning for Emission lines), a code designed to infer key interstellar medium physical properties from emission li…

astro-ph.GA2018★ 131 cited

Dusty galaxies in the Epoch of Reionization: simulations

C. Behrens, A. Pallottini, A. Ferrara +2

The recent discovery of dusty galaxies well into the Epoch of Reionization (redshift ) poses challenging questions about the properties of the interstellar medium in these pri…