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20122026
most citedThe ALPINE-ALMA [CII] Survey: data processing, catalogs, and statistical source properties

245 citations · 5.8k across the 91 of their papers we have counts for

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Showing 2019Show all

12 papers · 1 filter

astro-ph.GA2019★ 159 cited

The ALPINE-ALMA [CII] Survey: Multi-Wavelength Ancillary Data and Basic Physical Measurements

A. L. Faisst, D. Schaerer, B. C. Lemaux +37

We present the ancillary data and basic physical measurements for the galaxies in the ALMA Large Program to Investigate C+ at Early Times (ALPINE) survey - the first large multi-wa…

astro-ph.GA2019★ 170 cited

The ALPINE-ALMA [CII] survey: Star-formation-driven outflows and circumgalactic enrichment in the early Universe

M. Ginolfi, G. C. Jones, M. Bethermin +29

We study the efficiency of galactic feedback in the early Universe by stacking the [C II] 158 um emission in a large sample of normal star-forming galaxies at 4 < z < 6 from the AL…

astro-ph.GA2019★ 45 cited

Impact of X-rays on CO emission from high-z galaxies

L. Vallini, A. G. G. M. Tielens, A. Pallottini +5

We study the impact of active galactic nuclei (AGN) on the CO Spectral Line Energy Distribution (SLED) of high- galaxies. In particular, we want to assess if the CO SLED can be…

astro-ph.GA2019★ 188 cited

Large Population of ALMA Galaxies at z>6 with Very High [OIII]88um to [CII]158um Flux Ratios: Evidence of Extremely High Ionization Parameter or PDR Deficit?

Yuichi Harikane, Masami Ouchi, Akio K. Inoue +20

We present our new ALMA observations targeting [OIII]88um, [CII]158um, [NII]122um, and dust continuum emission for three Lyman break galaxies at z=6.0293-6.2037 identified in the S…

astro-ph.GA2019★ 42 cited

The ALPINE-ALMA [CII] Survey: A Triple Merger at z~4.56

G. C. Jones, M. Bethermin, Y. Fudamoto +29

We report the detection of [CII]158um emission from a system of three closely-separated sources in the COSMOS field at z~4.56, as part of the ALMA Large Program to INvestigate CII…

astro-ph.GA2019★ 109 cited

A physical model for [CII] line emission from galaxies

A. Ferrara, L. Vallini, A. Pallottini +5

A tight relation between the [CII]158m line luminosity and star formation rate is measured in local galaxies. At high redshift (), though, a much larger scatter is observed…

astro-ph.GA2019★ 110 cited

Kinematics of galaxies from [CII] line emission

M. Kohandel, A. Pallottini, A. Ferrara +5

We study the kinematical properties of galaxies in the Epoch of Reionization via the [CII] 158m line emission. The line profile provides information on the kinematics as well as…

astro-ph.GA2019★ 144 cited

Deep into the structure of the first galaxies: SERRA views

A. Pallottini, A. Ferrara, D Decataldo +6

We study the formation and evolution of a sample of Lyman Break Galaxies in the Epoch of Reionization by using high-resolution (), cosmological zoom-in simulati…

astro-ph.GA2019★ 44 cited

Photoevaporation of Jeans-unstable molecular clumps

D. Decataldo, A. Pallottini, A. Ferrara +2

We study the photoevaporation of Jeans-unstable molecular clumps by isotropic FUV (6 eV < 13.6 eV) radiation, through 3D radiative transfer hydrodynamical simulations…

astro-ph.GA2019★ 93 cited

Resolved UV and [CII] structures of luminous galaxies within the epoch of reionisation

J. Matthee, D. Sobral, L. A. Boogaard +7

We present new deep ALMA and HST/WFC3 observations of MASOSA and VR7, two luminous Ly emitters (LAEs) at , for which the UV continuum level differ by a factor four. No IR…

astro-ph.GA2019★ 38 cited

Lyα emission from galaxies in the Epoch of Reionization

Christoph Behrens, Andrea Pallottini, Andrea Ferrara +2

The intrinsic strength of the Ly line in young, star-forming systems makes it a special tool for studying high-redshift galaxies. However, interpreting observations remains chal…

astro-ph.GA2019★ 35 cited

Constraints on high-J CO emission lines in quasars

S. Carniani, S. Gallerani, L. Vallini +10

We present Atacama Large Millimiter/submillimiter Array (ALMA) observations of eight highly excited CO (J) lines and continuum emission in two quasars: SDSS J…