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20152022
most citedThe ALPINE-ALMA [CII] Survey: data processing, catalogs, and statistical source properties

245 citations · 1.6k across the 18 of their papers we have counts for

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18 papers · 1 filter

astro-ph.GA2022★ 15 cited

The ALPINE-ALMA [CII] Survey: Investigation of 10 Galaxies at with [OII] and [CII] Line Emission ISM Properties and [OII]SFR Relation

Brittany N. Vanderhoof, A. L. Faisst, L. Shen +23

We present main-sequence ALPINE galaxies (log() = 9.2-11.1 and ) at with optical [OII] measurements from Ke…

astro-ph.GA2021★ 33 cited

A High-Resolution Investigation of the Multi-Phase ISM in a Galaxy during the First Two Billion Years

S. Dye, S. A. Eales, H. L. Gomez +20

We have carried out the first spatially-resolved investigation of the multi-phase interstellar medium (ISM) at high redshift, using the z=4.24 strongly-lensed sub-millimetre galaxy…

astro-ph.GA2021★ 59 cited

The ALPINE-ALMA [CII] survey: The contribution of major mergers to the galaxy mass assembly at z~5

M. Romano, P. Cassata, L. Morselli +25

Galaxy mergers are thought to be one of the main mechanisms of the mass assembly of galaxies. Recently, many works have suggested a possible increase in the fraction of major merge…

astro-ph.GA2021★ 43 cited

The ALPINE-ALMA [CII] survey: Dust mass budget in the early Universe

F. Pozzi, F. Calura, Y. Fudamoto +32

The dust content of normal galaxies and the dust mass density (DMD) at high-z (z>4) are unconstrained given the source confusion and the sensitivity limitations of previous observa…

astro-ph.GA2021★ 80 cited

The ALPINE-ALMA [CII] Survey: Kinematic Diversity & Rotation in Massive Star Forming Galaxies at z~4.4-5.9

G. C. Jones, D. Vergani, M. Romano +21

While the kinematics of galaxies up to z~3 have been characterized in detail, only a handful of galaxies at high redshift (z>4) have been examined in such a way. The Atacama Large…

astro-ph.GA2020★ 200 cited

The ALPINE-ALMA [CII] Survey: The nature, luminosity function and star formation history of dusty galaxies up to z~6

C. Gruppioni, M. Bethermin, F. Loiacono +30

We present the detailed characterisation of a sample of 56 sources serendipitously detected in ALMA band 7, as part of the ALMA Large Program to INvestigate CII at Early Times (ALP…

astro-ph.GA2020★ 122 cited

The ALPINE-ALMA [CII] survey: Molecular gas budget in the Early Universe as traced by [CII]

M. Dessauges-Zavadsky, M. Ginolfi, F. Pozzi +32

The molecular gas content of normal galaxies at z>4 is poorly constrained, because the commonly used molecular gas tracers become hard to detect. We use the [CII]158um luminosity,…

astro-ph.GA2020★ 28 cited

The ALPINE-ALMA [CII] Survey: On the nature of an extremely obscured serendipitous galaxy

Michael Romano, P. Cassata, L. Morselli +31

We report the serendipitous discovery of a bright galaxy (Gal-A) observed as part of the ALMA Large Program to INvestigate [CII] at Early times (ALPINE). While this galaxy is detec…

astro-ph.GA2020★ 173 cited

The ALPINE-ALMA [CII] survey. Little to no evolution in the [CII]-SFR relation over the last 13 Gyr

D. Schaerer, M. Ginolfi, M. Bethermin +34

The [CII] 158 micron line is one of the strongest IR emission lines, which has been shown to trace the star-formation rate (SFR) of galaxies in the nearby Universe and up to $z \si…

astro-ph.GA2020★ 245 cited

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

M. Bethermin, Y. Fudamoto, M. Ginolfi +33

The ALPINE-ALMA large program targets the [CII] 158 m line and the far-infrared continuum in 118 spectroscopically confirmed star-forming galaxies between z=4.4 and z=5.9. It re…

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★ 27 cited

Detection of a high-redshift molecular outflow in a primeval hyperstarburst galaxy

G. C. Jones, R. Maiolino, P. Caselli +1

We report the discovery of a high-redshift, massive molecular outflow in the starburst galaxy SPT0346-52 () via the detected absorption of high-excitation water transition…

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★ 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.GA2018★ 83 cited

Starburst to quiescent from HST/ALMA: Stars and dust unveil minor mergers in submillimeter galaxies at

C. Gómez-Guijarro, S. Toft, A. Karim +32

Dust-enshrouded, starbursting, submillimeter galaxies (SMGs) at have been proposed as progenitors of compact quiescent galaxies (cQGs). To test this connectio…

astro-ph.GA2017★ 17 cited

Molecular gas in AzTEC/C159: a star-forming disk galaxy 1.3Gyr after the Big Bang

E. F. Jiménez-Andrade, B. Magnelli, A. Karim +23

We studied the molecular gas properties of AzTEC/C159, a star-forming disk galaxy at . We secured CO molecular line detections for the and trans…

astro-ph.GA2017★ 30 cited

Galaxy Formation Through Filamentary Accretion at z=6.1

G. C. Jones, C. J. Willott, C. L. Carilli +3

We present ALMA observations of the dust continuum and [C II] 158um line emission from the z=6.0695 Lyman Break Galaxy WMH5. These observations at 0.3" spatial resolution show a co…

astro-ph.GA2015★ 99 cited

ALMA constraints on the faint millimetre source number counts and their contribution to the cosmic infrared background

S. Carniani, R. Maiolino, G. De Zotti +20

We have analysed 18 ALMA continuum maps in Bands 6 and 7, with rms down to 7.8Jy, to derive differential number counts down to 60Jy and 100Jy at 1.3 mm and 1.1 mm,…