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20002026
most citedThe lesser role of starbursts for star formation at z=2

867 citations · 13.7k across the 180 of their papers we have counts for

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Showing 2019Show all

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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★ 36 cited

The dust mass function from z~0 to z~2

F. Pozzi, F. Calura, G. Zamorani +3

We derive for the first time the dust mass function (DMF) in a wide redshift range, from z~0.2 up to z~2.5. In order to trace the dust emission, we start from a far-IR (160-um) Her…

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★ 15 cited

Broad-band X-ray analysis of local mid-infrared selected Compton-thick AGN candidates

M. -M. La Caria, C. Vignali, G. Lanzuisi +2

The estimate of the number and space density of obscured AGN over cosmic time still represents an open issue. While the obscured AGN population is a key ingredient of the X-ray bac…