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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…
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…
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…
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…
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…
AGN in Dusty Starbursts at Z=2: Feedback Still To Kick In
G. Rodighiero, A. Enia, I. Delvecchio +18
We investigate a sample of 152 dusty sources at 1:5 < z < 2:5 to understand the connection of enhanced Star-Formation-Rate (SFR) and Black-Hole-Accretion-Rate (BHAR). The sources a…