867 citations · 13.7k across the 180 of their papers we have counts for
10 papers · 2 filters
The ALPINE-ALMA [CII] survey: double stellar population and AGN activity in a galaxy at
L. Barchiesi, M. Dessauges-Zavadsky, C. Vignali +16
GDS J033218.92-275302.7 (here GS-14) is a galaxy detected in [CII] as part of the ALPINE survey with unusual UV spectral features that have been interpreted as signature…
The resolved scaling relations in DustPedia: Zooming in on the local Universe
Viviana Casasola, Simone Bianchi, Laura Magrini +18
We perform a homogeneous analysis of an unprecedented set of spatially resolved scaling relations (SRs) between ISM components and other properties in the range of scales 0.3-3.4 k…
Spritz is sparkling: simulated CO and [CII] luminosities
L. Bisigello, L. Vallini, C. Gruppioni +6
We present a new prediction of the luminosity functions of the [CII] line at 158 m, of the CO lines from J=0 to J=24, and of the molecular gas mass density up to z=10, using the…
Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium
R. Gilli, C. Norman, F. Calura +12
We combine results from deep ALMA observations of massive () galaxies at different redshifts to show that the column density of their inter stellar medium (…
Compton-Thick AGN in the NuSTAR era VIII: A joint NuSTAR-XMM-Newton monitoring of the changing-look Compton-thick AGN NGC 1358
Stefano Marchesi, Xiurui Zhao, Núria Torres-Albà +18
We present the multi-epoch monitoring with NuSTAR and XMM-Newton of NGC 1358, a nearby Seyfert 2 galaxy whose properties made it a promising candidate X-ray changing look AGN, i.e.…
The ALMA REBELS Survey: Average [CII] sizes of Star-Forming Galaxies from to
Y. Fudamoto, R. Smit, R. A. A. Bowler +36
We present the average [CII] emission line sizes of UV-bright star-forming galaxies at . Our results are derived from a stacking analysis of [CII] $158\,\rm{…
ALPINE: A Large Survey to Understand Teenage Galaxies
A. L. Faisst, L. Yan, M. Béthermin +13
A multiwavelength study of galaxies is important to understand their formation and evolution. Only in the recent past, thanks to the Atacama Large (Sub) Millimeter Array (ALMA), we…
The molecular gas properties in local Seyfert 2 galaxies
F. Salvestrini, C. Gruppioni, E. Hatziminaoglou +8
We present a multi-wavelength study of the molecular gas properties of a sample of local Seyfert 2 galaxies to assess if, and to what extent, the presence of an active galactic nuc…
IR characteristic emission and dust properties of star-forming galaxies at 4.5 z 6.2
D. Burgarella, J. Bogdanoska, A. Nanni +31
The luminosity functions at z < 4 - 5 suggest that most galaxies have a relatively low stellar mass (logM_star = 10) and a low dust attenuation (A_FUV = 1.0). The physical properti…
AGN impact on the molecular gas in galactic centers as probed by CO lines
Federico Esposito, Livia Vallini, Francesca Pozzi +5
We present a detailed analysis of the X-ray, infrared, and carbon monoxide (CO) emission for a sample of 35 local (), active ( erg s) galaxies…