66 citations · 214 across the 7 of their papers we have counts for
16 papers
Being KLEVER at cosmic noon: ionised gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts
Alice Concas, Roberto Maiolino, Mirko Curti +13
We investigate the presence of ionised gas outflows in a sample of 141 main-sequence star-forming galaxies at from the KLEVER (KMOS Lensed Emission Lines and VElocity R…
The ALPINE-ALMA [CII] Survey: the population of [CII]-undetected galaxies and their role in the -SFR relation
Michael Romano, L. Morselli, P. Cassata +22
The [CII] 158m emission line represents so far one of the most profitable tools for the investigation of the high-redshift galaxies in the early Universe. Being one of the brig…
What drives galaxy quenching? A deep connection between galaxy kinematics and quenching in the local Universe
Simcha Brownson, Asa F. L. Bluck, Roberto Maiolino +1
We develop a 2D inclined rotating disc model, which we apply to the stellar velocity maps of 1862 galaxies taken from the MaNGA survey (SDSS public Data Release 15). We use a rando…
Kinematics and Star Formation of High-Redshift Hot Dust-Obscured Quasars as Seen by ALMA
Tanio Diaz-Santos, Roberto J. Assef, Peter R. M. Eisenhardt +9
Hot, dust-obscured galaxies (Hot DOGs) are a population of hyper-luminous obscured quasars identified by WISE. We present ALMA observations of the [CII] fine-structure line and und…
Resolving Disks & Mergers in Heavily Reddened Quasars and their Companion Galaxies with ALMA
Manda Banerji, Gareth C. Jones, Stefano Carniani +2
We present sub-arcsecond resolution ALMA imaging of the CO(3-2) emission in two heavily reddened quasars (HRQs) - ULASJ1234+0907 and ULASJ2315+0143 - and their companion…
Gas and Star Formation from HD and Dust Emission in a Strongly Lensed Galaxy
Gareth C. Jones, Roberto Maiolino, Paola Caselli +1
The molecular gas content of high-redshift galaxies is a highly sought-after property. However, H is not directly observable in most environments, so its mass is probed through…