[HTML][HTML] From clusters to proto-clusters: the infrared perspective on environmental galaxy evolution
Environment is one of the primary drivers of galaxy evolution; via multiple mechanisms, it
can control the critical process of transforming galaxies from star forming to quiescent …
can control the critical process of transforming galaxies from star forming to quiescent …
The [C ii] emission as a molecular gas mass tracer in galaxies at low and high redshifts
We present ALMA Band 9 observations of the [C ii] 158 m emission for a sample of 10 main-
sequence galaxies at redshift∼ 2, with typical stellar masses (log M⋆/M⊙∼ 10.0–10.9) and …
sequence galaxies at redshift∼ 2, with typical stellar masses (log M⋆/M⊙∼ 10.0–10.9) and …
The properties of the interstellar medium of galaxies across time as traced by the neutral atomic carbon [C i]
The Properties of the Interstellar Medium of Galaxies across Time as Traced by the Neutral
Atomic Carbon [C i] - IOPscience This site uses cookies. By continuing to use this site you …
Atomic Carbon [C i] - IOPscience This site uses cookies. By continuing to use this site you …
Discovery of four apparently cold dusty galaxies at z= 3.62–5.85 in the COSMOS field: direct evidence of cosmic microwave background impact on high-redshift galaxy …
Abstract We report Atacama Large Millimeter Array (ALMA) observations of four high-redshift
dusty star-forming galaxy candidates selected from far-infrared (FIR)/submillimeter …
dusty star-forming galaxy candidates selected from far-infrared (FIR)/submillimeter …
Diagnosing deceivingly cold dusty galaxies at 3.5< z< 6: A substantial population of compact starbursts with high infrared optical depths
Using NOEMA and ALMA 3mm line scans, we measured spectroscopic redshifts of six new
dusty galaxies at 3.5< z< 4.2 by solidly detecting [CI](1-0) and CO transitions. The sample …
dusty galaxies at 3.5< z< 4.2 by solidly detecting [CI](1-0) and CO transitions. The sample …
Three Lyman-α-emitting filaments converging to a massive galaxy group at z= 2.91: discussing the case for cold gas infall
E Daddi, F Valentino, RM Rich, JD Neill… - Astronomy & …, 2021 - aanda.org
We have discovered a 300 kpc-wide giant Lyman-α (Lyα) nebula centered on the massive
galaxy group RO-1001 at z= 2.91 in the Cosmic Evolution Survey field. Keck Cosmic Web …
galaxy group RO-1001 at z= 2.91 in the Cosmic Evolution Survey field. Keck Cosmic Web …
A contribution of star-forming clumps and accreting satellites to the mass assembly of z ∼ 2 galaxies
A Zanella, E Le Floc'h, CM Harrison… - Monthly Notices of …, 2019 - academic.oup.com
We investigate the contribution of clumps and satellites to the galaxy mass assembly. We
analysed spatially resolved HubbleSpace Telescope observations (imaging and slitless …
analysed spatially resolved HubbleSpace Telescope observations (imaging and slitless …
The DIANOGA simulations of galaxy clusters: characterising star formation in protoclusters
L Bassini, E Rasia, S Borgani, GL Granato… - Astronomy & …, 2020 - aanda.org
Aims. We studied the star formation rate (SFR) in cosmological hydrodynamical simulations
of galaxy (proto-) clusters in the redshift range 0< z< 4, comparing them to recent …
of galaxy (proto-) clusters in the redshift range 0< z< 4, comparing them to recent …
A massive quiescent galaxy in a group environment at z= 4.53
T Kakimoto, M Tanaka, M Onodera… - The Astrophysical …, 2024 - iopscience.iop.org
We report on the spectroscopic confirmation of a massive quiescent galaxy at z spec= 4.53
in the COSMOS field. The object was first identified as a galaxy with suppressed star …
in the COSMOS field. The object was first identified as a galaxy with suppressed star …
The X-shooter GRB afterglow legacy sample (XS-GRB)
In this work we present spectra of all γ-ray burst (GRB) afterglows that have been promptly
observed with the X-shooter spectrograph until 31/03/2017. In total, we have obtained …
observed with the X-shooter spectrograph until 31/03/2017. In total, we have obtained …