350 citations · 1.8k across the 33 of their papers we have counts for
33 papers
CHAMPS: The COSMOS High-Redshift ALMA-MIRI Population Survey - A New Census of the Dusty Early Universe
Andreas L. Faisst, Felix Martinez, Jeyhan S. Kartaltepe +86
Understanding how dust forms and evolves over cosmic time is a key open problem in extragalactic astrophysics. Galaxies in the early Universe were once thought to be mostly dust-po…
Noema formIng Cluster survEy (NICE): A Census of Star Formation and Cold Gas Properties in Massive protoclusters at 1.5<z<4
Luwenjia Zhou, Tao Wang, Emanuele Daddi +36
Massive protoclusters at z~1.5-4, the peak of the cosmic star formation history, are key to understanding the formation mechanisms of massive galaxies in today's clusters. However,…
Revealing the hidden cosmic feast: A z=4.3 galaxy group hosting two optically dark, efficiently star-forming galaxies
Malte Brinch, Shuowen Jin, Raphael Gobat +11
We present the confirmation of a compact galaxy group candidate, CGG-z4, at in the COSMOS field. This structure was identified by two spectroscopically confirmed $K…
The Cosmic Evolution Early Release Science Survey (CEERS)
Steven L. Finkelstein, Micaela B. Bagley, Pablo Arrabal Haro +96
We present the Cosmic Evolution Early Release Science (CEERS) Survey, a 77.2 hour Director's Discretionary Early Release Science Program. CEERS demonstrates, tests, and validates e…
Behind the dust veil: A panchromatic view of an optically dark galaxy at z=4.82
Nikolaj B. Sillassen, Shuowen Jin, Georgios E. Magdis +30
Optically dark dusty star-forming galaxies (DSFGs) play an essential role in massive galaxy formation at early cosmic time, however their nature remains elusive. Here we present a…
Size - Stellar Mass Relation and Morphology of Quiescent Galaxies at in Public Fields
Kei Ito, Francesco Valentino, Gabriel Brammer +19
We present the results of a systematic study of the rest-frame optical morphology of quiescent galaxies at using the Near-Infrared Camera (NIRCam) onboard . Based…
The IR Compactness of Dusty Galaxies Set Star-formation and Dust Properties at z~0-2
Jed McKinney, Alexandra Pope, Allison Kirkpatrick +9
Surface densities of gas, dust and stars provide a window into the physics of star-formation that, until the advent of high-resolution far-infrared/sub-millimeter observations, has…
Extremely red galaxies at with MIRI and NIRSpec: dusty galaxies or obscured AGNs?
Guillermo Barro, Pablo G. Perez-Gonzalez, Dale D. Kocevski +27
We study a new population of extremely red objects (EROs) recently discovered by JWST based on their NIRCam colors F277WF444W mag. We find 37 EROs in the CEERS field with…
Insight Into a Lensed -dark Galaxy and its Quiescent Companion at
Vasily Kokorev, Shuowen Jin, Georgios E. Magdis +13
Using the novel /NIRCam observations in the Abell 2744 field, we present a first spatially resolved overview of an -dark galaxy, spectroscopically confirmed at …
An Atlas of Color-selected Quiescent Galaxies at in Public Fields
Francesco Valentino, Gabriel Brammer, Katriona M. L. Gould +24
We present the results of a systematic search for candidate quiescent galaxies in the distant Universe in eleven fields with publicly available observations collected during…
A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS Imaging
Steven L. Finkelstein, Micaela B. Bagley, Pablo Arrabal Haro +117
We report the discovery of a candidate galaxy with a photo-z of z~12 in the first epoch of the JWST Cosmic Evolution Early Release Science (CEERS) Survey. Following conservative se…
Starbursts with suppressed velocity dispersion revealed in a forming cluster at z=2.51
Mengyuan Xiao, Tao Wang, David Elbaz +19
One of the most prominent features of galaxy clusters is the presence of a dominant population of massive ellipticals in their cores. Stellar archaeology suggests that these gigant…
The bending of the star-forming main sequence traces the cold- to hot-accretion transition mass over 0<z<4
E. Daddi, I. Delvecchio, P. Dimauro +8
We analyse measurements of the evolving stellar mass (M0) at which the bending of the star-forming main sequence (MS) occurs over 0<z<4. We find M0~10^10Msun over 0<z<1, then M0 ri…
The Evolving Interstellar Medium of Star-Forming Galaxies, as traced by
Vasily Kokorev, Georgios Magdis, Iary Davidzon +13
We analyse the far-infrared properties of 5,000 star-forming galaxies at , drawn from the deepest, super-deblended catalogues in the GOODS-N and COSMOS fields. We dev…
The effect of active galactic nuclei on the cold interstellar medium in distant star-forming galaxies
Francesco Valentino, Emanuele Daddi, Annagrazia Puglisi +17
In the framework of a systematic ALMA study of IR-selected main-sequence and starburst galaxies at z~1-1.7 at typical ~1" resolution, we report on the effects of mid-IR- and X-ray-…
An ancient massive quiescent galaxy found in a gas-rich z ~ 3 group
Boris S. Kalita, Emanuele Daddi, Chiara D'Eugenio +9
Deep ALMA and HST observations reveal the presence of a quenched massive galaxy within the galaxy group RO-1001. With a mass-weighted stellar age of Gyr th…
Sub-millimetre compactness as a critical dimension to understand the Main Sequence of star-forming galaxies
Annagrazia Puglisi, Emanuele Daddi, Francesco Valentino +11
We study the interstellar medium (ISM) properties as a function of the molecular gas size for 77 infrared-selected galaxies at . Molecular gas sizes are measured on ALM…
Feedback Factory: Multiple faint radio-jets detected in a cluster at z=2
Boris S. Kalita, Emanuele Daddi, Rosemary T. Coogan +8
We report the detection of multiple faint radio sources, that we identify as AGN-jets, within CLJ1449+0856 at z=2 using 3 GHz VLA observations. We study the effects of radio-jet ba…
The Fundamental Plane of Massive Quiescent Galaxies at z~2
Mikkel Stockmann, Inger Jørgensen, Sune Toft +11
We examine the Fundamental Plane (FP) and mass-to-light ratio () scaling relations using the largest sample of massive quiescent galaxies at to date. The FP ($r_{e…
Fast rotating and low-turbulence discs at : Dynamical evidence of their evolution into local early-type galaxies
F. Fraternali, A. Karim, B. Magnelli +3
Massive starburst galaxies in the early Universe are estimated to have depletion times of Myr and thus be able to convert their gas very quickly into stars, possibly lea…
Knocking on giants' doors: I. The evolution of the dust-to-stellar mass ratio in distant dusty galaxies
D. Donevski, A. Lapi, K. Małek +11
The dust-to-stellar mass ratio (/) is a crucial yet poorly constrained quantity to understand the production mechanisms of dust, metals and stars in ga…
CO emission in distant galaxies on and above the main sequence
Francesco Valentino, Emanuele Daddi, Annagrazia Puglisi +17
We present the detection of multiple CO line transitions with ALMA in a few tens of infrared-selected galaxies on and above the main sequence at z=1.1-1.7. We reliably detected the…
How primordial magnetic fields shrink galaxies
Sergio Martin-Alvarez, Adrianne Slyz, Julien Devriendt +1
As one of the prime contributors to the interstellar medium energy budget, magnetic fields naturally play a part in shaping the evolution of galaxies. Galactic magnetic fields can…
The BUFFALO HST Survey
Charles L. Steinhardt, Mathilde Jauzac, Ana Acebron +91
The Beyond Ultra-deep Frontier Fields and Legacy Observations (BUFFALO) is a 101 orbit + 101 parallel Cycle 25 Hubble Space Telescope Treasury program taking data from 2018-2020. B…