98 citations · 165 across the 10 of their papers we have counts for
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A Cosmic Archipelago of lensed metal-poor galaxies at
A. Bolamperti, M. Messa, A. Zanella +21
The Cosmic Archipelago is an ensemble of galaxies, strongly lensed by the cluster MACSJ0416, showing extreme physical properties at . We combine JWST/NIRCam with deep VL…
First Statistical Study of Over 100 Magnified Stellar Events at Redshift with JWST
J. M. Palencia, Fengwu Sun, J. M. Diego +25
Highly magnified stars at cosmological distances () become detectable thanks to microlensing by intracluster stars near the critical curves of galaxy clusters. Multi…
Euclid: Scaled-up little red dots and other sources with v-shaped spectral energy distributions at z>4
Euclid Collaboration, A. A. Tumborang, K. I. Caputi +169
Little Red Dots (LRDs) are some the most intriguing galaxy populations recently identified at z>~4 with JWST. They constitute the most extreme class of a more abundant population o…
Constraining the geometry of the gas surrounding a typical galaxy at with Ly polarization
A. Bolamperti, S. -J. Chang, J. Vernet +6
Ly emission is the strongest tracer of recombining ionized hydrogen in young, star-forming galaxies, but its origin is still debated. Ly arises when emitted photons scatter i…
Unveiling [CII] clumps in a lensed star-forming galaxy at z ~ 3.4
A. Zanella, E. Iani, M. Dessauges-Zavadsky +15
Observations at UV and optical wavelengths have revealed that galaxies at z~1-4 host star-forming regions, dubbed "clumps", which are believed to form due to the fragmentation of g…
CEERS Key Paper VI: JWST/MIRI Uncovers a Large Population of Obscured AGN at High Redshifts
G. Yang, K. I. Caputi, C. Papovich +35
Mid-infrared observations are powerful in identifying heavily obscured Active Galactic Nuclei (AGN) which have weak emission in other wavelengths. Data from the Mid-Infrared Instru…
Scrutiny of a very young, metal-poor star-forming Lyα-emitter at z ~ 3.7
E. Iani, A. Zanella, J. Vernet +9
The origin of the Lyman- (Ly) emission in galaxies is a long-standing issue: despite several processes known to originate this line (e.g. AGN, star formation, cold accretion,…
Differential attenuation in star-forming galaxies at 0.3 1.5 in the SHARDS/CANDELS field
L. Rodríguez-Muñoz, G. Rodighiero, P. G. Pérez-González +21
We use a sample of 706 galaxies, selected as [OII]3727 ([OII]) emitters in the Survey for High- Absorption Red and Dead Sources (SHARDS) on the CANDELS/GOODS-N field, to stud…
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…
Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.20.9
L. Rodríguez-Muñoz, G. Rodighiero, C. Mancini +21
We quantify the star formation (SF) in the inner cores (/0.3) of 24 massive galaxy clusters at 0.20.9 observed by the …