activity
20232026
most citedA Milky Way-like barred spiral galaxy at a redshift of 3

70 citations · 342 across the 26 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

26 papers · 1 filter

astro-ph.GA2026

The gradual decline of Ly visibility in the CANDELS fields: evidence for the combined effects of galaxy evolution and reionization

L. Napolitano, L. Pentericci, A. Ferrara +35

We investigate the evolution of Ly visibility and the physical properties of Ly emitters (LAEs) across the five CANDELS fields using publicly available JWST/NIRSpec PRISM spe…

astro-ph.GA2026

The Collective Voice of Ly Emitters: Insights from JWST Stacked Spectroscopy

R. Tripodi, L. Napolitano, L. Pentericci +20

We present a spatially resolved stacked analysis of 287 LAEs at observed with JWST/NIRSpec prism spectroscopy. By constructing a two-dimensional stack from public surveys (CA…

astro-ph.GA2026

Investigating the role of mergers in galaxy assembly in the early Universe (z > 5)

A. Calabrò, L. Pentericci, M. Llerena +20

Galaxy mergers play a crucial role in shaping the morphology, the star formation, and the mass growth of galaxies across cosmic time. While mergers have been extensively investigat…

astro-ph.GA2025★ 1 cited

HELM's deep: Highly Extincted Low-Mass galaxies seen by JWST

L. Bisigello, G. Gandolfi, A. Grazian +25

The dust content of star-forming galaxies is generally positively correlated with their stellar mass. However, some recent JWST studies have shown the existence of a population of…

astro-ph.GA2025★ 1 cited

Searching Within Galaxies for the Earliest Signs of Quenching With Spatially Resolved Star Formation Histories in UVCANDELS Galaxies at z< 0.3

Charlotte Olsen, Eric Gawiser, Charlotte Welker +18

Understanding the complicated processes that regulate star formation and cause a galaxy to become quiescent is key to our comprehension of galaxy evolution. We used eight well reso…

astro-ph.GA2025★ 29 cited

Density modulated star formation efficiency: implications for the observed abundance of ultra-violet luminous galaxies at z>10

Rachel S. Somerville, L. Y. Aaron Yung, Lachlan Lancaster +3

The number density of UV luminous galaxies discovered by the James Webb Space Telescope at ultra high redshift () is higher, and declines much more slowly with increa…

astro-ph.GA2025★ 13 cited

ΛCDM is still not broken: empirical constraints on the star formation efficiency at z ~ 12-30

L. Y. Aaron Yung, Rachel S. Somerville, Kartheik G. Iyer

The James Webb Space Telescope continues to push back the redshift frontier to ever earlier cosmic epochs, with recent announcements of galaxy candidates at redshifts of $15 \lesss…

astro-ph.GA2025★ 13 cited

Pushing JWST to the extremes: search and scrutiny of bright galaxy candidates at z15-30

M. Castellano, A. Fontana, E. Merlin +50

We designed customized Lyman-break color selection techniques to identify galaxy candidates in the redshift ranges and . The selection was pe…

astro-ph.GA2025★ 3 cited

Extended Enriched Gas in a Multi-Galaxy Merger at Redshift 6.7

Weida Hu, Casey Papovich, Lu Shen +5

Recent JWST observations have uncovered high-redshift galaxies characterized by multiple star-forming clumps, many of which appear to be undergoing mergers. Such mergers, especiall…

astro-ph.GA2025★ 1 cited

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…

astro-ph.GA2024★ 41 cited

ASTRODEEP-JWST: NIRCam-HST multiband photometry and redshifts for half a million sources in six extragalactic deep fields

E. Merlin, P. Santini, D. Paris +52

We present a set of photometric catalogs primarily aimed at providing the community with a comprehensive database for the study of galaxy populations in the high redshift Universe.…

astro-ph.GA2024

UVCANDELS: Catalogs of photometric redshifts and galaxy physical properties

Vihang Mehta, Marc Rafelski, Ben Sunnquist +76

The UltraViolet imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey Fields (UVCANDELS) program provides deep HST F275W and F435W imaging over four CANDELS…

astro-ph.GA2024★ 8 cited

NGDEEP: The Star Formation and Ionization Properties of Galaxies at

Lu Shen, Casey Papovich, Jasleen Matharu +23

We use JWST/NIRISS slitless spectroscopy from the Next Generation Deep Extragalactic Exploratory Public (NGDEEP) Survey to investigate the physical condition of star-forming galaxi…

astro-ph.GA2024★ 2 cited

The Abundance and Properties of Barred Galaxies out to 4 Using CEERS Data

Yuchen Guo, Shardha Jogee, Eden Wise +26

We present the first estimate of the observed fraction and properties of bars out to using CEERS NIRCam images. We analyze 1770 galaxies with $M_\star > 1…

astro-ph.GA2024★ 8 cited

Physical properties of strong 1 < z < 3 Balmer and Paschen lines emitters observed with JWST

L. -M. Seillé, V. Buat, V. Fernández +16

The ultraviolet continuum traces young stars while the near-infrared unveils older stellar populations and dust-obscured regions. Balmer emission lines provide insights on gas prop…

astro-ph.GA2024★ 26 cited

Physical properties of extreme emission-line galaxies at from the JWST CEERS survey

M. Llerena, R. Amorín, L. Pentericci +22

Extreme emission line galaxies (EELGs) are typically characterized by high equivalent widths (EWs) which are driven by elevated specific star formation rates (sSFR) in low-mass gal…

astro-ph.GA2024★ 49 cited

Peering into cosmic reionization: the Ly visibility evolution from galaxies at = 4.5-8.5 with JWST

L. Napolitano, L. Pentericci, P. Santini +28

The resonant scattering interaction between Ly photons and neutral hydrogen implies that a partially neutral IGM can significantly impact the detectability of Ly emission in…

astro-ph.GA2024★ 28 cited

The evolution of the SFR and Sigma-SFR of galaxies in cosmic morning (4 < z < 10)

A. Calabrò, L. Pentericci, P. Santini +28

The galaxy integrated star-formation rate (SFR) surface density () has been proposed as a valuable diagnostic of the mass accumulation in galaxies as being more tightl…

astro-ph.GA2023★ 8 cited

CEERS: Increasing Scatter along the Star-Forming Main Sequence Indicates Early Galaxies Form in Bursts

Justin W. Cole, Casey Papovich, Steven L. Finkelstein +29

We present the star-formation-rate -- stellar-mass (SFR-M) relation for galaxies in the CEERS survey at . We model the \jwst\ and \hst\ rest-UV and rest-op…

astro-ph.GA2023★ 4 cited

Evidence for a Shallow Evolution in the Volume Densities of Massive Galaxies at to from CEERS

Katherine Chworowsky, Steven L. Finkelstein, Michael Boylan-Kolchin +36

We analyze the evolution of massive (log [] ) galaxies at 4--8 selected from the JWST Cosmic Evolution Early Release Science (CEERS) survey. W…

astro-ph.GA2023★ 70 cited

A Milky Way-like barred spiral galaxy at a redshift of 3

Luca Costantin, Pablo G. Pérez-González, Yuchen Guo +30

The majority of massive disk galaxies in the local Universe show a stellar barred structure in their central regions, including our Milky Way. Bars are supposed to develop in dynam…

astro-ph.GA2023★ 17 cited

The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ~ 8.5-14.5

Steven L. Finkelstein, Gene C. K. Leung, Micaela B. Bagley +52

We present a sample of 88 candidate z~8.5-14.5 galaxies selected from the completed NIRCam imaging from the Cosmic Evolution Early Release Science (CEERS) survey. These data cover…

astro-ph.GA2023★ 2 cited

Evolution of the Size-Mass Relation of Star-forming Galaxies Since Revealed by CEERS

Ethan M. Ward, Alexander de la Vega, Bahram Mobasher +19

We combine deep imaging data from the CEERS early release JWST survey and HST imaging from CANDELS to examine the size-mass relation of star-forming galaxies and the morphology-que…

astro-ph.GA2023

Galaxies Going Bananas: Inferring the 3D Geometry of High-Redshift Galaxies with JWST-CEERS

Viraj Pandya, Haowen Zhang, Marc Huertas-Company +53

The 3D geometry of high-redshift galaxies remains poorly understood. We build a differentiable Bayesian model and use Hamiltonian Monte Carlo to efficiently and robustly infer the…