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researcher

A. Ferrara

4 papers hereh-index 5167 citations13 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA4
same name
  • A. Ferrara — 14 papers, h 12
  • A. Ferrara — 12 papers, h 7
  • A. Ferrara — 5 papers, h 4
  • A. Ferrara — 4 papers, h 3
  • A. Ferrara — 4 papers, h 7
  • A. Ferrara — 3 papers, h 18

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

collaborators

4 papers

astro-ph.GA2025

How much gas and dust is in the z=5.7 Lyman Break Galaxy HZ10? An ALMA Band 10 to 4 and JWST/NIRSpec study of its interstellar medium

H. S. B. Algera, R. Herrera-Camus, M. Aravena +26

A complete overview of the stellar, gas and dust contents of galaxies is key to understanding their assembly at early times. However, an estimation of molecular and atomic gas rese…

astro-ph.GA2025

The ALMA REBELS survey: [OIII]88I^¼m​ line scans of UV-bright z≳7.6 galaxies

I. F. van Leeuwen, R. J. Bouwens, J. A. Hodge +17

We present the [OIII]88I^¼m​ spectral scan results from the ALMA Large Program REBELS (Reionization Era Bright Emission Line Survey). The generally high luminosity of [OI…

astro-ph.GA2025

Spatially resolved [CII]-gas conversion factor in early galaxies

L. Vallini, A. Pallottini, M. Kohandel +12

Determining how efficiently gas collapses into stars at high-redshift is key to understanding galaxy evolution in the Epoch of Reionization (EoR). Globally, this process is quantif…

astro-ph.GA2024

A hidden active galactic nucleus powering bright [O III] nebulae in a protocluster at z=4.5 revealed by JWST

M. Solimano, J. González-López, M. Aravena +48

Galaxy protoclusters are sites of rapid growth, with a high density of massive galaxies driving elevated rates of star formation and accretion onto supermassive black holes. Here,…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.