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A. Zanella

24 papers hereh-index 694 citations30 works total

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

author position
  • first author1
  • middle author15
  • last author6

Across the 22 of 24 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA23
  • astro-ph.CO1
same name
  • A. Zanella — 59 papers, h 43
  • A. Zanella — 50 papers, h 20
  • A. Zanella — 23 papers, h 4
  • A. Zanella — 8 papers, h 3
  • A. Zanella — 6 papers, h 36
  • A. Zanella — 1 paper, h 2

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

activity
20232026
most citedDynamically cold disks in the early Universe: myth or reality?

51 citations · 204 across the 22 of their papers we have counts for

collaborators
Showing 2026Show all

4 papers · 1 filter

astro-ph.GA2026

GA-NIFS view of LAP1: Assembly of Pop~III stellar clusters during EoR

J. Scholtz, R. Maiolino, S. Carniani +28

Lensed and Pristine 1 (LAP1) is one of the most promising candidates for the detection of so-called Pop~III stars at z∼6.6. In this work, we present new high-spectral-resoluti…

astro-ph.GA2026

DREAMS: Taking the Temperature of a Massive Galaxy at z ~ 11

L. Parente, E. Vanzella, M. Messa +15

We present a detailed photometric and spectroscopic analysis of Janus-11, a z=10.7933±0.0006 galaxy magnified by a factor 1.6 by the galaxy cluster MACS J0416. It was observ…

astro-ph.GA2026

A Cosmic Archipelago of lensed metal-poor galaxies at z∼6

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 z∼6.14. We combine JWST/NIRCam with deep VL…

astro-ph.GA2026

A first [CII] view of high-z quiescent galaxies

C. D'Eugenio, E. Daddi, R. Gobat +10

We present ALMA detections (or stringent upper limits) of the [CII] 158 μm emission line and underlying dust continuum from five massive quenched galaxies (QGs) at 2<z<4.7. We fi…

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