activity
19962025
most citedEuclid. I. Overview of the Euclid mission

550 citations · 1.3k across the 19 of their papers we have counts for

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Showing astro-ph.GAShow all

7 papers · 1 filter

astro-ph.GA2025★ 2 cited

The HST-Hyperion Survey: Companion Fraction and Overdensity in a z ~ 2.5 Proto-supercluster

F. Giddings, B. C. Lemaux, B. Forrest +22

We present a study of the galaxy merger and interaction activity within the Hyperion Proto-supercluster at z~2.5 in an effort to assess the occurrence of galaxy mergers and interac…

astro-ph.GA2023

Identification and Characterization of Six Spectroscopically Confirmed Massive Protostructures at

Ekta A. Shah, Brian Lemaux, Benjamin Forrest +22

We present six spectroscopically confirmed massive protostructures, spanning a redshift range of in the Extended Chandra Deep Field South (ECDFS) field discovered as pa…

astro-ph.GA2023★ 20 cited

WEAVE-StePS. A stellar population survey using WEAVE at WHT

A. Iovino, B. M. Poggianti, A. Mercurio +44

The upcoming new generation of optical spectrographs on four-meter-class telescopes will provide valuable opportunities for forthcoming galaxy surveys through their huge multiplexi…

astro-ph.GA2022★ 18 cited

Euclid preparation. XXI. Intermediate-redshift contaminants in the search for galaxies within the Euclid Deep Survey

Euclid Collaboration, S. E. van Mierlo, K. I. Caputi +203

(Abridged) The Euclid mission is expected to discover thousands of z>6 galaxies in three Deep Fields, which together will cover a ~40 deg2 area. However, the limited number of Eucl…

astro-ph.GA2021★ 43 cited

The ALPINE-ALMA [CII] survey: Dust mass budget in the early Universe

F. Pozzi, F. Calura, Y. Fudamoto +32

The dust content of normal galaxies and the dust mass density (DMD) at high-z (z>4) are unconstrained given the source confusion and the sensitivity limitations of previous observa…

astro-ph.GA2020★ 11 cited

The ALPINE-ALMA [C II] survey: the luminosity function of serendipitous [C II] line emitters at

Federica Loiacono, Roberto Decarli, Carlotta Gruppioni +32

We present the first [CII] 158 m luminosity function (LF) at from a sample of serendipitous lines detected in the ALMA Large Program to INvestigate [CII] at Early time…