activity
20172024
most citedX-shooter Spectroscopy and HST Imaging of 15 Ultra Massive Quiescent Galaxies at

44 citations · 149 across the 8 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

16 papers · 1 filter

astro-ph.GA20245 cited

RUBIES Reveals a Massive Quiescent Galaxy at z=7.3

Andrea Weibel, Anna de Graaff, David J. Setton +26

We report the spectroscopic discovery of a massive quiescent galaxy at , just Myr after the Big Bang. RUBIES-UDS-QG-z7 was selected from public…

astro-ph.GA2024

ALMA Lensing Cluster Survey: Physical characterization of near-infrared-dark intrinsically faint ALMA sources at z=2-4

Akiyoshi Tsujita, Kotaro Kohno, Shuo Huang +33

We present results from Atacama Large Millimeter/submillimeter Array (ALMA) spectral line-scan observations at 3-mm and 2-mm bands of three near-infrared-dark (NIR-dark) galaxies b…

astro-ph.GA2024

The cold interstellar medium of a normal sub- galaxy at the end of reionization

F. Valentino, S. Fujimoto, C. Giménez-Arteaga +21

We present the results of a ~60-hr observational campaign with ALMA targeting a spectroscopically confirmed and lensed sub- galaxy at z=6.07, identified during the ALMA Le…

astro-ph.GA202310 cited

ALMACAL. XI. Over-densities as signposts to proto-clusters? A cautionary tale

Jianhang Chen, R. J. Ivison, Martin A. Zwaan +6

It may be unsurprising that the most common approach to finding proto-clusters is to search for over-densities of galaxies. Upgrades to submillimetre (submm) interferometers and th…

astro-ph.GA2023

ALMA Lensing Cluster Survey: Deep 1.2 mm Number Counts and Infrared Luminosity Functions at

Seiji Fujimoto, Kotaro Kohno, Masami Ouchi +40

We present a statistical study of 180 dust continuum sources identified in 33 massive cluster fields by the ALMA Lensing Cluster Survey (ALCS) over a total of 133 arcmin area…

astro-ph.GA20207 cited

The Fundamental Plane of Massive Quiescent Galaxies at z~2

Mikkel Stockmann, Inger Jørgensen, Sune Toft +11

We examine the Fundamental Plane (FP) and mass-to-light ratio () scaling relations using the largest sample of massive quiescent galaxies at to date. The FP ($r_{e…