activity
20242026
collaborators

9 papers

astro-ph.IM2026

ALMA publication statistics

Felix Stoehr, María Díaz Trigo, Evanthia Hatziminaoglou +9

The success of an astronomical facility is measured by its scientific impact. A principal metric for this impact is the ensemble of peer-reviewed publications based on the observat…

astro-ph.GA2026

PAHSPECS: Spatially Resolved PAH Spectroscopy at cosmic noon with JWST MIRI MRS

Fergus R. Donnan, Karin Sandstrom, Irene Shivaei +10

We present spatially resolved spectroscopy with JWST/MIRI MRS of a representative sample of normal star-forming galaxies at as part of the PAHSPECS program. To extract e…

astro-ph.IM2026

Towards ALMA2040: An update from the European community and invitation to contribute

Stefano Facchini, Jacqueline Hodge, Jes Jørgensen +27

Over the last 15 years, the Atacama Large Millimeter/submillimeter Array (ALMA) has revolutionized astrophysics by providing unprecedented resolution and sensitivity in observing t…

astro-ph.GA2025

A search for cold molecular outflows in cosmic noon galaxies

Ivanna Langan, Gergö Popping, Michele Ginolfi +4

The flow of baryons in and out of galaxies is the primary driver for galaxy evolution. In addition to depleting the gas reservoir of galaxies, outflows also enrich their circumgala…

astro-ph.GA2025

Predicting the resolved CO emission of star-forming galaxies

Ravishankar Anirudh, Melanie Kaasinen, Gergö Popping +3

(Abridged) Resolved observations of the CO emission from star-forming galaxies are becoming increasingly common, with new high-resolution surveys on the horizon. We aim to…

astro-ph.GA2025

Do cosmological simulations reproduce the [OIII] 88 m line emission and properties of JWST-discovered galaxies at ?

Shengqi Yang, Adam Lidz, Hui Li +3

Recent ALMA observations of the [OIII] 88 m line provide spectroscopic confirmation of two JWST photometric candidates, GS-z14 and GHZ2, at and , respectively.…