activity
20052026
most citedThe James Webb Space Telescope Mission

490 citations · 3.3k across the 72 of their papers we have counts for

collaborators

73 papers

astro-ph.SR2026

The CepA disk-outflow system at <=0.2'' or <=100au resolution

H. Beuther, C. Gieser, V. Aberham +21

Context: Although there has been significant progress, the physical properties and potential fragmentation of accretion disks around high-mass protostars remain poorly constrained.…

astro-ph.SR2023★ 18 cited

JOYS: Disentangling the warm and cold material in the high-mass IRAS 23385+6053 cluster

C. Gieser, H. Beuther, E. F. van Dishoeck +20

(abridged) We study and compare the warm (>100 K) and cold (<100 K) material toward the high-mass star-forming region IRAS 23385+6053 (IRAS 23385 hereafter) combining high angular…

astro-ph.GA2023★ 115 cited

PDRs4All IV. An embarrassment of riches: Aromatic infrared bands in the Orion Bar

Ryan Chown, Ameek Sidhu, Els Peeters +136

(Abridged) Mid-infrared observations of photodissociation regions (PDRs) are dominated by strong emission features called aromatic infrared bands (AIBs). The most prominent AIBs ar…

astro-ph.IM2023★ 19 cited

Progress in the Design of the Atacama Large Aperture Submillimeter Telescope

Tony Mroczkowski, Claudia Cicone, Matthias Reichert +13

The Atacama Large Aperture Submillimeter Telescope (AtLAST) aims to be the premier next generation large diameter (50 meter) single dish observatory capable of observations across…

astro-ph.IM2023

Geometric distortion and astrometric calibration of the JWST MIRI Medium Resolution Spectrometer

P. Patapis, I. Argyriou, D. R. Law +12

The Medium-Resolution integral field Spectrometer (MRS) of MIRI on board JWST performs spectroscopy between 5 and 28~m. The optics of the MRS introduce substantial distortion, a…

astro-ph.GA2023★ 25 cited

High resolution modeling of [CII], [CI], [OIII] and CO line emission from the ISM and CGM of a star forming galaxy at z ~ 6.5

Alice Schimek, Davide Decataldo, Sijing Shen +10

The circumgalactic medium (CGM) is a crucial component of galaxy evolution, but thus far its physical properties are highly unconstrained. As of yet, no cosmological simulation has…