activity
20002026
most citedObservations of the Icy Universe

1k citations · 5.4k across the 65 of their papers we have counts for

collaborators

66 papers

astro-ph.GA2026

Dust Absorption towards Supernova Remnant W44

Tian-Yu Tu, Adwin Boogert, Yang Chen +1

Supernova remnants (SNRs) can strongly affect the chemical composition of the interstellar dust. In this paper we investigate to what degree the dust and ices are modified by obser…

astro-ph.GA2026

Ice chemistry that can be unveiled with the JWST: SynthIceSpec, a synthetic spectrum generator to test spectral limits. Solid CO_2 as a dust thermometer and solid CH_3CN detectability in cold cores

A. Taillard, P. Gratier, J. A. Noble +7

As the (JWST) pursues its observing journey, several thousands of icy-grain spectra are expected to be measured and analysed. The inventory of ices in particular, via the observati…

astro-ph.SR2026

The Outflow of the B335 Protostar II: After the Outburst

Klaus W. Hodapp, Adwin Boogert, Doug Johnstone +6

The B335 protostar has recently undergone a major, still ongoing, outburst detected in scattered light from its outflow cavity, offering a rare opportunity to study its impact on a…

astro-ph.GA2026

Backlighting young stellar objects in the Central Molecular Zone: an ensemble-averaged abundance structure of methanol ices

Yewon Kang, Deokkeun An, Jiwon Han +5

The Central Molecular Zone (CMZ) contains a substantial reservoir of dense molecular gas, where numerous young stellar objects (YSOs) and dense cloud cores have been identified. Ho…

astro-ph.SR2025

A Comprehensive Analysis of Rovibrational CO in the Era of JWST

D. Annie Dickson-Vandervelde, Colette Salyk, Geoffrey A. Blake +3

We present an analysis of CO rovibrational emission lines in the 183 infrared spectra of nearby Class II objects obtained with the NIRSPEC instrument on the Keck II telescope over…

astro-ph.SR2025★ 11 cited

HDO ice detected toward an isolated low-mass protostar with JWST

Katerina Slavicinska, Łukasz Tychoniec, María Gabriela Navarro +15

Water is detected in environments representing every stage of star and solar system formation, but its chemical evolution throughout these stages remains poorly constrained. Deuter…