Low-temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues. II. Mg and Fe-rich amorphous silicates (Corrigendum)

K. Demyk (1) , C. Meny (1) , H. Leroux (2) , C. Depecker (2) , J. -B. Brubach (3) , P. Roy (3) , C. Nayral (4) , W. -S. Ojo (4) , F. Delpech (4)

1 IRAP - Institut de recherche en astrophysique et planétologie
2 UMET - Unité Matériaux et Transformations - UMR 8207
3 SSOLEIL - Synchrotron SOLEIL
4 LPCNO - Laboratoire de physique et chimie des nano-objets

Data from this article are publicly available through the STOPCODA (SpecTroscopy and Optical Properties of Cosmic Dust Analogues) database of the SSHADE infrastructure of solid spectroscopy (https://doi.org/10.26302/SSHADE/STOPCODA). The dataset are accessible via the following links: https://www.sshade.eu/data/experiment/EXPERIMENT_KD_20170822 and https://www.sshade.eu/data/experiment/EXPERIMENT_KD_20170823

Keywords: astrochemistry; errata; addenda; dust; extinction; submillimeter: ISM; infrared: ISM; methods: laboratory: solid state

Domains: Sciences of the Universe [physics]; Astrophysics [astro-ph]

K. Demyk, C. Meny, H. Leroux, C. Depecker, J. -B. Brubach, et al.. Low-temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues. II. Mg and Fe-rich amorphous silicates (Corrigendum). Astronomy and Astrophysics - A&A, 2022, 666, ⟨10.1051/0004-6361/201730944e⟩. ⟨insu-03867385⟩