Low-temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues. II. Mg and Fe-rich amorphous silicates (Corrigendum) - INSU - Institut national des sciences de l'Univers Access content directly
Journal Articles Astronomy and Astrophysics - A&A Year : 2022

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

Abstract

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
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insu-03867385 , version 1 (23-11-2022)

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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⟩
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