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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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https://hal-insu.archives-ouvertes.fr/insu-03867385
Contributor : Nathalie POTHIER Connect in order to contact the contributor
Submitted on : Wednesday, November 23, 2022 - 1:17:20 PM
Last modification on : Thursday, November 24, 2022 - 4:05:39 AM

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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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