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Low temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues. I. Mg-rich glassy silicates (Corrigendum)

Abstract : Data from this article are publicly available through the STOP-CODA (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 is accessible via the following link: https://www.sshade.eu/data/experiment/EXPERIMENT_KD_20170711
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https://hal-insu.archives-ouvertes.fr/insu-03867386
Contributor : Nathalie POTHIER Connect in order to contact the contributor
Submitted on : Wednesday, November 23, 2022 - 1:21:42 PM
Last modification on : Tuesday, December 6, 2022 - 12:42:14 PM

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Distributed under a Creative Commons Attribution 4.0 International License

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K. Demyk, C. Meny, X. -H. Lu, G. Papatheodorou, M. J. Toplis, et al.. Low temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues. I. Mg-rich glassy silicates (Corrigendum). Astronomy and Astrophysics - A&A, 2022, 666, ⟨10.1051/0004-6361/201629711e⟩. ⟨insu-03867386⟩

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