| Issue |
A&A
Volume 666, October 2022
|
|
|---|---|---|
| Article Number | C4 | |
| Number of page(s) | 4 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/201730944e | |
| Published online | 18 October 2022 | |
Low-temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues
II. Mg and Fe-rich amorphous silicates★ (Corrigendum)
1
IRAP, Université de Toulouse, CNRS, UPS,
9 avenue colonel Roche,
BP 44346,
31028
Toulouse cedex 4, France
e-mail: karine.demyk@irap.omp.eu
2
UMET, UMR 8207,
Université Lille 1, CNRS,
59655
Villeneuve d’Ascq, France
3
Ligne AILES – Synchrotron SOLEIL, L’Orme des Merisiers,
91192
Gif-sur-Yvette, France
4
LPCNO, Université de Toulouse, CNRS, INSA, UPS,
135 avenue de Rangueil,
31077
Toulouse, France
This article has no abstract.
Key words: dust, extinction / submillimeter: ISM / infrared: ISM / methods: laboratory: solid state / astrochemistry / errata, addenda
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
© K. Demyk et al. 2022
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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