| Issue |
A&A
Volume 666, October 2022
|
|
|---|---|---|
| Article Number | C3 | |
| Number of page(s) | 2 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/201629711e | |
| Published online | 18 October 2022 | |
Low temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues
I. Mg-rich glassy silicates★ (Corrigendum)
1
IRAP, Université de Toulouse, CNRS, UPS, IRAP,
9 avenue colonel Roche,
BP 44346,
31028
Toulouse Cedex 4, France
e-mail: karine.demyk@irap.omp.eu
2
Institute of Chemical Engineering Sciences, FORTH,
PO Box 1414,
26504
Patras, Greece
3
Department of Chemical Engineering, University of Patras,
26504
Patras, Greece
4
UMET, UMR 8207,
Université Lille 1, CNRS,
59655
Villeneuve d'Ascq, France
5
Ligne AILES - Synchrotron SOLEIL, L'Orme des Merisiers,
91192
Gif-sur-Yvette, France
6
Université de Toulouse, INSA, CNRS, LPCNO,
31077
Toulouse, France
7
Space Research Institute, RAS,
84/32 Profsoyuznaya,
117810
Moscow, Russia
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 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
© 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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