Oxygen K-edge cross sections (Psaradaki+, 2020)

The dust samples analysed in this work are laboratory analogues of silicates and oxides of astronomical interest. Here, we present the calculated dust extinction cross sections. The data were acquired using the electron microscope facility located at the University of Cadiz in Spain. Among the samples, four of them are natural and six are commercial products. The rest of the silicate samples are synthesised in the laboratories at the Astrophysikalisches Institut, Universitats-Stenwarte (AIU), and Osaka University.

Identifier
Source http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/642/A208
Related Identifier https://ui.adsabs.harvard.edu/abs/2020A&A...642A.208P
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_datacite&identifier=ivo://CDS.VizieR/J/A+A/642/A208
Provenance
Creator Psaradaki I., Costantini E., Mehdipour M., Rogantini D., de Vries C.P., de Groot F., Mutschke H., Trasobares S., Waters L.B.F.M., Zeegers S.T.
Publisher CDS
Contributor International Virtual Observatory Alliance (IVOA)
Publication Year 2021
Rights public
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Format text/xml+votable
Version 26-Sep-2020
Discipline Stellar Astronomy;Interdisciplinary Astronomy