Characterising pre-main-sequence stars in the large magellanic cloud with machine and deep learning techniques
Gespeichert in:
| 1. Verfasser: | |
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| Dokumenttyp: | Buch/Monographie Hochschulschrift |
| Sprache: | Englisch |
| Veröffentlicht: |
Heidelberg
19 Jul. 2021
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| DOI: | 10.11588/heidok.00030216 |
| Schlagworte: | |
| Online-Zugang: | Resolving-System, kostenfrei: https://nbn-resolving.de/urn:nbn:de:bsz:16-heidok-302167 Resolving-System, kostenfrei: http://dx.doi.org/10.11588/heidok.00030216 Verlag, kostenfrei, Volltext: http://www.ub.uni-heidelberg.de/archiv/30216 Resolving-System: https://doi.org/10.11588/heidok.00030216 Resolving-System: https://nbn-resolving.org/urn:nbn:de:bsz:16-heidok-302167 Langzeitarchivierung Nationalbibliothek: https://d-nb.info/1237270855/34 Verlag, kostenfrei: http://www.ub.uni-heidelberg.de/archiv/30216 |
| Verfasserangaben: | put forward by Victor Francisco Ksoll ; referees: Prof. Dr. Ralf Klessen [und ein weiterer Gutachter] |
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