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Pluto's Opposition Surge during 2018 and 2019, V1.0
- DOI:
- 10.26007/feev-qn61
- LID:
- Not yet assigned
- Authors:
- Burratti, B.; Hicks, M.; Bauer, J.; Ciardi, D.; Lund, M.; Lawrence, K.
- Abstract:
- Pluto and Charon were observed in 2018 and 2019 at small solar phase angles. Data were taken with the 5 m Hale telescope using the Palomar High Angular Resolution Observer (PHARO; Hayward et al. 2001) adaptive optics (AO; Dekany et al. 2013) system at Palomar Observatory. This data set contains raw image files of the Pluto-Charon system, associated dark frames, flat fields and standard stars.
This data set is being prepared for review, anticipated in June 2021. Following lien resolution, the data will be posted to the SBN archive pages as part of the Transneptunian, Centaur, and Pluto Data Sets collections.
If you have questions about these data before they are posted, please contact the SBN archive manager ("SBN Mgr.") listed below.
