Using HARPS-N to characterise the long-period planets in the PH-2 and Kepler-103 systems (2019)
Attributed to:
Astronomy at St Andrews 2018-2021
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1910.03518
Publication URI: https://arxiv.org/abs/1910.03518
Type: Other