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Using HARPS-N to characterise the long-period planets in the PH-2 and Kepler-103 systems (2019)

First Author: Dubber S

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