Using HARPS-N to characterize 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/10.1093/mnras/stz2856

Publication URI: http://dx.doi.org/10.1093/mnras/stz2856

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 4