Using HARPS-N to characterize the long-period planets in the PH-2 and Kepler-103 systems (2019)
Attributed to:
Astronomy at St Andrews 2015-2018
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