The TESS-Keck Survey. VIII. Confirmation of a Transiting Giant Planet on an Eccentric 261 Day Orbit with the Automated Planet Finder Telescope* *Some of the data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation.
The Astronomical Journal American Astronomical Society 163:2 (2022) 61
Quantifying the poor purity and completeness of morphological samples selected by galaxy colour
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 510:3 (2022) 4126-4133
Quantifying Uncertainty in Deep Learning Approaches to Radio Galaxy Classification
ArXiv 2201.01203 (2022)
Optimization of the Observing Cadence for the Rubin Observatory Legacy Survey of Space and Time: A Pioneering Process of Community-focused Experimental Design
The Astrophysical Journal Supplement Series American Astronomical Society 258:1 (2022) 1
TESS Eclipsing Binary Stars. I. Short-cadence Observations of 4584 Eclipsing Binaries in Sectors 1–26
The Astrophysical Journal Supplement Series American Astronomical Society 258:1 (2022) 16