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A Planetary System around the nearby M Dwarf GJ 667C with At Least One Super-Earth in Its Habitable Zone, , , , , , , , , and 7 other author(s). \apjl, (May 2012)Signals embedded in the radial velocity noise. Periodic variations in the $\tau$ Ceti velocities, , , , , , , , , and 5 other author(s). \aap, (March 2013)Two Super-Earths Orbiting the Solar Analog HD 41248 on the Edge of a 7:5 Mean Motion Resonance, , , , and . \apj, (July 2013)Surface stress in d-band metal surfaces, and . Journal of Physics: Condensed Matter, 22 (13): 135007 (2010)A dynamically-packed planetary system around GJ667C with three super-Earths in its habitable zone, , , , , , , , , and 1 other author(s). ArXiv e-prints, (June 2013)A multiple planet system of super-Earths orbiting the brightest red dwarf star GJ887, , , , , , , , , and 22 other author(s). (2020)cite arxiv:2006.16372Comment: Published by Science.The effect of ISM absorption on stellar activity measurements and its relevance for exoplanet studies, , , , , , , , , and 3 other author(s). (2017)cite arxiv:1702.02883Comment: Accepted for publication in A&A.Frequency of planets orbiting M dwarfs in the Solar neighbourhood, , , , , , , , , and 9 other author(s). (2019)cite arxiv:1906.04644Comment: Manuscript submitted to AAS journals. 341 pages, including 66 pages of tables summarising data properties, target properties, and selected parameter estimates.