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Stellar and Orbital Characterization of Three Low Mass M Dwarf Binary Stars with Dynamical Spectroscopy from the Habitable Zone Planet Finder

  • Authors: Suhani Surana, Chad F. Bender, Caleb I. Cañas, Daniel M. Krolikowski, William D. Cochran, Mark Everett, Arvind F. Gupta, Shubham Kanodia, Suvrath Mahadevan, Andrew Monson, Joe P. Ninan, Leonardo A. Paredes, Paul Robertson, Arpita Roy, Christian Schwab, Gudmundur Stefansson

Suhani Surana et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 6.

RV vs. orbital phase for NLTT 45468. Upper panel: open black circles and open red triangles show primary HPF V﹩{}_{{pre}}﹩ and Vpost, respectively, corrected for the relative offset to be plotted on the same plot. The solid lines show the best orbital solution (Table 3). Lower panels: observed − calculated residuals for the HPF pre- and post-primary RVs.

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