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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 1.

Contrast curves and reconstructed images from the NESSI speckle imager for (a) LSPM 0515+5911, (b) NLTT 45468, and (c) NLTT 43564. Neither LSPM 0515+5911 nor NLTT 43564 show companions within the field that could contaminate the HPF observations. NLTT 45468 shows a nearby star at 2﹩\mathop{.}\limits^{\unicode{x02033}}﹩1 in the lower left of the inset in (b); the signal in the upper right is an artifact of the speckle processing.

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