Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT Format

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 3.

Speckle imaging contrast curves for NLTT 43564 (GAI 1645+6057) obtained with the ’Alopeke Speckle Imaging at Gemini at 562 nm (blue) and 832 nm (red). The curves show the 5σ detection limits (Δm) as a function of angular separation. The inset of 1″ × 1″ shows the reconstructed speckle image at 832 nm. No nearby companions are detected within 1﹩\mathop{.}\limits^{\unicode{x02033}}﹩2 angular separation of the target.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse