Image Details
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.
© 2026. The Author(s). Published by the American Astronomical Society.