Published 2019
“…We determine the possibility of a companion star and false positive detection to be extremely low using both archival images and high-contrast adaptive optics images from the
Palomar observatory. The brightness of the host star makes Wolf 503b a prime target for prompt radial velocity follow-up, and with the small stellar radius (0.690 ± 0.025R [subscript ⊕]), it is also an excellent target for HST transit spectroscopy and detailed atmospheric characterization with JWST. …”
Get full text
Article