We detect a candidate fifth planet in the HR 8799 system, directly imaged with the JWST/NIRISS Aperture Masking Interferometer (AMI). The detected source lies just above a $3\sigma$ contrast curve at a contrast of $\sim2\times10^{-4}$ in the F380M filter at a projected separation of $\sim150$ mas, corresponding to a fe...
Jayke S. Nguyen, L. Desdoigts, A. Greenbaum et al.· 0 citations
The detection of orbiting exoplanets by way of astrometric monitoring of the host star to reveal gravitationally induced reflex motion requires extreme precision and measurement stability when targeting Earth-mass objects. Despite this, astrometry is widely regarded as the most promising avenue for the most desired of...
P. Tuthill, George Ayad, Donald G. Dansereau et al.· Astronomical Telescopes + In...· 0 citations
ADORA provides a flexible framework for studying astrometric extraction, calibration-bias diagnosis, and future SHERA requirements, and Pixel-position errors across the tested range remain near the matched-model recovery scale indicating robustness to certain detector calibration errors.
Dylan M. McKeithen, S. Shaklan, G. Vasisht et al.· Astronomical Telescopes + In...· 0 citations
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