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20202026
most citedThe infrared colors of 51 Eridani b: micrometereoid dust or chemical disequilibrium?

9 citations · 32 across the 10 of their papers we have counts for

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astro-ph.EP2026

A Sulfur-Rich Atmosphere for the Young Jupiter Analog AF Lep b Reveals Significant Solid Accretion

Jerry W. Xuan, William O. Balmer, Yayaati Chachan +25

AF Lep b is one of the closest analogs to Jupiter in terms of mass () and semi-major axis ( AU) amenable to spectroscopic characterization. We present JWST/NIR…

astro-ph.EP2026

Discovery of an Exterior Third Planet Orbiting Pictoris

Aidan Gibbs, Jean-Baptiste Ruffio, Alexis Bidot +9

We report the discovery of Pictoris d ( Pic d), a third giant planet in the Pictoris system, which now becomes only the second directly imaged system with more than two…

astro-ph.EP2026

Worlds Next Door. IV. Mapping the Late Stages of Giant Planet Evolution with a Precise Dynamical Mass and Luminosity for Ind Ab

Aniket Sanghi, William Thompson, James Mang +21

We present new JWST/NIRCam 4-5 m (F410M, F430M) and JWST/MIRI 18-25 m (F1800W, F2100W, F2550W) imaging detections of the nearby (3.6 pc) cold (275 K) gas giant exoplanet …

astro-ph.EP2025★ 8 cited

Direct Spectroscopy of 51 Eridani b with JWST NIRSpec

Alexander Madurowicz, Jean-Baptiste Ruffio, Bruce Macintosh +4

We present high-contrast direct spectroscopy of the low-mass, cool exoplanet 51 Eridani b (2-4 M, 750 K) using JWST / NIRSpec in a fixed-slit configuration (F2…

astro-ph.EP2023★ 9 cited

The infrared colors of 51 Eridani b: micrometereoid dust or chemical disequilibrium?

Alexander Madurowicz, Sagnick Mukherjee, Natasha Batalha +3

We reanalyze near-infrared spectra of the young extrasolar giant planet 51 Eridani b which was originally presented in (Macintosh et al. 2015) and (Rajan et al. 2017) using modern…

astro-ph.EP2021★ 8 cited

Multiwavelength Mitigation of Stellar Activity in Astrometric Planet Detection

Avi Kaplan-Lipkin, Bruce Macintosh, Alexander Madurowicz +4

Astrometry has long been a promising technique for exoplanet detection. At the theoretical limits, astrometry would allow for the detection of smaller planets than previously seen…