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20012024
most citedAccreting Protoplanets in the LkCa 15 Transition Disk

302 citations · 2.8k across the 58 of their papers we have counts for

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astro-ph.IM2020★ 1 cited

Betelgeuse scope: Single-mode-fibers-assisted optical interferometer design for dedicated stellar activity monitoring

Narsireddy Anugu, Katie M. Morzinski, Josh Eisner +12

Betelgeuse has gone through a sudden shift in its brightness and dimmed mysteriously. This is likely caused by a hot blob of plasma ejected from Betelgeuse and then cooled to obscu…

astro-ph.IM2018

The Wide Integral Field Infrared Spectrograph: Commissioning Results and On-sky Performance

Suresh Sivanandam, Dae-Sik Moon, R. Elliot Meyer +11

We have recently commissioned a novel infrared ( m) integral field spectrograph (IFS) called the Wide Integral Field Infrared Spectrograph (WIFIS). WIFIS is a unique in…

astro-ph.IM2016★ 37 cited

iLocater: A Diffraction-limited Doppler Spectrometer for the Large Binocular Telescope

Justin R. Crepp, Jonathan Crass, David King +31

We are developing a stable and precise spectrograph for the Large Binocular Telescope (LBT) named "iLocater." The instrument comprises three principal components: a cross-dispersed…

astro-ph.IM2014★ 16 cited

High contrast imaging at the LBT: the LEECH exoplanet imaging survey

Andrew J. Skemer, Philip Hinz, Simone Esposito +34

In Spring 2013, the LEECH (LBTI Exozodi Exoplanet Common Hunt) survey began its 130-night campaign from the Large Binocular Telescope (LBT) atop Mt Graham, Arizona. This surv…

astro-ph.IM2013★ 29 cited

Simultaneous Exoplanet Characterization and deep wide-field imaging with a diffractive pupil telescope

Olivier Guyon, Josh A. Eisner, Roger Angel +12

High-precision astrometry can identify exoplanets and measure their orbits and masses, while coronagraphic imaging enables detailed characterization of their physical properties an…

astro-ph.IM2013★ 41 cited

High precision astrometry with a diffractive pupil telescope

Olivier Guyon, Eduardo A. Bendek, Thomas D. Milster +11

Astrometric detection and mass determination of Earth-mass exoplanets requires sub-microarcsec accuracy, which is theoretically possible with an imaging space telescope using field…