works on

From the 2 of 8.2k papers with an AI index.

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20022026
most citedQuantum ESPRESSO: a modular and open-source software project for quantum simulations of materials

29.3k citations

Showing 2019 · astro-ph.EPShow all

41 papers · 2 filters

astro-ph.EP2019★ 40 cited

Phase Curve of the Hot Jupiter WASP-19b

Ian Wong, Björn Benneke, Avi Shporer +13

We analyze the phase curve of the short-period transiting hot Jupiter system WASP-19, which was observed by the Transiting Exoplanet Survey Satellite () in Sector 9. WASP-19…

astro-ph.EP2019★ 73 cited

A sub-Neptune sized planet transiting the M2.5-dwarf G 9-40: Validation with the Habitable-zone Planet Finder

Gudmundur Stefansson, Caleb Cañas, John Wisniewski +32

We validate the discovery of a 2 Earth radii sub-Neptune-size planet around the nearby high proper motion M2.5-dwarf G 9-40 (EPIC 212048748), using high-precision near-infrared (NI…

astro-ph.EP2019★ 7 cited

Atmospheric Characterization and Further Orbital Modeling of And b

Taichi Uyama, Thayne Currie, Yasunori Hori +18

We present Andromeda b's photometry and astrometry taken with Subaru/SCExAO+HiCIAO and Keck/NIRC2, combined with recently published SCExAO/CHARIS low-resolution spectroscopy an…

astro-ph.EP2019★ 174 cited

The Orbit of WASP-12b is Decaying

Samuel W. Yee, Joshua N. Winn, Heather A. Knutson +6

WASP-12b is a transiting hot Jupiter on a 1.09-day orbit around a late-F star. Since the planet's discovery in 2008, the time interval between transits has been decreasing by $29\p…

astro-ph.EP2019★ 30 cited

TOI-132 b: A short-period planet in the Neptune desert transiting a G-type star

Matías R. Díaz, James S. Jenkins, Davide Gandolfi +45

The Neptune desert is a feature seen in the radius-mass-period plane, whereby a notable dearth of short period, Neptune-like planets is found. Here we report the {\it TESS} discove…

astro-ph.EP2019★ 28 cited

Gravity-Darkening Analysis of Misaligned Hot Jupiter MASCARA-4 b

John P. Ahlers, Ethan Kruse, Knicole D. Colon +17

MASCARA-4 b is a hot Jupiter in a highly-misaligned orbit around a rapidly-rotating A3V star that was observed for 54 days by the Transiting Exoplanet Survey Satellite (\tess). We…