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19972026
most citedWide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report

1k citations · 5.2k across the 111 of their papers we have counts for

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astro-ph.EP20231 cited

The PEPSI Exoplanet Transit Survey (PETS) IV: Assessing the atmospheric chemistry of KELT-20b

Sydney Petz, Marshall C. Johnson, Anusha Pai Asnodkar +11

Most ultra hot Jupiters (UHJs) show evidence of temperature inversions, in which temperature increases with altitude over a range of pressures. Temperature inversions can occur whe…

astro-ph.EP2023

A Comparison of the Composition of Planets in Single- and Multi-Planet Systems Orbiting M dwarfs

Romy Rodríguez Martínez, David V. Martin, B. Scott Gaudi +4

We investigate and compare the composition of M-dwarf planets in systems with only one known planet (``singles") to those residing in multi-planet systems (``multis") and the funda…

astro-ph.IM2023

Roman CCS White Paper: Adding Fields Hosting Globular Clusters To The Galactic Bulge Time Domain Survey

Samuel K. Grunblatt, Robert F. Wilson, Andrew Winter +9

Despite multiple previous searches, no transiting planets have yet been identified within a globular cluster. This is believed to be due to a combination of factors: the low metall…

astro-ph.HE2023

K2 Optical Emission from OJ 287 and Other Gamma-Ray Blazars on Hours-to-Weeks Timescales from 2014-2018

Ann E. Wehrle, Michael Carini, Paul J. Wiita +5

We present second observations by K2 of OJ~287 and 7 other -ray AGNs obtained in 2017-2018, second and third observations of the lobe-dominated, steep spectrum quasar 3C~207, an…

astro-ph.EP20231 cited

Exoplanet Nodal Precession Induced by Rapidly Rotating Stars: Impacts on Transit Probabilities and Biases

Alexander P. Stephan, B. Scott Gaudi

For the majority of short period exoplanets transiting massive stars with radiative envelopes, the spin angular momentum of the host star is greater than the planetary orbital angu…

astro-ph.EP202316 cited

The PEPSI Exoplanet Transit Survey. III: The detection of FeI, CrI and TiI in the atmosphere of MASCARA-1 b through high-resolution emission spectroscopy

G. Scandariato, F. Borsa, A. S. Bonomo +19

Hot giant planets like MASCARA-1 b are expected to have thermally inverted atmospheres, that makes them perfect laboratory for the atmospheric characterization through high-resolut…