output
19962026
most citedA Framework for Prioritizing the TESS Planetary Candidates Most Amenable to Atmospheric Characterization

593 citations

Showing 2017 · astro-ph.EPShow all

6 papers · 2 filters

astro-ph.EP2017★ 44 cited

Constraining Hot Jupiter Atmospheric Structure and Dynamics through Doppler Shifted Emission Spectra

Jisheng Zhang, Eliza Kempton, Emily Rauscher

We present a coupled 3-D atmospheric dynamics and radiative transfer model to predict the disk-integrated thermal emission spectra of transiting exoplanets in edge-on orbits. We ca…

astro-ph.EP2017★ 75 cited

A Statistical Comparative Planetology Approach to the Hunt for Habitable Exoplanets and Life Beyond the Solar System

Jacob L. Bean, Dorian S. Abbot, Eliza M. -R. Kempton

The search for habitable exoplanets and life beyond the Solar System is one of the most compelling scientific opportunities of our time. Nevertheless, the high cost of building fac…

astro-ph.EP2017★ 64 cited

An Observational Diagnostic for Distinguishing Between Clouds and Haze in Hot Exoplanet Atmospheres

Eliza M. -R. Kempton, Jacob L. Bean, Vivien Parmentier

The nature of aerosols in hot exoplanet atmospheres is one of the primary vexing questions facing the exoplanet field. The complex chemistry, multiple formation pathways, and lack…

astro-ph.EP2017★ 6 cited

Quantifying the Impact of Spectral Coverage on the Retrieval of Molecular Abundances from Exoplanet Transmission Spectra

John W. Chapman, Robert T. Zellem, Michael R. Line +14

Using forward models for representative exoplanet atmospheres and a radiometric instrument model, we have generated synthetic observational data to explore how well the major C- an…

astro-ph.EP2017★ 15 cited

KELT-18b: Puffy Planet, Hot Host, Probably Perturbed

Kim K. McLeod, Joseph E. Rodriguez, Ryan J. Oelkers +53

We report the discovery of KELT-18b, a transiting hot Jupiter in a 2.87d orbit around the bright (V=10.1), hot, F4V star BD+60 1538 (TYC 3865-1173-1). We present follow-up photomet…

astro-ph.EP2017★ 39 cited

Challenges to Constraining Exoplanet Masses via Transmission Spectroscopy

Natasha E. Batalha, Eliza M. -R. Kempton, Rostom Mbarek

MassSpec, a method for determining the mass of a transiting exoplanet from its transmission spectrum alone, was proposed by \citet{dew13}. The premise of this method relies on the…