activity
20152023
most citedOrigin of the resistive anisotropy in the electronic nematic phase of BaFeAs revealed by optical spectroscopy

47 citations · 176 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.EP2023★ 27 cited

Exoplanet Volatile Carbon Content as a Natural Pathway for Haze Formation

E. A. Bergin, E. Kempton, M. Hirschmann +5

We explore terrestrial planet formation with a focus on the supply of solid-state organics as the main source of volatile carbon. For the water-poor Earth, the water ice line, or i…

astro-ph.EP2022★ 32 cited

Evaluating the Plausible Range of N2O Biosignatures on Exo-Earths: An Integrated Biogeochemical, Photochemical, and Spectral Modeling Approach

Edward W. Schwieterman, Stephanie L. Olson, Daria Pidhorodetska +7

Nitrous oxide (N2O) -- a product of microbial nitrogen metabolism -- is a compelling exoplanet biosignature gas with distinctive spectral features in the near- and mid-infrared, an…

astro-ph.EP2022★ 9 cited

The Role of Atmospheric Exchange in False-Positive Biosignature Detection

Ryan C. Felton, Sandra T. Bastelberger, Kathleen E. Mandt +3

Saturn's Moon Titan receives volatiles into the top of its atmosphere-including atomic oxygen-sourced from cryovolcanoes on Enceladus. Similar types of atmosphere exchange from one…

astro-ph.EP2022

The Outer Edge of the Venus Zone Around Main-Sequence Stars

Monica R. Vidaurri, Sandra T. Bastelberger, Eric T. Wolf +2

A key item of interest for planetary scientists and astronomers is the habitable zone, or the distance from a host star where a terrestrial planet can maintain necessary temperatur…

astro-ph.EP2022★ 38 cited

Effects of UV stellar spectral uncertainty on the chemistry of terrestrial atmospheres

D. J. Teal, Eliza M. -R. Kempton, Sandra Bastelberger +2

The upcoming deployment of JWST will dramatically advance our ability to characterize exoplanet atmospheres, both in terms of precision and sensitivity to smaller and cooler planet…

astro-ph.SR2021★ 23 cited

The high-energy spectrum of the nearby planet-hosting inactive mid-M dwarf LHS 3844

Hannah Diamond-Lowe, Allison Youngblood, David Charbonneau +5

To fully characterize the atmospheres, or lack thereof, of terrestrial exoplanets we must include the high-energy environments provided by their host stars. The nearby mid-M dwarf…

cond-mat.supr-con2015★ 47 cited

Origin of the resistive anisotropy in the electronic nematic phase of BaFeAs revealed by optical spectroscopy

C. Mirri, A. Dusza, S. Bastelberger +5

We perform, as a function of uniaxial stress, an optical-reflectivity investigation of the representative 'parent' ferropnictide BaFeAs in a broad spectral range, across th…