activity
20182020
most citedMass-Metallicity Trends in Transiting Exoplanets from Atmospheric Abundances of HO, Na, and K

231 citations · 448 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2020★ 10 cited

The nearby magnetic cool DZ white dwarf PM J08186-3110

Adela Kawka, Stéphane Vennes, Nicole F. Allard +2

We present an analysis of photometric, spectroscopic and spectropolarimetric data of the nearby, cool, magnetic DZ white dwarf PM J08186-3110. High dispersion spectra show the pres…

astro-ph.EP2019★ 231 cited

Mass-Metallicity Trends in Transiting Exoplanets from Atmospheric Abundances of HO, Na, and K

Luis Welbanks, Nikku Madhusudhan, Nicole F. Allard +3

Atmospheric compositions can provide powerful diagnostics of formation and migration histories of planetary systems. We investigate constraints on atmospheric abundances of HO,…

astro-ph.SR2019★ 145 cited

New study of the line profiles of sodium perturbed by H2

N. F. Allard, F. Spiegelman, T. Leininger +1

The opacity of alkali atoms, most importantly of Na and K, plays a crucial role in the atmospheres of brown dwarfs and exoplanets. We present a comprehensive study of NaH2 collisio…

cond-mat.str-el2019★ 18 cited

A Wigner molecule at extremely low densities: a numerically exact study

Miguel Escobar Azor, Léa Brooke, Stefano Evangelisti +4

In this work we investigate Wigner localization at very low densities by means of the exact diagonalization of the Hamiltonian. This yields numerically exact results. In particular…

cond-mat.other2018★ 33 cited

A simple position operator for periodic systems

Emilia Aragao Valença, Diego Moreno, Stefano Battaglia +5

We present a position operator that is compatible with periodic boundary conditions (PBC). It is a one-body operator that can be applied in calculations of correlated materials by…

astro-ph.SR2018★ 11 cited

Line shapes of the magnesium resonance lines in cool DZ white dwarf atmospheres

N. F. Allard, J. F. Kielkopf, S. Blouin +4

Line shapes of the magnesium resonance lines in white dwarf spectra are determined by the properties of magnesium atoms and the structure of the white dwarf atmosphere. Through the…