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Henrique Reggiani
Henrique Reggiani
Johns Hopkins University
Astrophysics
Physics
Metallicity
Stars
Milky Way
5
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1
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The relationship between photometric and spectroscopic oscillation amplitudes from 3D stellar atmosphere simulations
2021
Monthly Notices of the Royal Astronomical Society
Yixiao Zhou
Thomas Nordlander
Luca Casagrande
Meridith Joyce
Yaguang Li
A. M. Amarsi
Henrique Reggiani
Martin Asplund
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Searching for new solar twins: The Inti survey for the Northern Sky
2021
Monthly Notices of the Royal Astronomical Society
Jhon Yana Galarza
Ricardo Lopez-Valdivia
Diego Lorenzo-Oliveira
Henrique Reggiani
Jorge Melendez
Daniel Gamarra-Sánchez
M. Flores
Jerry Portal-Rivera
P. Miquelarena
Geisa Ponte
Kevin C. Schlaufman
Teófilo Vargas Auccalla
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The relationship between photometric and spectroscopic oscillation amplitudes from 3D stellar atmosphere simulations
2021
arXiv: Solar and Stellar Astrophysics
Yixiao Zhou
Thomas Nordlander
Luca Casagrande
Meridith Joyce
Yaguang Li
A. M. Amarsi
Henrique Reggiani
Martin Asplund
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The Most Metal-poor Stars in the Magellanic Clouds are $r$-process Enhanced
2021
arXiv: Astrophysics of Galaxies
Henrique Reggiani
Kevin C. Schlaufman
Andrew R. Casey
Joshua D. Simon
andAlexander P. Ji
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The Most Metal-poor Stars in the Inner Bulge
2020
arXiv: Solar and Stellar Astrophysics
Henrique Reggiani
Kevin C. Schlaufman
Andrew R. Casey
Alexander P. Ji
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