The Citing articles tool gives a list of articles citing the current article. The citing articles come from EDP Sciences database, as well as other publishers participating in CrossRef Cited-by Linking Program. You can set up your personal account to receive an email alert each time this article is cited by a new article (see the menu on the right-hand side of the abstract page).
Degenerate Interpretations of O3 Spectral Features in Exoplanet Atmosphere Observations Due to Stellar UV Uncertainties: A 3D Case Study with TRAPPIST-1 e
HAZMAT. IX. An Analysis of the UV and X-Ray Evolution of Low-mass Stars in the Era of Gaia
Tyler Richey-Yowell, Evgenya L. Shkolnik, Adam C. Schneider, Sarah Peacock, Lori A. Huseby, James A. G. Jackman, Travis Barman, Ella Osby and Victoria S. Meadows The Astrophysical Journal 951(1) 44 (2023) https://doi.org/10.3847/1538-4357/acd2dc
Accurate Modeling of Lyα Profiles and Their Impact on Photolysis of Terrestrial Planet Atmospheres
Sarah Peacock, Travis S. Barman, Adam C. Schneider, Michaela Leung, Edward W. Schwieterman, Evgenya L. Shkolnik and R. O. Parke Loyd The Astrophysical Journal 933(2) 235 (2022) https://doi.org/10.3847/1538-4357/ac77f2
Reconstructing the Extreme Ultraviolet Emission of Cool Dwarfs Using Differential Emission Measure Polynomials
Girish M. Duvvuri, J. Sebastian Pineda, Zachory K. Berta-Thompson, Alexander Brown, Kevin France, Adam F. Kowalski, Seth Redfield, Dennis Tilipman, Mariela C. Vieytes, David J. Wilson, Allison Youngblood, Cynthia S. Froning, Jeffrey Linsky, R. O. Parke Loyd, Pablo Mauas, Yamila Miguel, Elisabeth R. Newton, Sarah Rugheimer and P. Christian Schneider The Astrophysical Journal 913(1) 40 (2021) https://doi.org/10.3847/1538-4357/abeaaf
Cloud Properties of Brown Dwarf Binaries across the L/T Transition
HAZMAT VI: The Evolution of Extreme Ultraviolet Radiation Emitted from Early M Stars
Sarah Peacock, Travis Barman, Evgenya L. Shkolnik, R. O. Parke Loyd, Adam C. Schneider, Isabella Pagano and Victoria S. Meadows The Astrophysical Journal 895(1) 5 (2020) https://doi.org/10.3847/1538-4357/ab893a
A 3D short-characteristics method for continuum and line scattering problems in the winds of hot stars
Distinguishing between Wet and Dry Atmospheres of TRAPPIST-1 e and f
Fabian Wunderlich, Markus Scheucher, M. Godolt, J. L. Grenfell, F. Schreier, P. C. Schneider, D. J. Wilson, A. Sánchez-López, M. López-Puertas and H. Rauer The Astrophysical Journal 901(2) 126 (2020) https://doi.org/10.3847/1538-4357/aba59c
Predicting the Extreme Ultraviolet Radiation Environment of Exoplanets around Low-mass Stars: GJ 832, GJ 176, and GJ 436
Sarah Peacock, Travis Barman, Evgenya L. Shkolnik, Peter H. Hauschildt, E. Baron and Birgit Fuhrmeister The Astrophysical Journal 886(2) 77 (2019) https://doi.org/10.3847/1538-4357/ab4f6f
Predicting the Extreme Ultraviolet Radiation Environment of Exoplanets around Low-mass Stars: The TRAPPIST-1 System
Sarah Peacock, Travis Barman, Evgenya L. Shkolnik, Peter H. Hauschildt and E. Baron The Astrophysical Journal 871(2) 235 (2019) https://doi.org/10.3847/1538-4357/aaf891
The Effects of Telluric Contamination in Iodine-calibrated Precise Radial Velocities
Pushing Automated Abundance Derivations into the Cool Dwarf Regime: A Test Using Three G and Two K Stars in Praesepe∗
Marwan Gebran, Marcel A. Agüeros, Keith Hawkins, Simon C. Schuler and Brett M. Morris The Astrophysical Journal 871(2) 142 (2019) https://doi.org/10.3847/1538-4357/aaf721
3D radiative transfer: Continuum and line scattering in non-spherical winds from OB stars
An open-source, massively parallel code for non-LTE synthesis and inversion of spectral lines and Zeeman-induced Stokes profiles
H. Socas-Navarro, J. de la Cruz Rodríguez, A. Asensio Ramos, J. Trujillo Bueno and B. Ruiz Cobo Astronomy & Astrophysics 577 A7 (2015) https://doi.org/10.1051/0004-6361/201424860
Determination of Atmospheric Parameters of B-, A-, F- and G-Type Stars
Maria Bergemann GeoPlanet: Earth and Planetary Sciences, Determination of Atmospheric Parameters of B-, A-, F- and G-Type Stars 187 (2014) https://doi.org/10.1007/978-3-319-06956-2_17
THREE-DIMENSIONAL SIMULATIONS OF PURE DEFLAGRATION MODELS FOR THERMONUCLEAR SUPERNOVAE