output
20102026
most citedVariations of the Similarity Function of TextRank for Automated Summarization

112 citations

researchers with a paper here

Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.

collaborating institutions
Showing astro-ph.SRShow all

11 papers · 1 filter

astro-ph.SR2023★ 5 cited

Modeling the Mg I from the NUV to MIR. II. Testing stellar models

J. I. Peralta, M. C. Vieytes, A. M. P. Mendez +1

Aims. We tested the new atomic model using atmospheric models of stars of different spectral types: the Sun (dG2), HD22049 (dK2, Epsilon Eridani), GJ 832 (dM2), and GJ 581 (dM3). M…

astro-ph.SR2022★ 5 cited

Enthalpy-based modeling of tomographically reconstructed quiet-Sun coronal loops

C. Mac Cormack, M. López Fuentes, C. H. Mandrini +2

The structure of the solar corona is made of magnetic flux tubes or loops. Due to the lack of contrast with their environment, observing and studying coronal loops in the quiet Sun…

astro-ph.SR2021★ 4 cited

Modeling the MgI from the NUV to MIR: I. The Solar Case

J. I. Peralta, M. C. Vieytes, A. M. P. Mendez +1

Semi-empirical models of the solar atmosphere are used to study the radiative environment of any planet in our solar system. There is a need for reliable atomic data for neutral at…

astro-ph.SR2020★ 25 cited

Semi-Empirical Modeling of the Atmospheres of the M Dwarf Exoplanet Hosts GJ 832 and GJ 581

Dennis Tilipman, Mariela Vieytes, Jeffrey L. Linsky +2

Stellar ultraviolet (UV) radiation drives photochemistry, and extreme-ultraviolet (EUV) radiation drives mass loss in exoplanet atmospheres. However, the UV flux is partly unobserv…

astro-ph.SR2020★ 2 cited

Three-Dimensional Reconstruction and Thermal Modelling of Observed Loops

F. A. Nuevo, C. Mac Cormack, M. López Fuentes +2

Due to their characteristic temperature and density, loop structures in active regions (ARs) can be seen bright in extreme ultraviolet (EUV) and soft X-ray images. The semiempirica…

astro-ph.SR2020★ 31 cited

Estimating the Ultraviolet Emission of M dwarfs with Exoplanets from Ca II and H

Katherine Melbourne, Allison Youngblood, Kevin France +29

M dwarf stars are excellent candidates around which to search for exoplanets, including temperate, Earth-sized planets. To evaluate the photochemistry of the planetary atmosphere,…

astro-ph.SR2020★ 20 cited

Thermodynamic Structure of the Solar Corona: Tomographic Reconstructions and MHD Modeling

D. G. Lloveras, A. M. Vásquez, F. A. Nuevo +5

We carry out a study of the global three-dimensional (3D) structure of the electron density and temperature of the quiescent inner solar corona () by means of tomog…

astro-ph.SR2020★ 29 cited

The UV surface habitability of Proxima b: first experiments revealing probable life survival to stellar flares

Ximena C. Abrevaya, Martin Leitzinger, Oscar oppezzo +5

We use a new interdisciplinary approach to study the UV surface habitability of Proxima under quiescent and flaring stellar conditions. We assumed planetary atmospheric composi…

astro-ph.SR2019★ 83 cited

Validation of the Alfvén Wave Solar atmosphere Model (AWSoM) with Observations from the Low Corona to 1 AU

N. Sachdeva, B. van der Holst, W. B. Manchester +9

We perform a validation study of the latest version of the Alfvén Wave Solar atmosphere Model (AWSoM) within the Space Weather Modeling Framework (SWMF). To do so, we compare the s…

astro-ph.SR2017★ 10 cited

Energy Input Flux in the Global Quiet-Sun Corona

C. Mac Cormack, A. M. Vásquez, M. López Fuentes +3

We present first results of a novel technique that provides, for the first time, constraints on the energy input flux at the coronal base () of the qui…

astro-ph.SR2016★ 18 cited

Mass Loss Evolution in the EUV Low Corona from SDO/AIA Data

Fernando M. López, Hebe Cremades, Federico A. Nuevo +2

We carry out an analysis of the evacuated mass from three coronal dimming regions observed by the {\it Atmospheric Imaging Assembly} (AIA) on board the {\it Solar Dynamics Observat…