activity
20162026
most citedHigh-precision analysis of binary stars with planets. I. Searching for condensation temperature trends in the HD 106515 system

22 citations · 99 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2026

PRICM3: A novel Polarization Ratio framework for three-dimensional CME reconstruction

Yara De Leo, Manuela Temmer, Fernando M. López +15

Coronal mass ejections (CMEs) are inherently three-dimensional (3D), but traditional white-light coronagraphs provide only two-dimensional (2D) projections. While the Polarization…

astro-ph.SR2020★ 8 cited

HATS: A Ground-Based Telescope to Explore the THz Domain

C. G. Giménez de Castro, J. -P. Raulin, A. Valio +11

The almost unexplored frequency window from submillimeter to mid-infrared (mid-IR) may bring new clues about the particle acceleration and transport processes and the atmospheric t…

astro-ph.SR2019★ 6 cited

Analysis of a long-duration AR throughout five solar rotations: Magnetic properties and ejective events

Francisco A. Iglesias, Hebe Cremades, Luciano A. Merenda +4

Coronal mass ejections (CMEs), which are among the most magnificent solar eruptions, are a major driver of space weather and can thus affect diverse human technologies. Different p…

astro-ph.SR2019★ 22 cited

High-precision analysis of binary stars with planets. I. Searching for condensation temperature trends in the HD 106515 system

C. Saffe, E. Jofre, P. Miquelarena +4

We explore the probable chemical signature of planet formation in the remarkable binary system HD 106515. The A star hosts a massive long-period planet with 9 MJup detected by radi…

astro-ph.SR2018★ 10 cited

Physical processes involved in the EUV "Surge" Event of 09 May 2012

Marcelo López Fuentes, Cristina H. Mandrini, Mariano Poisson +4

We study an EUV confined ejection observed on 09 May 2012 in active region (AR) NOAA 11476. For the analysis we use observations in multiple wavelengths (EUV, X-rays, H, and mag…

astro-ph.SR2018★ 14 cited

Using non-solar-scaled opacities to derive stellar parameters. Toward high-precision parameters and abundances

C. Saffe, M. Flores, P. Miquelarena +5

We implemented non-solar-scaled opacities in a simultaneous derivation of fundamental parameters and abundances. We carried out a high-precision stellar parameters and abundance de…

astro-ph.SR2017★ 21 cited

Moreton and EUV Waves Associated with an X1.0 Flare and CME Ejection

Carlos Francile, Fernando M. López, Hebe Cremades +3

A Moreton wave was detected in active region (AR) 12017 on 29 March 2014 with very high cadence with the Halpha Solar Telescope for Argentina (HASTA) in association with an X1.0 fl…

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…