424 citations
- Tel Aviv UniversityIL60 papers
- Universidad Andrés BelloCL26 papers
- European Southern ObservatoryCL16 papers
- Pontificia Universidad Católica de ChileCL14 papers
- University of ConcepciónCL14 papers
- Centre National de la Recherche ScientifiqueFR13 papers
- National Institute for AstrophysicsIT11 papers
- Max Planck Institute for AstrophysicsDE8 papers
- Texas A&M UniversityUS8 papers
- University of PotsdamDE8 papers
- Carnegie Institution for ScienceUS7 papers
- Heidelberg UniversityDE7 papers
171 papers
Consensus In Asynchrony: Strictly Formal
Ivan Klianev
In this paper, we resolve the apparent contradiction between the proven possibility of deterministic crash-tolerant consensus in a fully asynchronous environment and the reconfirma…
4MOST ChANGES: Catalog of high-redshift quasar candidates (4.5 < < 7) selected with SED fitting
T. Mkrtchyan, C. Mazzucchelli, R. J. Assef +12
The identification of high-redshift quasars () is critical for studying the early Universe, supermassive black hole growth, and cosmic reionization. Most known high-redshi…
Constraining an exoplanets magnetic field using star-planet interactions
D. Revilla, P. J. Amado, R. Luque +17
Theory predicts that a planet with a sufficiently strong magnetic field orbiting close to its host star could induce star-planet magnetic interactions. This is potentially observab…
Search for TeV emission from spider millisecond pulsars with HAWC
R. Alfaro, E. Anita-Rangel, M. Araya +90
Millisecond pulsars (MSPs) are observed to emit multi-wavelength radiation, from radio to GeV. Spider MSPs, which interact with their low-mass companion in close orbit (orbital per…
Kinematical and dynamical properties of recently discovered bulge and disc star clusters with WINERED
Ilaria Petralia, Dante Minniti, José G. Fernández-Trincado +8
Context. Galactic globular clusters are a very important tool in explaining the characteristics of the Milky Way. Therefore it is essential to determine the kinematical and dynamic…
Hydrogen photoionization in a magnetized medium: the rigid-wavefunction approach revisited
René D. Rohrmann
Realistic modeling of stellar spectra requires accurate radiative opacity coefficients. Owing to the fragmentary nature of existing data from rigorous quantum-mechanical calculatio…