253 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- University of ViennaAT10 papers
- Centre National de la Recherche ScientifiqueFR5 papers
- Comenius University BratislavaSK5 papers
- Konkoly ObservatoryHU5 papers
- Sorbonne UniversitéFR5 papers
- Natural History MuseumGB4 papers
- University of GenevaCH4 papers
- University of StuttgartDE4 papers
- European Space Research and Technology CentreNL3 papers
- HUN-REN Research Centre for Astronomy and Earth SciencesHU3 papers
- Institut de Mécanique Céleste et de Calcul des ÉphéméridesFR3 papers
- Université Paris-SaclayFR3 papers
19 papers
Linking Young Stellar Object Morphology to Evolutionary Stages with Self-Organizing Maps
David Hernandez, Odysseas Dionatos, Marc Audard +5
Studies in the past few decades have investigated young stellar object evolution based on their spectral energy distribution (SED). The SED is heavily influenced not only by evolut…
Catastrophic disruption of asteroid 2023 CX1 and implications for planetary defense
Auriane Egal, Denis Vida, François Colas +94
Mitigation of the threat from airbursting asteroids requires an understanding of the potential risk they pose for the ground. How asteroids release their kinetic energy in the atmo…
Exploring Young Stellar Variability with Gaia DR3 light curves
Chloé Mas, Julia Roquette, Marc Audard +5
Context: Photometric variability is a defining characteristic of young stellar objects (YSO), which can be traced back to a range of physical processes taking place at different st…
The NEMESIS Catalogue of Young Stellar Objects for the Orion Star Formation Complex. I. General description of data curation
J. Roquette, M. Audard, D. Hernandez +5
The past decade has seen a rise in the use of Machine Learning methods in the study of young stellar evolution. This trend has led to a growing need for a comprehensive database of…
Spectral properties of ablating meteorite samples for improved meteoroid composition diagnostics
Pavol Matlovič, Adriana Pisarčíková, Veronika Pazderová +7
Emission spectra and diagnostic spectral features of a diverse range of ablated meteorite samples with a known composition are presented. We aim to provide a reference spectral dat…
Improved absolute abundance estimates from spatial count data with simulation and microfossil case studies
Chris Mays, Marcos Amores, Anthony Mays
Many fundamental parameters of biological systems -- eg. productivity, population sizes and biomass -- are most effectively expressed in absolute terms. In contrast to proportional…
The new Herschel/PACS Point Source Catalogue
Gábor Marton, Ilknur Gezer, Máté Madarász +6
Herschel operated as an observatory, therefore it did not cover the whole sky, but still observed ~8% of it. The first version of an overall Herschel/PACS Point Source Catalogue wa…
The Fireball of November 24, 1970, as the Most Probable Source of the Ischgl Meteorite
Maria Gritsevich, Jarmo Moilanen, Jaakko Visuri +13
In June 1976, a pristine meteorite stone weighing approximately 1 kg, fully covered with a fresh black fusion crust, was collected on a mountain road in the high-altitude Alpine en…
Analysis of CN emission as a marker of organic compounds in meteoroids using laboratory simulated meteors
Adriana Pisarčíková, Pavol Matlovič, Juraj Tóth +5
Fragments of small solar system bodies entering Earth's atmosphere have possibly been important contributors of organic compounds to the early Earth. The cyano radical (CN) emissio…
Hydrogen emission from meteors and meteorites: mapping traces of HO molecules and organic compounds in small Solar system bodies
Pavol Matlovič, Adriana Pisarčíková, Juraj Tóth +8
The hydrogen emission from meteors is assumed to originate mainly from the meteoroid composition, making it a potential tracer of HO molecules and organic compounds. H lin…
Luminous efficiency based on FRIPON meteors
Esther Drolshagen, Theresa Ott, Detlef Koschny +36
In meteor physics the luminous efficiency is used to convert the meteor's magnitude to the corresponding meteoroid's mass. However, lack of sufficiently accurate verification m…
The active lives of stars: a complete description of rotation and XUV evolution of F, G, K, and M dwarfs
Colin P. Johnstone, Michael Bartel, Manuel Güdel
Aims. We study the evolution of rotation and high energy X-ray, extreme ultraviolet (EUV), and Ly-alpha emission for F, G, K, and M dwarfs, with masses between 0.1 and 1.2 Msun, an…
Microtextures in the Chelyabinsk impact breccia reveal the history of Phosphorus-Olivine-Assemblages in chondrites
Craig R. Walton, Ioannis Baziotis, Ana Černok +4
The geochemistry and textural associations of chondritic phosphate minerals can provide insights into the geological histories of parental asteroids, but the processes governing th…
Hydrodynamic escape of water vapor atmospheres near very active stars
Colin P. Johnstone
When exposed to the high energy X-ray and ultraviolet radiation of a very active star, water vapor in the upper atmospheres of planets can be photodissociated and rapidly lost to s…
Dust of comet 67P/Churyumov-Gerasimenko collected by Rosetta/MIDAS: classification and extension to the nanometre scale
T. Mannel, M. S. Bentley, P. D. Boakes +9
The properties of the smallest subunits of cometary dust contain information on their origin and clues to the formation of planetesimals and planets. Compared to IDPs or particles…
IDEAS: Immersive Dome Experiences for Accelerating Science
Jacqueline K. Faherty, Mark SubbaRao, Ryan Wyatt +29
Astrophysics lies at the crossroads of big datasets (such as the Large Synoptic Survey Telescope and Gaia), open source software to visualize and interpret high dimensional dataset…
Aggregate dust particles at comet 67P/Churyumov-Gerasimenko
Mark S. Bentley, Roland Schmied, Thurid Mannel +9
Comets are thought to preserve almost pristine dust particles, thus providing a unique sample of the properties of the early solar nebula. The microscopic properties of this dust p…
Chromium isotope evidence in ejecta deposits for the nature of Paleoproterozoic impactors
Berengere Mougel, Frederic Moynier, Christa Gopel +1
Non-mass dependent chromium isotopic signatures have been successfully used to determine the presence and identification of extra-terrestrial materials in terrestrial impact rocks.…
A statistical dynamical study of meteorite impactors: a case study based on parameters derived from the Bosumtwi impact event
M. A. Galiazzo, Á. Bazsó, M. S. Huber +3
The study of meteorite craters on Earth provides information about the dynamic evolution of bodies within the Solar System. Bosumtwi crater is a well studied, 10.5 km in diameter,…