3.8k citations
- Centre National de la Recherche ScientifiqueFR1.2k papers
- European Southern ObservatoryCL792 papers
- Max Planck Institute for AstronomyDE674 papers
- California Institute of TechnologyUS485 papers
- Leiden UniversityNL459 papers
- Sorbonne UniversitéFR414 papers
- Center for Astrophysics Harvard & SmithsonianUS409 papers
- Osservatorio Astronomico di PadovaIT407 papers
- National Institute for AstrophysicsIT403 papers
- Instituto de Astrofísica de CanariasES391 papers
- Université Grenoble AlpesFR390 papers
- Max Planck Institute for Extraterrestrial PhysicsDE386 papers
30 papers · 2 filters
The Success of Optical Variability in Uncovering AGNs in Low-stellar Mass Galaxies
S. Bernal, P. Sánchez-Sáez, P. Arévalo +3
We used random forest algorithms to classify all objects in a large portion of the sky, using optical light curves obtained, or built from images provided, by the Zwicky Transient…
Feedback from intermediate mass black holes on dwarf galaxy morphology at z=2
Da Bi, Dominik R. G. Schleicher, Andres Escala
This study investigates the influence of intermediate-mass black holes (IMBHs) on galactic morphology, focusing on their evolution within dwarf galaxies at high redshift (z~2). Usi…
A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
D. Stoppacher, A. D. Montero-Dorta, M. C. Artale +4
Investigating the assembly history of the most massive and passive galaxies will enhance our understanding of why galaxies exhibit such a remarkable diversity in structure and morp…
ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- XIX. The origin of SiO emission
Rong Liu, Tie Liu, Izaskun Jiménez-Serra +23
The production of silicon monoxide (SiO) can be considered as a fingerprint of shock interaction. In this work, we use high-sensitivity observations of the SiO (2-1) and HCO…
Compact and High Excitation Molecular Clumps in the Extended Ultraviolet Disk of M83
Jin Koda, Francoise Combes, Monica Rubio +9
The extended ultraviolet (XUV) disks of nearby galaxies show ongoing massive star formation, but their parental molecular clouds remain mostly undetected despite searches in CO(1-0…
Machine learning the gap between real and simulated nebulae: A domain-adaptation approach to classify ionised nebulae in nearby galaxies
Francesco Belfiore, Michele Ginolfi, Guillermo Blanc +8
Classifying ionised nebulae in nearby galaxies is crucial to studying stellar feedback mechanisms and understanding the physical conditions of the interstellar medium. This classif…