1.9k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- University of TurkuFI349 papers
- Centre National de la Recherche ScientifiqueFR112 papers
- Aalto UniversityFI109 papers
- University of PaduaIT102 papers
- Instituto de Astrofísica de AndalucíaES94 papers
- California Institute of TechnologyUS92 papers
- Instituto de Astrofísica de CanariasES84 papers
- Center for Astrophysics Harvard & SmithsonianUS78 papers
- Hiroshima UniversityJP75 papers
- National Institute for AstrophysicsIT74 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di PisaIT72 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di TorinoIT71 papers
6 papers · 2 filters
Modeling of the nebular-phase spectral evolution of stripped-envelope supernovae. New grids from 100 to 450 days
Luc Dessart, D. John Hillier, S. E. Woosley +1
We present an extended grid of multi-epoch 1D nonlocal thermodynamic equilibrium radiative transfer calculations for nebular-phase Type Ibc supernovae (SNe) from He-star explosions…
A characterization of ASAS-SN core-collapse supernova environments with VLT+MUSE: I. Sample selection, analysis of local environments, and correlations with light curve properties
Thallis Pessi, Jose L. Prieto, Joseph P. Anderson +17
The analysis of core-collapse supernova (CCSN) environments can provide important information on the life cycle of massive stars and constrain the progenitor properties of these po…
Dynamical mass of the white dwarf in XY Ari: a test for intermediate polar X-ray spectral models
A. Álvarez-Hernández, M. A. P. Torres, P. Rodríguez-Gil +7
We present a dynamical study of the eclipsing intermediate polar XY Ari based on time-resolved near-infrared spectroscopy obtained with the EMIR spectrograph on the 10.4-m Gran Tel…
The broad-lined Type-Ic supernova SN 2022xxf with extraordinary two-humped light curves
H. Kuncarayakti, J. Sollerman, L. Izzo +60
We report on our study of supernova (SN) 2022xxf based on observations obtained during the first four months of its evolution. The light curves (LCs) display two humps of similar m…
The morphing of decay powered to interaction powered Type II supernova ejecta at nebular times
Luc Dessart, Claudia P. Gutierrez, Hanindyo Kuncarayakti +2
Much excitement surrounds the intense mass loss that seems to take place in some massive stars immediately before core collapse. However, occurring too late, it has a negligible im…
Near-infrared evolution of the equatorial ring of SN 1987A
T. Kangas, A. Ahola, C. Fransson +4
We use adaptive-optics imaging and integral field spectroscopy from the Very Large Telescope, together with images from the \emph{Hubble Space Telescope}, to study the near-infrare…