568 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Institute of Space SciencesES9 papers
- Universitat de BarcelonaES9 papers
- Institut d'Estudis Espacials de CatalunyaES8 papers
- Universitat Politècnica de CatalunyaES6 papers
- Institut de Ciències del CosmosES4 papers
- Osservatorio Astronomico di PadovaIT4 papers
- Astronomy and SpaceAU3 papers
- Brera Astronomical ObservatoryIT3 papers
- Chongqing University of Posts and TelecommunicationsCN3 papers
- Collurania Teramo ObservatoryIT3 papers
- University of Chinese Academy of SciencesCN3 papers
- University of North Carolina at Chapel HillUS3 papers
5 papers · 1 filter
SN 2022ngb: A faint, slowly evolving Type IIb supernova with a low-mass envelope
J. -W. Zhao, S. Benetti, Y. -Z. Cai +35
An extensive photometric and spectroscopic follow-up campaign of the Type IIb SN 2022ngb is presented in the article. Through detailed modeling of this dataset, we aim to constrain…
SN 2016iog: A fast declining Type II-L supernova with an ultra-faint tail, persistently interacting with circumstellar material
Z. -H. Peng, S. Benetti, Y. -Z. Cai +26
We present optical photometric and spectroscopic observations of the rapidly declining Type IIL supernova (SN) 2016iog. SN 2016iog reached its peak 14 days after explosion,…
SN2017ckj: A linearly declining Type IIb supernova with a relatively massive hydrogen envelope
L. -H. Li, S. Benetti, Y. -Z. Cai +26
We present optical observations of the Type IIb supernova (SN) 2017ckj, covering approximately 180 days after the explosion. Its early-time multi-band light curves display no clear…
Can we reveal the core-chemical composition of ultra-massive white dwarfs through their magnetic fields?
Maria E. Camisassa, Roberto Raddi, Leandro G. Althaus +5
Ultra-massive white dwarfs () are particularly interesting objects that allow us to study extreme astrophysical phenomena such as type Ia superno…
The HADES RV Programme with HARPS-N@TNG IV. Time resolved analysis of the Ca ii H&K and Hα chromospheric emission of low-activity early-type M dwarfs
G. Scandariato, J. Maldonado L. Affer, K. Biazzo +22
M dwarfs are prime targets for planet search programs, particularly of those focused on the detection and characterization of rocky planets in the habitable zone. Understanding the…