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
4 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…
Modelling the Milky Way's exoplanet population based on cosmological galaxy simulations
Chloé Padois, Daniel del Ser, Friedrich Anders +7
In this paper we aim to simulate realistic exoplanet populations across different regions of the MW by combining state-of-the-art cosmological simulations of our Galaxy with exopla…
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…