F. Nappo
University of Insubria
20 Papers
227 Citations
F. Nappo is an academic researcher from University of Insubria. The author has contributed to research in topics: Gamma-ray burst & Computer science. The author has an hindex of 12, co-authored 12 publications. Previous affiliations of F. Nappo include INAF.
Chat about Author
Papers
Short gamma-ray bursts at the dawn of the gravitational wave era
Giancarlo Ghirlanda,Om Sharan Salafia,Om Sharan Salafia,A. Pescalli,A. Pescalli,Gabriele Ghisellini,Ruben Salvaterra,E. Chassande Mottin,Monica Colpi,Monica Colpi,F. Nappo,F. Nappo,P. D'Avanzo,A. Melandri,M. G. Bernardini,M. Branchesi,Sergio Campana,Riccardo Ciolfi,Stefano Covino,D. Gotz,S. D. Vergani,S. D. Vergani,Matteo Zennaro,Matteo Zennaro,G. Tagliaferri +24 more
TL;DR: In this paper, the authors derived the luminosity function φ (L ) and redshift distribution Ψ(z ) of short gamma-ray bursts (SGRBs) using all the available observer-frame constraints (i.e., peak flux, fluence, peak energy and duration distributions) and the rest-frame properties of a complete sample of SGRBs detected by Swift.
156
Short GRBs at the dawn of the gravitational wave era
G. Ghirlanda,Om Sharan Salafia,A. Pescalli,G. Ghisellini,Ruben Salvaterra,E. Chassande-Mottin,M. Colpi,F. Nappo,P. D'Avanzo,A. Melandri,M. G. Bernardini,M. Branchesi,Sergio Campana,Riccardo Ciolfi,Stefano Covino,Diego Götz,S. D. Vergani,Matteo Zennaro,G. Tagliaferri +18 more
TL;DR: In this article, the authors derived the luminosity function and redshift distribution of short Gamma Ray Bursts (SGRBs) using all the available observer-frame constraints (i.e. peak flux, fluence, peak energy and duration distributions) of the large population of Fermi SGRBs and the rest-frame properties of a complete sample of Swift SGRB.
Unveiling the population of orphan Gamma Ray Bursts
G. Ghirlanda,Ruben Salvaterra,Sergio Campana,S. D. Vergani,J. Japelj,M. G. Bernardini,D. Burlon,P. D'Avanzo,A. Melandri,A. Gomboc,F. Nappo,R. Paladini,A. Pescalli,Om Sharan Salafia,G. Tagliaferri +14 more
TL;DR: In this paper, the authors estimate the expected flux of the population of orphan afterglows in the mm, optical and X-ray bands through a population synthesis code of GRBs and the standard afterglow emission model.
The high-redshift gamma-ray burst GRB140515A
A. Melandri,M. G. Bernardini,P. D'Avanzo,R. Sanchez-Ramirez,F. Nappo,Lara Nava,J. Japelj,A. de Ugarte Postigo,S. R. Oates,Sergio Campana,Stefano Covino,V. D'Elia,G. Ghirlanda,E. Gafton,G. Ghisellini,Nickolay Y. Gnedin,P. Goldoni,J. Gorosabel,Tine Libbrecht,D. Malesani,Ruben Salvaterra,C. C. Thöne,S. D. Vergani,Da Xu,G. Tagliaferri +24 more
TL;DR: In this article, the authors presented the multi-wavelength analysis of the high-z$ Swift gamma-ray burst GRB140515A ($z = 6.327$).
The 999th Swift Gamma-Ray Burst: some like it thermal
F. Nappo,A. Pescalli,Gor Oganesyan,G. Ghirlanda,Marcello Giroletti,A. Melandri,Sergio Campana,G. Ghisellini,Om Sharan Salafia,P. D'Avanzo,M. G. Bernardini,Stefano Covino,E. Carretti,Annalisa Celotti,V. D'Elia,Lara Nava,E. Palazzi,S. Poppi,Isabella Prandoni,Simona Righini,A. M. Rossi,Ruben Salvaterra,G. Tagliaferri,Vincenzo Testa,Tiziana Venturi,S. D. Vergani +25 more
TL;DR: In this paper, a multi-wavelength study of GRB 151027A is presented, which is the 999th GRB detected by the Swift satellite and it has a densely sampled emission in the X-ray and optical band and has been observed and detected in the radio up to 140 days after the prompt.