1 code implementation • 23 Dec 2020 • David R. Young, Marco Landoni, Stephen J. Smartt, Sergio Campana, Riccardo Claudi, Pietro Schipani, Matteo Aliverti, Andrea Baruffolo, Sagi Ben-Ami, Federico Biondi, Giulio Capasso, Rosario Cosentino, Francesco D'Alessio, Paolo D'Avanzo, Ofir Hershko, Hanindyo Kuncarayakti, Matteo Munari, Giuliano Pignata, Adam Rubin, Salvatore Scuderi, Fabrizio Vitali, Jani Achrén, José Antonio Araiza-Duran, Iair Arcavi, Anna Brucalassi, Rachel Bruch, Enrico Cappellaro, Mirko Colapietro, Massimo Della Valle, Marco De Pascale, Rosario Di Benedetto, Sergio D'Orsi, Avishay Gal-Yam, Matteo Genoni, Marcos Hernandez, Jari Kotilainen, Gianluca Li Causi, Seppo Mattila, Michael Rappaport, Kalyan Radhakrishnan, Davide Ricci, Marco Riva, Bernardo Salasnich, Ricardo Zanmar Sanchez, Maximilian Stritzinger, Hector Ventura
The SOXS is a dual-arm spectrograph (UV-VIS & NIR) and AC due to mounted on the ESO 3. 6m NTT in La Silla.
Instrumentation and Methods for Astrophysics
no code implementations • 23 Dec 2020 • Achille Fiore, Ting-Wan Chen, Anders Jerkstrand, Stefano Benetti, Riccardo Ciolfi, Cosimo Inserra, Enrico Cappellaro, Andrea Pastorello, Giorgos Leloudas, Steve Schulze, Marco Berton, Claudia Patricia Gutiérrez, Jamison Burke, Mariusz Gromadzki, Matt Nicholl, Arne Rau, Jesper Sollerman, Curtis McCully, Wen-fai Fong, Lluís Galbany, Daichi Hiramatsu, D. Andrew Howell, Erkki Kankare, Ragnhlid Lunnan, Tomás E. Müller-Bravo, David O Neill, David R. Young, Giacomo Terreran, Stefano Valenti
A CSM interaction scenario would imply a CSM mass of 5 Msun and an ejecta mass of 12 Msun.
High Energy Astrophysical Phenomena Solar and Stellar Astrophysics