no code implementations • 12 Jan 2021 • Main Pal, Neeraj Kumari, Pankaj Kushwaha, K. P. Singh, Alok C. Gupta, Sachindra Naik, G. C. Dewangan, P. Tripathi, Rathin Adhikari, O. Adegoke, H. Nandan
Both observations show extremely variable soft and hard X-ray emission that are correlated with each other.
High Energy Astrophysical Phenomena
no code implementations • 16 Oct 2020 • Piotr Homola, Dmitriy Beznosko, Gopal Bhatta, Lukasz Bibrzycki, Michalina Borczynska, Lukasz Bratek, Nikolai Budnev, Dariusz Burakowski, David E. Alvarez-Castillo, Kevin Almeida Cheminant, Aleksander Cwikla, Punsiri Dam-o, Niraj Dhital, Alan R. Duffy, Piotr Glownia, Krzysztof Gorzkiewicz, Dariusz Gora, Alok C. Gupta, Zuzana Hlavkova, Martin Homola, Joanna Jalocha, Robert Kaminski, Michal Karbowiak, Marcin Kasztelan, Renata Kierepko, Marek Knap, P eter Kov acs, Szymon Kuli nski, Bartosz L ozowski, Marek Magrys, Mikhail V. Medvedev, Justyna Mkedrala, Jerzy W. Mietelski, Justyna Miszczyk, Alona Mozgova, Antonio Napolitano, Vahab Nazari, Y. Jack Ng, Michal Niedzwiecki, Cristina Oancea, Boguslaw Ogan, Gabriela Opila, Krzysztof Oziomek, Maciej Pawlik, Marcin Piekarczyk, Bozena Poncyliusz, Jerzy Pryga, Matias Rosas, Krzysztof Rzecki, Jilberto Zamora-Saa, Katarzyna Smelcerz, Karel Smolek, Weronika Stanek, Jaroslaw Stasielak, Slawomir Stuglik, Jolanta Sulma, Oleksandr Sushchov, Manana Svanidze, Kyle Tam, Arman Tursunov, Jose M. Vaquero, Tadeusz Wibig, Krzysztof W. Wozniak
The Cosmic Ray Extremely Distributed Observatory (CREDO) is a newly formed, global collaboration dedicated to observing and studying cosmic rays (CR) and cosmic ray ensembles (CRE): groups of a minimum of two CR with a common primary interaction vertex or the same parent particle.
High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics
no code implementations • 4 Mar 2020 • Arkadipta Sarkar, Alok C. Gupta, Varsha R. Chitnis, Paul J. Wiita
We report the detection ($>4\sigma$) of a Quasi-Periodic Oscillation (QPO) in the $\gamma$-ray light curve of 3C 454. 3 along with a simultaneous marginal QPO detection ($>2. 4\sigma$) in the optical light curves.
High Energy Astrophysical Phenomena
