A multi-wavelength pipeline for pulsar searches
Abstract
Pulsar studies in the recent years have shown, more than others, to have benefited from a multi-wavelength approach. The INAF - Astronomical Observatory in Cagliari (INAF-OAC) is a growing facility with a young group devoted to pulsar and fast transients studies across the electromagnetic spectrum. Taking advantage of this expertise we have worked to provide a suite of multi-wavelength software and databases for the observations of pulsars and compact Galactic objects at the Sardinia Radio Telescope (SRT). In turn, radio pulsar observations at SRT will be made available, in a processed format, to gamma-ray searches using AGILE and Fermi gamma-ray satellite and, in a near future, they will be complementary to polarimetric X-ray observations with IXPE.
Cite
@article{arxiv.1904.02686,
title = {A multi-wavelength pipeline for pulsar searches},
author = {Maura Pilia and Alessio Trois and Matteo Bachetti and Alberto Pellizzoni and Giuseppe Atzeni and Elise Egron and Maria Noemi Iacolina and Sara Loru and Antonio Poddighe and Valentina Vacca},
journal= {arXiv preprint arXiv:1904.02686},
year = {2019}
}
Comments
Accepted for publications in Rendiconti Lincei as Proceedings of "A Decade of AGILE: Results, Challenges and Prospects of Gamma-Ray Astrophysics"