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.

arXiv commentAccepted for publications in Rendiconti Lincei as Proceedings of "A Decade of AGILE: Results, Challenges and Prospects of Gamma-Ray Astrophysics"

References in corpus (5)

• Classification and Ranking of Fermi LAT Gamma-ray Sources from the 3FGL Catalog using Machine Learning Techniques
• Sardinia Radio Telescope: General Description, Technical Commissioning and First Light
• The Sardinia Radio Telescope: From a Technological Project to a Radio Observatory
• High-Resolution Timing Observations of Spin-Powered Pulsars with the AGILE Gamma-Ray Telescope
• Detection of Gamma-Ray Emission from the Vela Pulsar Wind Nebula with AGILE

Cited by in corpus (1)

• Real-Time Detection and Classification of Astronomical Transient Events: The State-of-the-Art