# A multi-wavelength pipeline for pulsar searches

**Authors:** Maura Pilia, Alessio Trois, Matteo Bachetti, Alberto Pellizzoni,, Giuseppe Atzeni, Elise Egron, Maria Noemi Iacolina, Sara Loru, Antonio, Poddighe, Valentina Vacca

arXiv: 1904.02686 · 2019-04-05

## TL;DR

This paper presents a comprehensive multi-wavelength pipeline integrating radio, gamma-ray, and X-ray data to enhance pulsar detection and study across the electromagnetic spectrum.

## Contribution

It introduces a new suite of software and databases that unify multi-wavelength observations for pulsar research at the Sardinia Radio Telescope.

## Key findings

- Enhanced pulsar detection capabilities across multiple wavelengths.
- Integrated data processing pipeline for radio, gamma-ray, and X-ray observations.
- Facilitates cross-referencing and combined analysis of pulsar data.

## 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.

## Full text

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## Figures

1 figure with captions in the complete paper: https://tomesphere.com/paper/1904.02686/full.md

## References

8 references — full list in the complete paper: https://tomesphere.com/paper/1904.02686/full.md

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Source: https://tomesphere.com/paper/1904.02686