A multi-wavelength pipeline for pulsar observations

The Astronomical Observatory in Cagliari (OAC) is a growing facility with a group devoted to pulsar 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, Bolli et al. 2015, Prandoni et al. 2017).

Coverage

Pulsar Astrophysics the Next Fifty Years

All editors

Weltevrede, P.; Perera, B.B.P.;Preston, L.L.; Sanidas, S.

Series

PROCEEDINGS OF THE INTERNATIONAL ASTRONOMICAL UNION

Volume

vol. 13, S337

Start page

394

Conferenece

Pulsar Astrophysics the Next Fifty Years

Conferenece place

Jodrell Bank Observatory, United Kingdom

Conferenece date

4-8 September, 2017

Uri

http://hdl.handle.net/20.500.12386/28193

Url

https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/multiwavelength-pipeline-for-pulsar-observations/B493CD58386DEBDBD1DB1EA7704AF7C2

Issn Identifier

1743-9213

Ads BibCode

2018IAUS..337..394P

Rights

open.access

File(s)

Name

Pilia18_IAUS.pdf

Description

Pdf editoriale

Size

159.7 KB

Format

Adobe PDF

Checksum (MD5)

9c03546e5833ffdc6aac222d4c39b41c

A multi-wavelength pipeline for pulsar observations

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