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Parkes observations for project P574 semester 2019APRS_06

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About this Collection

Parkes observations for project P574 semester 2019APRS_06


We request time to observe 260 pulsars on a regular basis to provide the accurate ephemerides necessary for the detection and characterisation of gamma-ray pulsars with the Fermi satellite. The primary science goals are to increase the number of known gamma-ray pulsars (both radio loud and radio quiet), to determine accurate pulse profiles, and to ... more


Astronomical and Space Sciences not elsewhere classified


https://doi.org/10.25919/5d649b501e70c


01 Apr 2019


30 Sep 2019


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pulsars neutron stars interstellar medium in and around the Milky Way P574_2019APRS


Creative Commons Attribution 4.0 International Licence


CSIRO (Australia)


Sobey, Charlotte; Possenti, Andrea; Manchester, Dick; Johnston, Simon; Hobbs, George; Weltevrede, Patrick; Kerr, Matthew; Shannon, Ryan; Dai, Shi; Ilie, Cristina-Diana; Kumamoto, Hiroki (2019): Parkes observations for project P574 semester 2019APRS_06. v1. CSIRO. Data Collection. https://doi.org/10.25919/5d649b501e70c


All Rights (including copyright) CSIRO 2019.


Access to this collection's metadata and/or files (if any) are restricted until 30 Mar 2021.

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More about this Collection

ivo://au.csiro.atnf/P574-2019APRS_06


About this Project

Australia Telescope National Facility


P574 - Pulsar timing and the GLAST mission


NASA are launching a new gamma-ray satellite in October 2007. It aims to detect several hundred pulsars (only 5 are known today) but it needs radio telescopes to tell them when the pulse from each pulsar arrives. The Parkes telescope will perform this task and, at the same time, extract lots of other pulsar science from the ensuing database.


Observation


Parkes


Charlotte Sobey


Andrea Possenti


Dick Manchester


Simon Johnston


George Hobbs


Patrick Weltevrede


Matthew Kerr


Ryan Shannon


Shi Dai


Cristina-Diana Ilie


Hiroki Kumamoto


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