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Parkes observations for project P574 semester 2018OCTS_04

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About this Collection

Parkes observations for project P574 semester 2018OCTS_04


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


Astronomical and Space Sciences not elsewhere classified


https://doi.org/10.25919/5c940abebba59


01 Oct 2018


01 Apr 2019


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pulsars neutron stars P574_2018OCTS


Creative Commons Attribution 4.0 International Licence


CSIRO (Australia)


Dai, Shi; Possenti, Andrea; Manchester, Dick; Johnston, Simon; Hobbs, George; Weltevrede, Patrick; Kerr, Matthew; Shannon, Ryan; Ilie, Cristina-Diana; Sobey, Charlotte (2018): Parkes observations for project P574 semester 2018OCTS_04. v1. CSIRO. Data Collection. https://doi.org/10.25919/5c940abebba59


All Rights (including copyright) CSIRO 2018.


Access to this collection's metadata and/or files (if any) are restricted until 01 Oct 2020.

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More about this Collection

ivo://au.csiro.atnf/P574-2018OCTS_04


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


Shi Dai


Andrea Possenti


Dick Manchester


Simon Johnston


George Hobbs


Patrick Weltevrede


Matthew Kerr


Ryan Shannon


Cristina-Diana Ilie


Charlotte Sobey


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