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Parkes observations for project P574 semester 2015APRS_BPSR_02

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Parkes observations for project P574 semester 2015APRS_BPSR_02


We request time to observe 230 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/10.4225/08/58dd14f15d2ac


01 Apr 2015


30 Sep 2015


CSIRO Enquiries
CSIROEnquiries@csiro.au
1300 363 400

pulsars neutron stars BPSR HIPSR


Creative Commons Attribution 3.0 Unported Licence


CSIRO (Australia)


Kerr, Matthew; Possenti, Andrea; Manchester, R; Johnston, Simon; Hobbs, George; Romani, Roger W.; Thompson, David J.; Weltevrede, Patrick; Shannon, Ryan; Petroff, Emily; Brook, Paul (2015): Parkes observations for project P574 semester 2015APRS_BPSR_02. v1. CSIRO. Data Collection. https://doi.org/10.4225/08/58dd14f15d2ac


All Rights (including copyright) CSIRO Australia 2015.


The metadata and files (if any) are available to the public.

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More about this Collection

ivo://au.csiro.atnf/P574-2015APRS_BPSR_02


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


Matthew Kerr


Andrea Possenti


Dick Manchester


Simon Johnston


George Hobbs


R Romani


David J. Thompson


Patrick Weltevrede


Ryan Shannon


Emily Petroff


Paul Brook


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