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Parkes observations for project P1013 semester 2019APRS_05

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About this Collection

Parkes observations for project P1013 semester 2019APRS_05


The paucity of known intermittent pulsars makes individual studies valuable from the perspective of understanding how these pulsars emit and how that emission is changing in time and as a function of frequency. The inherent difficulty in detecting these objects implies that their small population may well simply be a sampling bias, thus studying in... more


Astronomical and Space Sciences not elsewhere classified


https://doi.org/10.25919/5d9e58d8c1f90


01 Apr 2019


30 Sep 2019


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pulsars neutron stars P1013_2019APRS


Creative Commons Attribution 4.0 International Licence


CSIRO (Australia)


Meyers, Bradley; Johnston, Simon; Hobbs, George; Bhat, Ramesh; Shannon, Ryan; Wang, Jingbo; Dai, Shi; Tremblay, Steven (2019): Parkes observations for project P1013 semester 2019APRS_05. v1. CSIRO. Data Collection. https://doi.org/10.25919/5d9e58d8c1f90


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/P1013-2019APRS_05


About this Project

Australia Telescope National Facility


P1013 - An ultra-wide-band study of the intermittent pulsar J1107-5907


Astronomers still do not fully understand how pulsars shine at radio wavelengths. On top of that, there are some special pulsars that don't shine continuously, and are instead mostly "off". One particular subclass of these objects are called intermittent pulsars, and they exhibit some of the most extreme examples of switching between "off" and "on"... more


Observation


Parkes


Bradley Meyers


Simon Johnston


George Hobbs


Ramesh Bhat


Ryan Shannon


Jingbo Wang


Shi Dai


Steven Tremblay


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