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Parkes observations for project P885 semester 2018APRS_04

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About this Collection

Parkes observations for project P885 semester 2018APRS_04


We propose to observe PSR J1622-4950 and 1E1547.0-5408 weekly, two of three magnetars known to currently emit radio pulsations, to track their rotation, flux density, and polarisation. Less frequently we will monitor XTE J1810-197, which used to emit radio pulsations, to be on the lookout for its revival - as just happened with PSR J1622-4950,... more


Astronomical and Space Sciences not elsewhere classified


https://doi.org/10.25919/5b3c2fb00b859


20 Jun 2018


22 Jun 2018


CSIRO Enquiries
CSIROEnquiries@csiro.au
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pulsars neutron stars P885_2018APRS


Creative Commons Attribution 4.0 International Licence


CSIRO (Australia)


Camilo, Fernando; Johnston, Simon; Sarkissian, John; Reynolds, John; Scholz, Paul (2018): Parkes observations for project P885 semester 2018APRS_04. v1. CSIRO. Data Collection. https://doi.org/10.25919/5b3c2fb00b859


All Rights (including copyright) CSIRO 2018.


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

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More about this Collection

ivo://au.csiro.atnf/P885-2018APRS_04


About this Project

Australia Telescope National Facility


P885 - Understanding the Remarkable Behaviour of Radio Magnetars


Neutron stars are extreme objects, the size of a city but containing the mass of the Sun. Pulsars are neutron stars with very strong magnetic fields that rotate rapidly and emit focused beams of radio waves that we may detect on Earth once with every turn of the star, in light-house-like fashion. While the typical pulsar has a magnetic field ... more


Observation


Parkes


Fernando Camilo


Simon Johnston


John Sarkissian


John Reynolds


Paul Scholz


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