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Parkes observations for project P965 semester 2018APRS_01

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Parkes observations for project P965 semester 2018APRS_01


The deployment of the new ultra-wide-band receiver UWL enables a plethora of experiments which were previously not possible or very difficult. One immediate benefit for pulsar timing studies is the significantly increased ratio of available radio frequency bandwidth to the decorrelation bandwidth as induced by the ionised interstellar medium (ISM).... more


Astronomical and Space Sciences not elsewhere classified


https://doi.org/10.25919/5bbc381842324


01 Aug 2018


17 Aug 2018


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pulsars neutron stars compact binaries and/or black-holes interstellar medium in and around the Milky Way P965_2018APRS


Creative Commons Attribution 4.0 International Licence


CSIRO (Australia)


Oslowski, Stefan; Verbiest, Joris P.W. (2018): Parkes observations for project P965 semester 2018APRS_01. v1. CSIRO. Data Collection. https://doi.org/10.25919/5bbc381842324


All Rights (including copyright) CSIRO 2018.


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More about this Collection

ivo://au.csiro.atnf/P965-2018APRS_01


About this Project

Australia Telescope National Facility


P965 - Wideband timing observations of J1933-6211


We are observing the millisecond pulsar J1933-6211. It is a city-sized compact object left after a star heavier than our Sun finished producing energy in its core and collapsed. We can see the star emitting radio waves in two beams that sweep past Earth, like the beams of a light house. We are hoping to measure the mass and determine the orbit of t... more


Observation


Parkes


Stefan Oslowski


Joris P.W. Verbiest


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