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Parkes observations for project P1016 semester 2019APRS_06

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Parkes observations for project P1016 semester 2019APRS_06


Understanding rotating radio transients (RRATs) has the potential to uproot our understanding of core-collapse supernovae and the overall evolution of neutron stars. Despite this, RRATs remain an enigma and has numerous potential and conflicting explanations in the literature. These observations will observe a sample of RRATs with the UWL receiver,... more


Astronomical and Space Sciences not elsewhere classified


https://doi.org/10.25919/5d63c20d8ed2a


01 Apr 2019


30 Sep 2019


CSIRO Enquiries
CSIROEnquiries@csiro.au
1300 363 400

pulsars neutron stars transients P1016_2019APRS


Creative Commons Attribution 4.0 International Licence


CSIRO (Australia)


Kaczmarek, Jane; Johnston, Simon; Hobbs, George; Oslowski, Stefan; Dai, Shi (2019): Parkes observations for project P1016 semester 2019APRS_06. v1. CSIRO. Data Collection. https://doi.org/10.25919/5d63c20d8ed2a


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/P1016-2019APRS_06


About this Project

Australia Telescope National Facility


P1016 - Instant GRRATificiation


Rotating radio transients, also known as RRATs, are an enigmatic class of spinning neutron star which occasionally emits bright flashes of light. Due to their intermittent nature, it is difficult to place RRATs amongst the larger population of rotating neutron stars and pulsars. Together with the world's largest radio telescope, FAST, this project ... more


Observation


Parkes


Jane Kaczmarek


Simon Johnston


George Hobbs


Stefan Oslowski


Shi Dai


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