Data

Parkes observations for project P892 semester 2017OCTS_BPSR_01

Commonwealth Scientific and Industrial Research Organisation
Keane, Evan ; Possenti, Andrea ; Green, James ; Johnston, Simon ; Kramer, Michael ; Burgay, Marta ; Bailes, Matthew ; Bhat, Ramesh ; Burke-Spolaor, Sarah ; Eatough, Ralph ; van Straten, Willem ; Stappers, Benjamin ; Levin, Lina ; Jameson, Andrew ; Ng, Cherry ; Tiburzi, Caterina ; Petroff, Emily ; Barr, Ewan ; Flynn, Chris ; Jankowski, Fabian ; Caleb, Manisha ; Morello, Vincent ; Bhandari, Shivani ; Venkatraman Krishnan, Vivek
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ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2FANDS&rft_id=info:doi10.4225/08/5a722a56cc468&rft.title=Parkes observations for project P892 semester 2017OCTS_BPSR_01&rft.identifier=10.4225/08/5a722a56cc468&rft.publisher=Commonwealth Scientific and Industrial Research Organisation (CSIRO)&rft.description=SUPERBx is an extension to the SUPERB survey which looks at the highest Galactic latitudes in a search for fast radio bursts (FRBs). We will focus our efforts at high Galactic latitudes where our previous work has shown FRB detectability to be as much as 3 times higher than in the plane. SUPERBx uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The FRBs discovered (we have already discovered five FRBs in this project) will have much more associated information than all previous detections. Firstly our discovery lag is ~1 second, rather than months/years. The Parkes observations will be shadowed by other radio telescopes (in particular the refurbished Molonglo which has now reached a level of performance where it has independently discovered 3 FRBs) to allow localisation of the discovered FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors and to exploit their many uses as tools for precision cosmology measurements.&rft.creator=Keane, Evan &rft.creator=Possenti, Andrea &rft.creator=Green, James &rft.creator=Johnston, Simon &rft.creator=Kramer, Michael &rft.creator=Burgay, Marta &rft.creator=Bailes, Matthew &rft.creator=Bhat, Ramesh &rft.creator=Burke-Spolaor, Sarah &rft.creator=Eatough, Ralph &rft.creator=van Straten, Willem &rft.creator=Stappers, Benjamin &rft.creator=Levin, Lina &rft.creator=Jameson, Andrew &rft.creator=Ng, Cherry &rft.creator=Tiburzi, Caterina &rft.creator=Petroff, Emily &rft.creator=Barr, Ewan &rft.creator=Flynn, Chris &rft.creator=Jankowski, Fabian &rft.creator=Caleb, Manisha &rft.creator=Morello, Vincent &rft.creator=Bhandari, Shivani &rft.creator=Venkatraman Krishnan, Vivek &rft.date=2018&rft.edition=v1&rft_rights=All Rights (including copyright) CSIRO 2018.&rft_rights=Creative Commons Attribution https://creativecommons.org/licenses/by/4.0/&rft_subject=pulsars, neutron stars, compact binaries and/or black-holes, interstellar medium in and around the Milky Way, magnetic fields, HIPSR, BPSR&rft_subject=Astronomical and Space Sciences not elsewhere classified&rft_subject=PHYSICAL SCIENCES&rft_subject=ASTRONOMICAL AND SPACE SCIENCES&rft.type=dataset&rft.language=English Access the data

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All Rights (including copyright) CSIRO 2018.

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Brief description

SUPERBx is an extension to the SUPERB survey which looks at the highest Galactic latitudes in a search for fast radio bursts (FRBs). We will focus our efforts at high Galactic latitudes where our previous work has shown FRB detectability to be as much as 3 times higher than in the plane. SUPERBx uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The FRBs discovered (we have already discovered five FRBs in this project) will have much more associated information than all previous detections. Firstly our discovery lag is ~1 second, rather than months/years. The Parkes observations will be shadowed by other radio telescopes (in particular the refurbished Molonglo which has now reached a level of performance where it has independently discovered 3 FRBs) to allow localisation of the discovered FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors and to exploit their many uses as tools for precision cosmology measurements.

Data time period: 2017-09-30 to 2018-03-31

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