A pilot ASKAP survey of radio transient events in the region around the intermittent pulsar PSR J1107-5907

G Hobbs,I Heywood,M E Bell,Michael A Kerr,A Rowlinson,S Johnston,R M Shannon,M A Voronkov,C P Ward,J Banyer,Paul J Hancock,Tara Murphy,J Allison,S W Amy,L Ball,K W Bannister,Douglas C J Bock, D Brodrick,A J Brown,John D Bunton,J D Chapman,A P Chippendale,Yuenli Chung,David R Deboer,P J Diamond,Philip G Edwards,R D Ekers,R H Ferris,R Forsyth,R G Gough, A Grancea,Navdeep Gupta,L Harveysmith,Stuart Hay,D B Hayman,A W Hotan,S Hoyle,Benjamin D Humphreys,Balthasar T Indermuehle, C E Jacka,Carole A Jackson, Susan E Jackson,Karthik B Jeganathan, Jayesh George Joseph,Richard Kendall, D Kiraly,Barbel S Koribalski,Martin O Leach,E Lenc, Andrew Macleod,S Mader, M Marquarding, J Marvil,N M Mccluregriffiths,David J Mcconnell,Peter Mirtschin, S Neuhold,A Ng,R P Norris, J D Osullivan,S Pearce,C J Phillips,Attila Popping, R Y Qiao,J E Reynolds,Patricia L Roberts,Robert J Sault,Antony Schinckel,P Serra, Rosalind Shaw,Timothy W Shimwell,Michelle C Storey, A W Sweetnam,A K Tzioumis,Tobias Westmeier,M T Whiting,Carol Wilson

Monthly Notices of the Royal Astronomical Society（2016）

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摘要

We use observations from the Boolardy Engineering Test Array (BETA) of the Australian Square Kilometre Array Pathfinder (ASKAP) telescope to search for transient radio sources in the field around the intermittent pulsar PSR J1107−5907. The pulsar is thought to switch between an ‘off’ state in which no emission is detectable, a weak state and a strong state. We ran three independent transient detec...

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关键词

pulsars: individual: J1107−5907

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