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The bright spiky emission of pulsar B0656+14 (vol 458, pg 269, 2006)

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PDF/44/aa5572-06e.pdf.url A&A 459, 597 (2006) DOI: 10.1051/0004-6361:20065572e c© ESO 2006 Astronomy &Astrophysics The bright spiky emission of pulsar B0656+14 P. Weltevrede1, G. A. E. Wright2,1, B. W. Stappers3,1, and J. M. Rankin4,1 1 Astronomical Institute “Anton Pannekoek”, University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands e-mail: 2 Astronomy Centre, University of Sussex, Falmer, BN1 9QJ, UK e-mail: 3 Stichting ASTRON, Postbus 2, 7990 AA Dwingeloo, The Netherlands e-mail: 4 Physics Department, 405 Cook Physical Science building, University of Vermont, Burlington 05405, USA e-mail: A&A 458, 269–283 (2006), DOI: 10.1051/0004-6361:20065572 Key words. stars: pulsars: individual: PSR B0656+14 – stars: pulsars: general – radiation mechanisms: non-thermal – errata, addenda A misprint was inserted in Table 2 during the printing process ([2mm] was wrongly placed before AO-P1). The correct table is as follows: Table 2. The parameters of the best fits to the pulse-energy distributions of the four observations. Besides the parameters of the fitted distribution (where fweak = Nweak/Ntot is the fraction of weak pulses that are added to the distribution), also the total χ2, the number of degrees of freedom and the significance probability are tabulated. REF σ µ fweak χ2 Nd.o.f P(χ2) AO-P1 0.99 −0.34 13% 105 32 1× 10−9 AO-P2 0.79 −0.34 0% 146 24 2× 10−19 AO-L 0.56 −0.13 0% 240 44 8× 10−29 WSRT-L 0.48 −0.03 8% 148 44 4× 10−13 Article published by EDP Sciences and available at or published by EDP Sciences and available at or

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