Affordable Access

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

Publication Date


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: [email protected] 2 Astronomy Centre, University of Sussex, Falmer, BN1 9QJ, UK e-mail: [email protected] 3 Stichting ASTRON, Postbus 2, 7990 AA Dwingeloo, The Netherlands e-mail: [email protected] 4 Physics Department, 405 Cook Physical Science building, University of Vermont, Burlington 05405, USA e-mail: [email protected] 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

There are no comments yet on this publication. Be the first to share your thoughts.


Seen <100 times