The glitch activity of neutron stars (Corrigendum)
Instituto de Astrofísica, Pontificia Universidad Católica de Chile, Av. Vicuña Mackenna 4860, 7820436 Macul, Santiago, Chile
2 Departamento de Física, Universidad de Santiago de Chile, Avenida Ecuador 3493, 9170124 Estación Central, Santiago, Chile
3 Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester, M13 9PL UK
Key words: stars: neutron / stars: magnetars / pulsars: general / stars: rotation / errata, addenda
The original article contains some errors, which are corrected below.
Introduction. Line of text number 10, shows , but it must be “”.
Figure 4. The y axis is labeled by “ (Hz s−1)”, but it must be “ (Hz s−1)”.
Section 4.2. Page number 5, “the 7th bin ” but it must be “7th bin ”.
where is the (Poisson) probability of observing a value smaller or equal to the expected value , based on the fixed ratio calculated above (and analogously for ).
where is the (Poisson) probability of obtaining a value x smaller or equal to the actual observed value , based on the fixed ratio calculated above, and the observation time of the pulsar (and analogously for ).
Discussion. Line of text number 1, shows “” but it must be “”.
© ESO 2018