Issue |
A&A
Volume 618, October 2018
|
|
---|---|---|
Article Number | C1 | |
Number of page(s) | 1 | |
Section | Astrophysical processes | |
DOI | https://doi.org/10.1051/0004-6361/201731519e | |
Published online | 05 October 2018 |
The glitch activity of neutron stars (Corrigendum)
1
Instituto de Astrofísica, Pontificia Universidad Católica de Chile, Av. Vicuña Mackenna 4860, 7820436 Macul, Santiago, Chile
e-mail: jrfuentes@uc.cl
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
”.
Equation (3) and its description is written as(3)
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
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