In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 48, no. 1
M. Yu
Detaily:
Rok, strany: 2018, 259 - 261
Kľúčové slová:
pulsars: general, stars: neutron
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2018/Vol_48/No_1/pp259-261_abstract.html
O článku:
Neutron star glitches are observed via artificially scheduled pulsar pulse arrival-time observations.
The detection probability density of glitch events for a given data set is an essentially required knowledge
for realizing glitch detectability with a specified observing system and schedule.
In Yu & Liu (2017), the detection probability density was derived for the Yu et al. (2013)
data set. In this proceeding, further discussions are presented.
Ako citovať:
ISO 690:
Yu, M. 2018. Have we seen all glitches?. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 48, no.1, pp. 259-261. 1335-1842.
APA:
Yu, M. (2018). Have we seen all glitches?. Contributions of the Astronomical Observatory Skalnaté Pleso, 48(1), 259-261. 1335-1842.