@inproceedings{c96af576a76a4550a7cf56d306adc9a5,
title = "Periodic nulls in pulsar B1133+16",
abstract = "Numerous studies of the brightest Cambridge pulsar, B1133+16, have revealed little order in its individual pulses, apart from a weak 30-odd-rotation-period fluctuation feature and that some 15% of the star's pulsars are {"}nulls.{"} New Arecibo observations confirm this fluctuation feature and that it modulates all the emission, not simply the {"}saddle{"} region. By replacing each pulse with a scaled version of the average profile we were able to quench all subpulse modulation and thereby demonstrate that the star's {"}null{"} pulses exhibit a similar periodicity. An unabridged analysis of periodic nulling (using the techniques in this paper) in pulsar B1133+16 is in Herfindal & Rankin (2007).",
keywords = "Data analysis, Methods, Miscellaneous, Pulsars: general, individual (B1133+16), periodicities",
author = "Herfindal, {Jeffrey L.} and Rankin, {Joanna M.}",
year = "2008",
doi = "10.1063/1.2900325",
language = "English",
isbn = "9780735405028",
series = "AIP Conference Proceedings",
pages = "82--84",
booktitle = "40 Years Of Pulsars",
note = "40 Years Of Pulsars: Millisecond Pulsars, Magnetars and More ; Conference date: 12-08-2007 Through 17-08-2007",
}