The MeerKAT PTA data release finds a common red noise signal with amplitude log10 A = -14.25 to -14.28, larger than other PTAs, and provides detailed noise models for 83 pulsars.
year = 1971, month = mar, volume =
3 Pith papers cite this work, alongside 59 external citations. Polarity classification is still indexing.
3
Pith papers citing it
59
external citations · Crossref
fields
astro-ph.HE 3representative citing papers
Wideband observations show M28A giant pulses differ from FRB 20200120E bursts in duration, luminosity, timing statistics, and spectral structure, yielding no strong evidence for a direct link.
A reported periodic fast radio burst is reclassified as Galactic pulsar emission due to CHIME calibration and beam-pointing error.
citing papers explorer
-
The MeerKAT Pulsar Timing Array: The $4.5$-year data release and the noise and stochastic signals of the millisecond pulsar population
The MeerKAT PTA data release finds a common red noise signal with amplitude log10 A = -14.25 to -14.28, larger than other PTAs, and provides detailed noise models for 83 pulsars.
-
Searching for links between energetic millisecond pulsars and repeating fast radio bursts
Wideband observations show M28A giant pulses differ from FRB 20200120E bursts in duration, luminosity, timing statistics, and spectral structure, yielding no strong evidence for a direct link.
-
A series of unfortunate events: CHIME/FRB misclassification of a Galactic pulsar as a periodic fast radio burst
A reported periodic fast radio burst is reclassified as Galactic pulsar emission due to CHIME calibration and beam-pointing error.