|Savitribai Phule Pune University||All Models Are False, Some Are Useful|
|Title||Inferring a characteristic timescale for pulsar microstructure|
Centre for Modeling and Simulation, Savitribai Phule Pune University, Pune 411 007, India
National Centre for Radio Astrophysics, Pune 411 007, India
Department of Physics, University of Vermont, Burlington, VT 05405 USA
|Abstract||We describe a method to extract quasiperiodicities observed in pulsar single pulses reliably, and then to infer their characteristic timescale. The method is applied to PSR B0301+19 data at time resolution of 59.5 μs from Arecibo Observatory.|
|Citing This Document||Mihir Arjunwadkar, Dipanjan Mitra, and Joanna Rankin , Inferring a characteristic timescale for pulsar microstructure . Technical Report CMS-TR-20131210 of the Centre for Modeling and Simulation, Savitribai Phule Pune University, Pune 411007, India (2013); available at http://cms.unipune.ac.in/reports/.|
|Notes, Published Reference, Etc.||
Work presented at the conference The Metre Wavelength Sky: Celebrating 50 years of Radio Astronomy at TIFR & 10 years of GMRT, 9-13 December 2013. To be published in Bulletin of the Astronomical Society of India.
An extended report on this work is available as CMS-TR-20150223.
|Contact||mihir AT cms.unipune.ac.in, dmitra AT ncra.tifr.res.in, Joanna.Rankin AT uvm.edu|