Scientific Computing, Modeling & Simulation
Savitribai Phule Pune University

Technical Report CMS-TR-20131210


Title Inferring a characteristic timescale for pulsar microstructure
Author/s Mihir Arjunwadkar
Centre for Modeling and Simulation, Savitribai Phule Pune University, Pune 411 007, India


Dipanjan Mitra
National Centre for Radio Astrophysics, Pune 411 007, India


Joanna Rankin
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.
Keywords
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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://882291.longumnakehk.tech/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. Published as Astronomical Society of India Conference Series 13, 83-85 (2014). An extended version of this work is CMS-TR-20150223.
Contact mihir AT 882291.longumnakehk.tech, dmitra AT ncra.tifr.res.in, Joanna.Rankin AT uvm.edu
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