# pinta

pinta is a data reduction pipeline for pulsar data taken using the upgraded Giant Metre-wave Radio Telescope (uGMRT). It takes the uGMRT raw pulsar data as input, does RFI mitigation and folding, and gives partially folded profile archives as output. It is now an observatory pipeline at GMRT. This pipeline was described in this paper.

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# ugmrt2fil

ugmrt2fil is a program to convert uGMRT raw pulsar data to sigproc-filterbank format. It is a part of the pinta pipeline.

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# GWecc

GWecc is a library used to compute Pulsar Timing Array (PTA) signals due to gravitational waves emitted by black hole binaries. It is designed to be called from PTA data analysis packages like ENTERPRISE. It can also be used to simulate pulsar time of arrivals using packages like libstempo and PINT. This code is described in this paper.

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# mikkola

This is an implementation of Mikkola’s method for solving the classical Kepler equation.

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