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Astrophysics Source Code Library

Making codes discoverable since 1999

Searching for codes credited to 'Ransom, S. M.'

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Found 2 codes.

[ascl:2011.017] RRATtrap: Rotating Radio Transient identifier
Karako-Argaman, C.; Kaspi, V. M.; Lynch, R. S.; Hessels, J. W. T.; Kondratiev, V. I.; McLaughlin, M. A.; Ransom, S. M.; Archibald, A. M.; Boyles, J.; Jenet, F. A.; Kaplan, D. L.; Levin, L.; Lorimer, D. R.; Madsen, E. C.; Roberts, M. S. E.; Siemens, X.; Stairs, I. H.; Stovall, K.; Swiggum, J. K.; van Leeuwen, J.
RRATtrap is a single-pulse sifting algorithm to identify Rotating Radio Transients (RRATs) and transients using output from the PRESTO (ascl:1107.017) routine single_pulse_search.py. It can be integrated into pulsar survey data analysis pipelines and, in addition to finding RRATs, it can also identify Fast Radio Bursts.
[ascl:1606.013] Pulse Portraiture: Pulsar timing
Pennucci, Timothy T.; Demorest, Paul B.; Ransom, Scott M.
Pulse Portraiture is a wideband pulsar timing code written in python. It uses an extension of the FFTFIT algorithm (Taylor 1992) to simultaneously measure a phase (TOA) and dispersion measure (DM). The code includes a Gaussian-component-based portrait modeling routine. The code uses the python interface to the pulsar data analysis package PSRCHIVE (ascl:1105.014) and also requires the non-linear least-squares minimization package lmfit (ascl:1606.014).