2011•AIP conference proceedingsOpen access
Pulsar Science with the Green Bank 43 m Telescope
M. B. Mickaliger, M. A. McLaughlin, D. R. Lorimer, G. I. Langston, A. V. Bilous, V. I. Kondratiev, S. M. Ransom, F. Crawford, M. Burgay, Nicolò D’Amico, P. Esposito, A. Pellizzoni, Andrea Possenti
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Abstract
The 43m telescope at the NRAO site in Green Bank, WV has recently been outfitted with a clone of the Green Bank Ultimate Pulsar Processing Instrument (GUPPI \cite{Ransom:2009}) backend, making it very useful for a number of pulsar related studies in frequency ranges 800-1600 MHz and 220-440 MHz. Some of the recent science being done with it include: monitoring of the Crab pulsar, a blind search for transient sources, pulsar searches of targets of opportunity, and an all-sky mapping project. For the Crab monitoring project, regular observations are searched for giant pulses (GPs), which are then correlated with $\gamma$-ray photons from the \emph{Fermi} spacecraft. Data from the all-sky mapping project are first run through a pipeline that does a blind transient search, looking for single pulses over a DM range of 0-500 pc~cm$^{-3}$. These projects are made possible by MIT Lincoln Labs.
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