The 43 m 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 [1]) 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 γ‐ray photons from the 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 These projects are made possible by MIT Lincoln Labs.
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18 August 2011
RADIO PULSARS: AN ASTROPHYSICAL KEY TO UNLOCK THE SECRETS OF THE UNIVERSE
10–15 October 2010
Chia, Sardinia, (Italy)
Research Article|
August 18 2011
Pulsar Science with the Green Bank 43 m Telescope Available to Purchase
M. B. Mickaliger;
M. B. Mickaliger
aDepartment of Physics, West Virginia University, Morgantown, WV 26506
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M. A. McLaughlin;
M. A. McLaughlin
aDepartment of Physics, West Virginia University, Morgantown, WV 26506
bNational Radio Astronomy Observatory, Green Bank, WV 24944
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D. R. Lorimer;
D. R. Lorimer
aDepartment of Physics, West Virginia University, Morgantown, WV 26506
bNational Radio Astronomy Observatory, Green Bank, WV 24944
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G. Langston;
G. Langston
bNational Radio Astronomy Observatory, Green Bank, WV 24944
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A. V. Bilous;
A. V. Bilous
cDepartment of Astronomy, University of Virginia, Charlottesville, VA 22904
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V. I. Kondratiev;
V. I. Kondratiev
dNetherlands Institue for Radio Astronomy (ASTRON), Postbus 2, 7990 AA Dwingeloo, The Netherlands
eAstro Space Center of the Lebedev Physical Institute, Profsoyuznaya str 84/32, Moscow 117997, Russia
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S. M. Ransom;
S. M. Ransom
fNational Radio Astronomy Observatory, Charlottesville, VA 22903
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F. Crawford
F. Crawford
gDepartment of Physics and Astronomy, Franklin and Marshall College, Lancaster, PA 17604
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M. B. Mickaliger
a
M. A. McLaughlin
a,b
D. R. Lorimer
a,b
G. Langston
b
A. V. Bilous
c
V. I. Kondratiev
d,e
S. M. Ransom
f
F. Crawford
g
aDepartment of Physics, West Virginia University, Morgantown, WV 26506
bNational Radio Astronomy Observatory, Green Bank, WV 24944
cDepartment of Astronomy, University of Virginia, Charlottesville, VA 22904
dNetherlands Institue for Radio Astronomy (ASTRON), Postbus 2, 7990 AA Dwingeloo, The Netherlands
eAstro Space Center of the Lebedev Physical Institute, Profsoyuznaya str 84/32, Moscow 117997, Russia
fNational Radio Astronomy Observatory, Charlottesville, VA 22903
gDepartment of Physics and Astronomy, Franklin and Marshall College, Lancaster, PA 17604
AIP Conf. Proc. 1357, 60–61 (2011)
Citation
M. B. Mickaliger, M. A. McLaughlin, D. R. Lorimer, G. Langston, A. V. Bilous, V. I. Kondratiev, S. M. Ransom, F. Crawford; Pulsar Science with the Green Bank 43 m Telescope. AIP Conf. Proc. 18 August 2011; 1357 (1): 60–61. https://doi.org/10.1063/1.3615079
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