@article{Shearer:1997:10.1086/310888,
author = {Shearer, A and Redfern, RM and Gorman, G and Butler, R and Golden, A and O'Kane, P and Beskin, G and Neizvestny, SI and Neustroev, VV and Plokhotnichenko, VL and Cullum, M},
doi = {10.1086/310888},
journal = {Astrophysical Journal Letters},
title = {Pulsed Optical Emission from PSR 0656+14},
url = {http://dx.doi.org/10.1086/310888},
volume = {487},
year = {1997}
}

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TY  - JOUR
AB  - Using data collected with the Special Astrophysical Observatory (SAO) 6 m telescope and the University College Galway (UCG) Transputer Instrument for Fast Image Deconvolution (TRIFFID) imaging photometer, we show that the radio, X-ray, and gamma -ray pulsar PSR 0656+14 exhibits pulsed optical emission. We observed that the pulsed fraction was consistent with 100% and that the flux was higher than that expected from a thermal source. The magnitude of PSR 0656+14 in the B band was observed to be 25.1 +/- 0.3, consistent with previous CCD observations. The peak of the optical signal is at phase 0.2 compared to the radio and in phase with the weak gamma -ray pulse.
AU  - Shearer,A
AU  - Redfern,RM
AU  - Gorman,G
AU  - Butler,R
AU  - Golden,A
AU  - O'Kane,P
AU  - Beskin,G
AU  - Neizvestny,SI
AU  - Neustroev,VV
AU  - Plokhotnichenko,VL
AU  - Cullum,M
DO  - 10.1086/310888
PY  - 1997///
TI  - Pulsed Optical Emission from PSR 0656+14
T2  - Astrophysical Journal Letters
UR  - http://dx.doi.org/10.1086/310888
VL  - 487
ER  - 

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