In this section
@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}
}
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 -