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Overview
The pulsar camera is a phase-binning CCD designed to determine photometric
and photo-polarimetric light-curves for objects with known periodicities, such
as pulsars.
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Recent Results on PSR 0656 This light curve was obtained over 2
nights at the Palomar 200 inch telescope in December, 2000. The light curve
shows a main peak and a clear interpeak. The light curve closely resembles
the gamma-ray light curve. |
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Recent Results on Vela The Vela pulsar was observed from the
CTIO 4 meter in Feb, 2000 to measure polarization. High noise prevented a
sensitive polarization measurement. |
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