![]() | ![]() |
Astron. Astrophys. 363, 617-628 (2000) 9. ConclusionDefinitive optical observations of the Crab and other pulsars have
to date been restricted - either by poor temporal resolution both in
terms of resolution and with respect to absolute UTC, and also by the
limited spatial information which is crucial in distinguishing the
pulsar's emission from the background. Using the TRIFFID high speed
photometer, we have obtained datasets uncompromised by these previous
limitations, and in addition to confirming many of the previous
conclusions of Eikenberry et al. (1997), we have determined several
new results uniquely due to the technology we have implemented,
including the fluxing of the unpulsed component of emission, the
absolute arrival times of the three light curves with respect to one
another, and the spatial extent of the plateau on the main peak. Our
photometric analysis was however limited by the reference data we used
to renormalize the flux ratios thus determined. It is clear that
further analysis using more photometrically accurate reference data
combined with further observations at extended wavebands, such as the
UV or
© European Southern Observatory (ESO) 2000 Online publication: December 11, 2000 ![]() |