Table 3: V-band data used for examining the secular decrease in luminosity of the Crab Pulsar.
Table 4: UBVRIz magnitudes of the eight field stars examined in the secular decrease of luminosity of the pulsar.
The stars that were chosen for relative photometry in the investigation of the secular decrease in luminosity. The numbering is the same as in Table 4 where the UBVRIz magnitudes for these stars are given. The numbering is also used in Table 3. The pulsar is number eight. This V-band image was acquired with the JKT on February 7, 1990. North is up and east is to the left. The field of view is approximately 3.2 by 2.1 arcmin.
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