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2. The observations

 

plate date tex2html_wrap_inline3375 emulsion/filter/exposure
U9362 84:06:03 12:27,13:30 IIIaJ/UG1/3 hr.
J4882 79:03:23 12:25,13:20 IIIaJ/GG395/1 hr.
J9229 84:04:26 12:27,13:30 IIIaJ/GG395/1 hr.
R2936 77:02:27 12:25,13:20 IIIaF/RG630/48 min.

Table 1: The UKST plates on which the VPC is based

 

The VPC is based on four photographic plates (one U, two tex2html_wrap_inline3309 and one tex2html_wrap_inline3311) of the same field; all of which were exposed on the 1.2-metre UK Schmidt Telescope (UKST) at Siding Spring Observatory in Australia. Details of all four plates are listed in Table 1 (click here). Each plate measured 356 mm square and covered an area of the sky tex2html_wrap_inline3389 by tex2html_wrap_inline3389 within an imaging area of dimensions 343 mm by 343 mm. The plate scale was therefore 67.12 arcsec/mm in each case. All of the plates were hypersensitised by successive soaking in nitrogen and hydrogen gas. Those plates taken after 1982 December 3 had the added advantage of being nitrogen flushed; that is exposed under a constant stream of nitrogen. The significance of this flushing process is dealt with in Sects. 3.7 (click here) and 6.2 (click here).


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