

S. Kim , L. Staveley-Smith , R.J. Sault , M.J. Kesteven , D. McConnell , M.A. Dopita , M. Bessell, PASA, 15 (1), 132
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H Observations and Data Reduction
 Observations and Data Reduction
  For the wide-field survey of H emission in the LMC, a 153 mm  f/5.0 camera lens from 2.3-m telescope at Siding Spring Observatory was mounted on the 16-inch telescope with a filter assembly and a cooled 2048
 emission in the LMC, a 153 mm  f/5.0 camera lens from 2.3-m telescope at Siding Spring Observatory was mounted on the 16-inch telescope with a filter assembly and a cooled 2048  2048 CCD. Each 15
 2048 CCD. Each 15  m pixel corresponds to 20.''63 on the sky, giving a total field size of
m pixel corresponds to 20.''63 on the sky, giving a total field size of  square. The H
 square. The H filter was centered at 6569 ц…\ with a FWHM of 15 ц…. Continuum subtraction was done with another image centered at 6620
 filter was centered at 6569 ц…\ with a FWHM of 15 ц…. Continuum subtraction was done with another image centered at 6620  . The exposure time for both H
. The exposure time for both H and continuum images was 4
 and continuum images was 4  900 s.
 900 s. 
| Next Section:  Results Title/Abstract Page: HI Supergiant Shells in Previous Section: HI Observations and Data | Contents Page: Volume 15, Number 1 | 
 
  
  
  
  
  
  
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