N. S. P. Sabalisck , M. Rozas, J. E. Beckman , J. H. Knapen, PASA, 15 (1), 161
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Observations
These were with the TAURUS II instrument, at the Cassegrain focus of the WHT, in May 1995. As M100 is so big, we required two data cubes whose region of overlap contained the galaxy centre. We had 0.29 "/pix, and velocity steps of 10 km s
, under photometric conditions with seeing of 1". Calibration followed the standard method of Atherton & Taylor (1984).
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