The peculiar velocity survey
Whole new scale of peculiar velocity survey - can rewrite rules
All spectra in principal good enough resolution and wavelength coverage for Dn-s
Limited by S/N, ellipticity, linewidth, redshift, spectral type?
Can reobserve suitable galaxies with marginally poor S/N (or alibi)
Aim for S/N = 20/A at MgB
May want to set selection criteria at this meeting