I have become very interested in the consistency of transformation coefficients derived from the standard red/blue stars in the PEP calibration list (see http://www.aavso.org/obtaining-your-pep-epsilonv-coefficient). The Leo Minor pair is now becoming observable, and will be accessible to northern hemisphere PEPers for three months. I would like to ask V band observers to make at least two eV determinations based on this pair (more would be better). Save your raw data, which should be taken on "photometric nights."
I don't think we presently have active V band observers in the southern hemisphere - raise your hand if I am wrong.
Tom Calderwood