PALFA, p2030, 23 March 2005

Observers: Jason Hessels, Julia Deneva

1. While cycling a known pulsar through the beams, it was showing up in the 
   wrong beam--rot.angle was left at 15deg (according to Michael Lerner, it
   shouldn't matter because the rot. angle is taken into account when centering
   a beam). Setting the rot.angle to zero and cycling again seemed to go 
   around this problem.

2. Sporadic overflows from wapp3: several in a row, about 20s apart. M.Lerner 
   has seen same problem in spectral line mode--due to timeout as data isn't 
   being taken but there are attempts to read it off. Stopping the 
   observation and restarting + quitting the quick processing helped. 

3. No overflows since quick processing was stopped.

4. Reobserved 2 single-pulse candidates:
	G189.84+01.71.N_53451_0044 (beam 6)
	G208.07+02.01.N_53451_0088 (beam 1)