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    No turkeys on the menu!

    From: Joe Patterson <jop_at_astro.columbia.edu>
    Date: Tue, 3 Dec 2002 13:39:10 -0500 (EST)
    Definitely not.  The campaign on Tau 2 is starting to yield its result.
    Our coverage is still dominated by USA longitudes (Dave S, Jerry F, Cap'n
    Bob, David Messier), but some contributions have come in from Bob Rea and
    Tonny (NZ and Belgium).  So we've overcome simple aliasing, though the
    domination by one longitude still inflicts avoidable noise on the power
    spectrum.  Anyway, the main story seems to be this: three signals in the
    power spectrum, a positive superhump at Po+3.4%, a negative superhump at
    Po-2.7%, and the nodal signal itself at 6 days.  Cute!  And damned
    interesting... at this Po, the positive superhump is expected at about
    Po+8%, so this implies a low mass ratio - which we can maybe make hay of.
    (Where did that expression come from, anyway?)
    
    We have to sharpen accuracy, and also explore the higher harmonics, which
    are still a bit weak.  We have about 12 more days before the Moon will
    interrupt us - let's try to get tree-to-tree coverage until then.
    Especially those treasured and exotic longitudes oh-so-far from 90 degrees
    west!
    
    The other great star is EC0422-20.  This one is *really* easy to do - very
    attractive target for small scopes, even if the declination is a trifle
    unappealing.  For this one, our dominant coverage is from Berto and Greg
    Bolt (Pretoria and Perth), so our more common artillery in the USA and NZ
    haven't yet arrived in force - except for Lew Cook, whose data breaks the
    cycle-count logjam.  The star shows BIG-TIME negative superhumps at 3.32
    hours.
    
    Those are the two CBA targets for the south.  For the north too - in a
    full display of hemispheric brotherhood I hope.  But we get some extra
    hours of darkness in the north.  I recommend short (1-2 hr) observations
    of FO Aqr and AO Psc if you'd like an early-evening target.
    
       Joe
    
    Received on 3 Dec 2002