May 25, 2007: Marcos Moya Lopez visited Bordeaux these last few weeks. With Damien, he wrote a note discussing which known pulsars are really the best candidates, which you can find here.
February 6, 2007: While at Stanford for the 1st GLAST Symposium, a meeting was held. Romani recapitulated needs and tactics. Lyne showed slides summarzing Jodrell observations for GLAST. Johnston spoke of Parkes observations (his rough notes here). Smith spoke of Nancay observations (see slides, Feb 2, below). Ransom and others intend to request GBT and/or Arecibo time for the radio-faint but gamma-likely targets. McLaughlin will use the 140' telescope to time noisier, louder gamma candidates. The consensus was that the timing needs for GLAST are on track for being met, even if much work remains to be done. (Attendees: Andrew Lyne, Simon Johnston, Scott Ransom, Maura McLaughlin, Mallory Roberts, Jim Cordes, Alberto Carramiñana, Roger Romani, Dave Thompson, Steve Thorsett, Peter Michelson, Steve Ritz, Denis Dumora, David Smith.)
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