Subject: [Fwd: Correlation of V094a] Date: Thu, 04 Feb 1999 16:31:05 -0800 From: "Sean M. Dougherty" Organization: University of Calgary/DRAO To: Dave Del Rizzo --------------------------------------------------------------------- Subject: Correlation of V094a Date: Fri, 5 Feb 1999 09:30:33 +0900 (JST) From: Jim Lovell To: Penticton , Brent Carlson , ped@drao.nrc.ca, Sean.Dougherty@hia.nrc.ca CC: Phil Edwards Hi, We've had a couple of requests from the PI of V094a that didn't make it to the schedule cover notes. I guess I was a bit slow in getting the PI letter out (shame on me!). The most important point is that this experiment is an observation of a four-image gravitational lens and the PI requires one correlator pass for each component. The four positions are: Component RA (J2000) Dec ------------------------------------------------- A1 04 14 37.76715 05 34 42.3424 A2 04 14 37.77613 05 34 42.7481 B 04 14 37.72772 05 34 44.2803 C 04 14 37.63684 05 34 42.6424 The PI has also requested an increrase to 64 channels per IF to reduce bandwidth smearing effects. Lastly, the PI's address has changed: e-mail: cmoore@astro.rug.nl Christopher Moore Kapteyn Institute Postbus 800 9700AV Groningen The Netherlands Cheers, Jim -- Jim Lovell, JSPS Fellow Phone: (+81) 427-59-8346 Institute of Space & Fax : (+81) 427-59-8340 Astronautical Science Email: jlovell@vsop.isas.ac.jp 3-1-1 Yoshinodai WWW : http://www.vsop.isas.ac.jp/~jlovell Sagamihara, Kanagawa 229-8510 Japan