GBT VLBA PROJECT SETUP

Observer's Name: Phil Diamond et al.
Project ID: GD017B ( AGD017B_01 )
Note: Correlate at Socorro
Receiver: Rcvr1_2
Stations : GBT, VLBA, VLA, Arecibo, Joddrell, Bonn,
Westerbork, Medicina, Noto, Torun
Description Monitoring the compact emission in Arp 220.
Receiver Tuning Frequency: 1646 MHz
Start Date/Time: Mon Mar 07, 2005 05:00 UT
End Date/Time: Mon Mar 07, 2005 17:38 UT
Number of tapes: 2 (autoallocate)
Tapes change times: 10:52
LO1 center F0:
phase cal? 		1550 MHz
Yes 1MHz 

Date: Tue, 25 Jan 2005 09:01:35 -0700 (MST)
From: Barry Clark 
To: pdiamond@jb.man.ac.uk
Subject: GD 17 = Arp 220  (Correction of typo)

This is scheduled on the EVN on March 6/7, 2100-1100 UT, on the VLBA
0500-1900 UT, on the GBT 0500-1900 UT, on Arecibo 0700-1100 UT, and
on the phased VLA 0830-2300 VLALST.  The observation is at 256 Mbits/sec,
but no more than two tapes per station.

This is segment B of the proposal.

I am herewith asking Lorant Sjouwerman to serve as local technical contact
person for this observation.
As part of the Global Session, observe files are due in both Bologna and
Socorro by January 27.