[daip] [Fwd: ACCOR output]

[lincoln greenhill]

Dear Leonid, Craig,


Attached is a plot showing output from ACCOR (3 VLBA stations, 8 IFs 
overplotted) for a 22 GHz phase referencing expt in Nov. 2004.

We used solint = -0.25 .

I have not previously see the signature shown here for OV, where 2 of 8 IFs
show a rapid and systematic variation in sampler statistics.  Is the
behavior familiar?  Do you know what could cause it?

Best, L.

-------- Original Message --------
Subject: ACCOR output
Date: Tue, 21 Apr 2009 13:04:10 -0400 (EDT)
From: Ingyin Zaw <iz6 at cosmo.nyu.edu>
To: lincoln greenhill <greenhill at cfa.harvard.edu>
References: <49EC83F6.1010101 at cfa.harvard.edu>

Hi Lincoln,

Here is the file of the ACCOR solutions for OV compared to MK and NL.
Please let me know what the NRAO people say about the arc.

Thanks,
Ingyin

-- 
Lincoln J. Greenhill               Harvard-Smithsonian Center for Astrophysics
Office:     1 617-495-7194         60 Garden St, Cambridge, MA 02138
Cell:       1 617 851 8918         E-mail:  greenhill at cfa.harvard.edu
FAX:        1 617-495-7345         http://cfa-www.harvard.edu/~lincoln
-------------- next part --------------
A non-text attachment was scrubbed...
Name: bb242d_astro_accor.ps
Type: application/postscript
Size: 2492509 bytes
Desc: not available
URL: <http://listmgr.nrao.edu/pipermail/daip/attachments/20090421/241d9595/attachment.ps>