From hiroimai@sci.kagoshima-u.ac.jpThu Nov  6 09:28:12 2003
Date: Thu, 06 Nov 2003 11:03:45 +0900
From: Hiroshi Imai <hiroimai@sci.kagoshima-u.ac.jp>
To: "VLBI Observers (Aspen only)" <vlbiobs@nrao.edu>
Cc: Lisa Foley <lfoley@nrao.edu>
Subject: Re: bi028a

Dear Lisa,

Previously I asked two correlation passes, the first for the coordinate
that has already been specified in the keyin file and the second for
another coordinate I would specify on basis of single dish observaitons.
Unfortunately, I have not yet obtained the second coordinate.

Therefore, I would like to ask to process only the first pass, but in which
the integration time is as short as possible. Hopefully, the output rate
now is 1Mbytes/s. I expect to use an integration time of 1 second. This
covers a wider field of view and the second pass is not necessary any more.

If some problem in my above proposal, please ask to me again. Because
I will be away in this week, I will reply in the next week.

Thank you very much for kind processing.

Best regards,

Hiroshi

> 
> Hello Hiroshi Imai,
> 
> We are preparing to correlate bi028a. Did you want to specify
> correlation coordinates that are different from those in the
> .sum file? Please let us know what you'd like done at your
> earliest convenience.
> 
> Thanks very much,
> 
> Lisa Foley
> NRAO Data Analyst
> 
>
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                      *
        <<<               *      Hiroshi Imai, Ph.D.
         >>>       *
        <<<                    Research associate
      /^^xx^^%          *      Department of Physics (astronomy)
     /   xx   %                Kagoshima University
    /     xxx  %          Tel./FAX: +81-(0)99-285-8960
   /     xx xx  %%        E-mail: hiroimai@sci.kagoshima-u.ac.jp
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   ~  ~   ~   ~   ~   ~        omodaka-nishio/member/imai/index.html
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From hiroimai@sci.kagoshima-u.ac.jpMon Sep 29 09:57:24 2003
Date: Mon, 29 Sep 2003 11:12:01 +0900
From: Hiroshi Imai <hiroimai@sci.kagoshima-u.ac.jp>
To: "VLBI Observers (Aspen only)" <vlbiobs@nrao.edu>
Subject: Re: BI 028 keyin file

Dear Lisa,

One more comment. my preference for the maser source positions has
not yet fixed. But I would like to set the coordinate used previously
in the keyin file. Maybe I will ask to add another source position,
which will be determied after a short VLA observation and before the
data correlation. The keyin file will be used in the whole our project.

Regards,

Hiroshi 


> 
> Hello Hiroshi Imai,
> 
> I've processed your key file for bi028. A new feature in the
> latest release of sched is a log of comments and warnings made
> as the program executes. The log for bi028 is pasted below;
> note the comment regarding DOPFQ. This may be indicative
> of a serious problem. Please let us know if you are concerned.
> 
> Also, your preference for source positions was not set. Can we
> assume 'standard'? And do you want this schedule used for all
> four epochs of bi028?
> 
> best regards,
> 
> Lisa Foley
> NRAO Data Analyst

--------------------------------------------------------------------------
                      *
        <<<               *      Hiroshi Imai, Ph.D.
         >>>       *
        <<<                    Research associate
      /^^xx^^%          *      Department of Physics (astronomy)
     /   xx   %                Kagoshima University
    /     xxx  %          Tel./FAX: +81-(0)99-285-8960
   /     xx xx  %%        E-mail: hiroimai@sci.kagoshima-u.ac.jp
=====================     Home page:  http://astro.sci.kagoshima-u.ac.jp/
   ~  ~   ~   ~   ~   ~        omodaka-nishio/member/imai/index.html
--------------------------------------------------------------------------