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<p>Dear Thomas and all,</p>
<p>The new <a class="moz-txt-link-abbreviated" href="mailto:LO@87.300GHz">LO@87.300GHz</a> that you propose for MK018 is perfectly
possible for the 30M. As you know it takes some time for the
tuning and new LO setting but that shouldn´t be a problem
according to the schedule block.</p>
<p>In the tst.vex that you attached I can see a different value
<a class="moz-txt-link-abbreviated" href="mailto:LO@87.500">LO@87.500</a> GHz for PV. What does it mean? Anyhow it is not a
problem and this value of LO is also possible at the 30M.</p>
<p>Best,</p>
<p>Salvador<br>
</p>
<p><br>
</p>
<div class="moz-cite-prefix">On 09/09/2020 18:06, Thomas Krichbaum
wrote:<br>
</div>
<blockquote type="cite"
cite="mid:ab380f7e-3da6-b1a4-d5d1-ff9e50bebcf5@mpifr-bonn.mpg.de">
<pre class="moz-quote-pre" wrap="">Hi Helge,
in the standard GMVA setup, we usually use firstlo =85500.0 MHz.
In the next session there is one experiments, which requires
observations at 88 GHz, with a different firstlo =87300.0 MHz. This LO
is one of the possible modes, which the VLBA can do.
Can you please confirm that this is possible for all GMVA stations.
I attach a skeleton for the new setup. I also note
that in the next GMVA run, we will need to change form
one setup to the other one:
FRNGTST 86 GHz standard
POLCAL1 86 GHz standard
MK018 88 GHz nonstandard
Eu 282 2200(08/10)-0530(09/10)
US 283 0400(09/10)-1030(09/10)
MK016A 86 GHz back to standard
best Thomas
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<pre class="moz-quote-pre" wrap="">_______________________________________________
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</pre>
</blockquote>
<pre class="moz-signature" cols="72">--
Salvador Sanchez <a class="moz-txt-link-abbreviated" href="mailto:sanchez@iram.es">sanchez@iram.es</a>
Telescope Engineer
IRAM-Instituto de Radioastronomia Milimetrica
Avda. Divina Pastora 7, NC
18012 Granada Spain
Tel: +34-958482002-332 (direct) +34-958482002 (central)
web: <a class="moz-txt-link-abbreviated" href="http://www.iram.es">www.iram.es</a>
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