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<p>Hi Ingyin,<br>
</p>
You can use VLBAMPCL to do both. Set:<br>
<br>
REFANT to an antenna that is present for calsour1 and calsour2.<br>
TIMERANG time range for calsour1<br>
CALSOUR calsour1<br>
OPCODE 'CALP'<br>
TIME2 time range for calsour2<br>
SOURCES calsour2<br>
ANTENNAS antenna number for VLA<br>
<br>
I'll stop by in a little while to see if you have any more
questions.<br>
<br>
Amy<br>
<br>
<div class="moz-cite-prefix">On 07/05/2018 12:30 PM, Ingyin Zaw
wrote:<br>
</div>
<blockquote type="cite"
cite="mid:CAOtp+V97oO+inG=GcEHUuBrBmQyy__zCC9pRTSJ7XmRQA9KiNg@mail.gmail.com">
<div dir="ltr">
<div>Hi,</div>
<div><br>
</div>
<div>I have a dataset where there were 2 calibrator sources
observed. The first is far stronger and good for all antennas
except VLA which did not observe it. The second is fine for
the VLA but not great for the others.</div>
<div><br>
</div>
<div>How can I run VLBAMPCL with the first source for all
antennas except the VLA and then rerun with the second source
for the VLA and have everything in the same CL table?</div>
<div><br>
</div>
<div>If that is not possible, could you let me know where I can
find the script so that I can run the steps on my own with the
two sources for different antennas?</div>
<div><br>
</div>
<div>I'm currently visiting Socorro and will leave after
tomorrow, so I'd like to get through this today, if possible.<br>
</div>
<div><br>
</div>
<div>Thanks,</div>
<div>Ingyin<br>
</div>
</div>
<br>
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