[daip] RUNNING RM synthesis tasks (or getting ready to do so)
Eric Perlman
eperlman at fit.edu
Thu Jun 9 16:47:12 EDT 2016
Hi Eric,
On 6/9/16 4:43 PM, Eric Greisen wrote:
> On 06/09/2016 02:36 PM, Eric Perlman wrote:
>> Hi Eric,
>>
>> Thanks for your response.
>>> Why are you running FQUBE or MCUBE?? You already have cubes in Q and
>>> U and I (V is of little use). These are the inputs to DOFARS (the Q
>>> and U images are INNAME and IN2NAME) which will transpose them and
>>> then run FARS. Note that you will need the transposed Q and U cubes
>>> for both FARS and RMFIT so it is probably better to use TRANS and then
>>> FARS directly rather than have to do the transposition over again for
>>> RMFIT.
>>>
>>> Be sure to study teh relevant portions of AIPS Memo 118 to learn about
>>> RMFIT. You do not have a particularly long freq axis so the FARS
>>> output will be disappointing. RMFIT may be able to pull some info out
>>> however...
>>>
>>
>> Primarily because I did not have AIPS Memo 118 and could not find it on
>> the Web! The Google searches did not link to it either and my former
>> grad student's (Sayali Avachat) notes weren't that helpful either,
>> probably because she did it years ago.
>>
>> Anyway, though, since it's recent VLBA data with the RDBE, isn't there
>> something like 128 channels in each band? In that case there is
>> significant leverage. Anyway, I'm reading through that memo now.
>>
>> Thanks,
>>
>> Eric
>
> You have AIPSMEM118.pdf in every AIPS installation so it should be
> easy to find or use the AIPS web site www.aips.nrao.edu.
>
> You have a bandwidth of 32 MHz at 4852 MHz. Bandwidth factors like
> 2:1 are much more productive in RM synthesis and frequencies < 1 GHz
> give much narrower RM synthesized beam widths. Go ahead and try it
> but do not pin much hope for it.
>
> Eric Greisen
Ok, good point, although I also have 1.5 GHz. When the OBSERVE file was
written RM synthesis was not planned for.
Eric
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