Re: LBA sensitivity calculator
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From: <Tasso.Tzioumis_at_email.protected>
Date: Mon, 21 Mar 2005 16:53:59 +1100
Hi Adam,
A couple of more points on the calculator that may be easy to implement:
When one uses telescopes very far apart, there is little mutual
uv-coverage. When there is no common time the baselines are flagged in
the list as N/A and no sensitivity is reported. However, the uv-plot it
is still scaled to maximum possible baseline.
Here is a couple of suggestions to improve things:
1. Rescale the uv-plot to use ONLY the baselines that exist, not the N/A
2. Change the listing to also report "Coverage (hrs)" for each
baseline. Then you can list the sensitivities for all baselines (it is
useful to know sometimes even if no mutual coverage) and make the
coverage 0 hrs (or N/A or an *, or red colour). This will give all the
information that there is now and a little more.
I think you already calculate the coverage times, so it should easy to
implement. I'll not do it if it requires major effort.
Cheers
Tasso
--------------------------------------------------------------------
Tasso Tzioumis, Australia Telescope National Facility, CSIRO
Location: Cnr Pembroke & Vimiera Rds, Marsfield, NSW, 2122, AUSTRALIA
Post: PO Box 76, Epping, NSW 1710, AUSTRALIA
Phone: +61 2 9372 4350 Fax: +61 2 9372 4450 or 4310
Email: Tasso.Tzioumis_at_csiro.au
URL: http://www.atnf.csiro.au/~atzioumi/
--------------------------------------------------------------------
Received on 2005-03-21 16:54:18
Date: Mon, 21 Mar 2005 16:53:59 +1100
Hi Adam,
A couple of more points on the calculator that may be easy to implement:
When one uses telescopes very far apart, there is little mutual
uv-coverage. When there is no common time the baselines are flagged in
the list as N/A and no sensitivity is reported. However, the uv-plot it
is still scaled to maximum possible baseline.
Here is a couple of suggestions to improve things:
1. Rescale the uv-plot to use ONLY the baselines that exist, not the N/A
2. Change the listing to also report "Coverage (hrs)" for each
baseline. Then you can list the sensitivities for all baselines (it is
useful to know sometimes even if no mutual coverage) and make the
coverage 0 hrs (or N/A or an *, or red colour). This will give all the
information that there is now and a little more.
I think you already calculate the coverage times, so it should easy to
implement. I'll not do it if it requires major effort.
Cheers
Tasso
--------------------------------------------------------------------
Tasso Tzioumis, Australia Telescope National Facility, CSIRO
Location: Cnr Pembroke & Vimiera Rds, Marsfield, NSW, 2122, AUSTRALIA
Post: PO Box 76, Epping, NSW 1710, AUSTRALIA
Phone: +61 2 9372 4350 Fax: +61 2 9372 4450 or 4310
Email: Tasso.Tzioumis_at_csiro.au
URL: http://www.atnf.csiro.au/~atzioumi/
--------------------------------------------------------------------
Received on 2005-03-21 16:54:18