Hi Andrew,
Your ISIS 'failure point' is where I assumed it would be. A couple of years
ago I tried to help Carl Sawicki use ISIS to reduce his SQUES (with Relco
cal line) ecelle spectra and that is where we also floundered. I recently
changed my eShel camera from an ST-8 (KAF-1603) to a QHY22 (ICX-694) and it
took a lot of fine tuning of the camera rotation angle and messing with the
alpha and gamma values before it all worked well. While I can't be 100%
confident I do feel that if we had persisted we could have got it to work
with ISIS, as I see no obvious reason why the programme could not handle it.
Cheers,
Bernard
-----Original Message-----
From: Andrew Smith
Sent: Monday, September 18, 2017 12:04 AM
To:
fg-spek-admin@vdsastro.de
Subject: [fg spektroskopie] ISIS and my echelle
Link zum neuen Beitrag:
http://forum.vdsastro.de/viewtopic.php?t=4918#p30258
Rather than hijack Daniels thread I will respond to Bernard here.
I had used ISIS with the first version of my spectrograph which used an
echelle with the same characteristics as the eShel. However, when I
updated it for my new telescope to a larger echelle I saved money by
getting an over stocked grating but it had a different blaze and
lines/mm to teh eShel.
I tried to use ISIS and worked at it for a considerable time but I
could not get past the camera rotation stage and the setting of the
alpha and gamma angles and hence the assignment of the orders. See
figures 22 to 26 here
http://www.astrosurf.com/buil/isis/eshel/tuto1.htm
I assume this was because ISIS used a model based on the spectrograph
characteristics. However, I could not prove this.
In the end I decided to use IRAF and got that working with help of this
forum.
Regards Andrew
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