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strange ISIS fault - displaying UVES Castor spectrum

Posted: Mon Jan 09, 2017 10:41 pm
by Robin Leadbeater
If you display the UVES Castor spectrum from the ISIS database, then save it and compare this saved version with the spectrum displayed straight from the database, you see a large (non constant) wavelength shift between the two versions of the same spectra. (see attached) It does not happen with other UVES spectra in the database though. Does anyone else see the same fault?

What is happening ???
Any ideas ?
Robin

Re: strange ISIS fault - displaying UVES Castor spectrum

Posted: Tue Jan 10, 2017 10:56 am
by Robin Leadbeater
I think I understand what is happening. I had replaced the original UVES Castor spectrum in the ISIS database with one with a wider wavelength range that I had generated from the UVES POP website using the plot function there. The problem is that spectra produced using this function do not have equal bin widths across the wavelength range. ISIS plots these correctly but saves them incorrectly with equal bin widths.

Does anyone know how to generate files (fits or dat) with equal bin width from the UVES POP spectra ?

Many Thanks
Robin

Re: strange ISIS fault - displaying UVES Castor spectrum

Posted: Tue Jan 10, 2017 8:13 pm
by Peter Somogyi
Hi Robin,

"Does anyone know how to generate files (fits or dat) with equal bin width from the UVES POP spectra ?"

I've already tried this feature in ISIS on .fit files with success:
resampling.png
resampling.png (9.94 KiB) Viewed 4499 times
"A/p" is matching with 'CRDELT1' value in the fits header. (However, never tried with .dat format.)

HTH
Peter

Re: strange ISIS fault - displaying UVES Castor spectrum

Posted: Tue Jan 10, 2017 11:58 pm
by Robin Leadbeater
That works, thanks Peter !

That tool can convert a dat file with unequal bin sizes to an equal bin size fits file. That can then be converted to a dat file using the tool in the same ISIS window

Thanks again!
Robin

Re: strange ISIS fault - displaying UVES Castor spectrum

Posted: Fri Jan 13, 2017 9:12 pm
by Christian Buil
Yes Peter is pointing the correct solution.

The UVES spectra variable sampling (presence of hole, ...) is always a problem.

Christian