Hello

I am measuring the reflectance of some coatings using a Perkin Elmer spectro (lamda 950). In order to increase the precision I bought (from PE also) a Al reference mirror. It cames with a CD with a .sp and a .dx file (dx I dont know what is for).

First time I collected the R spectrum for the mirror (using standard 100% T and 0%T baselines) Indeed there are important discrepancies between the collected spetrum and one coming with the reference mirror (NIST +' .... certified). So I decided to measure the R for my films using this reference mirror.

The mathematics beyond is logic:

Corrected sample R = Collected sample Rx(Collected Mirror R/Standard mirror R)

HAving many samples to analyze and being lazy I prefer to use the automatic method suggested in the documentation coming woth mirror. However the explanation here are a little foggy:

" 1. Obtain a baseline spectrum using the Calibration Reference Mirror

2. Obtain a spectrum for the sample

3. Multiply them"

They ask me to do 2 measurements so I will have 2 files in the end. But in this case how I am inserting in this process the 3rd file from the CD - the standard spectra for mirror? How I can obtain a baseline spectrum from the reference mirror? If I am using the import option for the baseline and I insert here the "official standard file from the CD" then where I am using the mirror collected spectra? I am missing something? Can someone explain me how to collect a baseline from the mirror and then how to correlate with the standard spectra?

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