What causes variations in redshift measurements?

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Variations in redshift measurements can occur due to the choice of spectral peaks used for calculations, leading to different results. For example, measuring a 20nm shift from different wavelengths can yield redshifts of 0.047 and 0.032, which can significantly impact subsequent calculations like recession speed. The shifts are proportional to wavelength, meaning that longer wavelengths will experience larger shifts. This discrepancy highlights the importance of consistent measurement practices in redshift analysis. Understanding these factors is crucial for accurate astrophysical interpretations.
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Hello!
I have a small question, in my textbook and everywhere I look online it states that to find the redshift of a receding galaxy from the spectrograph you divide the change in wavelength by the original point you are measuring from.
The problem I have is, if there is a 20nm shift for example across the whole graph then you get different results depending on which peaks you decide to take the measure from.
For instance if you had 420nm > 440nm the redshift would be 0.047 3.d.p but if you used another peak at 620nm shifting to 640nm you would get a redshift of 0.032 3.d.p
Completely different figures that would alter any future calculations such as recession speed but for the same redshift.

I'm sure that as usual I'm missing something obvious, but after much searching I can still not work out what it is.. Can anyone help please? Thanks!
 
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Do all peaks shift the same number of nm?
 
The shifts are proportional to wavelength.
 
Exactly. Unfortunately, it seems that we are too late, as the original poster was last logged in less than an hour after the original post.
 
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