Anyone who is interested in reading more on how to estimate the signal-to-noise ratios (SNRs) and the uncertainties in digital photometry can take a look at :
The IRAF equation for error estimation is an approximation for SNR>>1. If someone doesn't trust that this is valid for all their data, it is better to manually calculate the errors using the SNR (see the first link for a brief explanation and the equations).
Can I quote the article (second link) as a valid reference for how IRAF calculates the final errors in a CCD photometry process*?
Thanks!
* Such as the one described in A User's Guide to Stellar CCD Photometry with IRAF by Massey & Davis (1992)
Joined: 10 Feb 2006 Posts: 135 Location: Flagstaff
Posted: Sat Jun 16, 2012 3:03 am Post subject:
Yes, these are about PSF fitting. Yes, two of the articles can't be found on-line, but you would have to try an astronomy library, where they have conference proceedings and observatory publications.
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