I was wondering if anyone has used the alpy photometry slit? Pictures I’ve seen on the web has it in a vertical position, spectroscopy slit at the top and the wider section at the bottom for photometry.
I have one but have not used it “in anger”. To produce a spectrum calibrated in absolute flux, two sets of spectra are taken, one as normal in the narrow slit, and one effectively “slitless” using the wider part.
The narrow slit spectrum has the fine detail and accurate wavelength calibration but only includes the fraction of flux which happens to pass through the slit so cannot be used to measure the absolute flux. The wide slit spectrum has lower resolution and poorer wavelength calibration but includes the total flux from the target. By combining the two a fully flux calibrated spectrum can be produced with accurate wavelength and good resolution. Christian Buil’s page here shows how to do this using ISIS.
The conventional photometric brightnesses can then be calculated by integrating the spectrum over the wavelength range of the standard photometric filters.
More commonly in the amateur realm, the reverse is done ie a spectrum is produced as normal using a narrow slit and then calibrated in absolute flux using brightness measurements obtained using photometric filters.
I use this slit as a matter of course, primarily as a means of getting the best definition of the continuum that I can with my equipment & set-up. Although it means 4 measurements instead of 2 it’s a very useful piece of kit just for this function alone. I don’t use it for photometry though I have processed some of my measurements following the examples given in the Christian Buil references Robin has given, just to see what sort of results were produced – the instructions in the references are straightforward & clear.