Question about how darks are handled by LSST

(Fergus Longbottom) #1

Hi Everyone,

I’m a student working on the Huntsman Telephoto array project (same concept as the dragonfly telescope) and we’ve been looking at using the LSST stack for our data reduction pipeline/developing our own obs_huntsman package. Ideally we will use as much as the stack functionality as is, as far as it is possible.

With the introduction out of the way, I have a quick question regarding how darks are handled.

Huntsman currently collects darks for flat-field and science exposures. We take an exposure time matched dark frame for each flat-field (we use twilight flats, so the darks are taken in a single batch after the end of the twilight flat window) and an exposure time matched dark for science frames. Science frames are uniformly 5 minute exposures at the moment.

The reason we do this is, is to get the bias and dark in the same exposure. This saves us an extra processing step and also avoids introduction of noise/errors from taking a separate bias to subtract from the dark exposures and then scaling the dark current etc. However, this appears to be how the LSST operates by default (bias subtract and then scale the dark current as required). My question is it is possible to use the LSST stack with our calibration strategy? One hacky work around would be to just treat our dark+bias frames as just the bias, as all we want is to subtract the dark+bias frame from the desired science/flat frame but I’m hoping there is a cleaner solution?

Thanks in advance for any help/advice,