Closed ericasaw closed 5 months ago
The bottom plot also nicely shows how the new flexure correction is leading to better telluric correction.
We reimplemented how v2.2.0 handles the synthetic Vega spectrum in v3.0. @ericasaw let me know if you want to reopen this issue, otherwise I'm closing it.
Here is an example of what the continuum looks like in the new pipeline for a .spec_a0v.fits file
This is what the continuum looks like in the old pipeline
We found that the new version of the pipeline is flattening the Vega spectrum (but we are unsure why this was implemented). Kyle just pushed a fix for this to the reimplement_cr_reject branch that removes the flattening.
This is what the continuum looks like for this branch of the pipeline with this fix
Additionally Kyle brought up the slight increase in the flux in the new pipeline (Issue #25; < 2%). We posited that as long as the A0 and the target were reduced with the same pipeline this flux difference wouldn't matter in the spec_a0v.fits files since the ratio between the target and standard would stay the same. Just want to note that things work out like we expected. Here is a single order in the old pipeline, blue, and the new pipeline (non-flattened Vega), orange, and we can see the flux doesnt have any consistent offset which is what we had hoped for
I'm basically raising this issue to document the issue occurring in the new pipeline and to ask @leejjoon if he would be upset if we turned the Vega flattening off in the next release.