Closed moustakas closed 2 years ago
I'm working on this ticket here by comparing my vdisp estimates against those derived by Khaled Soliman using pPXF-- https://data.desi.lbl.gov/desi/users/ioannis/fastspecfit/pv-vdisp/fujilupe/qa/
Lots of bugs (both algorithmic and in the QA code) now fixed in #69. Also, vdisp is now computed if solve_vdisp=True
or if: (S/N_B>3 or S/N_R>3) and (redshift < 1)
, where S/N_B
and S/N_R
is the signal-to-noise ratio per pixel in the B and R camera, respectively.
One medium-term goal is to improve the velocity dispersion estimates. But first we need to fix issues like this, which suggest that velocity dispersion isn't being handled correctly at all. In detail, with the nominal
vdisp=150 km/s
, the Ca H+K lines in the model are clearly over-broadened. However, the implied broadening is more like20-30 km/s
, which can't be right for a relatively luminous & massive system like this. So, I need to check that I'm doing the broadening correctly in the first place.