Quasar spectra carry the imprint of foreground intergalactic medium (IGM) through absorption systems. In particular, absorption caused by neutral hydrogen gas, the "Ly$\alpha$ forest," is a key spectroscopic tracer for cosmological analyses used to measure cosmic expansion and test physics beyond the standard model. SpenderQ is a ML-based framework for reconstructing intrinsic quasar spectra and measuring the Lyα forest from observations. SpenderQ uses the Spender spectrum autoencoder to learn a compact and redshift-invariant latent encoding of quasar spectra, combined with an iterative procedure to identify and mask absorption regions. It is entirely data-driven (e.g., not calibrated on simulations) and makes no assumptions on the shape of the intrinsic quasar continuum.
Here's a schematic diagram of the SpenderQ framework:
and an example on a mock spectrum (grey/black) where we know the truth (blue):
Here's SpenderQ in action on real public DESI data:
Here's another for a spectrum with a Broad Absoprtion Line, which was not
masked
ChangHoon Hahn (Princeton; changhoon.hahn[at]princeton.edu)
Satya Gontcho A Gontcho (Berkeley)
Peter Melchior (Princeton)
Abby Bault (Princeton)
Hiram Herrera (CEA)