This project represents a major observational effort to characterize the galaxy morphologies and the line-emitting gas kinematics using a multi-wavelength and multi-scale approach. The observations available are the following:
- 7 QSO2s observed with ALMA in CO(2-1) at 0.2 arcsec resolution (2018.1.00870.S)
- 5 QSO2s to be observed with JWST/MIRI/MRS (program 3566, 30 hours)
- 44 QSO2s observed in the K-band with GTC/EMIR – seeing limited long-slit spectroscopy (GTC77-18A, GTC62-18B, GTCMULTIPLE2G-19A, GTC83-19B, GTC55-20A)
- 9 QSO2s observed in the K-band with VLT/SINFONI or Gemini/NIFS – seeing limited integral field spectroscopy (ESO and Gemini archives).
- 5 QSO2s observed in the optical with Keck/KCWI – seeing limited integral field spectroscopy (U052, 4 half nights, PI: Canalizo).
- 5 QSO2s observed in the optical with GTC/MEGARA – seeing limited integral field spectroscopy (GTC62-20B).
- 48 QSO2s with SDSS optical spectra.
- 48 QSO2s observed in the R-band with WFC/INT – seeing limited deep imaging (multiple observing runs, see Pierce et al. 2023).