spectroscopy

https://docs.google.com/spreadsheets/d/1p_Thr5zWqoERwhbO3Ud8AlLJWVeFNXUZEmEtTX9NI18

UV line strengths (Stark+17): detections are a few e-18 erg / cm^2 / s

Planning to consider:

– BC03 + CLOUDY nebular emission lines

– MegaSaura (Rigby): z ~ 2 lensed

– LYCAN (Zackrisson): z = 7 models

– (observed line widths of CIII], etc.)

could also include:

Senchyna, Stark, et al. 2017:

Ultraviolet spectra of extreme nearby star-forming regions - approaching a local reference sample for JWST

– BPASS: binaries and rotation

– MAPPINGS: photoionization radiative transfer code (Lisa Kewley & David Nicholls)

Brett's spectral library cheat sheet:

https://docs.google.com/spreadsheets/d/1346FJ3-HFr0hFw9ePbu-0I03aT9KOo0o4RV81p-tZFU