Core research program
Lead developerSLICK
From gas physics to emission-line observables
SLICK predicts molecular and atomic emission from the physical conditions of gas in cosmological simulations, rather than relying solely on empirical galaxy-wide luminosity relations. Combining gas modeling with radiative-transfer calculations, it allows us to investigate not only how galaxies emit light, but why.
Related publications
- Garcia, K. et al. (2024), SLICK: Modeling a Universe of Molecular Line Luminosities in Hydrodynamical Simulations, ApJ.
- Garcia, K. et al., in preparation — SLICK-2 (multiphase, multi-line framework).
- Anirudh et al., including Garcia, K. (2025), Predicting the resolved CO emission of z = 1–3 star-forming galaxies, A&A.
Research directions built on SLICK
Line-Intensity Mapping
Predicting cosmic emission fields and interpreting multi-line surveys across cosmic time.
Related publications
- Bracks et al., including Garcia, K. (2026), ApJ.
- Agrawal et al., including Garcia, K. (2026), arXiv preprint.
- Karoumpis et al., including Garcia, K. (2024), A&A.
AGN & Gas Physics
Investigating how black hole radiation changes gas conditions and emission-line diagnostics.
Current work
- Garcia, K. et al., in preparation — SLICK-AGN.
CAMELS & Galaxy Formation
Testing how uncertain galaxy formation and feedback prescriptions affect observable line emission.
Current work
- CAMELS + SLICK — ongoing research.