The abundance and emission of PAHs from the local to early Universe
astro-ph.GA, astro-ph.CO
Submitted: 2026-09-28
Updated: 2026-09-28
Project page: https://lgalaxiespublicrelease.github.io/index.html
Terminology
Sources
- A panchromatic view of N2CLS GOODS-N: the evolution of the dust cosmic density since z~7
- Ashes of FIRE: Modeling Dust Grain Size Evolution in the Local Group with FIRE
- PAHSPECS: Spatially Resolved PAH Spectroscopy at cosmic noon with JWST MIRI MRS
- Cosmic Noon Galaxies in the Hubble Ultra Deep Field with MIRI Wide-Field Slitless Spectroscopy
- PAHSPECS: Polycyclic aromatic hydrocarbon properties at cosmic noon with JWST/MIRI MRS
- The Lifecycle and Emission Properties of PAHs in Cosmological Hydrodynamic Galaxy Formation Simulations
- Modeling Dust in Galaxy Evolution Simulations
- Dust and Grain Size Evolution in Galaxy Simulations: What Matters and What Does Not
- PAH Emission Spectra and Band Ratios for Arbitrary Radiation Fields with the Single Photon Approximation
- CALIMA: On-the-fly dust and PAH evolution for radiation-hydrodynamics galaxy formation simulations
- PAHSPECS: JWST/MIRI Spectroscopy of PAHs at Cosmic Noon
- Growth of Aromatic Hydrocarbon Dust Particles in the Extremely Metal-poor Galaxy Sextans A
- Resolved Dust in z about1 Galaxies with JWST/MIRI MRS: Survey Description and First View on PAHs, Mid-IR Atomic Emission, and Warm H 2
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