Cosmic Sands II: Challenges in Predicting and Measuring High-z Dust Temperatures

TL;DR

This paper examines the challenges and uncertainties in modeling and measuring dust temperatures in high-redshift galaxies, highlighting limitations of current methods and the impact on interpreting early universe observations.

Contribution

It provides a detailed analysis of the limitations in both forward and backward modeling of high-z galaxy dust temperatures using simulations and observational data.

Findings

Simulations can predict dust evolution but depend on free parameters.

Common SED fitting models often fail to capture galaxy complexity.

Uncertainties in models and observations limit the interpretability of high-z dust measurements.

Abstract

In the current era of high-z galaxy discovery with JWST and ALMA, our ability to study the stellar populations and ISM conditions in a diverse range of galaxies at Cosmic Dawn has rapidly improved. At the same time, the need to understand the current limitations in modeling galaxy formation processes and physical properties in order to interpret these observations is critical. Here, we study the challenges in modeling galaxy dust temperatures, both in the context of forward modeling galaxy spectral properties from a hydrodynamical simulation and via backwards modeling galaxy physical properties from mock observations of far-infrared dust emission. Using the Simba model for galaxy formation combined with Powderday radiative transfer, we can accurately predict the evolution of dust at high redshift, though several aspects of the model are essentially free parameters (dust composition, sub-resolution dust in star-forming regions) that dull the predictive power of the model dust temperature distributions. We also highlight the uncertainties in the backwards modeling methods, where we find the commonly used models and assumptions to fit FIR SEDs and infer dust temperatures (e.g., single temperature, optically thin modified blackbody) largely fail to capture the complexity of high-z dusty galaxies. We caution that conclusions inferred from both simulations -- limited by resolution and post-processing techniques -- and observations -- limited by sparse data and simplistic model parameterizations -- are susceptible to unique and nuanced uncertainties that can limit the usefulness of current high-z dust measurements.