On the impact of intergalactic dust on cosmology with type Ia supernovae

TL;DR

This paper examines how intergalactic dust affects supernova-based cosmological measurements, revealing biases in parameter estimation and proposing methods to mitigate these effects for future surveys.

Contribution

It identifies biases caused by intergalactic dust in supernova cosmology and evaluates their impact on cosmological parameters, suggesting observational strategies to reduce these biases.

Findings

Color corrections are biased by intergalactic dust.

Cosmological parameters like Omega_M and w are biased by a few percent.

Future observations can detect and correct for intergalactic dust effects.

Abstract

Supernova measurements have become a key ingredient in current determinations of cosmological parameters. These sources can however be used as standard candles only after correcting their apparent brightness for a number of effects. In this paper we discuss some limitations imposed by the formalism currently used for such corrections and investigate the impact on cosmological constraints. We show that color corrections are, in general, expected to be biased. In addition, color excesses which do not add a significant scatter to the observed SN brightnesses affect the value of cosmological parameters but leave the slope of the color-luminosity relation unchanged. We quantify these biases in the context of the redshift-dependent dust extinction suggested by the recent detection of intergalactic dust by Menard et al. (2009). Using a range of models for the opacity of the Universe as a function of redshift, we find that color-magnitude-stretch scaling relations are virtually insensitive to the presence of cosmic dust while cosmological parameters such as Omega_M and w are biased at the level of a few percent, i.e. offsets comparable to the current statistical errors. Future surveys will be able to limit the impact of intergalactic extinction by observing at larger wavelengths. In addition such datasets will provide direct detections of intergalactic dust by cross-correlating SN colors and the density of foreground galaxies, which can be used as a consistency check on the cosmic dust extinction correction. Alternatively, such biases could be avoided by correcting the colors of supernovae on an object-by-object basis with accurate photometry.