Maximum likelihood spectral fitting and its application to EBL constraints

TL;DR

This paper applies a maximum-likelihood spectral fitting method to VHE gamma-ray data from blazars to derive model-dependent constraints on the extragalactic background light, advancing indirect measurement techniques.

Contribution

It introduces a maximum-likelihood approach to fit blazar spectra and extract EBL constraints, incorporating theoretical models as free parameters.

Findings

Preliminary EBL constraints obtained from VERITAS data.

Method demonstrates potential for indirect EBL measurement.

Framework allows for model-dependent analysis of EBL shape and intensity.

Abstract

The extragalactic background light (EBL) is the second-most-intense form of cosmic background light (the first being the cosmic microwave background) and contains the redshifted optical radiation, from infra-red to ultraviolet, emitted across all epochs, making it of great cosmological interest. While direct measurements of the EBL are hampered by foreground contamination, observations of VHE emission from distant sources can be used to obtain indirect measurements of the EBL. In this work a maximum-likelihood fit is applied to the energy spectra of blazars observed by VERITAS, an array of ground-based imaging atmospheric Cherenkov telescopes sensitive to very-high-energy (VHE; E>100 GeV) gamma rays. Using theoretical models of the EBL shape and intensity, the EBL normalization is treated as a free parameter, allowing for model-dependent constraints to be obtained. Details of this maximum-likelihood analysis and preliminary model-dependent constraints on the EBL, are presented.