Quasar Lensing: the Observer's Point of View

TL;DR

This paper discusses how quasar lensing and time-delay measurements can be used to determine the Hubble constant H_0 accurately, emphasizing observational constraints and the method's independence from standard candles.

Contribution

It explains the fundamentals of the time-delay method in quasar lensing and highlights how high-precision observations improve H_0 measurement accuracy.

Findings

Time-delay method provides competitive H_0 estimates.

High-quality observations enhance measurement precision.

The method is independent of standard candles.

Abstract

The determination of the Hubble parameter H_0 is probably one of the most important applications of quasar lensing. The method, based on the measurement of the so-called ``time-delay'' between the lensed images of distant sources, e.g., quasars, and on detailed mass modeling of the potential well responsible for the multiple images, yields an accuracy at least comparable with other techniques and that can be improved further with high precision observations, as can be obtained with intrumentation of constantly increasing quality. The basics of the ``time-delay'' method are described, and the emphasis is put on the observational constraints available to the astrophysicist in order to implement the method and to derive an accurate value for H_0, independent of any standard candle or any strong prior on the other cosmological parameters.