Gravitational Lensing as Signal and Noise in Lyman-alpha Forest Measurements
Marilena LoVerde, Stefanos Marnerides, Lam Hui, Brice Menard, Adam, Lidz

TL;DR
Gravitational lensing affects Lyman-alpha forest measurements by introducing bias and providing a new signal to probe the mass density field, challenging assumptions and enabling tests of cosmic structure models.
Contribution
This paper reveals how gravitational lensing impacts Lyman-alpha forest data analysis and proposes methods to extract the lensing signal for cosmological insights.
Findings
Lensing causes a 0.1-1% bias in flux measurements.
Correlations between quasar brightness and flux spectra can reveal mass distribution.
Lensing effects can test whether forest fluctuations are driven by mass or other factors.
Abstract
In Lyman-alpha forest measurements it is generally assumed that quasars are mere background light sources which are uncorrelated with the forest. Gravitational lensing of the quasars violates this assumption. This effect leads to a measurement bias, but more interestingly it provides a valuable signal. The lensing signal can be extracted by correlating quasar magnitudes with the flux power spectrum and with the flux decrement. These correlations will be challenging to measure but their detection provides a direct measure of how features in the Lyman-alpha forest trace the underlying mass density field. Observing them will test the fundamental hypothesis that fluctuations in the forest are predominantly driven by fluctuations in mass, rather than in the ionizing background, helium reionization or winds. We discuss ways to disentangle the lensing signal from other sources of such…
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