# Time-delay cosmographic forecasts with strong lensing and JWST stellar kinematics

## TL;DR

This paper introduces a joint strong lensing and stellar dynamics framework using JWST-like data to precisely measure cosmological distances and the Hubble constant from individual lens systems, enhancing future cosmological constraints.

## Contribution

It develops a novel method combining pixelated source reconstruction with axisymmetric Jeans equations, demonstrating high-precision $H_0$ and distance measurements with upcoming telescope data.

## Key findings

- Time-delay distance constrained to 3.1% uncertainty.
- Potential to measure $H_0$ with < 2.0% uncertainty from multiple lenses.
- Distance to lens constrained with 2.4% precision.

## Abstract

We present a joint strong lensing and stellar dynamical framework for future time-delay cosmography purposes. Based on a pixelated source reconstruction and the axisymmetric Jeans equations, we are capable of constraining cosmological distances and hence the current expansion rate of the Universe ($H_0$) to the few percent level per lens, when high signal-to-noise integral field unit (IFU) observations from the next generation of telescopes become available. For illustrating the power of this method, we mock up IFU stellar kinematic data of the prominent lens system RXJ1131-1231, given the specifications of the James Webb Space Telescope. Our analysis shows that the time-delay distance ($D_{\Delta t}$) can be constrained with 3.1% uncertainty at best, if future IFU stellar kinematics are included in the fit and if the set of candidate model parameterisations contains the true lens potential. These constraints would translate to a 3.2% precision measurement on $H_0$ in flat $\Lambda$CDM cosmology from the single lens RXJ1131-1231, and can be expected to yield an $H_0$ measure with < 2.0% uncertainty, if similar gains in precision can be reached for two additional lens systems. Moreover, the angular diameter distance ($D_\mathrm{d}$) to RXJ1131-1231 can be constrained with 2.4% precision, providing two distance measurements from a single lens system, which is extremely powerful to further constrain the matter density ($\Omega_\mathrm{m}$). The measurement accuracy of $D_\mathrm{d}$, however, is highly sensitive to any systematics in the measurement of the stellar kinematics. For both distance measurements, we strongly advise to probe a large set of physically motivated lens potentials in the future, to minimise the systematic errors associated with the lens mass parameterisation.