Simulating time-varying strong lenses
arXiv:2106.04344 · doi:10.1093/mnras/stac268
Abstract
We present a self-consistent and versatile forward modelling software package that can produce time series and pixel-level simulations of time-varying strongly lensed systems. The time dimension, which needs to take into account different physical mechanisms for variability such as microlensing, has been missing from existing approaches and it is of direct relevance to time delay, and consequently H0, measurements and caustic crossing event predictions. Such experiments are becoming more streamlined, especially with the advent of time domain surveys, and understanding their systematic and statistical uncertainties in a model-aware and physics-driven way can help improve their accuracy and precision. Here we demonstrate the software's capabilities by exploring the effect of measuring time delays from lensed quasars and supernovae in many wavelengths and under different microlensing and intrinsic variability assumptions. In this initial application, we find that the cadence of the observations and combining information from different wavelengths plays an important role in the correct recovery of the time delays. The Mock Lenses in Time (MOLET) software package is available at: \url{https://github.com/gvernard/molet}
14 pages, 8 figures, submitted to MNRAS
References in corpus (17)
- First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole
- Modeling the Time Variability of SDSS Stripe 82 Quasars as a Damped Random Walk
- Active Galactic Nuclei: what's in a name?
- Testing thermal reprocessing in AGN accretion discs
- H0LiCOW IV. Lens mass model of HE 0435-1223 and blind measurement of its time-delay distance for cosmology
- The Sloan Lens ACS Survey. VI: Discovery and analysis of a double Einstein ring
- H0LiCOW III. Quantifying the effect of mass along the line of sight to the gravitational lens HE 0435-1223 through weighted galaxy counts
- Microlensing Makes Lensed Quasar Time Delays Significantly Time Variable
- Accretion Disk Size Measurement and Time Delays in the Lensed Quasar WFI 2033-4723
- Toward an internally consistent astronomical distance scale
- Quasar microlensing light curve analysis using deep machine learning
- GERLUMPH Data Release 2: 2.5 billion simulated microlensing light curves
- Adventures in the microlensing cloud: large datasets, eResearch tools, and GPUs
- Microlensing flux ratio predictions for Euclid
- Imprints of the quasar structure in time-delay light curves: Microlensing-aided reverberation mapping
- The effect of macromodel uncertainties on microlensing modelling of lensed quasars
- Exploiting flux ratio anomalies to probe warm dark matter in future large scale surveys
Cited by in corpus (5)
- Using wavelets to capture deviations from smoothness in galaxy-scale strong lenses
- The Very Knotty Lenser: exploring the role of regularization in source and potential reconstructions using Gaussian Process Regression
- AI-driven spatio-temporal engine for finding gravitationally lensed type Ia supernovae
- Modeling lens potentials with continuous neural fields in galaxy-scale strong lenses
- Time delay estimation in unresolved lensed quasars