Testing strong lensing subhalo detection with a cosmological simulation. Issue 1 (29th September 2022)

• Record Type: Journal Article
• Authors: He, Qiuhan; Nightingale, James; Robertson, Andrew; Amvrosiadis, Aristeidis; Cole, Shaun; Frenk, Carlos S; Massey, Richard; Li, Ran; Amorisco, Nicola C; Metcalf, R Benton; Cao, Xiaoyue; Etherington, Amy
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 518:Issue 1(2023)
• Page Start: 220
• Page End: 239
• Publication Date: 2022-09-29
• Subjects: (cosmology:) dark matter -- gravitational lensing: strong; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stac2779
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: Strong gravitational lensing offers a compelling test of the cold dark matter paradigm, as it allows for subhaloes with masses of ∼10 9 M⊙ and below to be detected. We test commonly used techniques for detecting subhaloes superposed in images of strongly lensed galaxies. For the lens we take a simulated galaxy in a ∼10 13 M⊙ halo grown in a high-resolution cosmological hydrodynamical simulation, which we view from two different directions. Though the resolution is high, we note the simulated galaxy still has an artificial core which adds additional complexity to the baryon dominated region. To remove particle noise, we represent the projected galaxy mass distribution by a series of Gaussian profiles which precisely capture the features of the projected galaxy. We first model the lens mass as a (broken) power-law density profile and then search for small haloes. Of the two projections, one has a regular elliptical shape, while the other has distinct deviations from an elliptical shape. For the former, the broken power-law model gives no false positives and correctly recovers the mass of the superposed small halo; however, for the latter we find false positives and the inferred halo mass is overestimated by ∼4–5 times. We then use a more complex model in which the lens mass is decomposed into stellar and dark matter components. In this case, we show that we can capture the simulated galaxy's complex projected structures and correctly infer the input small halo.