2020ApJ...892L..27B


Query : 2020ApJ...892L..27B

2020ApJ...892L..27B - Astrophys. J., 892, L27-L27 (2020/April-1)

Could quasar lensing time delays hint to a core component in halos, instead of H0 tension?

BLUM K., CASTORINA E. and SIMONOVIC M.

Abstract (from CDS):

The time delay measured between the images of gravitationally lensed quasars probes a combination of the angular diameter distance to the source-lens system and the mass density profile of the lens. Observational campaigns to measure such systems have reported a determination of the Hubble parameter H0 that shows significant tension with independent determination based on the cosmic microwave background (CMB) and large-scale structure (LSS). We show that lens mass models that exhibit a cored component, coexisting with a cusp, probe a degenerate direction in the lens model parameter space, being an approximate mass sheet transformation. This family of lens models has not been considered by the cosmographic analyses. Once added to the model, the cosmographic error budget should become dependent on stellar kinematics uncertainties. We propose that a core component coexisting with a cusp could bring the lensing measurements of H0 into accordance with the CMB/LSS value.

Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.

Journal keyword(s): Gravitational lensing - Strong gravitational lensing - Hubble constant - Galaxy structure

Simbad objects: 7

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Number of rows : 7
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 [ALB2017] DES J0408-5354 gLS 04 08 21.70 -53 53 59.6           ~ 37 0
2 [VV2006] J043814.8-122314 QSO 04 38 14.88 -12 17 14.6     17.15     ~ 245 2
3 QSO B1115+080A QSO 11 18 16.951 +07 45 58.23   16.61 16.44     ~ 703 2
4 2MASS J11315154-1231588 Sy1 11 31 51.5387 -12 31 58.716           ~ 304 1
5 [OIH2005] SDSS J1206+4332 gLS 12 06 29.6 +43 32 17           ~ 63 0
6 M 60 GiC 12 43 39.9708251934 +11 33 09.688174067   10.3       ~ 1395 1
7 [VV2006] J203342.1-472343 QSO 20 33 42.12 -47 23 43.9           ~ 135 1

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