{ "id": "1908.02892", "version": "v1", "published": "2019-08-08T00:56:02.000Z", "updated": "2019-08-08T00:56:02.000Z", "title": "Measuring the distances to quasars at high redshifts with strong lensing", "authors": [ "Kai Liao" ], "comment": "7 pages, 5 figures, to appear in ApJ", "categories": [ "astro-ph.CO" ], "abstract": "Strongly lensed quasars with time-delay measurements are well known to provide the \"time-delay distances\" $D_{\\Delta t}=(1+z_L)D_LD_S/D_{LS}$ and the angular diameter distances to lens galaxies $D_L$. These two kinds of distances give stringent constraints on cosmological parameters. In this work, we explore a different use of time-delay observables: Under the assumption of a flat Universe, strong lensing observations can accurately measure the angular diameter distances to sources $D_S$. The corresponding redshifts of quasars may be up to $z_S\\sim4$ according to the forecast. The high-redshift distances would sample the Hubble diagram between SNe Ia and CMB, cosmological-model-independently providing direct information on the evolution of the nature of our Universe, for example, the dark energy Equation-of-State parameter $w(z)$. We apply our method to the existing lensing system SDSS 1206+4332 and get $D_S=2388_{-978}^{+2632}Mpc$ at $z_S=1.789$. We also make a forecast for the era of LSST. The uncertainty of $D_S$ depends on the redshifts of lens and source, the uncertainties of $D_{\\Delta t}$ and $D_L$, and the correlation between $D_{\\Delta t}$ and $D_L$ as well. Larger correlation would result in tighter $D_S$ determination.", "revisions": [ { "version": "v1", "updated": "2019-08-08T00:56:02.000Z" } ], "analyses": { "keywords": [ "high redshifts", "strong lensing", "angular diameter distances", "dark energy equation-of-state parameter", "high-redshift distances" ], "note": { "typesetting": "TeX", "pages": 7, "language": "en", "license": "arXiv", "status": "editable" } } }