Analysis of 204 lensed quasars yields mean source crossing time of 2.59 years, Einstein radius crossing time of 11.29 years, average quasar half-light radius of 5.4 light-days, microlens mass fraction lower limit of 0.15, and 9% probability of high-magnification events.
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An updated strong lensing model of SDSSJ1110+6459 using JWST-resolved clumps yields M(<250 kpc) = 1.21^{+0.09}_{-0.04} imes 10^{14} M_/sun, heta_E = 10.8^{+0.3}_{-0.4} arcsec, and \mu_tot = 24.2^{+3.4}_{-1.2} with 2-8 imes better magnification precision than prior models.
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Microlensing time-scales and flux magnification probabilities of a sample of 204 lensed quasars
Analysis of 204 lensed quasars yields mean source crossing time of 2.59 years, Einstein radius crossing time of 11.29 years, average quasar half-light radius of 5.4 light-days, microlens mass fraction lower limit of 0.15, and 9% probability of high-magnification events.
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LEGGOS II: A Strong Lens Model and Source-Plane Projection of the Clumpy Star-Forming Galaxy SGASJ111020.0+645950.8 at z=2.48
An updated strong lensing model of SDSSJ1110+6459 using JWST-resolved clumps yields M(<250 kpc) = 1.21^{+0.09}_{-0.04} imes 10^{14} M_/sun, heta_E = 10.8^{+0.3}_{-0.4} arcsec, and \mu_tot = 24.2^{+3.4}_{-1.2} with 2-8 imes better magnification precision than prior models.