RT Journal Article ID 43f7081512461bf8 A1 Butuzova, M. S. T1 PARAMETER DETERMINATION OF KILOPARSEC JETS AT LARGE REDSHIFTS BY THEIR RADIO AND X-RAY EMISSION JF Radio Physics and Radio Astronomy JO RPRA YR 2012 FD 2012-05-15 VO 3 IS 2 SP 123 OP 130 K1 kiloparsec jet K1 radio and X-ray emission K1 jet to line of sight angle K1 inverse Compton scattering K1 quasar 1745+624 K1 quasar PKS 1127-14 AB The 1745+624 and PKS 1127−14 quasar jets are considered. The X-ray emission of the near-central source knots is produced by the inverse Compton scattering of quasar radiation, while the inverse Compton scattering on the cosmic microwave background occurs at distant knots. The competition of these mechanisms has allowed to estimate the angles between the jets and the line of sight. The ratio of X-ray to radio flux densities of distant knots is shown to conform to the theoretical dependence on the redshift. PB Begell House LK https://www.dl.begellhouse.com/journals/6fd1549c0e2c05da,6f536281699b948c,43f7081512461bf8.html