We propose for deep Chandra-HST observations of 3 hybrid MOJAVE quasars. As these sources have jets with different powers (Fanaroff-Riley type I & II) on either side of the central engine they could be the touchstone for ideas put forth to explain the question of the FR dichotomy and the nature of AGN jets in general. These deep observations will constrain unambiguously the X-ray emission mechanisms in these jets through the construction and modeling of broad-band SEDs at multiple jet positions. The X-ray imaging may reveal asymmetries in the hot gas on either side of the AGN, telling us about jet propagation in low/high power sources. The lack of such features may provide support to the idea of highly magnetized jets, which could be examined further through broad-band SED modeling. We will observe the 3 quasars with arcsecond-scale radio jets, viz., 1045-188, 1849+670 and 2216-038, through the Wide Field Camera 3 (WFC3) on board HST, through the F160W (IR channel) and the F475W (UVIS channel) filters. The aim is to detect optical emission at various locations or knots along the jets of these quasars. Spectral index images will be made for these jet knots to understand the jet emission mechanism(s). Each target will be observed through each of the 2 filters (F160W and F475W) for 1 HST orbit each, giving a total of 6 orbits. Each orbit/visit is divided into 3 (sub-)exposures to create a 3-point LINE DITHER pattern. 12 false false 0.0 0.0 false false false SUPPORTED GALAXY ELLIPTICAL JET QUASAR J2000 J2000 GALAXY ELLIPTICAL JET QUASAR J2000 J2000 GALAXY ELLIPTICAL JET QUASAR J2000 J2000 WFC3/IR Imaging No No F160W WFC3/UVIS Imaging No No F475W WFC3/IR Imaging No No F160W WFC3/UVIS Imaging No No F475W WFC3/IR Imaging No No F160W WFC3/UVIS Imaging No No F475W POS-TARG DITHER 0.605 LINE false false 3 41.788 WFC3-IR-DITHER-LINE-3PT 1 false POS-TARG DITHER 0.135 LINE false false 3 46.84 WFC3-UVIS-DITHER-LINE-3PT 2 false The scheduling data was generated by CASM 21.0. CASM was run in Phase II mode. Observing 1045-188 through IR filter F160W and UVIS filter F475W Jet PA = 127 deg (Tic-Visit :proposal-id 13116 :visit-id "01" :proposal-version -1 :trans-version "20121031" :date "01-Apr-2013 09:50:51.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 1440720 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13116 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13116 :visit-id "01" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2875 :al-overhead-at-end 0 :internal-dur-at-end 65 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3244 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13116 :visit-id "01" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3021 :al-overhead-at-end 116 :internal-dur-at-end 352 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3244 :pcs-gap 0 ) true 2 0 The scheduling data was generated by CASM 21.0. CASM was run in Phase II mode. Observing 1849+670 through IR filter F160W and UVIS filter F475W Jet PA = 7 deg (Tic-Visit :proposal-id 13116 :visit-id "02" :proposal-version -1 :trans-version "20121031" :date "01-Apr-2013 09:50:53.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 1492944 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13116 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13116 :visit-id "02" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3175 :al-overhead-at-end 0 :internal-dur-at-end 65 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3582 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13116 :visit-id "02" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3360 :al-overhead-at-end 116 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3582 :pcs-gap 0 ) true 2 0 The scheduling data was generated by CASM 21.0. CASM was run in Phase II mode. Observing 2216-038 through IR filter F160W and UVIS filter F475W Jet PA = 140 deg (Tic-Visit :proposal-id 13116 :visit-id "03" :proposal-version -1 :trans-version "20121031" :date "01-Apr-2013 09:50:54.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 1440720 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13116 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13116 :visit-id "03" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2875 :al-overhead-at-end 0 :internal-dur-at-end 65 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13116 :visit-id "03" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3006 :al-overhead-at-end 116 :internal-dur-at-end 352 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) false 2 0