# Inverse-Compton scattering in the resolved jet of the high-redshift quasar PKS J1421-0643

D. M. Worrall*, M. Birkinshaw, H. L. Marshall, D. A. Schwartz, A. Siemiginowska, J. F. C. Wardle

*Corresponding author for this work

Research output: Contribution to journalArticle (Academic Journal)peer-review

7 Citations (Scopus)

## Abstract

Despite the fact that kpc-scale inverse-Compton (iC) scattering of cosmic microwave background (CMB) photons into the X-ray band is mandated, proof of detection in resolved quasar jets is often insecure. High redshift provides favourable conditions due to the increased energy density of the CMB, and it allows constraints to be placed on the radio synchrotron-emitting electron component at high energies that are otherwise inaccessible. We present new X-ray, optical and radio results from Chandra, HST and the VLA for the core and resolved jet in the $z=3.69$ quasar PKS J1421-0643. The X-ray jet extends for about $4.5''$ (32 kpc projected length). The jet's radio spectrum is abnormally steep and consistent with electrons being accelerated to a maximum Lorentz factor of about 5000. Results argue in favour of the detection of inverse-Compton X-rays for modest magnetic field strength of a few nT, Doppler factor of about 4, and viewing angle of about $15^\circ$, and predict the jet to be largely invisible in most other spectral bands including the far- and mid-infrared and high-energy gamma-ray. The jet power is estimated to be about $3 \times 10^{46}$ erg s$^{-1}$ which is of order a tenth of the quasar bolometric power, for an electron--positron jet. The jet radiative power is only about 0.07 per cent of the jet power, with a smaller radiated power ratio if the jet contains heavy particles, so most of the jet power is available for heating the intergalactic medium.
Original language English staa1975 988–1000 13 Monthly Notices of the Royal Astronomical Society 497 1 8 Jul 2020 https://doi.org/10.1093/mnras/staa1975 Published - 1 Sep 2020

### Bibliographical note

16 pages, 14 figures. Accepted for publication in MNRAS

## Keywords

• galaxies: active
• galaxies: jets
• quasars: individual: PKS J1421-0643