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This study presents Chandra observations of a high-redshift flat-spectrum radio quasar (FSRQ) with a FRII morphology, featuring a kiloparsec-scale jet. The analysis reveals a jet angle of approximately 4 degrees, with a magnitude in the V-band of 16.1 and a black hole mass of 4.6 x 10^8 solar masses. The Chandra observation conducted in 2003 for 70.12 ks, cleaned for 68.36 ks, utilized the ACIS-S detector with a 1/8 subarray to minimize core pileup. The study highlights core extended emission related to the kiloparsec-scale jet and knots. Additionally, it discusses X-ray, optical, and radio emissions at varying distances from the core.
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1136-135: Chandra observation • FSRQ at z=0.554 • FRII morphology, with kpc-scale jet • 4 deg • mV=16.1 • MBH=4.6 108 M • Chandra observation: 2003, 70.12 ks 68.36 ks cleaned • ACIS-S, 1/8 subarray to reduce core pileup (4%), Tframe=0.44 s Laboratorio Alte Energie - 2008
core extended emission kpc-jet and knots Laboratorio Alte Energie - 2008
X-ray optical radio Laboratorio Alte Energie - 2008
increasing distance from the core X-ray emission Laboratorio Alte Energie - 2008
increasing distance from the core radio emission Laboratorio Alte Energie - 2008