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PRODID:-//Heidelberg University//HePhySTO//EN
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BEGIN:VEVENT
DTEND:20270204T111500Z
UID:5159f491c0b80a0240346b62b6e4cfd5@physik.uni-heidelberg.de
DTSTAMP:20261007T213855Z
LOCATION:ARI\, Moenchhofstrasse 12-14\, Seminarraum 1.OG
DESCRIPTION:Studying the impact of Active Galactic Nuclei (AGN) on the inte
 rstellar medium at high redshift\nis crucial for understanding how galaxies
  evolve. In this talk\, I will first present results from 4C +03.24\, a pow
 erful radio galaxy at z ~ 3.5\, using integral-field spectroscopy obtained 
 with JWST/NIRSpec. The joint analysis of our observations with archival VLT
 /MUSE and HST data reveals extended continuum emission (~14 kpc)\, possibly
  arising from recent star formation and associated with nearby companions. 
 The presence of a gap in the [CII] emission within the bipolar region domin
 ated by AGN photo-ionization may provide direct evidence of negative AGN fe
 edback. We further find that the outflow power associated with the kinemati
 cally\ndisturbed ionized gas peaks ~ 2 kpc from the nucleus\, with a low ki
 netic coupling efficiency of ~0.0063%. In the second part\, I will discuss 
 new results on AGN across different epochs (1 < z < 6)\, obtained from arch
 ival JWST data.\n\nImported from https://www.physik.uni-heidelberg.de/hephy
 sto/ (no warranty for accuracy).
URL;VALUE=URI:https://www.physik.uni-heidelberg.de/hephysto/index.php?s=tal
 k&id=13018
SUMMARY:ARI Institute Colloquium: Bruno Dall’Agnol de Oliveira - Exploring 
 AGN Feedback at different epochs with JWST
DTSTART:20270204T101500Z
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