BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:From Radio to γ-rays: Emission Processes in Relativistic AGN Jets
  [Astrophysics Seminar]
DTSTART:20260202T100000Z
DTEND:20260202T110000Z
DTSTAMP:20260418T033700Z
UID:indico-event-400@events.iiap.res.in
DESCRIPTION:Speakers: Sanna Gulati (NCRA-TIFR)\n\nAbstractActive Galactic 
 Nuclei (AGN) powered by supermassive black holes launch relativistic jets 
 that emit across the electromagnetic spectrum. Studying this broad emissio
 n helps us understand particle acceleration\, jet structure\, and how ener
 gy is released in these extreme environments. In this talk\, I will presen
 t recent multiwavelength studies that combine radio\, X-ray\, and gamma-ra
 y observations of different AGN systems. This includes low-frequency uGMRT
  results from the Palomar-Green (PG) quasar sample\, which provide new ins
 ights into extended radio emission and its connection to accretion and jet
  power\; broadband modeling of sources such as NGC 1275 and Pictor A\, rev
 ealing complex jet components and high-energy behavior\; and constraints o
 n the gamma-ray emission region in the quasar 3C 380 using radio-gamma cor
 relations and SED modeling. Together\, these results show how observations
  from MHz radio to GeV gamma-rays can uncover the physical conditions with
 in AGN jets and improve our understanding of their emission processes and 
 unification.\n\nhttps://events.iiap.res.in/event/400/
LOCATION:Auditorium
URL:https://events.iiap.res.in/event/400/
END:VEVENT
END:VCALENDAR