From Nearby Low Luminosity AGN to High Redshift Radio Galaxies: Science Interests with SKA
P. Kharb (NCRA-TIFR, IIA), D. V. Lal (NCRA), V. Singh (PRL), J. Bagchi, (IUCAA), C. H. Ishwara Chandra (NCRA), A. Hota (CBS), C. Konar (Amity Univ),, Y. Wadadekar (NCRA), P. Shastri (IIA), M. Das (IIA), K. Baliyan (PRL), B. B., Nath (RRI), M. Pandey-Pommier (Univ Lyon)
TL;DR
This paper discusses the scientific opportunities with the SKA for studying active galactic nuclei across a wide range of luminosities and redshifts, emphasizing unresolved questions and current surveys.
Contribution
It outlines detailed science cases for the Indian AGN community utilizing SKA, covering low luminosity AGN to high redshift radio galaxies, and highlights ongoing GMRT surveys.
Findings
Identification of key science questions in AGN physics.
Potential of SKA to advance understanding of AGN across cosmic time.
Current GMRT surveys provide valuable data for future SKA studies.
Abstract
We present detailed science cases that a large fraction of the Indian AGN community is interested in pursuing with the upcoming Square Kilometre Array (SKA). These interests range from understanding low luminosity active galactic nuclei in the nearby Universe to powerful radio galaxies at high redshifts. Important unresolved science questions in AGN physics are discussed. Ongoing low-frequency surveys with the SKA pathfinder telescope GMRT, are highlighted.
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