From Nearby Low Luminosity AGN to High Redshift Radio Galaxies: Science Interests with Square Kilometre Array

Journal of astrophysics and astronomy

P. Kharb1 2³  B. B. Nath⁴  D. V. Lal³  M. Das⁷  Y. Wadadekar³  P. Shastri⁷  V. Singh⁷  C. H. Ishwara Chandra³  J. Bagchi⁵  M. Pandey-Pommier⁸  K. Baliyan¹  C. Konar⁶  A. Hota² 

[1] Astronomy & Astrophysics Division, Physical Research Laboratory, Ahmedabad 380 009, India.$$;UM-DAE Centre for Excellence in Basic Sciences, Vidyanagari, Mumbai 400 098, India.$$;National Centre for Radio Astrophysics – TIFR, Post Bag 3, Ganeshkhind, Pune 411 007, India.$$;Raman Research Institute, C. V. Raman Avenue, Sadashivanagar, Bangalore 560 080, India.$$;Inter-University Centre for Astronomy and Astrophysics, Pune, India.$$;Amity Institute of Applied Sciences, Amity University Uttar Pradesh, Sector-125, Noida, India.$$;Indian Institute of Astrophysics, II Block, Koramangala, Bangalore 560 034, India.$$;Centre de Recherche Astrophysique de Lyon UMR5574, Univ Lyon, Univ Lyon1, Ens de Lyon, CNRS, 9 av Charles Andr, 69230, Saint-Genis-Laval, France.$$

关键词: Galaxies: active;    galaxies: Seyfert;    quasars: general;    BL Lacertae objects: general;    radio continuum: galaxies.;   

DOI  :  

学科分类：天文学(综合)

来源: Indian Academy of Sciences

【 摘 要 】

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.

【 授权许可】

Unknown