Items where Author is "Arnaudova, M. I."

Number of items: 6.
Article
  • The DESI View of the Faint Radio Source Population in LoTSS DR2. (2026) M. I. Arnaudova, L. R. Holden, D. J. B. Smith, P. N. Best, R. Kondapally, K. J. Duncan, A. Bushi, S. Das, S. R. Flury, C. L. Hale, M. J. Hardcastle, H. J. A. Rottgering and S. Shenoy
  • The LOFAR Two-metre Sky Survey Deep Fields : new probabilistic spectroscopic classifications and the accretion rates of radio galaxies. (2025) M. I. Arnaudova, D. J. B. Smith, M. J. Hardcastle, P. N. Best, S. Das, S. Shenoy, K. J. Duncan, L. R. Holden, R. Kondapally, L. K. Morabito and H. J. A. Rottgering
  • A novel Bayesian approach for decomposing the radio emission of quasars : II. Link between quasar radio emission and black hole mass. (2025) B. -H. Yue, K. J. Duncan, P. N. Best, M. I. Arnaudova, L. K. Morabito, J. W. Petley, H. J. A. Röttgering, S. Shenoy and D. J. B. Smith picture_as_pdf
  • Radio-AGN activity across the galaxy population : dependence on stellar mass, star-formation rate, and redshift. (2024) R. Kondapally, P. N. Best, K. J. Duncan, H. J. A. Röttgering, D. J. B. Smith, I. Prandoni, M. J. Hardcastle, T. Holc, A. L. Patrick, M. I. Arnaudova, B. Mingo, R. K. Cochrane, S. Das, Paul Haskell, M. Magliocchetti, K. Małek, G. K. Miley, C. Tasse and W. L. Williams picture_as_pdf
  • Ubiquitous radio emission in quasars: Predominant AGN origin and a connection to jets, dust, and winds. (2024) G. Calistro Rivera, D. M. Alexander, C. M. Harrison, V. A. Fawcett, P. N. Best, W. L. Williams, M. J. Hardcastle, D. J. Rosario, D. J. B. Smith, M. I. Arnaudova, E. Escott, G. Gürkan, R. Kondapally, G. Miley, L. K. Morabito, J. Petley, I. Prandoni, H. J. A. Röttgering and B.-H. Yue
  • Exploring the radio-loudness of SDSS quasars with spectral stacking. (2024) M. I. Arnaudova, D. J. B. Smith, M. J. Hardcastle, Soumyadeep Das, A. Drake, Kenneth Duncan, G. Gürkan, M. Magliocchetti, L. K. Morabito, J. W. Petley, S. Shenoy and C. Tasse
  • This list was generated on Sun Aug 23 02:18:43 2026 BST.