VLT adaptive optics imaging of QSO host galaxies and their close environment at z ∼ 2.5: Results from a pilot program
Falomo, R. Kotilainen, J. K. Scarpa, R. Treves, A. 2005 A&A 434, 469
The luminous host galaxies of high redshift BL Lac objects
Kotilainen, J. K. Hyvönen, T. Falomo, R.. 2005 A&A 440, 831
ESO Very Large Telescope Optical Spectroscopy of BL Lacertae Objects. I. New Redshifts
Sbarufatti, B. Treves, A. Falomo, R. Heidt, J.; Kotilainen, J. Scarpa, R. 2005 AJ 129, 559
Imaging Redshifts of BL Lacertae Objects
Sbarufatti, B. Treves, A. Falomo, R. 2005 ApJ 635, 173 (PDF)
Hubble Space Telescope ultraviolet spectroscopy of blazars: emission-line properties and black hole masses
Pian, E. Falomo, R. Treves, A. 2005 MNRAS 361, 919
The cosmic evolution of quasar host galaxies
R. Falomo, J. K. Kotilainen , C. Pagani, R. Scarpa, A. Treves, 2004, ApJ 604 495
The optical-near-infrared colour of the host galaxies of BL Lacertae objects
Kotilainen, J.K & Falomo R. 2004 A&A, 424, 107
Host galaxies of low z radio loud quasars: A search of Hubble space telescope archives.
Pagani, C. Falomo, R, and Treves, A. 2003 ApJ, 596 830
Black Hole Masses and The Fundamental Plane of BL Lacertae Objects
Luminosities of radio loud active galaxies: Black hole masses and host galaxy luminosity functions
Falomo, R., Carangelo, N. Treves, A. 2003 MNRAS, 343 505
The host galaxy - AGN connection at low and high redshift.
Falomo, R. 2002 Proc. High Energy Blazar Astronomy, Turku 2003, ASP Vol 299 p. 279
The black hole mass in low redshift radiogalaxies
Bettoni, D. Falomo R., Fasano G, Govoni F. 2003, A&A, 399 869
The fundamental plane of radiogalaxies
Bettoni, D. Falomo R., Fasano G, Govoni F. 2003, A&A, 380 471 (PDF)
The black hole mass of BL Lacs from the stellar velocity dispersion of the host galaxy.
Falomo, R. Kotilainen, J., & Treves, A. 2002 ApJ, 569, L35.
Optical identi cations of High Frequency Peakers PDF Dallacasa, D., Falomo, R. and C. Stanghellini 2002 AA 382 53
Near-infrared imaging of the host galaxies of three radio-loud quasars at z = 1.5
