Structured jets in TeV BL Lac objects and radiogalaxies-Implications for the observed properties G Ghisellini, F Tavecchio, M Chiaberge Astronomy & Astrophysics 432 (2), 401-410, 2005 | 774 | 2005 |
Large-scale jets in active galactic nuclei: multiwavelength mapping A Celotti, G Ghisellini, M Chiaberge Monthly Notices of the Royal Astronomical Society 321 (1), L1-L5, 2001 | 386 | 2001 |
An optical spectroscopic survey of the 3CR sample of radio galaxies with z 0.3-II. Spectroscopic classes and accretion modes in radio-loud AGN S Buttiglione, A Capetti, A Celotti, DJ Axon, M Chiaberge, FD Macchetto, ... Astronomy & Astrophysics 509, A6, 2010 | 378* | 2010 |
The HST view of FR I radio galaxies: evidence for non-thermal nuclear sources M Chiaberge, A Capetti, A Celotti arXiv preprint astro-ph/9907064, 1999 | 354 | 1999 |
Extreme synchrotron BL Lac objects-Stretching the blazar sequence L Costamante, G Ghisellini, P Giommi, G Tagliaferri, A Celotti, ... Astronomy & Astrophysics 371 (2), 512-526, 2001 | 322 | 2001 |
Rapid variability in the synchrotron self-Compton model for blazars M Chiaberge, G Ghisellini Monthly Notices of the Royal Astronomical Society 306 (3), 551-560, 1999 | 272 | 1999 |
The soft X-ray/NLR connection: a single photoionized medium? S Bianchi, M Guainazzi, M Chiaberge Astronomy & Astrophysics 448 (2), 499-511, 2006 | 270 | 2006 |
Does the unification of BL Lac and FR I radio galaxies require jet velocity structures? M Chiaberge, A Celotti, A Capetti, G Ghisellini arXiv preprint astro-ph/0003197, 2000 | 234 | 2000 |
Chandra unveils a binary active galactic nucleus in Mrk 463 S Bianchi, M Chiaberge, E Piconcelli, M Guainazzi, G Matt Monthly Notices of the Royal Astronomical Society 386 (1), 105-110, 2008 | 201 | 2008 |
Radio loud AGNs are mergers M Chiaberge, R Gilli, JM Lotz, C Norman The Astrophysical Journal 806 (2), 147, 2015 | 172 | 2015 |
Optical photometric monitoring of γ-ray loud blazars.-I. Observations from November 1994 to November 1995 M Villata, CM Raiteri, G Ghisellini, G De Francesco, S Bosio, G Latini, ... Astronomy and Astrophysics Supplement Series 121 (1), 119-138, 1997 | 171 | 1997 |
X-ray emission of markarian 421: New clues from its spectral evolution. ii. spectral analysis and physical constraints G Fossati, A Celotti, M Chiaberge, YH Zhang, L Chiappetti, G Ghisellini, ... The Astrophysical Journal 541 (1), 166, 2000 | 166 | 2000 |
How complex is the obscuration in active galactic nuclei? New clues from the suzaku monitoring of the X-ray absorbers in NGC 7582 S Bianchi, E Piconcelli, M Chiaberge, EJ Bailón, G Matt, F Fiore The Astrophysical Journal 695 (1), 781, 2009 | 152 | 2009 |
Double-peak structure in the cyclic optical outbursts of blazar OJ 287. A Sillanpaa, LO Takalo, T Pursimo, K Nilsson, P Heinamaki, S Katajainen, ... Astronomy and Astrophysics, v. 315, p. L13-L16 315, L13-L16, 1996 | 150 | 1996 |
The BL lac heart of centaurus A M Chiaberge, A Capetti, A Celotti Monthly Notices of the Royal Astronomical Society 324 (4), L33-L37, 2001 | 132 | 2001 |
On the origin of radio loudness in active galactic nuclei and its relationship with the properties of the central supermassive black hole M Chiaberge, A Marconi Monthly Notices of the Royal Astronomical Society 416 (2), 917-926, 2011 | 128 | 2011 |
X-ray emission of Markarian 421: New clues from its spectral evolution. I. temporal analysis G Fossati, A Celotti, M Chiaberge, YH Zhang, L Chiappetti, G Ghisellini, ... The Astrophysical Journal 541 (1), 153, 2000 | 122 | 2000 |
Understanding the nature of FR II optical nuclei: A new diagnostic plane for radio galaxies M Chiaberge, A Capetti, A Celotti Astronomy & Astrophysics 394 (3), 791-800, 2002 | 109 | 2002 |
The concave X-ray spectrum of the blazar ON 231: the signature of intermediate BL Lacertae objects G Tagliaferri, G Ghisellini, P Giommi, L Chiappetti, L Maraschi, A Celotti, ... Astronomy and Astrophysics, v. 354, p. 431-438 (2000) 354, 431-438, 2000 | 101 | 2000 |
The hst view of the fr I/fr II dichotomy M Chiaberge, A Capetti, A Celotti arXiv preprint astro-ph/0002018, 2000 | 98 | 2000 |