Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Dip. di Fisica, II Universita' di Roma
Physics Department, II University of Rome
STScI / ESA
ESO
SAX Data Center, Roma
II Univ. di Roma, Italy
European Southern Observatory, D-85748 Garching bei München, Germany Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA; ESA Space Telescope Division II, University
on behalf of the Virtual Observatory Systems department at ESO European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748 Garching bei München, Germany Telescope Science Institute;, ESA Space Telescope Division
Space Telescope Science Institute; Department of Astronomy, University of California, Berkeley, CA 94720; Department of Physics and Astronomy, San Francisco State University, San Francisco, CA 94132. Telescope Institute, Baltimore, USA
Space Telescope Science Institute, Baltimore, USA
Space Telescope Science Institute, Baltimore, MD
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, Maryland 21218PaoloPadovaniEuropean Southern Observatory, Karl-Schwarzschild-Str. 2, D-8046 Garching bei München, Germany
STScI
ESA / STScI
ESA--STScI, Baltimore, USA
ST-Ecf / ESO
ESO, Germany
European Southern Observatory, Garching bei München
ST-ECF / ESO
University of Roma
ST-ECF, EUROPEAN SOUTHERN OBSERVATORY
Space Telescope Science Institute, Baltimore, MD; Padova, Università, Padua, Italy
European Southern Observatory
ESA, STScI
STScI, MAST
European Southern Observatory, Garching bei München, Germany
ESA, STScI / II University of Rome
ESO, Garching bei München, Germany
ESO, Garching bei München, Germany; Roma II, Univ., Rome; SISSA, Trieste, Italy
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA; Affiliated to the Space Telescope Division of the European Space Agency, ESTE
A catalogue of BL Lacertae objects (Padovani+ 1995)
A New Population of Radio Quasars
A New Population of Radio Quasars
A Physical Classification Scheme for Blazars
A pilot study for the creation of a large BL Lac sample
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Profile ID: LFWR-SCP-P-17297