THE AFTERGLOWS OF<i>SWIFT</i>-ERA GAMMA-RAY BURSTS. II. TYPE I GRB VERSUS TYPE II GRB OPTICAL AFTERGLOWS
Д. А. Канн(Thüringer Landessternwarte Tautenburg), K. Wiersema(University of Leicester), S. Klose(Thüringer Landessternwarte Tautenburg), P. D’Avanzo(Brera Astronomical Observatory), N. Butler(University of California, Berkeley), L. Stella(Astronomical Observatory of Rome), G. Tagliaferri(Brera Astronomical Observatory), Ehud Nakar(Tel Aviv University), D. Malesani(University of Copenhagen), M. Della Valle(Centre National de la Recherche Scientifique), V. D’Elia(Agenzia Spaziale Italiana), G. L. Israel(National Institute for Astrophysics), F. Mannucci(Arcetri Astrophysical Observatory), S. Piranomonte(Astronomical Observatory of Rome), S. Covino(Brera Astronomical Observatory), B. E. Cobb(George Washington University), S. Schulze(Northwestern University), L. A. Antonelli(Astronomical Observatory of Rome), P. Ferrero(Thüringer Landessternwarte Tautenburg), Bing Zhang(University of Nevada, Las Vegas), A. C. Wilson(The University of Texas at Austin), J. Gorosabel(Consejo Superior de Investigaciones Científicas), G. Chincarini(Brera Astronomical Observatory), D. Fugazza(National Institute for Astrophysics)
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