A&A 582, A3 (2015) Astronomy DOI: 10.1051/0004-6361/201525868 & c ESO 2015 Astrophysics A comparative study of Type II-P and II-L supernova rise times as exemplified by the case of LSQ13cuw E. E. E. Gall1,J.Polshaw1,R.Kotak1, A. Jerkstrand1, B. Leibundgut2, D. Rabinowitz3, J. Sollerman5, M. Sullivan6, S. J. Smartt1, J. P. Anderson7, S. Benetti8,C.Baltay9,U.Feindt10,11, M. Fraser4, S. González-Gaitán12,13 ,C.Inserra1, K. Maguire2, R. McKinnon9,S.Valenti14,15, and D. Young1 1 Astrophysics Research Centre, School of Mathematics and Physics, Queen’s University Belfast, Belfast BT7 1NN, UK e-mail:
[email protected] 2 ESO, Karl-Schwarzschild-Strasse 2, 85748 Garching, Germany 3 Center for Astronomy and Astrophysics, Yale University, New Haven, CT 06520, USA 4 Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, UK 5 Department of Astronomy, The Oskar Klein Centre, Stockholm University, AlbaNova, 10691 Stockholm, Sweden 6 School of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ, UK 7 European Southern Observatory, Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago, Chile 8 INAF Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, 35122 Padova, Italy 9 Department of Physics, Yale University, New Haven, CT 06250-8121, USA 10 Institut für Physik, Humboldt-Universität zu Berlin, Newtonstr. 15, 12489 Berlin, Germany 11 Physikalisches Institut, Universität Bonn, Nußallee 12, 53115 Bonn, Germany 12 Millennium Institute of Astrophysics, Casilla 36-D, Santiago, Chile 13 Departamento