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Nicholl, M.Smartt, S. J.Jerkstrand, A.Inserra, C.Sim, S. A.Chen, T. W.Benetti, S.Fraser, M.Gal Yam, AvishayKankare, E.Maguire, K.Smith, K.Sullivan, M.Valenti, S.Young, D. R.Baltay, C.Bauer, F. E.Baumont, S.Bersier, D.Botticella, M. T.Childress, M.Dennefeld, M.Della Valle, MassimoElias Rosa, N.Feindt, U.Galbany, LluisHadjiyska, E.Le Guillou, L.Leloudas, G.Mazzali, P.McKinnon, R.Polshaw, J.Rabinowitz, D.Rostami, S.Scalzo, R.Schmidt, B. P.Schulze, S.Sollerman, J.Taddia, F.Yuan, F.[On the diversity of superluminous supernovae: ejected mass as the dominant factor]

Context. Afterglows of gamma-ray bursts (GRBs) are simple in the most basic model, but can show many complex features. The ultra-long duration GRB 111209A, one of the longest GRBs ever detected, also has the best-monitored afterglow in this rare class of GRBs. Aims. We want to address the questio...


Kann, D.A.Schady, P.Olivares, E.F.Klose, S.Rossi, A.Perley, D.A.Zhang, B.Krühler, T.Greiner, J.Nicuesa Guelbenzu, A.Elliott, J.Knust, F.Cano, Z.Filgas, R.Pian, E.Mazzali, P.Fynbo, J.P.U.Leloudas, G.Afonso, P.M.J.Delvaux, C.Graham, J.F.Rau, A.Schmidl, S.Schulze, S.Tanga, M.Updike, A.C.Varela, K.[The optical/NIR afterglow of GRB 111209A: Complex yet not unprecedented]The optical/NIR afterglow of GRB 111209A: Complex yet not unprecedented

Tomasella, L.Cappellaro, E.Pumo, M.L.Jerkstrand, A.Benetti, S.Elias-Rosa, N.Fraser, M.Inserra, C.Pastorello, A.Turatto, M.Anderson, J.P.Galbany, L.Gutiérrez, C.P.Kankare, E.Pignata, G.Terreran, G.Valenti, S.Barbarino, C.Bauer, F.E.Botticella, M.T.Chen, T.-W.Gal-Yam, A.Harutyunyan, A.Howell, D.A.Maguire, K.Garoffolo, A.M.Ochner, P.Smartt, S.J.Schulze, S.Young, D.R.Zampieri, L.[SNe 2013K and 2013am: Observed and physical properties of two slow, normal Type IIP events]SNe 2013K and 2013am: Observed and physical properties of two slow, normal Type IIP events
Buchner, J.Schulze, S.Bauer, Franz Erik[Galaxy gas as obscurer - I. GRBs x-ray galaxies and find an NH^3 propto M_{star} relation]Galaxy gas as obscurer - I. GRBs x-ray galaxies and find an NH^3 propto M_{star} relation

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