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Phillips, M. M.Simon, Joshua D.Morrell, NidiaBurns, Christopher R.Cox, NickFoley, Ryan J.Karakas, AmandaPatat, F.Sternberg, A.Williams, R.Gal Yam, AvishayHsiao, EricLeonard, D.Persson, SvenStritzinger, MaximilianThompson, I.Campillay, AbdoContreras, CarlosFolatelli, GastónFreedman, Wendy L.Hamuy Wackenhut, MarioRoth, MiguelShields, GregorySuntzeff, Nicholas B.Chomiuk, LauraIvans, IneseMadore, BarryPenprase, B.Perley, DanielPignata Libralato, GiulianoPreston, G.Soderberg, Alicia[On the Source of the Dust Extinction in Type Ia Supernovae and the Discovery of Anomalously Strong Na I Absorption]

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]

Scalzo, R. A.Aldering, G.Antilogus, P.Aragón, C.Bailey, S.Baltay, C.Bongard, S.Buton, C.Childress, M.Chotard, N.Copin, Y.Fakhouri, H. K.Gal Yam, AvishayGangler, E.Hoyer, SergioKasliwal, M.Loken, S.Nugent, P.Pain, R.Pécontal, E.Pereira, R.Perlmutter, S.Rabinowitz, DavidRau, A.Rigaudier, G.Runge, K.Smadja, G.Tao, C.Thomas, R. C.Weaver, B.Wu, C.[NEARBY SUPERNOVA FACTORY OBSERVATIONS OF SN 2007IF: FIRST TOTAL MASS MEASUREMENT OF A SUPER-CHANDRASEKHAR-MASS PROGENITOR]

Perets, Hagai B.Gal Yam, AvishayMazzali, PaoloArnett, D.Kagan, D.Filippenko, Alexei V.Li, WeidongArcavi, I.Cenko, S. BradleyFox, D. B.Leonard, D. C.Moon, D.-S.Sand, D. J.Soderberg, A. M.Anderson, Joseph P.James, P. A.Foley, Ryan J.Ganeshalingam, MohanOfek, E. O.Bildsten, L.Nelemans, G.Shen, K. J.Weinberg, N. N.Metzger, B. D.Piro, A. L.Quataert, E.Kiewe, M.Poznanski, Dovi[A faint type of supernova from a white dwarf with a helium-rich companion]

Barbarino, C.Dall'Ora, M.Botticella, M. T.Della Valle, MassimoZampieri, L.Maund, J.Pumo, M.Jerkstrand, A.Benetti, S.Elias Rosa, N.Fraser, M.Gal Yam, AvishayHamuy Wackenhut, MarioInserra, C.Knapic, C.LaCluyze, A.Molinaro, M.Ochner, P.Pastorello, A.Pignata Libralato, GiulianoReichart, D.Ries, C.Riffeser, A.Schmidt, B.Schmidt, M.Smareglia, R.Smartt, S.Smith, K.Sollerman, J.Sullivan, M.Tomasella, L.Turatto, M.Valenti, S.Yaron, O.Young, D.[SN 2012ec: mass of the progenitor from PESSTO follow-up of the photospheric phase]

Nicholl, M.Smartt, S. J.Jerkstrand, A.Sim, S. A.Inserra, C.Anderson, J. P.Baltay, C.Benetti, S.Chambers, K.Chen, T. W.Elias Rosa, N.Feindt, U.Flewelling, H. A.Fraser, M.Gal Yam, AvishayGalbany, LluisHuber, M. E.Kangas, T.Kankare, E.Kotak, R.Kruehler, T.Maguire, K.McKinnon, R.Rabinowitz, D.Rostami, S.Schulze, SteveSmith, K.W.Sullivan, M.Tonry, J. L.Valenti, S.Young, D. R.[LSQ14bdq: A Type Ic super-luminous supernova with a double-peaked light curve]

Smith, M.Sullivan, M.D'Andrea, C. B.Castander, F. J.Casas, R.Prajs, S.Papadopoulos, A.Nichol, R. C.Karpenka, N. V.Bernard, S. R.Brown, P.Cartier Ugarte, RegisCooke, J.Curtin, C.Davis, T. M.Finley, D. A.Foley, R. J.Gal Yam, AvishayGoldstein, D. A.González Gaitán, SantiagoGupta, R. R.Howell, D. A.Inserra, C.Kessler, R.Lidman, C.Marriner, J.Nugent, P.Pritchard, T. A.Sako, M.Smartt, S.Smith, R. C.Spinka, H.Thomas, R. C.Wolf, R. C.Zenteno, A.Abbott, T. M.Benoit Levy, A.Bertin, E.Brooks, D.Buckley Geer, E.Carnero Rosell, A.Kind, CarrascoCarretero, J.Crocce, M.Cunha, C. E.da Costa, L. N.Desai, S.Fosalba, P.Frieman, J.Gerdes, D. W.Gruen, D.Gruendl, R. A.Marshall, J. L.Martini, P.Miller, C. J.Miquel, R.Nord, B. B.Ogando, R.Plazas, A. A.Reil, K.Romer, A. K.Roodman, A.Rykoff, E. S.Sánchez, E.Scarpine, V.Schubnell, M.Sevilla Noarbe, I.Soares Santos, M.Sobreira, F.Suchyta, E.Swanson, M. E. C.Tarle, G.Walker, A. R.Wester, W.[DES14X3taz: A type i superluminous supernova showing a luminous, rapidlycooling initial pre-peak bump]

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.Valle, M. DellaElías-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, SteveSollerman, J.Taddia, F.Yuan, F.[Erratum: On the diversity of superluminous supernovae: ejected mass as the dominant factor]

Foley, Ryan J.Simon, Joshua D.Burns, Christopher R.Gal Yam, AvishayHamuy Wackenhut, MarioKirshner, Robert P.Morrell, Nidia I.Phillips, Mark M.Shields, Gregory A.Sternberg, Assaf[Linking type Ia supernova progenitors and their resulting explosions]

Lyman, J. D.James, P. A.Perets, Hagai B.Anderson, J. P.Gal Yam, AvishayMazzali, PaoloPercival, S. M.[Environment-derived constraints on the progenitors of low-luminosity Type I supernovae]

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