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Hsiao, EricBurns, C.R.Contreras, C.Höflich, P.Sand, D.Marion, G.H.Phillips, M. M.Stritzinger, M.González Gaitán, SantiagoMason, R. E.Folatelli, GastónParent, E.Gall, C.Amanullah, R.Anupama, G. C.Arcavi, I.Banerjee, D. P. K.Beletsky, Y.Blanc Mendiberri, GuillermoBloom, J. S.Brown, P. J.Campillay, A.Cao, Y.Cia, A. deDiamond, T.Freedman, W. L.González, C.Goobar, A.Holmbo, S.Howell, D. A.Johansson, J.Kasliwal, M. M.Kirshner, R. P.Krisciunas, K.Kulkarni, S. R.Maguire, K.Milne, P. A.Morrell, N.Nugent, P. E.Ofek, E. O.Osip, D.Palunas, P.Perley, D. A.Persson, S. E.Piro, A. L.Rabus, M.Roth, M.Schiefelbein, J. M.Srivastav, S.Sullivan, M.Suntzeff, Nicholas B.Surace, J.Wózniak, P. R.Yaron, O.[Strong near-infrared carbon in the Type Ia supernova iPTF13ebh]

The enigmatic near-infrared transient VVV-WIT-06 underwent a large-amplitude eruption of unclear origin in 2013 July. Based on its light curve properties and late-time post-outburst spectra, various possibilities have been proposed in the literature for the origin of the object, namely a Type I s...


Banerjee, D.P.K.Hsiao, E.Y.Diamond, T.Galbany, L.Morrell, N.Minniti, D.Kuncarayakti, H.Mattila, S.Harmanen, J.[Unraveling the Infrared Transient VVV-WIT-06: The Case for the Origin as a Classical Nova]Unraveling the Infrared Transient VVV-WIT-06: The Case for the Origin as a Classical Nova

Hsiao, EricBurns, C. R.Contreras, C.Höflich, P.Sand, D.Marion, G. H.Phillips, M. M.Stritzinger, M.González Gaitán, FranciscoMason, R. E.Folatelli, GastónParent, E.Gall, C.Amanullah, R.Anupama, G. C.Arcavi, I.Banerjee, D. P. K.Beletsky, Y.Blanc Mendiberri, GuillermoBloom, J. S.Brown, P. J.Campillay, A.Cao, Y.De Cia, A.Diamond, T.Freedman, W. L.González, C.Goobar, A.Holmbo, S.Howell, D. A.Johansson, J.Kasliwal, M. M.Kirshner, R. P.Krisciunas, K.Kulkarni, S. R.Maguire, K.Milne, P. A.Morrell, N.Nugent, P. E.Ofek, E. O.Osip, D.Palunas, P.Perley, D. A.Persson, S. E.Piro, A. L.Rabus, M.Roth, M.Schiefelbein, J. M.Srivastav, S.Sullivan, M.Suntzeff, Nicholas B.Surace, J.Woźniak, P. R.Yaron, O.[Strong near-infrared carbon in the Type Ia supernova iPTF13ebh]

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