Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the $Kepler$ 2 Observations

ePESSTO,; Wang, X.; Vinkó, J.; Sand, D.~J J.; Zhang, J.; Zhang, T.; Wang, L.; Zhang, X.; Xiang, D.; Zhang, K.; Rui, L.; Zhao, X.; Sai, H.; Valenti, S.; Rest, A.; Tucker, B.~E E.; Shaya, E.; Ucsc,; Zenteno, A.; Villar, A.; Riess, A.~G G.; Rojas-Bravo, C.; Shappee, Benjamin J.; Stanek, K.~Z Z.; Shields, J.; Tallon, D.; Thompson, T.~A A.; Starrs, Pan; Vallely, P.~J J.; Villanueva, Jr. S.; Smartt, S.~J J.; Smith, K.~W W.; Waters, C.~Z Z.; Schultz, A.~S.~B S. B.; Willman, M.; Sárneczky, K.; Wheeler, J.~C C.; Sódor, A.; Szabó, R.; Szakáts, R.; Zsidi, G.; Swift,; Smith, N.; Williams, S.~C C.; Reding, J.~S S.; Tonry, J.~L L.; Vinícius de Miranda Cardoso, J.; Weiland, H.; Stalder, B.; Team, Kepler Spacecraft; Van Cleve, J.~E E.; Ross, S.~E E.; Reedy, L.~H H.; Wheaton, A.; Spencer, B.; Steward, K.; Weschler, T.; Redick, M.; Li, W.; Mo, J.; Hosseinzadeh, G.; Lin, H.; Ptss/Tnts,; Chen, Z.; Huang, F.; Li, X.; Li, L.; Baron, E.; Derkacy, J.~M M.; Lco,; Howell, D.~A A.; McCully, C.; Arcavi, I.; Kegs,; Hiramatsu, D.; Burke, J.; Garnavich, P.; Narayan, G.; Margheim, S.; Holoien, T.~W-S.; Dimitriadis, G.; Foley, R.~J J.; Pan, Y.-C.; Coulter, D.~A A.; Fox, O.~D D.; Jha, S.~W W.; Jones, D.~O O.; Kasen, D.~N N.; Kilpatrick, C.~D D.; Piro, A.~L L.; Asas-Sn,; Holoien, T. W.-S.; Drout, M.~R R.; Auchettl, K.; Kochanek, C.~S S.; Brown, J.~S S.; Bose, S.; Bersier, D.; Brimacombe, J.; Chen, P.; Dong, S.; Holmbo, S.; Muñoz, J.~A A.; Mutel, R.~L L.; Post, R.~S S.; Prieto, J.~L L.; Chambers, K.~C C.; Flewelling, H.~A A.; Huber, M.~E E.; Magnier, E.~A A.; Bulger, J.; Konkoly/Texas,; Lowe, T.~B B.; Pál, A.; Bódi, A.; Bognár, Z.-S.; Csák, B.; Cseh, B.; Csörnyei, G.; Hanyecz, O.; Ignácz, B.; Kalup, C.-S.; Könyves-Tóth, R.; Kriskovics, L.; Ordasi, A.; Arizona, U.~o; Rajmon, I.; Holoien, Thomas W.-S.; Milne, P.; Andrews, J.~E E.; Bilinski, C.; Brown, P.~J J.; Nordin, J.; Galbany, L.; Palmerio, J.; Hook, I.~M M.; Inserra, Cosimo; Maguire, K.; Cartier, Régis; Gutiérrez, C.~P P.; North Carolina, U.~o; Hermes, J.~J J.; Kaiser, B.~C C.; Atlas,; Heinze, A.~N N.; Denneau, L.; K2, Mission Team; Barentsen, G.; Dotson, J.; Barclay, T.; Gully-Santiago, M.; Hedges, C.; Cody, A.~M M.; Howell, S.; Coughlin, J.; Larson, K.~A A.; Cardoso, J.~V.~d.~M Vinícius de Miranda; McCalmont-Everton, K.~M M.; Peterson, C.~A A.; Razza, Alessandro; Osborne, D.; McGinn, C.; Kohnert, L.; Migliorini, L.; Cleve, J. E.; Labonde, C.; Castillo, G.; Beerman, G.; Avendano, Claudia Patricia Gutierrez; Hanley, M.; Larsen, R.; Gangopadhyay, R.; Kloetzel, R.; Nystrom, V.; Moffatt, J.; Griest, K.; Packard, M.; Muszynski, M.; Kampmeier, J.; Bjella, R.; Flynn, S.; Elsaesser, B.; Et, A. L.

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Jozsef Vinko
ePESSTO et al., 2018

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@article{ePESSTO2018,
  author = {ePESSTO,  and Wang, X. and Vinkó, J. and Sand, D.~J J. and Zhang, J. and Zhang, T. and Wang, L. and Zhang, X. and Xiang, D. and Zhang, K. and Rui, L. and Zhao, X. and Sai, H. and Valenti, S. and Rest, A. and Tucker, B.~E E. and Shaya, E. and Ucsc,  and Zenteno, A. and Villar, A. and Riess, A.~G G. and Rojas-Bravo, C. and Shappee, Benjamin J. and Stanek, K.~Z Z. and Shields, J. and Tallon, D. and Thompson, T.~A A. and Starrs, Pan and Vallely, P.~J J. and Villanueva, Jr. S. and Smartt, S.~J J. and Smith, K.~W W. and Waters, C.~Z Z. and Schultz, A.~S.~B S. B. and Willman, M. and Sárneczky, K. and Wheeler, J.~C C. and Sódor, A. and Szabó, R. and Szakáts, R. and Zsidi, G. and Swift,  and Smith, N. and Williams, S.~C C. and Reding, J.~S S. and Tonry, J.~L L. and Vinícius de Miranda Cardoso, J. and Weiland, H. and Stalder, B. and Team, Kepler Spacecraft and Van Cleve, J.~E E. and Ross, S.~E E. and Reedy, L.~H H. and Wheaton, A. and Spencer, B. and Steward, K. and Weschler, T. and Redick, M. and Li, W. and Mo, J. and Hosseinzadeh, G. and Lin, H. and Ptss/Tnts,  and Chen, Z. and Huang, F. and Li, X. and Li, L. and Baron, E. and Derkacy, J.~M M. and Lco,  and Howell, D.~A A. and McCully, C. and Arcavi, I. and Kegs,  and Hiramatsu, D. and Burke, J. and Garnavich, P. and Narayan, G. and Margheim, S. and Holoien, T.~W-S. and Dimitriadis, G. and Foley, R.~J J. and Pan, Y.-C. and Coulter, D.~A A. and Fox, O.~D D. and Jha, S.~W W. and Jones, D.~O O. and Kasen, D.~N N. and Kilpatrick, C.~D D. and Piro, A.~L L. and Asas-Sn,  and Holoien, T. W.-S. and Drout, M.~R R. and Auchettl, K. and Kochanek, C.~S S. and Brown, J.~S S. and Bose, S. and Bersier, D. and Brimacombe, J. and Chen, P. and Dong, S. and Holmbo, S. and Muñoz, J.~A A. and Mutel, R.~L L. and Post, R.~S S. and Prieto, J.~L L. and Chambers, K.~C C. and Flewelling, H.~A A. and Huber, M.~E E. and Magnier, E.~A A. and Bulger, J. and Konkoly/Texas,  and Lowe, T.~B B. and Pál, A. and Bódi, A. and Bognár, Z.-S. and Csák, B. and Cseh, B. and Csörnyei, G. and Hanyecz, O. and Ignácz, B. and Kalup, C.-S. and Könyves-Tóth, R. and Kriskovics, L. and Ordasi, A. and Arizona, U.~o and Rajmon, I. and Holoien, Thomas W.-S. and Milne, P. and Andrews, J.~E E. and Bilinski, C. and Brown, P.~J J. and Nordin, J. and Galbany, L. and Palmerio, J. and Hook, I.~M M. and Inserra, Cosimo and Maguire, K. and Cartier, Régis and Gutiérrez, C.~P P. and North Carolina, U.~o and Hermes, J.~J J. and Kaiser, B.~C C. and Atlas,  and Heinze, A.~N N. and Denneau, L. and K2, Mission Team and Barentsen, G. and Dotson, J. and Barclay, T. and Gully-Santiago, M. and Hedges, C. and Cody, A.~M M. and Howell, S. and Coughlin, J. and Larson, K.~A A. and Cardoso, J.~V.~d.~M Vinícius de Miranda and McCalmont-Everton, K.~M M. and Peterson, C.~A A. and Razza, Alessandro and Osborne, D. and McGinn, C. and Kohnert, L. and Migliorini, L. and Cleve, J. E. and Labonde, C. and Castillo, G. and Beerman, G. and Avendano, Claudia Patricia Gutierrez and Hanley, M. and Larsen, R. and Gangopadhyay, R. and Kloetzel, R. and Nystrom, V. and Moffatt, J. and Griest, K. and Packard, M. and Muszynski, M. and Kampmeier, J. and Bjella, R. and Flynn, S. and Elsaesser, B. and Et, A. L.},
  month = {dec},
  title = {Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the $Kepler$ 2 Observations},
  year = {2018}
}

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