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Article

Rho, J, Evans, A ORCID: https://orcid.org/0000-0002-3142-8953, Geballe, T, Banerjee, D, Hoeflich, P, Shahbandeh, M, Valenti, S, Yoon, S-C, Jin, H, Williamson, M, Modjaz, M, Hiramatsu, D, Howell, DA, Pellegrino, C, Vinko, J, Carter, R, Burke, J, McCully, C, An, H, Cha, H, Pritchard, T, Wang, X, Andrews, J, Galbany, L, Van Dyk, S, Graham, ML, Blinnikov, S, Joshi, V, Pal, A, Kriskovics, L, Ordash, A, Szakats, R, Vida, K, Chen, Z, Li, X, Zhang, J and Yan, S (2021) Near-Infrared and Optical Observations of Type Ic SN2020oi and broad-lined Ic SN2020bvc: Carbon Monoxide, Dust and High-Velocity Supernova Ejecta. Astrophysical Journal.

Kozyreva, A, Gilmer, M, Hirschi, R, Frohlich, C, Blinnikov, S, Wollaeger, R, Noebauer, U, van Rossum, D, Heger, A, Even, W, Waldman, R, Tolstov, A, Chatzopoulos, E and Sorokina, E (2017) Fast evolving pair-instability supernova models: evolution, explosion, light curves. Monthly Notices of the Royal Astronomical Society, 464 (3). pp. 2854-2865.

Kozyreva, A, Hirschi, R, Blinnikov, S and Hartogh, JD (2016) How much radioactive nickel does ASASSN-15lh require? Monthly Notices of the Royal Astronomical Society, 459 (1).

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