More Like this

1. SN 2017ens: The Metamorphosis of a Luminous Broadlined Type Ic Supernova into an SN IIn

   https://doi.org/10.3847/2041-8213/aaeb2e  

   Chen, T.-W. ; Inserra, C. ; Fraser, M. ; Moriya, T. J. ; Schady, P. ; Schweyer, T. ; Filippenko, A. V. ; Perley, D. A. ; Ruiter, A. J. ; Seitenzahl, I. ; et al ( November 2018 , The Astrophysical Journal)
2. The double-peaked Type Ic supernova 2019cad: another SN 2005bf-like object

   https://doi.org/10.1093/mnras/stab1009  

   Gutiérrez, C P ; Bersten, M C ; Orellana, M ; Pastorello, A ; Ertini, K ; Folatelli, G ; Pignata, G ; Anderson, J P ; Smartt, S ; Sullivan, M ; et al ( May 2021 , Monthly Notices of the Royal Astronomical Society)

   ABSTRACT We present the photometric and spectroscopic evolution of supernova (SN) 2019cad during the first ∼100 d from explosion. Based on the light-curve morphology, we find that SN 2019cad resembles the double-peaked Type Ib/c SN 2005bf and the Type Ic PTF11mnb. Unlike those two objects, SN 2019cad also shows the initial peak in the redder bands. Inspection of the g-band light curve indicates the initial peak is reached in ∼8 d, while the r-band peak occurred ∼15 d post-explosion. A second and more prominent peak is reached in all bands at ∼45 d past explosion, followed by a fast decline from ∼60 d. During the first 30 d, themore »spectra of SN 2019cad show the typical features of a Type Ic SN, however, after 40 d, a blue continuum with prominent lines of Si ii λ6355 and C ii λ6580 is observed again. Comparing the bolometric light curve to hydrodynamical models, we find that SN 2019cad is consistent with a pre-SN mass of 11 M⊙, and an explosion energy of 3.5 × 1051 erg. The light-curve morphology can be reproduced either by a double-peaked 56Ni distribution with an external component of 0.041 M⊙, and an internal component of 0.3 M⊙ or a double-peaked 56Ni distribution plus magnetar model (P ∼ 11 ms and B ∼ 26 × 1014 G). If SN 2019cad were to suffer from significant host reddening (which cannot be ruled out), the 56Ni model would require extreme values, while the magnetar model would still be feasible.« less
3. The Exotic Type Ic Broad-lined Supernova SN 2018gep: Blurring the Line between Supernovae and Fast Optical Transients

   https://doi.org/10.3847/1538-4357/ac00bc  

   Pritchard, T. A. ; Bensch, Katarzyna ; Modjaz, Maryam ; Williamson, Marc ; Thöne, Christina C. ; Vinkó, J. ; Bianco, Federica B. ; Bostroem, K. Azalee ; Burke, Jamison ; García-Benito, Rubén ; et al ( July 2021 , The Astrophysical Journal)
4. A GRB and Broad-lined Type Ic Supernova from a Single Central Engine

   https://doi.org/10.3847/1538-4357/aabf84  

   Barnes, Jennifer ; Duffell, Paul C. ; Liu, Yuqian ; Modjaz, Maryam ; Bianco, Federica B. ; Kasen, Daniel ; MacFadyen, Andrew I. ( June 2018 , The Astrophysical Journal)
5. A potential progenitor for the Type Ic supernova 2017ein

   https://doi.org/10.1093/mnras/sty2022  

   Kilpatrick, Charles D ; Takaro, Tyler ; Foley, Ryan J ; Leibler, Camille N ; Pan, Yen-Chen ; Campbell, Randall D ; Jacobson-Galan, Wynn V ; Lewis, Hilton A ; Lyke, James E ; Max, Claire E ; et al ( July 2018 , Monthly Notices of the Royal Astronomical Society)