Abstract
We study a sample of 11 Type II supernovae (SNe) discovered by the OGLE-IV survey. All objects have well-sampled I-band light curves, and at least one spectrum. We find that two or three of the 11 SNe have a declining light curve, and spectra consistent with other SNe II-L, while the rest have plateaus that can be as short as 70 d, unlike the 100 d typically found in nearby galaxies. The OGLE SNe are also brighter, and show that magnitude-limited surveys find SNe that are different than usually found in nearby galaxies.We discuss this sample in the context of understanding Type II SNe as a class and their suggested use as standard candles.
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Poznanski, D., Kostrzewa-Rutkowska, Z., Wyrzykowski, L., & Blagorodnova, N. (2015). Bright but slow - Type II supernovae from OGLE-IV - Implications for magnitude-limited surveys. Monthly Notices of the Royal Astronomical Society, 449(2), 1753–1759. https://doi.org/10.1093/mnras/stv428
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