Title: Discovery of Two Supernovae in the Nuclear Regions of the Luminous Infrared Galaxy IC 883 Authors: E. Kankare, S. Mattila, S. Ryder, P. Vaisanen, A. Alberdi, A. Alonso-Herrero, L. Colina, A. Efstathiou, J. Kotilainen, J. Melinder, M.-A. Perez-Torres, C. Romero-Canizales, A. Takalo
We report the discovery of two consecutive supernovae (SNe), 2010cu and 2011hi, located at 0.37" (180 pc) and 0.79" (380 pc) projected distance respectively from the centre of the K-band nucleus of the luminous infrared galaxy IC 883. The SNe were discovered in an ongoing near-infrared K-band search for core-collapse SNe in such galaxies using the ALTAIR/NIRI adaptive optics system with laser guide star at the Gemini-North Telescope. These are thus the closest SNe yet discovered to a LIRG nucleus in optical or near-infrared wavelengths. The near-infrared light curves and colours of both SNe are consistent with core-collapse events. Both SNe seem to suffer from relatively low host galaxy extinction suggesting that regardless of their low projected galactocentric distances, they are not deeply buried in the nuclear regions of the host galaxy.
A possible magnitude 16.9 supernova was discovered by E. Kankare, S. Ryder, S. Mattila (Gemini-North Telescope) on the 11th February, 2011, in the galaxy Arp 193 (IC 883) in the constellation Canes Venatici. The supernova is located 0.65" east and 0.45" south from the center of the galaxy. As yet the type is unknown.
Position(2000): RA = 13 20 35.38, Dec = +34°08'22.23" z = 0.023299