@article {230,
	title = {{Diversity in extinction laws of Type Ia supernovae measured between 0.2 and 2 {$μ$}m}},
	journal = {MNRAS},
	volume = {453},
	year = {2015},
	pages = {3300-3328},
	keywords = {circumstellar matter, dust, extinction, supernovae: general, supernovae: individual: 2012cu, supernovae: individual: SNe 2012cg},
	doi = {10.1093/mnras/stv1505},
	url = {http://adsabs.harvard.edu/abs/2015MNRAS.453.3300A},
	author = {Amanullah, R. and Johansson, J. and Goobar, A. and Ferretti, R. and Papadogiannakis, S. and Petrushevska, T. and Brown, P.~J. and Cao, Y. and Contreras, C. and Dahle, H. and Elias-Rosa, N. and Fynbo, J.~P.~U. and Gorosabel, J. and Guaita, L. and Hangard, L. and Howell, D.~A. and Hsiao, E.~Y. and Kankare, E. and Kasliwal, M. and Leloudas, G. and Lundqvist, P. and Mattila, S. and Nugent, P. and Phillips, M.~M. and Sandberg, A. and Stanishev, V. and Sullivan, M. and Taddia, F. and {\"O}stlin, G. and Asadi, S. and Herrero-Illana, R. and Jensen, J.~J. and Karhunen, K. and Lazarevic, S. and Varenius, E. and Santos, P. and Sridhar, S.~S. and Wallstr{\"o}m, S.~H.~J. and Wiegert, J.}
}
@article {2012ApJ...756..111M,
	title = {{Core-collapse Supernovae Missed by Optical Surveys}},
	journal = {The Astrophysical Journal},
	volume = {756},
	year = {2012},
	month = {sep},
	pages = {111},
	abstract = {We estimate the fraction of core-collapse supernovae (CCSNe) that remain undetected by optical SN searches due to obscuration by large amounts of dust in their host galaxies. This effect is especially important in luminous and ultraluminous infrared galaxies, which are locally rare but dominate the star formation at redshifts of z \~{} 1-2. We perform a detailed investigation of the SN activity in the nearby luminous infrared galaxy Arp 299 and estimate that up to 83\% of the SNe in Arp 299 and in similar galaxies in the local universe are missed by observations at optical wavelengths. For rest-frame optical surveys we find the fraction of SNe missed due to high dust extinction to increase from the average local value of \~{}19\% to \~{}38\% at z \~{} 1.2 and then remain roughly constant up to z \~{} 2. It is therefore crucial to take into account the effects of obscuration by dust when determining SN rates at high redshift and when predicting the number of CCSNe detectable by future high-z surveys such as LSST, JWST, and Euclid. For a sample of nearby CCSNe (distances 6-15 Mpc) detected during the last 12 yr, we find a lower limit for the local CCSN rate of 1.5$^{+0.4}$ $_{- 0.3}$ {\times} 10$^{-4}$ yr$^{-1}$ Mpc$^{-3}$, consistent with that expected from the star formation rate. Even closer, at distances less than \~{}6 Mpc, we find a significant increase in the CCSN rate, indicating a local overdensity of star formation caused by a small number of galaxies that have each hosted multiple SNe.},
	keywords = {galaxies: individual: Arp 299, galaxies: starburst, infrared: galaxies, supernovae: general, supernovae: individual: SN 2005at SN 2010P},
	doi = {10.1088/0004-637X/756/2/111},
	url = {http://adsabs.harvard.edu/abs/2012ApJ...756..111M},
	author = {Mattila, S. and Dahlen, T. and Efstathiou, A. and Kankare, E. and Melinder, J. and Alonso-Herrero, A. and M. A. P{\'e}rez-Torres and Ryder, S. and V{\"a}is{\"a}nen, P. and {\"O}stlin, G.}
}
