Swift UVOT Observations of Core‐Collapse SNe

We review recent UV observations of core‐collapse supernovae (SNe) with the Swift Ultra‐violet/Optical Telescope (UVOT) during its first two years. Rest‐frame UV photometry is useful for differentiating SN types by exploiting the UV‐optical spectral shape and more subtle UV features. This is useful for the real‐time classification of local and high‐redshift SNe using only photometry. Two remarkable SNe Ib/c were observed with UVOT — SN2006jc was a UV bright SN Ib. Swift observations of GRB060218/SN2006aj began shortly after the explosion and show a UV‐bright peak followed by a UV‐faint SN bump. UV observations are also useful for constraining the temperature and ionization structure of SNe IIR Rest‐frame UV observations of all types are important for understanding the extinction, temperature, and bolometric luminosity of SNe and to interpret the observations of high redshift SNe observed at optical wavelengths.