The study of supernovae (SNe) and their environments in host galaxies at the highest possible angular resolution in a number of wavelength regimes is providing vital clues to the nature of their progenitor stars. We are observing SNe in the radio using the Very Large Array (VLA) and VLBI, in the X-rays with Chandra , and in the optical at the subarcsecond resolution of HST .
Schuyler D. Van Dyk, Chien Y. Peng, Aaron J. Barth, Alexei V Filippenko, Roger A. Chevalier, Robert A. Fesen, Claes Fransson, R. Kirshner, B. Leibundgut
R. J. Foley, P. J. Challis, R. Chornock, M. Ganeshalingam, Wenyu Li, G. H. Marion, N. Morrell, G. Pignata, M. Stritzinger, J. M. Silverman, Xiaofeng Wang, J. P. Anderson, Alexei V Filippenko, Wendy L. Freedman, M. Hamuy, Saurabh W. Jha, R. Kirshner, C. McCully, S. E. Persson, M. M. Phillips, D. Reichart, A. M. Soderberg
R. J. Foley, P. J. Challis, R. Chornock, M. Ganeshalingam, Weifei Li, G. H. Marion, N. I. Morrell, G. Pignata, M. Stritzinger, Jacob Silverman, Xiaofeng Wang, J. P. Anderson, Alexei V Filippenko, Wendy L. Freedman, M. Hamuy, S. W. Jha, R. P. Kirshner, C. McCully, S. E. Persson, M. M. Phillips, D. Reichart, Anne‐Marie Søderberg
Tamás Szalai, Ori D. Fox, Richard G. Arendt, E. Dwek, Jennifer E. Andrews, Geoffrey C. Clayton, Alexei V Filippenko, J. Johansson, Patrick L. Kelly, Kelsie Krafton, A. P. Marston, Jon C. Mauerhan, Schuyler D. Van Dyk
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