Figure 2 from A Spectropolarimetric View on the Nature of the Peculiar Type I SN 2005hk

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A Spectropolarimetric View on the Nature of the Peculiar Type I SN 2005hk

Authors: Justyn R. Maund, J. Craig Wheeler, Lifan Wang, Dietrich Baade, Alejandro Clocchiatti, Ferdinando Patat, Peter Höflich, Jason Quinn, and Paula Zelaya

MAUND et al. 2010 The Astrophysical Journal 722 1162.

Provider: AAS Journals

Caption: Figure 2.

Flux spectra of SN 2005hk at 2005 November 9 and 2005 November 23, or approximately at B light curve maximum and 14 days after maximum. Line identifications are based on those provided by Chornock et al. (2006), Phillips et al. (2007), and Branch et al. (2004) and fits to the spectra using the SYNOW code. The wavelength scale has been corrected for the recessional velocity of the host galaxy.

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