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Multiepoch Spectropolarimetry of SN 2011fe

  • Authors: Peter A. Milne, G. Grant Williams, Amber Porter, Paul S. Smith, Nathan Smith, Mark D. Leising, Buell T. Jannuzi, and E. M. Green

2017 The Astrophysical Journal 835 100.

  • Provider: AAS Journals

Caption: Figure 6.

Upper panel: flux spectrum of Epoch 3 fit with SYNAPPS algorithm. The flux spectrum is shown with a black solid line, and the SYNAPPS fit is shown as a red dashed line. Fit parameters are listed in Table 2. Lower panels: polarization and ﹩\theta ﹩ spectra compared against individual ions from SYNAPPS fits for Epoch 3. The ion flux values are plotted to different scales, as shown on the right-hand axis. See text for explanation of A, B, C, and D labels.

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