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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 10.

The time evolution of the polarization of the Si IIλ6355 Å absorption feature. Whereas some SNe Ia studied in Wang et al. (2007) were found to reach the largest Si II polarization roughly 5 days before the optical maximum, SN 2011fe clearly reaches the largest polarization after the optical maximum, if assuming a parabolic fit to the data with a shape similar to Wang et al. (2007; dashed line). Error bars were generated by determining the standard deviation of PSi II estimations when q(ISP) and u(ISP) change according to the averages from Epochs 4–9, as shown in Figure 2. A continuum polarization level of ∼0.08% was not subtracted from PSi II.

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