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Figure 9: Illustrative example showing the calculation of the NCRPVF index for SN2002A in UGC 3804. The larger points/thicker curved line shows the ranked pixel values plotted against number in the ranked pixel sequence; the smaller points/thinner line shows the cumulative counts for each pixel, vertically scaled to fit. The pixel containing the location of SN2002A has a value of 4.5 counts, corresponding to an NCRPVF index of 0.401 as shown. |
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Figure 10:
Histograms of the positions of the SN-containing pixels
within the cumulative H![]() |
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Figure 11:
Histogram of the positions of the SN-containing pixels within
the cumulative H![]() |
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Figure 12:
a) Histograms of fractional H![]() |
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Figure 13:
Histogram of a) fractional H![]() |
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Figure 6:
a) Histograms of the locations of galaxies in the
ranked cumulative H![]() |
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Figure 7:
Histogram of the locations of the galaxies hosting the 12 type Ia supernovae in a) the ranked cumulative H![]() |
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Figure 8:
a) Histograms of the locations of galaxies in the
ranked cumulative H![]() |
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Figure 1:
Positions of type II supernovae (circles) overlaid on negative images
showing the distribution of H![]() ![]() |
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Figure 2:
Positions of type II supernovae (circles) overlaid on negative images
showing the distribution of H![]() ![]() |
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Figure 3:
Positions of type Ib and Ic supernovae (circles) overlaid on negative images
showing the distribution of H![]() ![]() |
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Figure 4:
Positions of type Ia supernovae (circles) overlaid on negative images
showing the distribution of H![]() ![]() |
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Figure 5:
Positions of unclassified supernovae (circles) overlaid on negative images
showing the distribution of H![]() ![]() |
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