Erratum to “Are Nuclear Star Clusters the Precursors of Massive Black Holes?”

---

The original paper had an erroneous value for the Srsic index of NGC 205, which was quoted as 𝑛=4. We used the surface brightness profile of [1] to derive Srsic 𝑛=2.05. The correct version of Figure 2 is reproduced below. This does not influence any of the conclusions.

Figure 2 

The mass of the BH against the Srsic index of the host bulge or disk. We plot the objects as listed in the text. The largest outliers are NGC205 (with   𝑛=2.05), POX52 (𝑛=3.6), NGC404 (𝑛=2.5), and NGC1493 (𝑛=2.4).