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Spin Measurements of Black Holes Thomas Dauser

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Robust <strong>Spin</strong> Estimation<br />

stellar mass BH Cyg X-1: Broad Band Spectrum<br />

νFν [10 −6 × ergs s −1 cm −2 ]<br />

χ<br />

10 XMM-Newton RXTE-PCA RXTE-HEXTE<br />

5<br />

2<br />

1<br />

5<br />

3<br />

1<br />

-1<br />

-3<br />

-5<br />

5 10 20 50<br />

Energy [keV]<br />

100<br />

Integral<br />

200<br />

500<br />

Duro & <strong>Dauser</strong> et al. (2013, in<br />

prep.)<br />

Broad Band<br />

Coverage<br />

(Simultaneous<br />

observations) ( first<br />

robust stellar mass BH spin<br />

measurement)<br />

Cygnus X-1 is a fast<br />

rotating black hole<br />

(a > 0.9), and<br />

compact emission<br />

region (h < 4rg)<br />

<strong>Spin</strong> in agreement<br />

with the “disk-spin”<br />

method (Gou et al., 2011)

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