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Ish: Testing the Kerr black hole hypothesis with the continuum-fitting and the iron line methods: the case of GRS 1915+105

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Black Hole Spin in X-Ray Binaries: Observational Consequences
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Testing the Kerr Black Hole Hypothesis with GRS 1716-249 by Combining the Continuum Fitting and the Iron-line Methods
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The effects of redshifts and focusing on the spectrum of an accretion disk around a Kerr black hole
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Testing the space-time geometry around black hole candidates with the analysis of the broad<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="bold">K</mml:mi><mml:mi>α</mml:mi></mml:math>iron line
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Stationary Black Holes: Uniqueness and Beyond
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The Spin of the Near‐Extreme Kerr Black Hole GRS 1915+105
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CONSTRAINTS ON THE SPACETIME GEOMETRY AROUND 10 STELLAR-MASS BLACK HOLE CANDIDATES FROM THE DISK'S THERMAL SPECTRUM
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XSPEC model for testing the Kerr black hole hypothesis using the continuum-fitting method
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Kerr Black Holes with Scalar Hair
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Impact of the reflection model on the estimate of the properties of accreting black holes
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<i>NuSTAR</i> SPECTROSCOPY OF GRS 1915+105: DISK REFLECTION, SPIN, AND CONNECTIONS TO JETS
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TESTING THE NO-HAIR THEOREM WITH OBSERVATIONS IN THE ELECTROMAGNETIC SPECTRUM. IV. RELATIVISTICALLY BROADENED IRON LINES
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TESTING THE KERR BLACK HOLE HYPOTHESIS
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Testing General Relativity with the Stellar-mass Black Hole in LMC X-1 Using the Continuum-fitting Method
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