Showing 1–20 of 30 results
/ Date/ Name
Apr 29, 2013Systematic Study of Event Horizons and Pathologies of Parametrically Deformed Kerr SpacetimesJan 12, 2015Photon Rings around Kerr and Kerr-like Black HolesJan 12, 2015X-ray Probes of Black Hole Accretion Disks for Testing the No-Hair TheoremOct 5, 2010Testing the No-Hair Theorem with Observations in the Electromagnetic Spectrum. III. Quasi-Periodic VariabilityMay 11, 2010Testing the No-Hair Theorem with Observations in the Electromagnetic Spectrum: II. Black-Hole ImagesAug 23, 2010Testing the No-Hair Theorem with Observations of Black Holes in the Electromagnetic SpectrumNov 17, 2010A Ray-Tracing Algorithm for Spinning Compact Object Spacetimes with Arbitrary Quadrupole Moments. I. Quasi-Kerr Black HolesOct 19, 2011A Ray-Tracing Algorithm for Spinning Compact Object Spacetimes with Arbitrary Quadrupole Moments. II. Neutron StarsSep 13, 2012Testing General Relativity in the Strong-Field Regime with Observations of Black Holes in the Electromagnetic SpectrumMar 13, 2008Constraints on the Size of Extra Dimensions from the Orbital Evolution of Black-Hole X-Ray BinariesFeb 24, 2016Testing the No-Hair Theorem with Observations of Black Holes in the Electromagnetic SpectrumDec 7, 2010Sgr A*: The Optimal Testbed of Strong-Field GravityMay 16, 2011A Metric for Rapidly Spinning Black Holes Suitable for Strong-Field Tests of the No-Hair TheoremOct 1, 2012A Metric for Testing the Nature of Black HolesAug 11, 2016Testing General Relativity with Accretion-Flow Imaging of Sgr A*Feb 27, 2012Testing the No-Hair Theorem with Observations in the Electromagnetic Spectrum. IV. Relativistically Broadened Iron LinesJan 3, 2012Masses of Nearby Supermassive Black Holes with Very-Long Baseline InterferometryDec 1, 2009Testing the No-Hair Theorem with Observations of Astrophysical Black Holes in the Electromagnetic SpectrumMar 17, 2010Testing the No-Hair Theorem with Observations in the Electromagnetic Spectrum: I. Properties of a Quasi-Kerr SpacetimeJan 12, 2015Regular Black Hole Metric with Three Constants of Motion