activity
20082016
most citedTesting the No-Hair Theorem with Observations in the Electromagnetic Spectrum: II. Black-Hole Images

412 citations · 3.1k across the 30 of their papers we have counts for

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Showing 2010Show all

6 papers · 1 filter

astro-ph.HE2010★ 35 cited

Sgr A*: The Optimal Testbed of Strong-Field Gravity

Dimitrios Psaltis, Tim Johannsen

The black hole in the center of the Milky Way has been observed and modeled intensely during the last decades. It is also the prime target of a number of new experiments that aim t…

astro-ph.HE2010★ 119 cited

A Ray-Tracing Algorithm for Spinning Compact Object Spacetimes with Arbitrary Quadrupole Moments. I. Quasi-Kerr Black Holes

Dimitrios Psaltis, Tim Johannsen

We describe a new numerical algorithm for ray tracing in the external spacetimes of spinning compact objects characterized by arbitrary quadrupole moments. Such spacetimes describe…

astro-ph.HE2010★ 130 cited

Testing the No-Hair Theorem with Observations in the Electromagnetic Spectrum. III. Quasi-Periodic Variability

Tim Johannsen, Dimitrios Psaltis

According to the no-hair theorem, astrophysical black holes are uniquely described by their masses and spins. An observational test of the no-hair theorem can be performed by measu…

astro-ph.HE2010★ 45 cited

Testing the No-Hair Theorem with Observations of Black Holes in the Electromagnetic Spectrum

Tim Johannsen, Dimitrios Psaltis

According to the no-hair theorem, astrophysical black holes are uniquely described by their mass and spin. In this paper, we review a new framework for testing the no-hair hypothes…

astro-ph.HE2010★ 412 cited

Testing the No-Hair Theorem with Observations in the Electromagnetic Spectrum: II. Black-Hole Images

Tim Johannsen, Dimitrios Psaltis

According to the no-hair theorem, all astrophysical black holes are fully described by their masses and spins. This theorem can be tested observationally by measuring (at least) th…

astro-ph.HE2010★ 128 cited

Testing the No-Hair Theorem with Observations in the Electromagnetic Spectrum: I. Properties of a Quasi-Kerr Spacetime

Tim Johannsen, Dimitrios Psaltis

According to the no-hair theorem, an astrophysical black hole is uniquely described by only two quantities, the mass and the spin. In this series of papers, we investigate a framew…