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Ish: On the Parameters of the Spherically Symmetric Parameterized Rezzolla–Zhidenko Spacetime through Solar System Tests, the Orbit of the S2 Star about Sgr A*, and Quasiperiodic Oscillations

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Constraints on Barrow Entropy from M87* and S2 Star Observations
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A test of general relativity using radio links with the Cassini spacecraft
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Discovery of a pulsar in a binary system
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Constraining wormhole geometries using the orbit of S2 star and the Event Horizon Telescope
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Radiation from relativistic particles in nongeodesic motion in a strong gravitational field
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High Proper‐Motion Stars in the Vicinity of Sagittarius A*: Evidence for a Supermassive Black Hole at the Center of Our Galaxy
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The accelerations of stars orbiting the Milky Way's central black hole
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Sgr A*: A Laboratory to Measure the Central Black Hole and Stellar Cluster Parameters
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Detection of the Schwarzschild precession in the orbit of the star S2 near the Galactic centre massive black hole
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Twin Peaks kHz QPOs: Mathematics of the 3:2 Orbital Resonance
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Geodesic motion of S2 and G2 as a test of the fermionic dark matter nature of our Galactic core
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S62 and S4711: Indications of a Population of Faint Fast-moving Stars inside the S2 Orbit—S4711 on a 7.6 yr Orbit around Sgr A*
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Constraints on self-dual black hole in loop quantum gravity with S0-2 star in the galactic center
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The Confrontation between General Relativity and Experiment
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Measurement of the Solar Gravitational Deflection of Radio Waves using Geodetic Very-Long-Baseline Interferometry Data, 1979–1999
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Gravitational anomalies in the solar system?
Lorenzo Iorio
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Post-Kerr black hole spectroscopy
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Calculation of the Uncertainties in the Planetary Precessions with the Recent EPM2017 Ephemerides and their Use in Fundamental Physics and Beyond
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Geodesic motion of S2 and G2 as a test of the fermionic dark matter nature of our Galactic core
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Sarlavhasiz
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Model for Gravity at Large Distances
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The Position of Sagittarius A*. III. Motion of the Stellar Cusp
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An abrupt drop in the coherence of the lower kHz quasi-periodic oscillations in 4U 1636−536
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