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Hunting for Cold Exoplanets via Microlensing
Published 2023-08-01“…Microlensing can detect planets at distances ranging from a few hundred parsecs all the way to the Galactic center. The maximum sensitivity is reached for systems that are located half way to the galactic center, with planets orbiting the lens star at a separation of few AUs. …”
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Time-resolved Hubble Space Telescope UV Observations of an X-Ray Quasiperiodic Eruption Source
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Evidence for AGN Feedback in Galaxy Clusters and Groups
Published 2012-01-01“…Instead of the initial idea that the thermal gas is cooling and flowing toward the center, the new picture envisages a complex dynamical evolution of the intracluster medium (ICM) regulated by the radiative cooling and the nongravitational heating from the active galactic nucleus (AGN). …”
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Observations of Radio Magnetars with the Deep Space Network
Published 2019-01-01“…When the DSN antennas are not communicating with spacecraft, they provide a valuable resource for performing observations of radio magnetars, searches for new pulsars at the Galactic Center, and additional pulsar-related studies. …”
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The Cosmic History of Black Hole Growth from Deep Multiwavelength Surveys
Published 2012-01-01Get full text
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Review of the Empirical Evidence for Superluminal Particles and the 3 + 3 Model of the Neutrino Masses
Published 2019-01-01“…Furthermore, this dark matter model is supported by several datasets: γ-rays from the galactic center, and the Kamiokande-II neutrino data on the day of SN 1987A. …”
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Your brain on art, nature, and meditation: a pilot neuroimaging study
Published 2025-01-01Get full text
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Mimetic Gravity: A Review of Recent Developments and Applications to Cosmology and Astrophysics
Published 2017-01-01Get full text
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Semianalytical Fokker–Planck Models for Nuclear Star Clusters
Published 2025-01-01“…This improves the rate estimates for extreme-mass ratio inspirals, and has interesting implications for a new class of galactic center transients called quasiperiodic eruptions.…”
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Little Red Dots: Rapidly Growing Black Holes Reddened by Extended Dusty Flows
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Extreme Scale Height Variations and Nozzle Shocks in Warped Disks
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Solar Modulation of Low-energy Cosmic-Ray Nitrogen and Its Comparison with Oxygen
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Recoiling Black Holes: Electromagnetic Signatures, Candidates, and Astrophysical Implications
Published 2012-01-01“…Supermassive black holes (SMBHs) may not always reside right at the centers of their host galaxies. This is a prediction of numerical relativity simulations, which imply that the newly formed single SMBH, after binary coalescence in a galaxy merger, can receive kick velocities up to several 1000 km/s due to anisotropic emission of gravitational waves. …”
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Data-driven Dynamics with Orbital Torus Imaging: A Flexible Model of the Vertical Phase Space of the Galaxy
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A Study of the Star Clusters’ Population in the Giant Molecular Cloud G174+2.5
Published 2025-01-01“…Then, for the detected clusters, we determine their general parameters: the center positions, radii, number of stars, and reddening. …”
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HCG 57: Evidence for Shock-heated Intergalactic Gas from X-Rays and Optical Emission Line Spectroscopy
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