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Late-time Radio Brightening and Emergence of a Radio Jet in the Changing-look AGN 1ES 1927+654
Published 2025-01-01Get full text
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First Results from the JWST Early Release Science Program Q3D: The Fast Outflow in a Red Quasar at z = 0.44
Published 2025-01-01Get full text
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A Dual Active Black Hole Candidate with Mass Ratio ~7:1 in a Disk Galaxy
Published 2025-01-01“…We identify the central BH with mass of 9.4 × 10 ^6 M _⊙ from its radio emission as well as AGN-driven galactic-scale biconical outflows. The off-centered BH generates obvious broad and narrow emission-line regions, which gives us a robust estimation of a 1.3 × 10 ^6 M _⊙ BH mass. …”
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No Galaxy-scale [C ii] Fast Outflow in the z = 6.72 Red Quasar HSC J1205–0000
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Strongly Magnetized Accretion with Low Angular Momentum Produces a Weak Jet
Published 2025-01-01“…In the lower-angular-momentum states, our results predict that there should be dynamically strong magnetic fields on horizon scales, but no powerful jet; this state may be consistent with Sgr A* in the Galactic center.…”
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Revisiting the Flaring Activity in Early 2015 of BL Lacertae Object S5 0716+714
Published 2025-01-01Get full text
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Generalized Centered Binomial Distribution for Bimodal Lattice Signatures
Published 2025-01-01“…As a generalized form of the centered binomial distribution (CBD), GCBD is simple and efficient in sampling integers from distributions with large standard deviations. …”
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Measurements of Cosmic Rays by a Mini‐Neutron Monitor at Neumayer III From 2014 to 2017
Published 2024-06-01Get full text
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Spectrum and Location of Ongoing Extreme Particle Acceleration in Cassiopeia A
Published 2025-01-01Get full text
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Quantifying Baryonic Feedback on the Warm–Hot Circumgalactic Medium in CAMELS Simulations
Published 2025-01-01Get full text
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The Disk Wind Contribution to the Gamma-Ray Emission from the Nearby Seyfert Galaxy GRS 1734−292
Published 2025-01-01Get full text
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MSA-3D: Metallicity Gradients in Galaxies at z ∼ 1 with JWST/NIRSpec Slit-stepping Spectroscopy
Published 2025-01-01Get full text
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