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- Maximal efficiency of geometric beaming and polarization of highly super-Eddington X-ray sources
- What can a uniform reflection pipeline establish about supermassive black hole spin? An audit and a corrected analysis of 57 AGN with XMM and NuSTAR
- Gamma-ray calorimetry of Seyfert winds
- How bright can a galaxy be? Extreme value predictions for high-redshift survey observables
- N-body simulations of the open cluster M67 -- I: global cluster properties
- The START mission: Probing the 2029 Apophis Flyby via a Low-Cost Geocentric SmallSat
- On the foundations of anthropic reasoning: Implications for life across the universe
- GASTRO−BH: Effects of a Central Black Hole in GSE-like Dwarf-galaxy Mergers Around Milky Way-like Hosts
- MIDSSAR: MId Dispersion Spectrograph for Stellar Activity Research
- Analytic and numerical study of dark matter halos in the Horndeski theory
- A Unified Solution to the Low-Mass X-ray Binary Diversity Puzzle: Saturated Magnetic Braking Coupled with Irradiation-Driven Winds
- Gaia in Technicolor. I. A Simple Variability-Encoded Color-Magnitude Diagram
- A Multiwavelength View of SPLUS J102139.31-282247.5: an X-ray Luminous and Eclipsing Dwarf Nova
- Laboratory Characterization of a Ge-CCD Prototype for Future Near-Infrared Astronomical Instrumentation
- Dust in Galaxies at z=10−15: Attenuation and Re-emission Predictions from the FirstLight Simulations
- Chemical Demographics of Star-forming Regions
- Dark Matter in the Galaxy: Insights from the Dynamics of Stellar Streams
- Missed Detections and False Alarms in a CNN Technosignature Detector on Breakthrough Listen Data
- Constrain the Size of Broad Line Region in NGC 1068 Using Sub-millimeter Excess
- The origin of the high heavy-element content of warm Jupiters
- Constraints from big bang nucleosynthesis and cosmological observations on varying Higgs vacuum expectation value
- Path-Degenerate Quantum Interferometry for Loss Resilience in Gravitational-Wave Detectors
- HURACAN: A comparison of stellar and interstellar proper motions inside L1688
- Bifrost spectral inversions: Fast non-LTE solar chromospheric diagnostics from 3D simulations
- An ALMA study of hub-filament systems II.Quiescent filaments converging towards highly dynamic hubs