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Unveiling dust, molecular gas, and high star-formation efficiency in extremely UV bright star-forming galaxies at z ∼ 2.1–3.6 |
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The multiple classes of ultra-diffuse galaxies: can we tell them apart?<SUP></SUP> |
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High-resolution observational analysis of flare ribbon fine structures |
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Evolution of the Accretion Disk and Corona during the Outburst of the Neutron Star Transient MAXI J1807+132 |
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A GTC spectroscopic study of three spider pulsar companions: line-based temperatures, a new face-on redback, and improved mass constraints |
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A possible misaligned orbit for the young planet AU Mic c |
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CHEX-MATE: Dynamical masses for a sample of 101 Planck Sunyaev-Zeldovich-selected galaxy clusters |
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Spider-Webb: JWST Near Infrared Camera resolved galaxy star formation and nuclear activities in the Spiderweb protocluster at z = 2.16 |
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Properties of Cosmic Deuterons Measured by the Alpha Magnetic Spectrometer |
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Kicking Time Back in Black Hole Mergers: Ancestral Masses, Spins, Birth Recoils, and Hierarchical-formation Viability of GW190521 |
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Large-scale stellar age-velocity spiral pattern in NGC 4030 |
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A Tale of Three: Magnetic Fields along the Orion Integral-shaped Filament as Revealed by the JCMT BISTRO Survey |
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CARMENES input catalogue of M dwarfs: VIII. Kinematics in the solar neighbourhood |
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Unveiling the ice and gas nature of active centaur (2060) Chiron using the James Webb Space Telescope |
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Characterisation of TOI-406 as a showcase of the THIRSTEE program: A two-planet system straddling the M-dwarf density gap |
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Chemo-dynamics of the stellar component of the Sculptor dwarf galaxy: I. Observed properties |
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Expanding the Ultracompacts: Gravitational-wave-driven Mass Transfer in the Shortest-period Binaries with Accretion Disks |
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Hints of a close outer companion to the ultra-hot Jupiter TOI-2109 b |
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Broadband multi-wavelength properties of M87 during the 2018 EHT campaign including a very high energy flaring episode |
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Constraints on compact objects from the Dark Energy Survey 5-yr supernova sample |
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Why do some ultra diffuse Galaxies have rich globular cluster systems? |
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Calibrating the Clock of JWST |
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Crimson Behemoth: A massive clumpy structure hosting a dusty AGN at z=4.91 |
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The CHEOPS view of the climate of WASP-3 b |
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