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Energy wrinkles and phase-space folds of the last major merger |
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Hace 2 weeks 3 days |
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HD 191939 revisited: New and refined planet mass determinations, and a new planet in the habitable zone |
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The Pristine survey - XIX. Cu and Zn abundances in metal-poor giants |
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The Robotic Multiobject Focal Plane System of the Dark Energy Spectroscopic Instrument (DESI) |
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Constraining the baryonic feedback with cosmic shear using the DES Year-3 small-scale measurements |
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Lessons learned from the two largest Galaxy morphological classification catalogues built by convolutional neural networks |
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Self-supervised clustering on image-subtracted data with deep-embedded self-organizing map |
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On the Presence of Metallofullerenes in Fullerene-rich Circumstellar Envelopes |
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Multiwavelength periodicity search in a sample of γ-ray bright blazars |
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Signs of environmental effects on star-forming galaxies in the Spiderweb protocluster at z = 2.16 |
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Towards the Identification and Classification of Solar Granulation Structures Using Semantic Segmentation |
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The JCMT BISTRO-2 Survey: Magnetic Fields of the Massive DR21 Filament |
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HD 20329b: An ultra-short-period planet around a solar-type star found by TESS |
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Optical design of an image-slicer integral field unit with two output slits |
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On the origin and evolution of the asteroid Ryugu: A comprehensive geochemical perspective |
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Pebbles and sand on asteroid (162173) Ryugu: In situ observation and particles returned to Earth |
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Fast Multipole Method for Gravitational Lensing: Application to High-magnification Quasar Microlensing |
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The JCMT BISTRO Survey: A Spiral Magnetic Field in a Hub-filament Structure, Monoceros R2 |
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Ultraviolet spectropolarimetry: investigating stellar magnetic field diagnostics |
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Unveiling the past evolution of the progenitor of the Helmi streams |
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CHEOPS finds KELT-1b darker than expected in visible light. Discrepancy between the CHEOPS and TESS eclipse depths |
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The messy death of a multiple star system and the resulting planetary nebula as observed by JWST |
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The Principle of Maximum Entropy and the Distribution of Mass in Galaxies |
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joshspeagle/dynesty: v1.2.3 |
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The uncertain interstellar medium of high-redshift quiescent galaxies: Impact of methodology |
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