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MMA Underground - The fight starts here.
Feb 4, 2025 · The fight starts here. Looking back at Francis Ngannou’s triumphant MMA return at PFL: Battle of the Giants
arxiv.org arXiv
arxiv.org › abs › 1709.05415v1
Mode-locking in advection-reaction-diffusion systems: an invariant manifold perspective
Fronts propagating in two-dimensional advection-reaction-diffusion (ARD) systems exhibit rich topological structure. When the underlying fluid flow is periodic in space and time, the reaction front ca...
arxiv.org arXiv
arxiv.org › abs › astro-ph › 0703640v1
Infrared Brightness Temperature of Mars, 1983-2103
The predicted infrared brightness temperature of Mars using the 1976 model of Wright is tabulated here for the period 1983 to 2103. This model was developed for far-infrared calibration, and is still ...
arxiv.org arXiv
arxiv.org › abs › 2112.02745v1
Potential Habitability as a Stellar Property: Effects of Model Uncertainties and Measurement Precision
Knowledge of a star's evolutionary history combined with estimates of planet occurrence rates allows one to infer its relative quality as a location in the search for biosignatures, and to quantify th...
arxiv.org arXiv
arxiv.org › abs › 2602.24229v1
Science Fiction and Fantasy in Wikipedia: Exploring Structural and Semantic Cues
Identifying which Wikipedia articles are related to science fiction, fantasy, or their hybrids is challenging because genre boundaries are porous and frequently overlap. Wikipedia nonetheless offers m...
arxiv.org arXiv
arxiv.org › abs › 1410.4680v2
Spectroscopy and laser cooling on the $^{1}S_{0}-\,^{3}P_{1}$ line in Yb via an injection-locked diode laser at 1111.6nm
We generate 555.8nm light with sub-MHz linewidth through the use of laser injection-locking of a semiconductor diode at 1111.6nm, followed by frequency doubling in a resonant cavity. The integrity of ...
arxiv.org arXiv
arxiv.org › abs › 1508.06444v1
HELP : The Herschel Extragalactic Legacy Project & The Coming of Age of Multi-Wavelength Astrophysics
How did galaxies form and evolve? This is one of the most challenging questions in astronomy today. Answering it requires a careful combination of observational and theoretical work to reliably determ...
arxiv.org arXiv
arxiv.org › abs › 1904.12498v1
HELP project - a dreamed-of multiwavelength dataset for SED fitting: the influence of used models for the main physical properties of galaxies
The Herschel Extragalactic Legacy Project (HELP) focuses to publish an astronomical multiwavelength catalogue of millions of objects over 1300~deg$^2$ of the Herschel Space Observatory survey fields. ...
arxiv.org arXiv
arxiv.org › abs › 1708.01291v1
Spin-Orbit Misalignments of Three Jovian Planets via Doppler Tomography
We present measurements of the spin-orbit misalignments of the hot Jupiters HAT-P-41 b and WASP-79 b, and the aligned warm Jupiter Kepler-448 b. We obtained these measurements with Doppler tomography,...
arxiv.org arXiv
arxiv.org › abs › 2509.09290v1
Modality-Agnostic Input Channels Enable Segmentation of Brain lesions in Multimodal MRI with Sequences Unavailable During Training
Segmentation models are important tools for the detection and analysis of lesions in brain MRI. Depending on the type of brain pathology that is imaged, MRI scanners can acquire multiple, different im...
arxiv.org arXiv
arxiv.org › abs › 1101.3480v3
Universal Quadratic Forms and Untwisting Whitney Towers
The first part of this paper completes the classification of Whitney towers in the 4-ball that was started in three related papers. We provide an algebraic framework allowing the computations of the g...