Results 51 to 60 of about 603 (179)
Abstract Background Force plates (FP) are considered the gold standard for quantitative equine gait evaluation but are limited to experimental use. An instrumented hoof boot (IHB) with pressure sensors and an inertial measurement unit would allow clinicians to objectively assess kinetic parameters and gait symmetry.
Jasmin Keller +3 more
wiley +1 more source
Origin of low surface brightness galaxies: a dynamical study [PDF]
Low Surface Brighness Galaxies (LSBs), inspite of being gas rich, have low star formation rates and are, therefore, low surface brightness in nature. We calculate Q$_{\rm{RW}}$, the 2-component disc stability parameter as proposed by Romeo \& Wiegert (2011), as a function of galactocentric radius $R$ for a sample of five LSBs, for which mass models,
Garg, Prerak, Banerjee, Arunima
openaire +2 more sources
Story2Board: A Training‐Free Approach for Expressive Visual Storytelling
Abstract We present Story2Board, a training‐free framework for expressive storyboard generation from natural language. Existing methods narrowly focus on subject identity, overlooking key aspects of visual storytelling such as spatial composition, background evolution, and narrative pacing.
D. Dinkevich +4 more
wiley +1 more source
H i Observations of Giant Low Surface Brightness Galaxies
Giant low surface brightness (gLSB) galaxies are galaxies with extremely extended, faint, optical disks over 50 kpc in radius and have high total masses, which can reach 10 ^12 M _⊙ .
Philip Lah +7 more
doaj +1 more source
MIGHTEE H I observations of low surface brightness and ultra-diffuse galaxies in the XMM-LSS field
Untargeted neutral hydrogen (H I) surveys are well suited to identifying low surface brightness galaxies (LSBGs) that are gas rich, and they offer a complementary view to optically selected populations.
Adams Elizabeth A. K. +10 more
doaj +1 more source
Star formation thresholds in Low Surface Brightness galaxies [PDF]
Low Surface Brightness (LSB) galaxies appear to have low star formation rates despite their often quite normal H I contents as judged from global H I properties such as M(H I)/L and M(H I)/M(T) ratios. H I imaging with the Very Large Array of the National Radio Astronomy Observatory (the NRAO is operated by Associated Universities Inc.
VAN DER HULST, J. M. +5 more
openaire +2 more sources
FaceIt: Real‐Time On‐Device Identity‐Preserving Portrait Animation
A real‐time, on‐device algorithm for animating a single portrait image using detailed facial expressions and motions from a driving video achieving visual quality that can outperform even techniques with significantly higher computational overhead. Abstract Recently, significant progress has been made in generating expressive and temporally coherent ...
M. Dvorožňák +7 more
wiley +1 more source
A Sample of Nearby Isolated Dwarf Galaxies: A First Look at the Mass Function of Field Dwarfs
We present the results of the Exploration of Local VolumE Survey-Field, a survey of the dwarf galaxies in the Local Volume (LV; D
Scott G. Carlsten +4 more
doaj +1 more source
The Properties of an Edge-On Low Surface Brightness Galaxies Sample
We analyzed the properties of a sample of edge-on low-surface brightness galaxies, which are referred to as Cao23 ELSBGs. Cao23 ELSBGs exhibit a wide range of luminosities (−22 < Mr < −13) with a mean scale length of 3.19 ± 1.48 kpc.
Tian-Wen Cao +7 more
doaj +1 more source
Low and high surface brightness galaxies at void walls [PDF]
Abstract We study the relative fraction of low and high surface brightness galaxies (LSBGs and HSBGs) at void walls in the Sloan Digital Sky Survey (SDSS) Data Release 7. We focus on galaxies in equal local density environments. We assume that the host dark matter halo mass (for which we use SDSS group masses) is a good indicator of ...
Ceccarelli, Maria Laura +4 more
openaire +8 more sources

