353 citations · 2.6k across the 26 of their papers we have counts for
26 papers
Ultra-compact Binary Neural Networks for Human Activity Recognition on RISC-V Processors
Francesco Daghero, Chen Xie, Daniele Jahier Pagliari +6
Human Activity Recognition (HAR) is a relevant inference task in many mobile applications. State-of-the-art HAR at the edge is typically achieved with lightweight machine learning…
Privacy-preserving Social Distance Monitoring on Microcontrollers with Low-Resolution Infrared Sensors and CNNs
Chen Xie, Francesco Daghero, Yukai Chen +6
Low-resolution infrared (IR) array sensors offer a low-cost, low-power, and privacy-preserving alternative to optical cameras and smartphones/wearables for social distance monitori…
The Low-Redshift Lyman Continuum Survey II: New Insights into LyC Diagnostics
Sophia R. Flury, Anne E. Jaskot, Harry C. Ferguson +44
The Lyman continuum (LyC) cannot be observed at the epoch of reionization (z {\gtrsim} 6) due to intergalactic H I absorption. To identify Lyman continuum emitters (LCEs) and infer…
A combined VANDELS and LEGA-C study: the evolution of quiescent galaxy size, stellar mass and age from to
M. L. Hamadouche, A. C. Carnall, R. J. McLure +13
We study the relationships between stellar mass, size and age within the quiescent population, using two mass-complete spectroscopic samples with $\mathrm{log_{10}}(M_{\star}/\math…
Analogs of primeval galaxies two billion years after the Big Bang
Ricardo Amorín, A. Fontana, E. Pérez-Montero +30
Deep observations are revealing a growing number of young galaxies in the first billion year of cosmic time. Compared to typical galaxies at later times, they show more extreme emi…
Fundamental physics with the Hubble Frontier Fields: constraining Dark Matter models with the abundance of extremely faint and distant galaxies
Nicola Menci, Alexander Merle, Maximilian Totzauer +4
We show that the measured abundance of ultra-faint lensed galaxies at in the Hubble Frontier Fields (HFF) provides stringent constraints on the parameter space of i) D…