output
20032025
most citedEEG machine learning with Higuchi fractal dimension and Sample Entropy as features for successful detection of depression

136 citations

29 papers

cond-mat.mes-hall2025★ 1 cited

Temperature anomaly of the V and V vacancy spin coherence time in 4H-SiC

P. Chrostoski, Ifeanyi I. Onwosi, D. H. Santamore

Increasing the spin coherence time (T2) is a major area of interest for spin defect systems such as the silicon (V) and carbon (V) vacancies in 4H-SiC. Usually as tem…

cs.CV2025

Cross Spatial Temporal Fusion Attention for Remote Sensing Object Detection via Image Feature Matching

Abu Sadat Mohammad Salehin Amit, Xiaoli Zhang, Md Masum Billa Shagar +3

Effectively describing features for cross-modal remote sensing image matching remains a challenging task due to the significant geometric and radiometric differences between multim…

cond-mat.mes-hall2022★ 16 cited

Surface roughness noise analysis and comprehensive noise effects on depth-dependent coherence time of NV centers in diamond

Philip Chrostoski, Pauli Kehayias, D. H. Santamore

Noise is a detrimental issue for nitrogen-vacancy (NV) centers in diamond, causing line broadening and decreasing the coherence time (T2). Following our previous electric and magne…

quant-ph2021★ 5 cited

Spin Squeezing Induced Enhancement of Sensitivity of an Atomic Clock using Coherent Population Trapping

Jinyang Li, Gregório R. M. da Silva, Schuyler Kain +3

The coherent population trapping (CPT) effect is used for making compact atomic clocks. There are two types of CPT clocks: the one in which the Raman beams are applied continuously…

cond-mat.mes-hall2021★ 16 cited

Magnetic field noise analyses generated by the interactions between a nitrogen vacancy center diamond and surface and bulk impurities

Philip Chrostoski, Bruce Barrios, D. H. Santamore

We investigated the mechanism of magnetic noise due to both surface and bulk impurities. For surface noise, we apply the Langevin method to spin fluctuation theory to calculate the…

astro-ph.CO2021

Core Mass Estimates in Strong Lensing Galaxy Clusters: a Comparison Between Masses Obtained from Detailed Lens Models, Single-Halo Lens Models, and Einstein Radii

J. D. Remolina González, K. Sharon, G. Mahler +7

The core mass of galaxy clusters is both an important anchor of the radial mass distribution profile and probe of structure formation. With thousands of strong lensing galaxy clust…