Results 91 to 100 of about 7,785,767 (337)
Rasch data evaluating an astronomy course [PDF]
<p>Binary data on 12 items for Rasch analysis for the evaluation of an astronomy course.</p ...
Evi Panou +2 more
core +1 more source
Bayesian Pulsar Timing and Noise Analysis with Vela.jl: An Overview
We present Vela.jl , an efficient, modular, easy-to-use Bayesian pulsar timing and noise analysis package written in Julia. Vela.jl provides an independent, efficient, and parallelized implementation of the full nonlinear pulsar timing and noise model ...
Abhimanyu Susobhanan
doaj +1 more source
A flexible and highly reliable piezoelectric pressure sensor based on GaN p–n homojunction microrod arrays on graphene is demonstrated. The sensor exhibits high sensitivity, rapid response, excellent cyclic durability, and stable performance after thermal aging and PBS immersion, highlighting its potential for harsh‐environment and biomedical pressure ...
Asad Ali +5 more
wiley +1 more source
PINT: Maximum-likelihood Estimation of Pulsar Timing Noise Parameters
PINT is a pure-Python framework for high-precision pulsar timing developed on top of widely used and well-tested Python libraries, supporting both interactive and programmatic data analysis workflows. We present a new frequentist framework within PINT to
Abhimanyu Susobhanan +23 more
doaj +1 more source
Reversible light‐induced gradients at solid–liquid interfaces enable controllable interfacial transport via light‐driven diffusioosmosis. We demonstrate directed particle manipulation based on dynamically generated concentration gradients. The mechanism is broadly applicable to cationic, anionic, and non‐ionic surfactants with varying hydrophobicity ...
Maren Umlandt +3 more
wiley +1 more source
Middle School Students’ Misconceptions about the Concepts of Astronomy [PDF]
The purpose of the current study is to conduct developmental comparison of the middle school students’ misconceptions about the concepts of astronomy. The sampling of the study is comprised of middle school students attending a private school located in ...
Gorecek Baybars, Meryem, Can, Sendil
core
A Simple but Powerful Method to Reduce Background Noise in Celestial Gamma-Ray Images
Reducing background noise is essential for clear data analysis and signal detection. In this study, we introduce a novel denoising algorithm tailored for gamma-ray astronomical data, utilizing local density sampling techniques.
H. Hedayati Kh., M. Soor, F. Akhondi
doaj +1 more source
Milled polycrystalline NMC811 cathode (MPC NMC) with smaller secondary particle and higher surface area had 1) greater cathode tortuosity, 2) reduced surface Ni on the cycled MPC cathodes consistent with surface reconstruction, and 3) increased Ni deposition from cathode‐anode crosstalk, manifesting in lower functional capacity and higher impedance ...
Edelmy J. Marin Bernardez +22 more
wiley +1 more source
Benchmarking Dimensionality Reduction Methods for High-dimensional ALMA Image Cubes
High-dimensional astronomical data cubes provide a wealth of spectral and structural information that can be used to study astrophysical and chemical processes.
Haley N. Scolati +3 more
doaj +1 more source
The opto‐electronic response of polycrystalline (PEA)2PbBr4 thin films is investigated by correlating macroscopic photodetector performance with nanoscale mapping techniques. Grain boundary density is systematically tuned through crystallization control and linked to device responsivity.
Camilla Bordoni +10 more
wiley +1 more source

