Simulation-based inference of galaxy properties from JWST pixels
The spectral energy distributions (SEDs) of galaxies offer detailed insights into their stellar populations, capturing key physical properties such as stellar...
Simulation-based inference of galaxy properties from JWST pixels
The spectral energy distributions (SEDs) of galaxies offer detailed insights into their stellar populations, capturing key physical properties such as stellar...
Simulations and laboratory performance results of the weighted Fourier phase slope centroiding algorithm in a Shack-Hartmann sensor
The performance of the "weighted Fourier phase slope" centroiding algorithm at the subpupil image of a Shack-Hartmann wavefront sensor for point-like...
The intergalactic magnetic field within filaments should be less polluted by magnetized outflows from active galaxies than magnetic fields in clusters...
Simulations of Magnetoacoustic Pulsations in Atmospheres of Rapidly Oscillating Ap Stars
Rapidly oscillating Ap (roAp) stars exhibit an astrophysically interesting combination of strong, dipolar-like magnetic fields and high-overtone p-mode...
Simulations of the Biermann battery mechanism in two-fluid partially ionised plasmas
Context. In the absence of an initial seed, the Biermann battery term of a non-ideal induction equation acts as a source that generates weak magnetic fields...
Simulations Predicting the Ability of Multi-color Simultaneous Photometry to Distinguish TESS Candidate Exoplanets from False Positives
The Transiting Exoplanet Survey Satellite (TESS) is currently concluding its 2 yr primary science mission searching 85% of the sky for transiting exoplanets...
Simultaneous longitudinal and transverse oscillations in filament threads after a failed eruption
Context. Longitudinal and transverse oscillations are frequently observed in the solar prominences and/or filaments. These oscillations are excited by a large...