<h3><strong>KraftShade 2: Mastering Shaders with KraftShade — Your Canvas on the GPU</strong></h3><p>Following our <a href="https://tech.pic-collage.com/kraftshade-1-unleashing-gpu-power-on-android-a-...
<p>To use the latest features of logging for Red Hat OpenShift 6.0, you must migrate from Elasticsearch to Loki. This article is a guide for users to test these changes in their development and test e...
arXiv:2508.21131v1 Announce Type: new Abstract: Recent pulsar timing array (PTA) analyses show evidence for a gravitational wave background (GWB) with angular correlations consistent with the Helling...
arXiv:2508.21126v1 Announce Type: new Abstract: We present the COLIBRE galaxy formation model and the COLIBRE suite of cosmological hydrodynamical simulations. COLIBRE includes new models for radiati...
arXiv:2508.21157v1 Announce Type: new Abstract: We investigate the impacts of the evolution of dust mass and grain size distribution within a Milky Way-like (MW-like) galaxy simulation on global atte...
arXiv:2508.21245v1 Announce Type: new Abstract: Recent advances in CMOS technology have potential to significantly increase the performance, at low-cost, of an astronomical space telescope. Arrays of...
arXiv:2508.21152v1 Announce Type: new Abstract: Star formation in galaxies is regulated by the interplay of a range of processes that shape the multiphase gas in the interstellar and circumgalactic m...
arXiv:2508.21282v1 Announce Type: new Abstract: Active galactic nuclei (AGN) jets are powerful drivers of galaxy evolution, depositing energy and momentum into the circumgalactic and intracluster med...
The degeneracy between microlensing wave effect and precession in strongly lensed gravitational wave
arXiv:2508.21262v1 Announce Type: new Abstract: Microlensing induced by the stellar field within a strong lensing galaxy can introduce fluctuations in the waveforms of strongly-lensed gravitational w...
arXiv:2508.21203v1 Announce Type: new Abstract: In this study, we present novel calculations of X-ray polarization from radio-quiet and unobscured active galactic nuclei (AGNs) using the Monte Carlo ...