<p>If you’ve just started learning Laravel, you’ve probably heard about <strong>Artisan commands</strong>.<br> But what exactly are they? And why should you use them?</p> <p>In this guide, we’ll walk...
arXiv:2509.07064v1 Announce Type: new Abstract: The James Webb Space Telescope (\textit{JWST}) opened a new observational window on the primordial Universe. Here we present new JWST NIRSpec integral ...
arXiv:2509.07065v1 Announce Type: new Abstract: Recent imaging of supermassive black holes by the Event Horizon Telescope (EHT) has relied on exhaustive parameter-space searches, matching observation...
arXiv:2509.07078v1 Announce Type: new Abstract: The stellar haloes and intra-cluster light around galaxies are crucial test beds for dark matter (DM) physics and galaxy formation models. We consider ...
arXiv:2509.07090v1 Announce Type: new Abstract: With pulsar timing arrays (PTAs) having observed a gravitational wave background (GWB) at nanohertz frequencies, the focus of the field is shifting tow...
arXiv:2509.07066v1 Announce Type: new Abstract: The satellite population of the Milky Way is shaped by a range of astrophysical processes including mergers, star formation, feedback, and cosmic reion...
arXiv:2509.07088v1 Announce Type: new Abstract: The Alfv\'en surface -- where the solar wind exceeds the local Alfv\'en speed as it expands into interplanetary space -- is now routinely probed by NAS...
arXiv:2509.07080v1 Announce Type: new Abstract: Supernovae that interact with hydrogen-poor, helium-rich circumstellar material (CSM), known as Type Ibn supernovae (SNe Ibn), present a unique opportu...
arXiv:2509.07091v1 Announce Type: new Abstract: We present a comprehensive spectroscopic and kinematic analysis of the very metal-poor ([Fe/H] = -2.60 $\pm$ 0.20 dex) giant star HE2159-0551. By inves...
arXiv:2509.07081v1 Announce Type: new Abstract: Following a binary neutron star (BNS) merger, the transient remnant is often a fast-spinning, differentially rotating, magnetised hypermassive neutron ...