arXiv:2509.05442v1 Announce Type: new Abstract: We present a follow-up study focused on cluster-scale diffuse radio emissions in 115 galaxy clusters in the Southern sky, using full-resolution (7.8") ...
arXiv:2509.05416v1 Announce Type: new Abstract: Strong gravitational lensing is a powerful cosmological probe, providing a direct tool to unveil the properties of dark matter (DM) on sub-galactic sca...
arXiv:2509.05499v1 Announce Type: new Abstract: We present measurements, analyses and results for the seventeen strongly carbon-chain depleted comets in Lowell Observatory's narrowband photometry dat...
arXiv:2509.05514v1 Announce Type: new Abstract: JWST has provided critical mid-infrared data for cold brown dwarfs. It has also provided low-resolution near-infrared spectra, and for faint sources th...
arXiv:2509.05457v1 Announce Type: new Abstract: The rotation periods of Ap stars range over five to six orders of magnitude. The origin of their differentiation remains unknown. We carry out a system...
arXiv:2509.05459v1 Announce Type: new Abstract: The JWST has enabled the discovery of Active Galactic Nuclei at high redshifts. The intrinsic UV spectrum of GN-z11 at redshift z = 10.6 has a spectral...
arXiv:2509.05434v1 Announce Type: new Abstract: New populations of red active galactic nuclei (known as ``Little Red Dots'') discovered by JWST exhibit remarkable spectral energy distributions. Lever...
arXiv:2509.05403v1 Announce Type: new Abstract: The Hydrogen-alpha (Ha) emission line in galaxies is a powerful tracer of their recent star formation activity. With the advent of JWST, we are now abl...
arXiv:2509.05419v1 Announce Type: new Abstract: Analytical templates for the covariance matrix of the 4-Point Correlation Function (4PCF) have been developed in the past assuming a Gaussian Random Fi...
arXiv:2509.05427v1 Announce Type: new Abstract: Accretion onto neutron stars (NSs) in X-ray pulsars (XRPs) results in intense X-ray emission, and under specific conditions, high-energy nuclear intera...