arXiv:2509.04573v1 Announce Type: new Abstract: As Radial velocity (RV) spectrographs reach unprecedented precision and stability below 1 m/s, the challenge of granulation in the context of exoplanet...
arXiv:2509.04572v1 Announce Type: new Abstract: For synchrotron radiation from relativistic electrons having a power-law energy distribution with a power-law index $p$ in an optically thin medium wit...
arXiv:2509.04570v1 Announce Type: new Abstract: Local galaxies follow scaling relations between mass and stellar population properties such as age and metallicity, which encode key information on the...
arXiv:2509.04551v1 Announce Type: new Abstract: The Einstein Probe is revolutionizing time-domain astrophysics through the discovery of new classes of X-ray transients associated with Type Ic-Broad L...
arXiv:2509.04531v1 Announce Type: new Abstract: OrbDot is a Python package for studying the secular (long-term) evolution of exoplanet orbits from observational data. It employs nested sampling algor...
arXiv:2509.04564v1 Announce Type: new Abstract: Neptunes and sub-Neptunes are typically modeled under the assumption that the interior is adiabatic and consists of distinct layers. However, formation...
arXiv:2509.04553v1 Announce Type: new Abstract: The origin of obscuration in Active Galactic Nuclei (AGN) is still a matter of contention. It is unclear whether obscured AGN are primarily due to line...
arXiv:2509.04552v1 Announce Type: new Abstract: In order to derive unbiased cosmological parameters from Stage-IV surveys, we need models that can predict the matter power spectrum for at least $k\,\...
arXiv:2509.04560v1 Announce Type: new Abstract: Episodic mass accretion is the dominant mechanism for mass assembly in the proto-stellar phase. Although prior optical time-domain searches have allowe...
arXiv:2509.04563v1 Announce Type: new Abstract: We report Giant Metrewave Radio Telescope (GMRT) \hii\ imaging of NGC\,4141, the host galaxy of FRB\,20250316A at $z=0.0063$. Our GMRT \hii\ images hav...