Is a 1D perturbative method sufficient for asteroseismic modelling of $\beta$ Cephei pulsators? Implications for measurements of rotation and internal magnetic fields arXiv:2511.09617
Think inside the box: cosmic variance and large-scale conformity of high-redshift massive galaxies in the FLAMINGO simulations arXiv:2511.09618
Changing-Look AGN Powered By Disk Tearing arXiv:2511.09626
A Submillimeter Survey of CS Excitation in Protoplanetary Disks: Evidence of X-ray-Driven Sulfur Chemistry arXiv:2511.09628
Dark Photons in the Radio Sky: I. Resonant Conversions in Halos arXiv:2511.09630
Prebiotic Chemistry Insights for Dragonfly: Thermodynamics of Amino Acid Synthesis in Selk Crater on Titan arXiv:2511.09636
Dark Photons in the Radio Sky: II. Resonant Conversions in the Intergalactic Medium arXiv:2511.09637
The SEEDZ Simulations: Methodology and First Results on Massive Black Hole Seeding and Early Galaxy Growth arXiv:2511.09640
Chandra and HST Observations of Radio-Selected (Wandering) Massive Black Hole Candidates in Dwarf Galaxies arXiv:2511.09641
statmorph-lsst: Quantifying and correcting morphological biases in galaxy surveys arXiv:2511.09644
Fractional Dynamics in Galactic Nuclei: Non-Local Transport, Transient Phenomena and the Nullification of the Schwarzschild Barrier arXiv:2511.09648
The origin of scatter in the X-ray luminosity - halo mass relation of galaxy clusters arXiv:2511.09649
Analysis of the TAIGA-HiSCORE Data Using the Latent Space of Autoencoders arXiv:2511.09655
Measuring the Dark Matter Self-Interaction Cross-Section with Deep Compact Clustering for Robust Machine Learning Inference arXiv:2511.09660
glitterin: Towards Replacing the Role of Lorenz-Mie Theory in Astronomy Using Neural Networks Trained on Light Scattering of Irregularly Shaped Grains arXiv:2511.09668
Planetary architectures under the influence of a stellar binary arXiv:2511.09676
Analyzing Exoplanet Transits Observed with the WFC3/UVIS G280 Grism arXiv:2511.09694
Towards a Machine Learning Solution for Hubble Tension: Physics-Informed Neural Network (PINN) Analysis of Tsallis Holographic Dark Energy in Presence of Neutrinos arXiv:2511.09706
Simulated Real-Time Testing of the Prototype Implementation of the SOFIE Model: The 2025 Space Weather Prediction Testbed Exercise arXiv:2511.09716
Type Ia supernova feedback effects on globular clusters of different masses arXiv:2511.09719
PEPSI Investigation, Retrieval, and Atlas of Numerous Giant Atmospheres (PIRANGA). IV. High-Resolution Phased-Resolved Spectroscopy of The Ultra Hot Jupiter KELT-20 b arXiv:2511.09720
Towards model-free stellar chemical abundances. Potential applications in the search for chemically peculiar stars in large spectroscopic surveys arXiv:2511.09733
Seasonal and Diurnal Variability of Atmospheric Pressure in Jezero Crater, Mars, from MEDA Measurements on the Perseverance Rover arXiv:2511.09743
Searching for Long-Period Radio Transients in ASKAP EMU Data with 10-Second Imaging arXiv:2511.09770
Simulating the Diffuse Neutrino Emission from the Milky Way with GALPROP arXiv:2511.09777
Modeling the Contact Surfaces Formed by Pebble Collisions: Application to Formation of Comet 67P/Churyumov--Gerasimenko arXiv:2511.09835
A precessing magnetic jet as the engine of GRB 250702B arXiv:2511.09850
GalaxyClusters from the DESILegacy ImagingSurveys. III.Star-forming Fraction of Brightest Cluster Galaxies arXiv:2511.09858
Mock Observations for the CSST Mission: CPI-C -- Targets for High Contrast Imaging arXiv:2511.09862
Topmetal-L: A Low Noise Charge-Sensitive Pixel Sensor for POLAR2/LPD arXiv:2511.09863
fiDrizzle-MU: A Fast Iterative Drizzle with Multiplicative Updates arXiv:2511.09881
findAbar: how astronomers may perceive the bar in galaxies differently arXiv:2511.09908
JWST View of the Supernebula in NGC 5253. I. Overview and Continuum Features arXiv:2511.09910
View of the Supernebula in NGC 5253. II. Nebular Lines arXiv:2511.09911
Slow neutrinos: non-linearity and momentum-space emulation arXiv:2511.09945
New ASKAP radio-continuum surveys of the Small Magellanic Cloud arXiv:2511.09954
Where Galaxies Point: First Measurement of the Large-Scale Axial Intrinsic Alignment arXiv:2511.10005
Composite Dissipation in Warm Inflation: Implications for the Primordial Power Spectrum arXiv:2511.10024
Impact of selection criteria on the structural parameters of the Galactic thin and thick discs arXiv:2511.10092
Fast Rotating Blue Straggler Stars in the globular cluster NGC 1851 arXiv:2511.10109
Synchrotron radiation from NGC 470 HLX1 - a hidden hyperluminous accreting neutron star? arXiv:2511.10183
Analysis of the magnetic fields in massive young stellar objects with masers arXiv:2511.10186
Estimating accretion times of halo substructures in the Milky Way arXiv:2511.10195
Probing AGN Disks Density Profiles through Gravitational Wave Observations arXiv:2511.10204
Systematic Analysis of Changing-look AGN Variability Using ZTF Light Curves arXiv:2511.10217
Fundamentals of interior modelling and challenges in the interpretation of observed rocky exoplanets arXiv:2511.10269
True spin-orbit obliquities distribution: data-driven confirmation of no clustering of misaligned planets arXiv:2511.10313
A Dynamical Scalar Field Model for Dark Energy: Addressing the Hubble Tension and Cosmic Evolution arXiv:2511.10317
Curious Case of CGRaBS J0211+1051: Observational Evidence of Lepto-Hadronic Origin of High-Energy Emission? arXiv:2511.10329
Alfven Waves in Partially Ionised Solar Steady-State Plasmas arXiv:2511.10330
Using the Cherenkov Telescope onboard EUSO-SPB2 for Target of Opportunity searches of very high energy neutrino sources arXiv:2511.10332
A predictive framework for realistic star planet radio emission in compact systems arXiv:2511.10350
Ginnungagap -- a massively parallel cosmological initial conditions generator arXiv:2511.10353
Extending the Frontier of Spatially-Resolved Supermassive Black Hole Mass Measurements to at $1\lesssim z\lesssim2$: Simulations with ELT/MICADO High-Resolution Mass Models and HARMONI Integral-Field Stellar Kinematics arXiv:2511.10427
How much can we learn from resolved stellar kinematics of galactic haloes using action-based dynamical models? arXiv:2511.10445
A scalable and accurate framework for self-calibrating null depth retrieval using neural posterior estimation arXiv:2511.10455
Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\lesssim$100 parsec in nearby star-forming galaxies from PHANGS arXiv:2511.10464
Disk warping and black hole X-ray binaries I. Tentative unification of low-frequency quasi-periodic oscillations arXiv:2511.10474
Collisional and magnetic effects on the polarization of the solar oxygen infrared triplet arXiv:2511.10476
Revealing the Connection Between the Filamentary Hierarchy and Star Cluster Formation in a Simulated NGC 628 Galaxy arXiv:2511.10486
Les Trente Glorieuses: 29 years of helioseismic observations with the Luminosity Oscillations Imager arXiv:2511.10491
Bayesian model comparison and validation with Gaussian Process Regression for interferometric 21-cm signal recovery arXiv:2511.10499
Shapiro Delay Measurements from Fifteen Years of PSR J1231$-$1411 Radio Observations arXiv:2511.10529
VELOCE III. Reconstructing Radial Velocity Curves of Classical Cepheids arXiv:2511.10534
Constraining the nature of the most extreme Galactic particle accelerator. H.E.S.S. observations of the microquasar V4641 Sgr arXiv:2511.10537
Carbox: an end-to-end differentiable astrochemical simulation framework arXiv:2511.10558
UHECRs Propagation and their Multimessengers: Upper limits and the Impact of the Extragalactic Magnetic Field arXiv:2511.10581
Co-evolution of baryons and dark matter halos of LYRA dwarf galaxies arXiv:2511.10582
The relationship between warm and hot gas-phase metallicity in massive elliptical galaxies and the influence of AGN feedback arXiv:2511.10587
The Local Group L-band Survey: Probing Cold Atomic Gas in IC10 with Neutral Hydrogen Absorption arXiv:2511.10602
A new multiprobe analysis of modified gravity and evolving dark energy arXiv:2511.10616
Dark Matter from Holography arXiv:2511.10617
The Atacama Cosmology Telescope. CMB Lensing from Daytime Data: A First Demonstration arXiv:2511.10620
A Bayesian Perspective on Evidence for Evolving Dark Energy arXiv:2511.10631
Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum arXiv:2511.10634
Flexible Simulation Based Inference for Galaxy Photometric Fitting with Synthesizer arXiv:2511.10640
Analytical approximations for curved primordial tensor spectra arXiv:2511.10644
Revisiting the maximum mass limit of strange stars in quadratic curvature-matter coupled gravity arXiv:2508.10524
The Non-thermal Energy Window for Laser-Driven Nuclear Reactions arXiv:2511.06657
Evading the BBN bound with a soft stiff period arXiv:2511.08384
Cosmological Limits on Strong Dark Forces arXiv:2511.09614
$L_\mu-L_\tau$ gauge bosons in beam dumps and supernovae arXiv:2511.09619
Ultralight Dark Matter from the Edge of Field Space arXiv:2511.09622
Freezing-in the Axiverse arXiv:2511.09631
Dark matter by design: $Q$-balls, neural networks and galaxy rotation curves arXiv:2511.09634
Photon counting readout for detection and inference of gravitational waves from neutron star merger remnants arXiv:2511.09656
Finite Populations & Finite Time: The Non-Gaussianity of a Gravitational Wave Background arXiv:2511.09659
Searching for screened scalar forces with long-baseline atom interferometers arXiv:2511.09750
Mitigating numerical dissipation in simulations of subsonic turbulent flows arXiv:2511.09806
CORONA-Fields: Leveraging Foundation Models for Classification of Solar Wind Phenomena arXiv:2511.09843
Rediscovering the Lunar Equation of the Centre with AI Feynman via Embedded Physical Biases arXiv:2511.09979
Trapped and Unstable: Axion-like particle fragmentation at finite temperature arXiv:2511.10086
Confronting dark energy in Harada's Conformal Killing Gravity with observational data arXiv:2511.10263
Electron Heat Flux and Whistler Instability in the Earth's Magnetosheath arXiv:2511.10275
Probing thermal leptogenesis and dark matter through primordial gravitational waves from a supercooled universe arXiv:2511.10288
Bubble Friction in Symmetry-Restoring Transitions arXiv:2511.10415
Generating optimal Gravitational-Wave template banks with metric-preserving autoencoders arXiv:2511.10466
A Fast Earth-scattering Formalism for Light Dark Matter with Dark Photon Mediators arXiv:2511.10589
Dark Matter and Baryon Asymmetry from Monopole-Axion Interactions arXiv:2511.10603
Challenging the AGN scenario for JWST/NIRSpec LRD and non-LRD broad H$\alpha$ emitters in light of non-detection of NIRCam photometric variability and X-ray arXiv:2407.04777
Extracting the Temperature Analytically In Hydrodynamics Simulations with Gas and Radiation Pressure arXiv:2501.18695
Evidence for a hot galactic halo around the Andromeda Galaxy using fast radio bursts along two sightlines arXiv:2503.02947
MOA-2010-BLG-328: Keck and HST Expose the Limits of Occams Razor in Microlensing arXiv:2504.06347
Perturbation Theory in the Minimally Extended Varying Speed of Light (meVSL) Model arXiv:2504.07975
The Host Galaxies of Fast Radio Bursts Track a Combination of Stellar Mass and Star Formation, Similar to Type Ia Supernovae arXiv:2504.08038
Spectroscopic r-Process Abundance Retrieval for Kilonovae III: Linking Spectral and Light Curve Modeling of the GW170817 Kilonova arXiv:2504.10696
Fast and accurate parameter estimation of high-redshift sources with the Einstein Telescope arXiv:2504.21087
The systemic recoil velocity distribution and the scale height of field millisecond pulsar systems: Implications on neutron star retention fractions in star clusters arXiv:2505.11357
Population demographics of white dwarf binaries with intermediate separations: Gaia constraints on post-AGB mass transfer arXiv:2505.14786
ASASSN-24fw: Candidate circumplanetary disk occultation of a main-sequence star arXiv:2507.05367
Neural-Network Chemical Emulator for First-Star Formation: Robust Iterative Predictions over a Wide Density Range arXiv:2508.16114
Studying the black widow pulsars PSR J0312$-$0921 and PSR J1627$+$3219 in the optical and X-rays arXiv:2509.01488
Relativistic Dissipative Magnetohydrodynamics for accretion disks arXiv:2509.02935
Can "premature collapse" form black holes in the upper and lower mass gaps? arXiv:2509.04574
Beyond No Tension: JWST z > 10 Galaxies Push Simulations to the Limit arXiv:2509.07695
The Physics of Cometary Anti-tails as Observed in 3I/ATLAS arXiv:2509.07771
Witnessing downsizing in the making: quiescent and breathing galaxies at the dawn of the Universe arXiv:2509.09764
Enhancing the development of Cherenkov Telescope Array control software with Large Language Models arXiv:2510.01299
Magnetic Field-Line Curvature and Its Role in Particle Acceleration by Magnetically Dominated Turbulence arXiv:2510.20628
Direct multi-model dark-matter search with gravitational-wave interferometers using data from the first part of the fourth LIGO-Virgo-KAGRA observing run arXiv:2510.27022
The effect of mass and morphology on the mass assembly of galaxies arXiv:2511.02715
Exploring the spectral characteristics of the periodic burster 4U 1323-62: Type-I X-ray burst and persistent emission arXiv:2511.03172
The Dark Energy Survey Supernova Program: A Reanalysis Of Cosmology Results And Evidence For Evolving Dark Energy With An Updated Type Ia Supernova Calibration arXiv:2511.07517
J-PLUS Reconstructing the Milky Way Disc's star formation history with twelve-filter photometry arXiv:2511.07596
Mock Observations for the CSST Mission: CPI-C -- Instrument Simulation arXiv:2511.08886
Mock Observations for the CSST Mission: HSTDM--Synthetic Data Generation arXiv:2511.09074
Adsorption of volatiles on dust grains in protoplanetary disks arXiv:2511.09481
From M100 to NGC 7331: A Multiband Study and Physical Parameters in Nearby Galaxies arXiv:2511.09482
Tests of General Relativity with GWTC-3 arXiv:2112.06861
Numerical gravitational backreaction on cosmic string loops from simulation arXiv:2411.10366
Detectability of Massive Boson Stars using Gravitational Waves from Fundamental Oscillations arXiv:2502.04068
Finite-temperature bubble nucleation with shifting scale hierarchies arXiv:2503.13597
Loops in inflation with strongly non-geodesic motion arXiv:2503.18516
Broadband Optical Modulation and Control at Millikelvin Temperatures arXiv:2504.06995
Linking the KM3-230213A Neutrino Event to Dark Matter Decay and Gravitational Wave signals arXiv:2504.16040
How gravitational waves change photon orbital angular momentum quantum states arXiv:2504.16452
$g$-mode oscillations of dark matter admixed neutron stars arXiv:2506.18892
Alexei Starobinsky and Modern Cosmology arXiv:2509.01675
Is the $\Lambda$CDM Model in Crisis? arXiv:2509.17124
Extracting Properties of Dark Dense Environments around Black Holes from Gravitational Waves arXiv:2510.27424