The Real-Time Data Processor Framework for Data Handling and Analysis of High-Energy Instruments arXiv:2511.03760
Dynamical Friction Constraints on the Dark Matter Hypothesis Across Astronomical Scales arXiv:2511.03776
Igniting galaxy formation in the post-reionization universe arXiv:2511.03785
Probing the dawn of galaxies: star formation and feedback in the JWST era through the GAEA model arXiv:2511.03787
Hot accretion onto spiral galaxies: the origin of extended and warped HI discs arXiv:2511.03793
Dark Matter in White Dwarfs: Implications for Their Structure arXiv:2511.03801
Making the most of pure parallels: Machine learning augmented photometric redshifts for sparse JWST filter sets arXiv:2511.03802
Effects of density stratification on Rossby waves in deep atmospheres arXiv:2511.03832
Photon Orbit Signatures in Spectra of Black Hole Accretion Disks arXiv:2511.03834
Do Planets Affect the Behavior of the Long-term Solar Activity? arXiv:2511.03889
Stellar Evolution with Radiative Feedback in AGN Disks arXiv:2511.03904
Energy-dependent SEP Fe/O abundances during the May 2024 superstorm arXiv:2511.03905
Event Reconstruction for Radio-Based In-Ice Neutrino Detectors with Neural Posterior Estimation arXiv:2511.03910
Revealing Hidden Cosmic Flows through the Zone of Avoidance with Deep Learning arXiv:2511.03919
Spectral Diversity in Type Ibn Supernovae and the Large Host Offset of SN2024acyl arXiv:2511.03926
Origin and Evolution of the $\Omega$ Structure in the Head-Tail Radio Galaxy of Abell 3322 arXiv:2511.03937
Non ideal Transport Processes in the Solar Atmosphere arXiv:2511.03949
SOFIA FEEDBACK Survey: The Eagle Nebula in [C II] and Molecular Lines arXiv:2511.03978
Cosmic voids and the kinetic analysis. V. Hubble tension, the cosmological constant and aperiodic filaments arXiv:2511.03990
Ultra-Diffuse, Ultra-Different: Observed vs. Simulated Ultra-Diffuse Galaxies Live in Fundamentally Different Halos arXiv:2511.04006
Low redshift observational constraints on dark energy models using ANN - CosmicANNEstimator arXiv:2511.04033
Super amplification of lunar response to gravitational waves driven by thick crust arXiv:2511.04067
Early evidence for isotropic planetary obliquities in young super-Jupiter systems arXiv:2511.04091
Exploring Cosmological Constraints of the Void-Lensing Cross-Correlation in the CSST Photometric Survey arXiv:2511.04099
Machine-Learning Estimation of Energy Fractions in MHD Turbulence Modes arXiv:2511.04119
Neural Network identification of Dark Star Candidates. I. Photometry arXiv:2511.04121
Neural Network identification of Dark Star Candidates. II. Spectroscopy arXiv:2511.04122
Limiting Eccentricity in Restricted Hierarchical Three-Body Systems with Short-Range Forces arXiv:2511.04146
TESS and ground-based observations of WZ Sge-type dwarf novae in outburst arXiv:2511.04175
Hadronic Processes in Advection-Dominated Accretion Flow as the Origin of TeV Excesses in BL Lac Objects arXiv:2511.04202
NANOGrav 15-year gravitational-wave signals from binary supermassive black-holes seeded by primordial black holes arXiv:2511.04210
Partial Null Point Reconnection of an Eruptive Filament arXiv:2511.04231
3D Non-LTE radiation transfer: theory and applications to stars, exoplanets, and kilonovae arXiv:2511.04254
Revealing an Oscillating and Contracting Compact Corona near the Event Horizon of the Supermassive Black Hole in 1ES 1927+654 arXiv:2511.04264
Cepheid Metallicity in the Leavitt Law (C- MetaLL) survey: IX: Spectroscopic detection of rare earth Dysprosium, Erbium, Lutetium and Thorium in Classical Cepheids arXiv:2511.04269
Constraining gravity with the decay rate of cosmological gravitational potential arXiv:2511.04279
The Initial mass function of field stars with mass $\leq$ 1 $M_{\odot}$ varies with metallicity arXiv:2511.04280
Discovery of a 9.67-s pulsar in an ultraluminous X-ray source in NGC 4631 with XMM-Newton arXiv:2511.04282
Massive stars exploding in a He-rich circumstellar medium XII. SN 2024acyl: A fast, linearly declining Type Ibn supernova with early flash-ionisation features arXiv:2511.04337
An alternative theory of magnetic flux tubes in strong fields via axion origin photons arXiv:2511.04346
The Apache Point Observatory extra-Galactic Evolution Experiment (APOeGEE): Chemical Abundance Trends for Seven Dwarf Spheroidal Galaxies in the APOGEE Survey arXiv:2511.04365
Magnetohydrodynamic simulation assessment of a potential near-ultraviolet early ingress in WASP-189b arXiv:2511.04372
Spectroscopic analysis of hydrogen and silicon in bright fireballs: New insights into meteoroid composition arXiv:2511.04373
Transiting Exoplanets from Sharjah Astronomical Observatory (SAO-M47): The Exoplanet HAT-P-25b Using L and V Filters arXiv:2511.04396
Artificial Precision Polarization Array: Sensitivity for the axion-like dark matter with clock satellites arXiv:2511.04400
How the gradient of $M_{\rm d}$ versus UV field strength yields insights into the ages of protoplanetary disc populations arXiv:2511.04410
Dust Collisions in Protoplanetary Disks: Atomic Simulations of the Surface Free Energy arXiv:2511.04423
Cutana: A High-Performance Tool for Astronomical Image Cutout Generation at Petabyte Scale arXiv:2511.04429
The TeV emission of 3C273: inverse Compton radiation from shear-accelerated high-energy electrons in the large-scale jet? arXiv:2511.04433
The AGORA High-resolution Galaxy Simulations Comparison Project. X: Formation and Evolution of Galaxies at the High-redshift Frontier arXiv:2511.04435
Study the nature of dynamical dark energy by measuring the CMB polarization rotation angle arXiv:2511.04459
The ALMA-ATOMS-QUARKS survey: Resolving a chemically rich massive protostellar outflow arXiv:2511.04504
Environmental effects in stellar mass gravitational wave sources II: Joint detections of eccentricity and phase shifts in binary sub-populations arXiv:2511.04540
2D unified atmosphere and wind simulations for a grid of O-type stars arXiv:2511.04542
Parameterizing Noise Covariance in Maximum-Likelihood Component Separation arXiv:2511.04546
Automatic detection of CMEs using synthetically-trained Mask R-CNN arXiv:2511.04589
The Pre-Outburst Properties of the FU Ori Object HBC 722 arXiv:2511.04592
Peculiarities in the infrared emission of PAH-C$_{60}$ adducts arXiv:2511.04606
Addressing the DESI DR2 Phantom-Crossing Anomaly and Enhanced $H_0$ Tension with Reconstructed Scalar-Tensor Gravity arXiv:2511.04610
Dynamical Masses of Young Stellar Multiple Systems with the VLBA (DYNAMO-VLBA) arXiv:2511.04642
$\texttt{unimpeded}$: A Public Grid of Nested Sampling Chains for Cosmological Model Comparison and Tension Analysis arXiv:2511.04661
Intermittency in Collisionless Large-Amplitude Turbulence arXiv:2511.04663
On the Exoplanet Yield of Gaia Astrometry arXiv:2511.04673
KGB-evolution: a relativistic $N$-body code for kinetic gravity braiding models arXiv:2511.04676
Dark Energy Survey Year 3 results: Simulation-based $w$CDM inference from weak lensing and galaxy clustering maps with deep learning. I. Analysis design arXiv:2511.04681
Demonstrating Agreement between Radio and Fluorescence Measurements of the Depth of Maximum of Extensive Air Showers at the Pierre Auger Observatory arXiv:2310.19963
Radio Measurements of the Depth of Air-Shower Maximum at the Pierre Auger Observatory arXiv:2310.19966
The Most Energetic Transients: Tidal Disruptions of High-Mass Stars arXiv:2405.08855
Astrophysical assumptions and equation of state framework have larger impact on equation of state inference than individual neutron star observations arXiv:2405.17326
Coronal hole picoflare jets are progenitors of both fast and Alfv\'enic slow solar wind arXiv:2411.16513
JWST PRIMER: A deep JWST study of all ALMA-detected galaxies in PRIMER COSMOS -- dust-obscured star-formation history back to z $\simeq$ 7 arXiv:2503.07774
Cosmology with supernova Encore in the strong lensing cluster MACS J0138$-$2155: photometry, cluster members, and lens mass model arXiv:2503.09718
Comprehensive JWST+ALMA Study on the Extended Ly$\alpha$ Emitters, Himiko and CR7 at $z\sim 7$: Blue Major Merger Systems in Stark Contrast to Submillimeter Galaxies arXiv:2504.03156
Higher-Order Mean-Motion Resonances Can Form in Type-I Disk Migration arXiv:2504.12596
Black Hole Survival Guide: Searching for Stars in the Galactic Center That Endure Partial Tidal Disruption arXiv:2504.14705
Starlight from JWST: Implications for star formation and dark matter models arXiv:2504.20043
Introducing the Descriptive Parametric Model: Gaseous Profiles for Galaxies, Groups, and Clusters arXiv:2505.14782
Non-minimal light-curvature couplings and black-hole imaging arXiv:2505.21431
Probing the accretion geometry of black hole X-ray binaries: A multi-mission spectro-polarimetric and timing study arXiv:2506.03774
Testing scalar dark matter clumps with Pulsar Timing Arrays arXiv:2506.08786
Testing Coasting Cosmologies with Large-Scale Structure Growth arXiv:2506.11826
Broadband Low-Resolution Spectrograph - SpectrumMate LR arXiv:2506.16153
An investigation into correlations between FRB and host galaxy properties arXiv:2506.23403
The validity of separate-universe approach in transient ultra-slow-roll inflation arXiv:2506.23571
Quantitative Morphology of Galactic Cirrus in Deep Optical Imaging arXiv:2507.05217
Cosmic Cartography II: completing galaxy catalogs for gravitational-wave cosmology arXiv:2507.12171
A Systematic Search for AGN Flares in ZTF Data Release 23 arXiv:2507.20232
Measuring the splashback feature: Dependence on halo properties and history arXiv:2507.22102
Hubble constant constraint using 117 FRBs with a more accurate probability density function for ${\rm DM}_{\rm diff}$ arXiv:2508.05161
MrMARTIAN: A Multi-resolution Mass Reconstruction Algorithm Combining Free-form and Analytic Components arXiv:2508.13262
Glitch analysis and asteroseismic modelling of subgiant $\mu$ Herculis: confirming and interpreting the $\Gamma_1$ peak as the helium glitch arXiv:2509.01577
A Dark Matter Model with Quadratic Equation of State: Background Evolution and Structure Formation arXiv:2509.11138
The SPAr burning: proton captures powering carbon-oxygen shell mergers in massive stars arXiv:2509.13749
Optical/infrared observations of the extraordinary GRB 250702B: a highly obscured afterglow in a massive galaxy consistent with multiple possible progenitors arXiv:2509.22784
The Tidal Torque Theory Revisited: II. Rotational Halo Properties arXiv:2509.26081
The Sunburst Arc with JWST. IV. The importance of interaction, turbulence, and feedback for Lyman-continuum escape arXiv:2510.11702
Dependency of the Bar Formation Timescale On The Halo Spin arXiv:2510.13153
Neural Posterior Estimation for Cataloging Astronomical Images from the Legacy Survey of Space and Time arXiv:2510.15315
Order-by-order Modeling of Exoplanet Radial Velocity Data arXiv:2510.16139
Pre-perihelion Development of Interstellar Comet 3I/ATLAS arXiv:2510.18769
Mass-radius relationship and gravitational wave emission from magnetized spheroidal quark stars arXiv:2510.20459
The cosmological analysis of DES 3$\times$2pt data from the Effective Field Theory of Large-Scale Structure arXiv:2510.24878
Stellar Spectroscopy Using Diffraction Grating, CMOS Monochrome Sensor, and Reflecting Telescopes arXiv:2510.26689
Properties of Carbon-rich AGB Stars in the LMC and the Milky Way arXiv:2511.00397
Determining the impact of post-main-sequence stellar evolution on the transiting giant planet population arXiv:2511.02896
Euclid Quick Data Release (Q1). The average far-infrared properties of Euclid-selected star-forming galaxies arXiv:2511.02989
Study of Four nulling pulsars with FAST arXiv:2511.03150
First Associated Neutrino Search for a Failed Supernova Candidate with Super-Kamiokande arXiv:2511.03470
The first year of LISA Galactic foreground arXiv:2511.03604
Prospects for Probing Sub-GeV Leptophilic Dark Matter with the Future VLAST arXiv:2505.05359
Graviton-photon conversion in stochastic magnetic fields arXiv:2505.10926
Inflation models selected by the swampland distance conjecture with the Lyth bound arXiv:2507.23320
Nuclear chiral density wave in neutron stars? arXiv:2509.10135
Equation of state for hyperonic neutron-star matter in SU(3) flavor symmetry arXiv:2509.16559
Ionospheric responses over the Antarctic region to Intense Space Weather events: Plasma Convection vs. Auroral Precipitation arXiv:2510.27372