Cosmological Constraints on 4D Einstein-Gauss-Bonnet Gravity and Kaniadakis Holographic Dark Energy: Implications for Black Hole Shadows arXiv:2511.21789
Globules and pillars in Cygnus X IV. Velocity-resolved [OI] 63 mu map of a peculiar proplyd-like object arXiv:2511.21800
Effects of Resolution and Local Stability on Galactic Disks: I. Multiple Spiral Mode Formation via Swing Amplification arXiv:2511.21805
Asteroseismic detection of an internal magnetic field in the B0.5V pulsator HD 192575 arXiv:2511.21812
APEX survey of interstellar HCl: $^{35}$Cl/$^{37}$Cl isotopic ratios in dense cores and outflows arXiv:2511.21813
Statistical Properties of Cold Streams In Massive Star-Forming Halos in IllustrisTNG-50 arXiv:2511.21814
The LMT 2 Millimeter Receiver System (B4R). I. Overview and Results of Science Demonstration arXiv:2511.21816
A Paradigm Shift in Exoplanet False Positive Identification with HIP-44302 arXiv:2511.21817
The impact of magnetic fields during tidal disruption events arXiv:2511.21818
Little Red Dots host Black Hole Stars: A unified family of gas-reddened AGN revealed by JWST/NIRSpec spectroscopy arXiv:2511.21820
J-PAS: A value-added catalogue of optical line intensities for nebular emission galaxies (JOLINES) arXiv:2511.21822
Probing Exotic Astrophysical Dark objects through Astrometric Microlensing from Gaia arXiv:2511.21823
LYRA ultra-faints: The emergence of faint dwarf galaxies in the presence of an early Lyman-Werner background arXiv:2511.21824
The HITRAN2024 methane update arXiv:2511.21840
The LMT 2 millimeter receiver system (B4R). II. Science demonstration observations toward Orion-KL/OMC-1 arXiv:2511.21845
Evaluating Star-Planet Interactions with Zeeman Doppler Imaging: Case Study in YZ Ceti arXiv:2511.21853
Intrinsic galaxy alignments in CAMELS simulations and the significant impact of baryon model arXiv:2511.21881
Gravitational Waves as a Probe of Core Collapse Supernova Progenitor Structure arXiv:2511.21895
Modeling Galaxy Formation in Cosmological Simulations with CRK-HACC arXiv:2511.21921
The relations between dust properties and galaxy global / integrated quantities in the nearby Universe arXiv:2511.21922
Data span and frequency coverage requirements for robust detection and inference in PTAs: A case study with EPTA DR2 arXiv:2511.21933
The Atacama Cosmology Telescope: $B$-mode delensing with DR6 data and external tracers of large-scale structure arXiv:2511.21949
Vibrationally excited H2 mutes the He i triplet line at 1.08 {\mu}m on warm exo-Neptunes arXiv:2511.21966
Interferometric view into RT Pav's long secondary period. binary vs oscillatory convective modes arXiv:2511.21987
Numerical implementation of flat FLRW models of cosmic expansion with Planck 2018 cosmological parameters arXiv:2511.21991
A Catalogue of Mid-infrared Variable Sources from unTimely arXiv:2511.22071
Characterizing Binary Black Hole Subpopulations in GWTC-4 with Binned Gaussian Processes: On the Origins of the $35M_{\odot}$ Peak arXiv:2511.22093
Deep insights into Abell 2163: unveiling the treasure trove of ICM plasma physics arXiv:2511.22124
Constraining the Properties of GRB Accreting Magnetar with $R/I$ Evolutionary Effects Using \emph{Swift}/XRT Data arXiv:2511.22149
A Novel Comb Generator for Frequency Phase Transfer arXiv:2511.22161
Probing CMB Polarization Gaussianity with the Statistics of Unpolarized Points: Non-Gaussianity of Planck Data and Prospects for Future B-Mode Measurements arXiv:2511.22220
Forecasting Primordial Non-Gaussianity from UNIONS Lyman-Break Galaxies and Planck CMB lensing arXiv:2511.22243
Galaxy rotation curve based on RGB stars from the Gaia DR3 catalogue arXiv:2511.22295
Recovering Intrinsic Pulsar Profiles and Scattering Parameters with a CLEAN-Based Algorithm for High-Precision Timing arXiv:2511.22299
Astrophysical constraints from future measurements of the kinetic Sunyaev-Zel'dovich power spectrum arXiv:2511.22309
The life of central radio galaxies in clusters: AGN-ICM studies of eRASS1 clusters in the ASKAP fields arXiv:2511.22319
The First Scientific Flight and Observations of the 50-mm Balloon-Borne White-Light Coronagraph arXiv:2511.22336
Euclid preparation: LXXXI. The impact of nonparametric star formation histories on spatially resolved galaxy property estimation using synthetic Euclid images arXiv:2511.22399
Manifestation of the stellar wind cycle in infrared images: Example of the heliosphere arXiv:2511.22401
Galaxy and Mass Assembly (GAMA): The Properties of Quasar Host Galaxies: Star Formation Histories and Stellar Populations arXiv:2511.22453
Differentiable N-body code for Galactic Dynamics -- Odisseo arXiv:2511.22468
The Solar Close Observations and Proximity Experiments (SCOPE) mission arXiv:2511.22472
Clustering in dynamical dark energy: observational constraints from DESI, CMB, and supernovae arXiv:2511.22478
Classical Cepheids in the Galactic thin disk. I. Abundance gradients through NLTE spectral analysis arXiv:2511.22491
Robust evidence for dynamical dark energy in light of DESI DR2 and joint ACT, SPT, and Planck data arXiv:2511.22512
Needle in a Poissonian haystack -- An X-ray astronomer's guide to QPE fishing arXiv:2511.22520
Spiral excitation in protoplanetary disks through gap-edge illumination: Distinctive kinematic signatures in CO isotopologues arXiv:2511.22527
Towards Understanding the Origin of Swift Gamma-Ray Bursts Driven by Magnetars arXiv:2511.22534
Laboratory Detection and Rotational Spectroscopy of $trans$-HNSO: Implications for Astronomical Observations arXiv:2511.22548
Cosmology of axion dark energy in supersymmetric models and constraints on high scale parameters arXiv:2511.22559
The network analysis of the cosmic web as a tool to constrain cosmology and cosmic magnetism arXiv:2511.22573
ALMACAL. XV. Band 3 ALMA Survey and Number Counts arXiv:2511.22574
Forecasting Constraint on Primordial Black Hole Properties with the CSST $3\times2$pt Analysis arXiv:2511.22575
Skew-spectra: a generalization to spin-$s$ arXiv:2511.22596
The NANOGrav 12.5-year Data Set: Chromatic Noise Characterization & Mitigation with Time-Domain Kernels arXiv:2511.22597
Identifying Transient Hosts in LSST's Deep Drilling Fields with Galaxy Catalogues arXiv:2511.22634
Non-Gaussianity in SMICA arXiv:2511.22641
Tracing Structure: Shape and Centroid Deviations in 39 Strong Lensing Clusters as a Test of Cluster Formation Predictions arXiv:2511.22661
Structure-Preserving Unpaired Image Translation to Photometrically Calibrate JunoCam with Hubble Data arXiv:2511.22668
Vortex Dynamics in the Neutron Star Inner Crust arXiv:2511.22670
The Parkes Observatory Pulsar Data Archive arXiv:2511.22702
Evading the dust fragmentation barrier with the streaming instability in protoplanetary disks arXiv:2511.22709
EMU and Euclid: Detection of a radio-optical galaxy clustering cross-correlation signal between the Evolutionary Map of the Universe and Euclid arXiv:2511.22732
Closing the gap: Follow-up observations of peculiar dusty objects close to Sgr A* using ERIS arXiv:2511.22761
The Hubble Ultracool Multiplicity (HUM) Survey. I. Characterizing Sensitivity to Companions at Sub-Diffraction Limit Separations with HST WFC3/IR arXiv:2511.22783
The Shear-to-Cosmology Paradigm I: Hybrid Field-Level and Simulation-Based Framework for Weak Lensing Surveys arXiv:2511.22851
BSN: The First Multiband Light Curve Analysis of the W UMa-type Contact Binary System EM Tucanae arXiv:2511.22907
SN 2021ukt: A Transitional Supernova with a Short Plateau and Persistent Interaction arXiv:2511.22923
Collapse of Axion Domain Wall Induced by Helical Primordial Magnetic Fields arXiv:2511.22949
Connecting Star Formation in the Milky Way and Nearby Galaxies -II. An Analytical Model to Predict Cloud-Scale Star Formation Rate arXiv:2511.22985
Incorporating neutron star physics into gravitational wave inference with neural priors arXiv:2511.22987
Blending-induced beating and emission in the symbiotic star Terz V 2513 arXiv:2511.22988
ExoJAX Retrievals of VLT/CRIRES Spectra of Luhman 16AB: C/O Ratios and Systematic Uncertainties arXiv:2511.23018
High-resolution cosmological simulations of primordial dark matter clustering under long-range and fractional forces arXiv:2511.23040
The observation of Ground Level Enhancement GLE 77 by the neutron detectors of the Experimental Complex NEVOD arXiv:2511.23048
Constraining dark matter halo profiles with symbolic regression arXiv:2511.23073
$\delta$ Circini: A massive hierarchical triple system with an eclipsing binary arXiv:2511.23089
Predictions from $s$-process AGB models of the isotopic variations of zirconium and neodymium for comparison to bulk meteorites arXiv:2511.23104
Consequences of radially correlated rotation curves for galaxy mass models arXiv:2511.23106
Young M dwarfs flare activity model: Towards better exoplanetary atmospheric characterisation arXiv:2511.23129
Blazar classification from multi-wavelength data using Deep Learning arXiv:2511.23134
Sulfur monoxide as a tracer of the Galactic $^{32}$S/$^{34}$S gradient arXiv:2511.23147
Large-amplitude Variability Driven by Giant Dust Storms on a Planetary-mass Companion arXiv:2511.23163
Bursty star formation, chemical enrichment, and star cluster formation in numerical analogues of GN-z11 arXiv:2511.23164
An improved formalism for measuring the dark matter subhalos mass by its gravitational wake arXiv:2511.23168
Primordial Black Holes as Dark Matter and the Tachyonic Trap During Inflation arXiv:2511.23182
Predictions on gravity mode pulsations of collisional blue straggler stars in globular clusters arXiv:2511.23189
Witten-O'Raifeartaigh potential revisited in the context of Warm Inflation arXiv:2511.23219
SlotFlow: Amortized Trans-Dimensional Inference with Slot-Based Normalizing Flows arXiv:2511.23228
Tools and Advancements towards Data Standardization of the MAGIC Collaboration arXiv:2511.23244
Macroscopic Dark Matter under siege: from White Dwarf Data to Gravitational Wave Detection arXiv:2511.23263
Simulating AGN feedback in galaxy clusters with pre-existing turbulence arXiv:2511.23267
Properties of Core Collapse Supernovae from Binary Population Synthesis arXiv:2511.23285
A Detection of Sulfur-Bearing Cyclic Hydrocarbons in Space arXiv:2511.23299
Calcium versus silicon ejecta velocities and decline rates in supernovae Ia: The role of high-velocity features arXiv:2511.23305
Stellar streams around dwarf galaxies in the Local Universe arXiv:2511.23314
CO observations in rotating circumbinary post-AGB disks arXiv:2511.23348
Synchrotron Self-Compton Model of TeV Afterglows in Gamma-Ray Bursts arXiv:2511.23349
Investigating the Impacts of AGN Activities on Dwarf Galaxies with FAST HI Observations arXiv:2511.23356
The Kinematic Properties of T\.ZO Candidate HV 11417 with Gaia DR3 arXiv:2511.23368
Identifying bars in galaxies using machine learning arXiv:2511.23383
Consensus based Algorithm for Nonparametric Detection of Star Clusters (CANDiSC) arXiv:2511.23414
Detection of the Pairwise Kinematic Sunyaev-Zel'dovich Effect and Pairwise Velocity with DESI DR1 Galaxies and ACT DR6 and Planck CMB Data arXiv:2511.23417
Inflation Driven by Scalar-Neutrino Coupling in a Mass-Varying Neutrino Framework arXiv:2511.23422
Variation of Microphysical Parameters in Reverse-shock Scenario arXiv:2511.23426
The EBLM Project XVIII. 3D Obliquities of Five Low-Mass Eclipsing Binaries arXiv:2511.23430
A measurement of $H_0$ from DESI DR1 using energy densities arXiv:2511.23432
From metallicity distributions to mutual information: A new perspective on stellar halo assembly arXiv:2511.23452
Baryon fraction from the BAO amplitude: a consistent approach to parameterizing perturbation growth arXiv:2511.23459
Kinetic Mixing and the Phantom Illusion: Axion-Dilaton Quintessence in Light of DESI DR2 arXiv:2511.23463
Observational constraints of diffusive dark-fluid cosmology arXiv:2301.02913
Total and dark mass from observations of galaxy centers with Machine Learning arXiv:2310.02816
Where do stars explode in the ISM? -- The distribution of dense gas around evolved massive stars in M33 arXiv:2310.17694
Cosmological Parameter Estimation with a Joint-Likelihood Analysis of the Cosmic Microwave Background and Big Bang Nucleosynthesis arXiv:2408.14531
LINX: A Fast, Differentiable, and Extensible Big Bang Nucleosynthesis Package arXiv:2408.14538
Deep Investigation of Neutral Gas Origins (DINGO): Options for the Processing and Storage of Radio Astronomy Data for robust Deep Spectral Line Imaging in the SKA-Era using uv-Grids arXiv:2410.02285
The galaxy-IGM connection in THESAN: observability and information content of the galaxy-Lyman-$\alpha$ cross-correlation at z$\geq$6 arXiv:2410.02850
Stochastic gravitational wave background anisotropies from inflation with non-Bunch-Davies states arXiv:2410.14664
Cosmological Model Independent Constraints on Lorentz Invariance Violation with Updated Gamma-Ray Burst Observations: An Artificial Neural Network Approach arXiv:2412.06159
Beyond MESA Defaults: The Impact of Structural Resolution Uncertainty in p-mode Asteroseismology arXiv:2501.13207
The dynamical and thermodynamic effects of turbulence for the cosmic baryonic fluid arXiv:2503.06593
A new approach for simulating PBH formation from generic curvature fluctuations with the Misner-Sharp formalism arXiv:2504.05813
Ultra-diffuse galaxies in the EAGLE simulation arXiv:2504.14973
A multi-messenger window into galactic magnetic fields and black hole mergers with LISA arXiv:2504.18986
A New Wavelet Scattering Transform-Based Statistic for Cosmological Analysis of Large-Scale Structure arXiv:2505.14400
Collisionless relaxation to equilibrium distributions in cold dark matter halos: origin of the Navarro-Frenk-White profile arXiv:2506.02104
JWST Spectroscopy of a Blue Binary Cold Classical Kuiper Belt Object arXiv:2506.11972
Hubble constant measurement from QPEs as electromagnetic counterparts to extreme mass ratio inspirals arXiv:2506.14150
Sulphur abundances in star-forming regions from optical emission lines: A new approach based on photoionization models consistent with the direct method arXiv:2506.14736
CosmoGLINT: Cosmological Generative Model for Line Intensity Mapping with Transformer arXiv:2506.16843
Cosmological abundance of primordial black holes in mixed dark matter scenarios incorporating Kaluza-Klein dark matter arXiv:2506.20391
HOLISMOKES XVIII: Detecting strongly lensed SNe Ia from time series of multi-band LSST-like imaging data arXiv:2506.22076
Dissecting Reionisation with the Cosmic Star Formation and Active Galactic Nuclei Luminosity History arXiv:2507.16112
Direct correlation of line intensity mapping and CMB lensing from evolution along the lightcone arXiv:2507.17752
MUSEQuBES: The Column Density, Covering Fraction, Mass, and Environmental Dependence of Cool HI Gas Around Low-Redshift Galaxies arXiv:2507.22283
The Filament Rift: $\Lambda$CDM's Structural Challenge Against Observation arXiv:2508.07480
Impact of Resonance, Raman, and Thomson Scattering on Hydrogen Line Formation in Little Red Dots arXiv:2508.08768
Field-level Reconstruction from Foreground-Contaminated 21-cm Maps arXiv:2508.13265
VIPCALs: A fully automated calibration pipeline for very long baseline interferometry data arXiv:2508.13282
Constraining deviations from $\Lambda$CDM in the Hubble expansion rate arXiv:2508.17848
SN2023syz and SN2025cbj: Two Type IIn Supernovae Associated with IceCube High-energy Neutrinos arXiv:2508.19080
Rethinking mass transfer: a unified semi-analytical framework for circular and eccentric binaries. I. Orbital evolution due to conservative mass transfer arXiv:2509.05243
The Hubble constant from the improved lens modeling of cluster-lensed supernova Refsdal with new spectroscopic redshifts and the Jackknife method arXiv:2509.09979
Sibling Sub-Neptunes Around Sibling M Dwarfs: TOI-521 and TOI-912 arXiv:2509.14782
A novel reverberation mapping method for blazars arXiv:2509.16927
Where did Heavy Binaries Go? Gravitational-wave Populations Using Delaunay Triangulation with Optimized Complexity arXiv:2509.19466
Impact of the latest 22Ne+{\alpha} reaction rates on nucleosynthesis in massive stars and galactic chemical evolution arXiv:2509.19583
A Less Terrifying Universe? Mundanity as an Explanation for the Fermi Paradox arXiv:2509.22878
Evidence for increasing dark energy in DESI from the Local Distance Ladder arXiv:2509.23168
Dark-Matter-Deficient Galaxies from Collisions: A New Probe of Bursty Feedback and Dark Matter Physics arXiv:2509.24270
The Tidal Torque Theory Revisited: II. Rotational Halo Properties arXiv:2509.26081
Measurements of the Birks' coefficient of GAGG:Ce using hard X-rays arXiv:2510.02920
SPYGLASS. VII-A. The Demographics and Ages of Small Nearby Young Associations arXiv:2510.21936
Mode Composition Shapes Magnetic Anisotropy in Solar Wind Turbulence arXiv:2510.25636
Cosmic voids and the kinetic analysis. V. Hubble tension, the cosmological constant and aperiodic filaments arXiv:2511.03990
Confirmation of SRGt 062340.2-265751 as a nova-like cataclysmic variable with a possible magnetic nature arXiv:2511.04738
Recoil-Enabled Energy Transfer from Coherent Neutrino Scattering in Core-Collapse Supernovae arXiv:2511.04896
Galaxy Clusters from the DESI Legacy Imaging Surveys. III.Star-forming Fraction of Brightest Cluster Galaxies arXiv:2511.09858
REBELS-IFU: Spatially Resolved Ionizing Photon Production Efficiencies of 12 Bright Galaxies in the Epoch of Reionization arXiv:2511.10743
PRIMA General Observer Science Book Volume 2 arXiv:2511.10927
Creation of Viscous Dark Energy by the Hubble Flow: Comparison with SNe Ia Master Sample Binned Data arXiv:2511.16130
Deep Investigation of Neutral Gas Origins (DINGO): Options for robust Deep Spectral Line Imaging in the SKA-Era arXiv:2511.17307
Measurement of Milli-Charged Particles with a running electromagnetic coupling constant at IceCube arXiv:2511.18881
Broad-band temporal and spectral study of TeV blazar TXS 0518+211 arXiv:2511.21182
Quantifying the differences in transmission and emission spectra for hot irradiated gaseous exoplanet atmospheres: A comparison of 1D and 3D modeling using JWST arXiv:2511.21454
Compton-induced $\gamma$-ray Cascade Emissions in Radio Galaxy NGC 1275 arXiv:2511.21463
Wideband search for axionlike dark matter using octupolar nuclei in a crystal arXiv:2410.02218
A Catalog of First-Order Electroweak Phase Transitions in the Standard Model Effective Field Theory arXiv:2410.23210
Post-adiabatic waveform-generation framework for asymmetric precessing binaries arXiv:2501.01413
Cosmological perturbation theory with trinity of scalar fields arXiv:2501.02991
Waveform models for the gravitational-wave memory effect: II. Time-domain and frequency-domain models for nonspinning binaries arXiv:2504.18635
Thermodynamics of magnetized BPS baryonic layers and the effects of the Isospin chemical potential arXiv:2505.18007
Gravitational waves in minimal Maxwell $f(R)$ gravity arXiv:2507.06094
Leptophilic dark matter in $U(1)_{L_{i}-L_{j}}$ models: a solution to the Fermi-LAT Galactic Center Excess consistent with cosmological and laboratory observations arXiv:2508.02775
QCD corrections to Minimal Dark Matter annihilations arXiv:2508.02778
Unified Framework for Geodesic Dynamics with Conservative, Dissipative, and GUP Effects arXiv:2509.14663
Gravity and the Hierarchy Problem arXiv:2510.12882
Bound State Perturbations in the Interior of Black Holes arXiv:2510.20305
Probing the nonstrange quark star equation of state with compact stars and gravitational waves arXiv:2510.24396
WallGo investigates: Theoretical uncertainties in the bubble wall velocity arXiv:2510.27691
Gravitational Bound State Perturbations Inside Black Holes and Isospectrality arXiv:2511.15140
Numerical tiling-based simulations of decoherence in multifield models of inflation arXiv:2511.16801
Ghost instabilities and strong coupling in quadratic non-metricity theories arXiv:2511.19101
$\mathbb Z_2$-Stable Dark Matter via Broken $\text{SU}(5)$ Gauge Bosons arXiv:2511.19462
A Bottom-Up EFT Approach To Superdense Baryonic Matter arXiv:2511.21141