Delayed Wind Onset in Pa 30, the Remnant of Type Iax SN 1181 arXiv:2511.14829
V570 Per: Characterization of a Benchmark Eclipsing Binary arXiv:2511.14830
Localized Deviations from the CO-PAH Relation in PHANGS-JWST Galaxies: Faint PAH Emission or Elevated CO Emissivity? arXiv:2511.14833
Mixing between AGN winds and ISM clouds produces luminous X-ray emission arXiv:2511.14834
First Mid-infrared Detection and Modeling of a Flare from Sgr A*. II. Mid-IR Spectral Energy Distribution and Millimeter Polarimetry arXiv:2511.14836
Stellar Obliquities of Young Systems, Atmospheres Undergoing Contraction and Escape (SOYSAUCE): a likely aligned orbit for the 3 Myr planet TIDYE-1 b arXiv:2511.14838
Variability-selected AGN in dwarf galaxies: the incidence of AGN in dwarf and massive galaxies is similar arXiv:2511.14842
Probing the influence of the protocluster environment on galaxy morphology at z = 2.23 arXiv:2511.14843
J-HERTz: J-PLUS Heritage Exploration of Radio Targets at z $<$ 5 arXiv:2511.14844
Mid-infrared extinction toward the Galactic center arXiv:2511.14850
Photometric Constraints on Intermediate-mass Black Holes in the Galactic Centre arXiv:2511.14856
Large Language Model Driven Analysis of General Coordinates Network (GCN) Circulars arXiv:2511.14858
Radio properties of the quasi-periodic eruption source RXJ1301.9+2747 at parsec scales arXiv:2511.14863
Tidal Disruption Events arXiv:2511.14911
Dynamics in the Cores of Self-Interacting Dark Matter Halos: Reduced Stalling and Accelerated Core Collapse arXiv:2511.14912
SN 2023taz: Implications for the UV Diversity of Superluminous Supernovae arXiv:2511.14916
Simulations of a Conducting Sphere Moving through Magnetized Plasma: Alfv\'en Wings, Slow Magnetosonic Wings, and Drag Force arXiv:2511.14932
Proton specific entropy as a proxy for the $O^{7+}/O^{6+}$ charge state ratio over heliocentric distance arXiv:2511.14938
Constraining the Jet Energetics of the Transient X-ray Binaries MAXI J1348-630 and MAXI J1820+070 through Calorimetry arXiv:2511.14941
Understanding the Origin and Dynamical Evolution of the Unique Open Star Cluster Berkeley 20 using FIRE Simulations arXiv:2511.14958
A Neural Network Approach to Preferred Event Selection for Low-Latency Gravitational-Wave Alerts arXiv:2511.14997
Toward Complete Merger Identification at Cosmic Noon with Deep Learning arXiv:2511.15006
Relative Strengths of Fundamental and Harmonic Emissions of Solar Radio Type II Bursts arXiv:2511.15011
Hyperaccretion-driven relativistic jets from massive collapsars in active galactic nucleus disks arXiv:2511.15056
Deep-learning mitigation of foregrounds and beam effects in 21-cm intensity mapping using hybrid frequency differencing and PCA arXiv:2511.15072
The ALMA-QUARKS survey: Evidence of a candidate high-mass prestellar core aside a bright-rimmed cloud IRAS 18290-0924 arXiv:2511.15079
Implications of the Two-Component Dark Energy Model for Hubble Tension arXiv:2511.15087
PHR~J1724-3859: A Bipolar Planetary Nebula in Open Cluster Trumpler 25 arXiv:2511.15115
Solar Periodic Companion and Random Stellar Flybys: Dynamical Perturbations of Highly Eccentric Comets in the Oort Cloud arXiv:2511.15121
Measuring the crust-superfluid coupling time-scale for 105 UTMOST pulsars with a Kalman filter arXiv:2511.15134
Electron Cyclotron Maser Emission as the Driving Mechanism in Long-Period Radio Transients arXiv:2511.15154
Non-thermal processes in standard big bang nucleosynthesis: III. Reactions with slow nuclei and the overall effect arXiv:2511.15158
Gravitational Wave Phase shifts of black hole mergers in AGN Disks arXiv:2511.15193
Evolution of action-space coherence in a Milky Way-like simulation arXiv:2511.15215
Changing-look Active Galactic Nuclei from the Dark Energy Spectroscopic Instrument. IV. Broad Emission Line Evolution Sequence Among H{\alpha}, Mg II, and H{\beta} arXiv:2511.15275
The Rotation Dip in the Envelope-Disk Transition of HH 111: Evidence for Magnetic Braking arXiv:2511.15309
Refractive indices of photochemical haze analogs for Solar System and exoplanet applications : a cross-laboratory comparative study between the PAMPRE and COSmIC experimental set-ups arXiv:2511.15310
A Method for Gamma-Ray Energy Spectrum Inversion and Correction arXiv:2511.15313
A JWST Transit of a Jupiter Analog: II. A Search for Exomoons arXiv:2511.15317
Origin of Galaxies arXiv:2511.15325
Interacting binaries on the Main Sequence as in-situ tracers of mass transfer efficiency and stability arXiv:2511.15347
Type Iax supernovae as a source of iron-rich silicate dust arXiv:2511.15349
Galaxy-Multiplet Clustering from DESI DR2 arXiv:2511.15354
Changing-look Active Galactic Nuclei from the Dark Energy Spectroscopic Instrument. V. Dramatic Variability in High-Ionization Broad Emission Lines arXiv:2511.15359
Simple relations from complex outflows: How the $M-\sigma$ relation emerges in a multi-phase environment arXiv:2511.15380
Insights on Gas Distribution and Dynamics in Massive Proto-cluster G358.46$-$0.39: Possible Multiplicity in G358.46$-$0.39 MM1a arXiv:2511.15400
Explosions in the Empty: A Survey of Transients in Local Void Galaxies arXiv:2511.15401
Elemental abundance ratios for the bulge of M31 arXiv:2511.15415
Viscous Dark Energy and Mass-Varying Dark Matter in Lyra Manifold: Cosmological Dynamics and Observational Constraints arXiv:2511.15422
21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter arXiv:2511.15430
Advancing Identification method of Gamma-Ray Bursts with Data and Feature Enhancement arXiv:2511.15470
Optical gains measurement with a gain scheduling camera: On-sky demonstration with PAPYRUS and perspectives arXiv:2511.15471
Challenging the $\omega_0\omega_a$CDM parametrization through rational expansions in view of DESI data release arXiv:2511.15472
LCS: A Learnlet-Based Sparse Framework for Blind Source Separation arXiv:2511.15475
Probing the disk-jet coupling in M87 arXiv:2511.15482
Efficient Exoplanet Imaging Simulations of the Habitable Worlds Observatory arXiv:2511.15511
Identification of periodic density structures in Solar Orbiter data: Radial evolution arXiv:2511.15518
Using Light Curve Derivatives to Estimate the Fill-out Factor of Overcontact Binaries arXiv:2511.15537
The VVVX quest for satellites around the Circinus galaxy arXiv:2511.15541
Is There New Physics Beyond 30 TeV in the BOAT? arXiv:2511.15542
Quadruple system HD 135160 in a unique 2+2 configuration arXiv:2511.15544
Excess of diffuse gamma-ray emission detected from the galaxy cluster Abell 119 from 14-year Fermi-LAT Data arXiv:2511.15559
Catching the 2021 {\gamma}-ray flare in the blazar TXS 2013+370 arXiv:2511.15601
Unified Kraft Break at ~6500 K: A Newly Identified Single-Star Obliquity Transition Matches the Classical Rotation Break arXiv:2511.15610
Reporting a Deficit of Intrinsic NV Absorbers in Core-dominated, Radio-loud Quasars arXiv:2511.15627
The Cherenkov Camera for the PBR mission arXiv:2511.15636
The data processing system of the POEMMA-Balloon with Radio mission arXiv:2511.15644
The JWST weather report from the nearest brown dwarfs III: Heterogeneous clouds and Thermochemical instabilities as possible drivers of WISE 1049AB's spectroscopic variability arXiv:2511.15667
Impact of cosmic expansion on gravitational wave spectra from strongly supercooled first-order phase transitions arXiv:2511.15687
The Relationship Between Emission Line and Continuum Luminosity and the Baldwin Effect in Blazars. I. The Case of the Mg II {\lambda}2798 {\AA} Emission Line arXiv:2511.15695
The Atacama Cosmology Telescope: Cross-correlation of kSZ and continuity equation velocity reconstruction with photometric DESI LRGs arXiv:2511.15701
Populating Galaxies Into Halos Via Machine Learning on the Simba Simulation arXiv:2406.16103
Formation of neutron stars inside planetary nebulae via accretion-induced collapse and core-merger-induced collapse from white dwarf binaries arXiv:2407.03985
A Novel Density Profile for Isothermal Cores of Dark Matter Halos arXiv:2411.11945
Isolated Binary Black Hole Formation and Merger Rates from Galaxy Evolution arXiv:2412.13318
Halo spin and orientation in Interacting Dark Matter Dark Energy Cosmology arXiv:2501.03750
UHECR deflections in the coherent Galactic magnetic field arXiv:2501.16158
Structure Formation with Warm White Noise: Effects of Finite Number Density and Velocity Dispersion in Particle and Wave Dark Matter arXiv:2503.20881
Denoising weak lensing mass maps with diffusion model: systematic comparison with generative adversarial network arXiv:2505.00345
Detection of a Type-C QPO during the soft-to-hard transition in Swift J1727.8-1613 arXiv:2505.07938
Smoking gun signature from axion and the constraints with radio telescopes arXiv:2506.05795
Spectroscopic Characterization of redMaPPer Galaxy Clusters with DESI arXiv:2506.06249
Analytical Transit Light Curves for Arbitrary Power-Law Limb Darkening: A Unified Framework arXiv:2506.18860
Understanding the Drag Torque in Common Envelope Evolution arXiv:2506.19547
Cool Gas in the Circumgalactic Medium of Massive Post Starburst Galaxies arXiv:2506.22287
JWST's PEARLS: A Candidate Massive Binary Star System in a Lensed Galaxy at Redshift 0.94 arXiv:2507.03098
Investigating the Growth of Little Red Dot Descendants at z<4 with the JWST arXiv:2507.04011
DELVE-ing into the Milky Way's Globular Clusters: Assessing extra-tidal features in NGC 5897, NGC 7492, and testing detectability with deeper photometry arXiv:2507.11629
Globular Clusters in the Galaxy Cluster MACS0416 at z = 0.397 arXiv:2508.03883
Dance to Demise -- How Massive Stars May Form Dense Circumstellar Shells Before Explosion arXiv:2508.04497
MrMARTIAN: A Multi-resolution Mass Reconstruction Algorithm Combining Free-form and Analytic Components arXiv:2508.13262
The source of the cosmic-ray excess in the Centaurus region -- constraints on possible candidates, mass composition and cosmic magnetic fields arXiv:2509.06594
Unlocking 21cm Cosmology with SBI: A Beginner friendly NRE for Inference of Astrophysical Parameters arXiv:2509.06834
Detecting Local and Integrated Relativistic Effects by Multi-Tracing a Single Galaxy Population in Harmonic Space arXiv:2509.08056
Gravitational Recoil and Suppression of Super Massive Black Hole Seeds in the Early Universe arXiv:2509.10564
Dust Attenuation of Lyman-Werner Feedback: Reassessing Early Super Massive Black Holes Seed Formation arXiv:2509.11111
A simple, flexible method for timing cross-calibration of space missions arXiv:2509.13865
Kinematics of Stellar Streams from Globular Clusters Depend on Black Hole Retention and Star Mass: A Selection Effect for Dark Matter Inference arXiv:2509.15307
Bayesian Gaussian Methods for Robust Background Modeling in CALorimetric Electron Telescope (CALET) Gravitational-Wave Searches arXiv:2509.25893
Cosmological constraints on nonphantom dynamical dark energy with DESI Data Release 2 Baryon Acoustic Oscillations: A 3$\sigma$+ lensing anomaly arXiv:2509.26144
Orbital decay candidates reconsidered: WASP-4 b is not decaying and Kepler-1658 b is not a planet arXiv:2510.05229
The ALPINE-CRISTAL-JWST Survey: Stellar and nebular dust attenuation of main-sequence galaxies at z~4-6 arXiv:2510.18248
Efficient analytic approximation for small-scale non-cold relic perturbations arXiv:2510.20821
XRISM Spectroscopy of the Stellar-mass Black Hole GRS 1915+105 arXiv:2510.25089
An extremely fast fading population II dwarf nova candidate: caught spectroscopically on the rise arXiv:2510.26682
The interstellar flux gap: From dust to kilometer-scale objects arXiv:2511.01957
Kerr Black Hole Shadows in Dispersive Plasma: Frequency-Dependent Geodesics and Shadow Distortions arXiv:2511.06466
JWST/NIRCam observations of HD~92945 debris disk: An asymmetric disk with a gap arXiv:2511.07561
Conservation laws in non-inertial frames and non-conservation of energy of relative motion in two-body problem arXiv:2511.08709
Occurrence rate of stellar Type II radio bursts from a 100 star-year search for coronal mass ejections arXiv:2511.09296
Recalibrating Inflation: Insights from Starobinsky Gravity arXiv:2511.11339
Foreground removal in HI 21 cm intensity mapping under frequency-dependent beam distortions arXiv:2511.13328
JWST observes the assembly of a massive galaxy at z~4 arXiv:2511.13650
Stellar Flares in the TESS Light Curves of Planet-hosting M dwarfs arXiv:2511.13716
Asteroseismic Imprints of Mass Transfer in Binary Stars: Probing the Interiors of Donors and Accretors with Gravity and Acoustic Modes arXiv:2511.14372
Magnetic Fields in the Shapley Supercluster Core with POSSUM: Challenging Model Predictions arXiv:2511.14377
Detector Response to Gravitational Wave Polarizations in Gravitational Quantum Field Theory arXiv:2504.01809
Understanding large-scale dynamos in unstratified rotating shear flows arXiv:2505.03660
Measuring spin precession from massive black hole binaries with gravitational waves: insights from time-domain signal morphology arXiv:2505.14573
A waveform and time digitization mainboard prototype for the hybrid digital optical module of TRIDENT neutrino experiment arXiv:2507.00548
Primordial regular black holes as all the dark matter. III. Covariant canonical quantum gravity models arXiv:2507.02396
Using tunable coherence for reaching micrometer coherence lengths and suppressing stray light in a power-recycled Michelson interferometer arXiv:2508.00503
Constraints on the Variation of the QCD Interaction Scale $\Lambda_{\text{QCD}}$ arXiv:2508.07266
Lightweight posterior construction for gravitational-wave catalogs with the Kolmogorov-Arnold network arXiv:2508.18698
A General Framework for the Spontaneous Scalarization of Regular Black Holes arXiv:2511.01544
Large-Scale Calculations of $\beta$-Decay Rates and Implications for $r$-Process Nucleosynthesis arXiv:2511.02999
Generating optimal Gravitational-Wave template banks with metric-preserving autoencoders arXiv:2511.10466