AstroArxiv

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The Environmental Switch in Black Hole Feeding: Bar-Driven vs. Merger-Driven Growth in IllustrisTNG50. Harsh Uttam et. al. https://arxiv.org/abs/2602.22875

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The MARTINI Platform (I): Se I-X atomic calculation and expansion opacity for early-stage kilonova spectral analysis. Matteo Bezmalinovich et. al. https://arxiv.org/abs/2602.22886

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Group Pre-processing in J1611+4026: Minor Rejuvenation of a Massive ETG fueled by Interaction-driven Gas Transfer. Yaosong Yu et. al. https://arxiv.org/abs/2602.22904

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Pulse-resolved Classification and Characteristics of Long-duration GRBs with \emph{Swift}-BAT Data.II. Main Burst versus Extended Emission. Liang Li et. al. https://arxiv.org/abs/2602.22926

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The Evolution of Nulling in Pulsars. P.R. Brook et. al. https://arxiv.org/abs/2602.22956

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Demonstrating Single Photon Counting with Kinetic Inductance Detectors from 3.8 to 25 $μ$m. Wilbert G. Ras-Vinke et. al. https://arxiv.org/abs/2602.22970

Reconstructed large-scale magnetic field map in flattened polar view. From the left, the radial, azimuthal, and meridional components of the magnetic field vector are illustrated. Concentric circles represent different stellar latitudes: -30\,$^{

Time series of Stokes~$V$ LSD profiles and the ZDI models for GJ~504. The observations are shown in black and the models in red. The numbers on the right indicate the rotational cycle computed from Eq.~ {eq:ephemeris

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Eating planets makes you younger: The magnetic dynamo rejuvenation of GJ 504 by planetary engulfment. S. Bellotti et. al. https://arxiv.org/abs/2602.22979

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Energy Deposition by Galactic Cosmic Rays and Implications for Ozone Chemistry. Luiz Augusto Stuani Pereia et. al. https://arxiv.org/abs/2602.22987

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A single void (the same as highlighted in white in Fig.~ {fig:Visualization

The void size function (VSF) model [Eqs.~ {eq:VSF_model

The void mass function (VMF) of ( {left

Cosmic voids as a probe of the nature of dark matter: simulations and galaxy survey forecasts. Alexander Spencer London et. al. https://arxiv.org/abs/2602.22990

Tight bounds on the Maxwell-Carroll-Field-Jackiw parameters using Fast Radio Bursts. Filipe S. Ribeiro et. al. https://arxiv.org/abs/2602.22996

Distribution of the $ $23\,000 sources after a sequential selection process, with colors indicating excluded objects and the dashed line denoting the white dwarf removal criterion.

The left panel shows the variability indices and thresholds for J022959.14+362405.6. The green dashed line represents the variability threshold, and the arrow indicates the position of the target source. The right panel shows the seasonal averages of W1 and W2 fluxes for the sample, with blue cir...

The relationship between the Gaia FoM and the signal-to-noise ratio (S/N) in the AllWISE W1 band for the 12 debris-disk candidates, with the color scale showing the positional offset between the Gaia and AllWISE positions.

Sample Selection and Screening Process

Warm Debris Disk Candidates around Nearby FGK Stars from LAMOST DR12. Xing Luo et. al. https://arxiv.org/abs/2602.23004

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Magnetic maps of DF Tau. The radial, azimuthal, and meridional fields are illustrated on the top, middle, and bottom panels, respectively. We used the same flattened polar view as Fig.~ {fig:di

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Characterising the magnetospheric accretion process of DF Tauri's primary. K. Pouilly et. al. https://arxiv.org/abs/2602.23015

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Phase-Induced Amplitude Apodization Complex Mask Coronagraph (PIAACMC) on-sky demonstration with MagAO-X. Elena Tonucci et. al. https://arxiv.org/abs/2602.23016

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Correlated residuals in Tully-Fisher and Fundamental Plane relations and their impact on peculiar velocity measurements. Tyann Dumerchat et. al. https://arxiv.org/abs/2602.23033

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Comparison of the {

The LOFAR sub-arcsecond view of the high-redshift radio relic in PSZ2G091.83+26.11. G. Di Gennaro et. al. https://arxiv.org/abs/2602.23046

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Measurements of the HI intensity mapping power spectrum at low redshifts with MIGHTEE data: comparison with detected HI galaxies. Junaid Townsend et. al. https://arxiv.org/abs/2602.23055

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A High-Throughput AES-GCM Implementation on GPUs for Secure, Policy-Based Access to Massive Astronomical Catalogs. Samuel Lemes-Perera et. al. https://arxiv.org/abs/2602.23067

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Noise-induced starburst dynamics driven by dark matter halo scatter. {Left:

Diagnostic of Galactic Death. {Top:

State at $T = 2.5$: Establishment of the central quenching radius and onset of disk starburst.

Stochastic Evolution of Galactic Star Formation with Halo Coupling, AGN Quenching and Hopf Bifurcation Dynamics. Sanjeev Kumar et. al. https://arxiv.org/abs/2602.23077

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TEPCat: The Transiting Extrasolar Planet Catalogue. John Southworth https://arxiv.org/abs/2602.23102

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Distribution functions for spheroids. James Binney https://arxiv.org/abs/2602.23127

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Searching for low-mass stars with magnetically-induced hyper-inflated radii. D. J. Mullan et. al. https://arxiv.org/abs/2602.23147

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Sulfur fractionation in coronal plumes as observed by Solar Orbiter/SPICE. Slimane Mzerguat et. al. https://arxiv.org/abs/2602.23170

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Optical spectra of SN 2022ywf. The epochs show the days with respect to r-maximum. The observation log of spectra can be found in Tab. {tab:22ywf_spectra

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Optical spectra of SN 2023zgx. The epochs show the days with respect to r-maximum. The observation log of spectra can be found in Tab. {tab:23zgx_spectra

The extremely low-luminosity Type Iax SNe 2022ywf and 2023zgx. Barnabás Barna et. al. https://arxiv.org/abs/2602.23175

A Lorentz-Covariant Spectral Universality of Stochastic Fields. Alexander G. Tevzadze https://arxiv.org/abs/2602.23195

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The photon survival probability $ {P

The photon survival probability $ {P

The Axion-Photon Mixing and the Extragalactic Magnetic Background: Plateau Regimes, Resonances, and Non-Gaussian Boosts. Andrea Addazi et. al. https://arxiv.org/abs/2602.23249

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Same as Fig.~ {fig: Per_Ecc_single_psMp

Time evolution of the protoplanet's semi-major axis in one representative simulation with $N_{0

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Elevated Eccentricities in the Radius Valley Hint at Water-Rich Mini-Neptunes. Sho Shibata et. al. https://arxiv.org/abs/2602.23250

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Tidal Synchronization of Binaries in Pleiades. Li Wang et. al. https://arxiv.org/abs/2602.23251

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Variability of the X-ray obscuring wind in Mrk 335 with XMM-Newton/RGS. Daniele Rogantini et. al. https://arxiv.org/abs/2602.23255

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Imprints of primordial magnetic fields on the late-time Universe. Jennifer Schober et. al. https://arxiv.org/abs/2602.23263

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Dyson spheres on H-R diagram. Amirnezam Amiri https://arxiv.org/abs/2602.23270