Obserwatorium Astronomiczne na Suhorze Strona główna
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ul. Podchorążych 2, 30-084 Kraków. tel.: (+48 12) 662 6301; fax: (+48 12) 637 2243; Obs. tel.: (+48) 502 113714
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Obserwatorium Astronomiczne na Suhorze

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 Wiadomości z astronet.pl
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RSS  Najnowsze prace na astro-ph:
› Orbital Stability of Closely-Spaced Four-planet Systems
› Exoplanet atmospheres and demographics in the 2040s
› Hedorah, the first yellow supergiant Kaiju star candidate at $z\approx3$ revealed by behind AS1063
› Inferring hemispheric asymmetries of stellar active regions through the information content of astrometric signals
› The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) I: Motivation, sample, data reduction, and results overview
› The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) IX: Gas-driven origin for the continuum arc in the debris disc of HD 121617
› Resonant Scattering of the He I 1.0833$\mu$m Triplet in H II Regions: Emission Spectra
› The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) VIII: A dust arc and non-Keplerian gas kinematics in HD 121617
› The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) IV: CO gas imaging and overview
› Blobs and Blurs: A Citizen Science-Identified Catalog of Diffuse Galaxies in the Fornax Cluster
› Discovery of High X-Ray Polarization from the Neutron Star Low-Mass X-Ray Binary Cyg X-2 in the Horizontal Branch
› The ALMA survey to Resolve exoKuiper belt Substructures (ARKS). X. Interpreting the peculiar dust rings around HD 131835
› Using Astrometry to Break Degeneracies in Stellar Surface Mapping
› Black hole accretion disks with outflows II. Time dependent Green's function solutions in Newtonian gravity
› The impact of attenuation on cosmic-ray chemistry: I. Abundances and chemical calibrators in molecular clouds
› The ALMA survey to Resolve exoKuiper belt Substructures (ARKS): VI. Asymmetries and offsets
› A Multi-Wavelength Study of Comet C/2022 E3 (ZTF): Complementary ALMA and JWST Investigations of Water and Methanol in Cometary Comae
› Einstein Probe discovery of EP J171159.4-333253: an eclipsing neutron star low-mass X-ray binary with clocked bursts
› Increased and Varied Radiation during the Sun's Encounters with Cold Clouds in the last 10 million years
› Habitable Worlds Observatory's Concept and Technology Maturation: Initial Feasibility and Trade Space Exploration
› The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) VII: Optically thick gas with broad CO gaussian local line profiles in the HD 121617 disc
› On the role of gravity, turbulence, and the magnetic field in angular momentum transfer within molecular clouds
› Template-free search for gravitational wave events using coincident anomaly detection
› Quiet, but not silent. The X-ray activity of the Maunder minimum star HD 166620
› Data Mining-Based Cislunar Escape-Family Analysis in The Multi-Body Models
› Prediction of Multi-Wavelength Afterglows Associated with FRB 20200120E and FRB 20201124A
› Possible Multi-band Afterglows of FRB 20171020A and its Implication
› Evidence for 1.01 s Pulsations of the Central Compact Object in the Supernova Remnant RCW 103 with ASCA, XMM-Newton, and NuSTAR
› Captured are circularized: A relativistic treatment of extreme mass ratio inspirals crossing accretion disks
› A Dynamo Confinement Scenario for the Solar Tachocline and its Implications for Spin-down in the Radiative Spreading Regime
› Pushchino Multibeam Pulsar Search. IX. Detection of a minute-long transient on the LPA antenna
› Euclid: Early Release Observations -- The extended stellar component of the IC10 dwarf galaxy
› The identification of new Herbig Ae/Be stars from LAMOST DR7
› Stability of equilibrium points in modified elliptic restricted three-body problem with various perturbation sources
› Interior dynamics of envelopes around disk-embedded planets
› Uncovering the Next Galactic Supernova with the Vera C. Rubin Observatory
› Detection of a Millisecond Periodicity in BATSE Short Gamma-Ray Bursts
› Timing analysis of a sample of five cataclysmic variable candidates observed by the XMM-Newton satellite
› The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) III: The vertical structure of debris disks
› Exploring Superfluid Angular Momentum Reservoir Effect on Pulsar Glitches and Forecasting Next Glitches of the Crab Pulsar
› Discovery of a soft X-ray lag in the tidal disruption event AT2021ehb
› Reconciling the Systemic Kicks of Observed Millisecond Pulsars, Spider Pulsars, and Low-mass X-ray Binaries
› The MAGPI Survey: co-evolution of baryons and dark matter in star-forming disk-like galaxies at $0.1 \lesssim z \lesssim 0.85$
› Unveiling the First O-Type Bloated Star Candidate through ALMA and EVLA Observations
› Revisiting the exoplanet radius valley with host stars from SWEET-Cat
› Updated indicators of oxygen metallicity for high-$z$ galaxies
› Probing Circumstellar Material and Shock Acceleration in Core-Collapse Supernovae with High-Energy Neutrinos
› Modified hadronic interactions in 3-dimensional simulations
› A long-term multiwavelength study of the flat spectrum radio quasar OP 313
› Evidence of energy conversion in weakly collisional plasma during an interplanetary coronal mass ejection
› Observational Signatures of Planetary Tidal Disruption Events Around Solar-Mass Stars
› Nuclear astrophysics
› Not so-dark: High resolution HI imaging of J0139+4328 and identification of an optical counterpart
› Magnetic field detections in massive systems at different stages of interaction
› Analytic Modeling of Tidally Locked Rocky Planet Atmospheres Across Dynamical Regimes
› Clouds and Chemistry Across the Brown Dwarf T-Y Sequence: Insights from JWST Atmospheric Retrievals
› On the accuracy of mass and size measurements of young protoplanetary disks
› The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) V: Comparison between scattered light and thermal emission
› The DESI Transients Survey: Legacy Classifications and Methodology
› LAMOST J113208.06-005052.3 and LAMOST J052957.56+344127.0: two new binaries with a hot white dwarf and a flaring companion star
› PyIRD: A Python-Based Data Reduction Pipeline for Subaru/IRD and REACH
› Rate of Repeating Tidal Disruption Events with 5--19 years interval constrained by CRTS and ZTF
› Optical Continuum Light Curves and Bolometric Energy Estimates of Solar White-light Flares
› Discovery of Multiple Ultra-Broad-Velocity Molecular Features Associated with the W44 Molecular Cloud
› Non-adiabatic Effect on Convective Mode
› The Feasibility of Potentially Hazardous Asteroids Flybys Using Multiple Venus Gravity Assists
› Testing Red Clump Models with the Asteroseismic Binary KIC 10841730
› Classical Be Stars and Classical Be Star Binaries from LAMOST DR12
› Identification of false positive double-lined spectroscopic binaries in LAMOST-MRS data due to moonlight contamination
› Project FOSSO I: Fates of the Known BDs in MS-BD Binaries
› Exploring rotational properties and the YORP effect in asteroid families
› Joint analysis of small-scale galaxy clustering and galaxy--galaxy lensing from BOSS galaxies
› BE Lyncis: An Extremely Eccentric Binary with the Nearest Known Black Hole
› Continuous-Time Modelling of Black Hole Binary Evolution with Neural ODEs
› Tracing cosmic structure with neutral hydrogen after the Epoch of Reionization
› The long-term evolution of Ultra Faint Dwarf Galaxies and observational implications
› Was the Early Universe Quantum? Falsifying Classical Stochastic Inflation
› Simulating the quasi-ballistic regime of a short Gamma-Ray Burst jet
› Antarctic Infrared Binocular Telescope: Early Data Release of observations in the 1.4 {\mu}m water-vapor-absorption band
› BOWIE-ALIGN: Sub-solar C/O ratio and metallicity atmosphere of the misaligned hot Jupiter HAT-P-30b
› Tidal capture and repeating partial tidal disruption events of giant stars
› Simulating radio emission from flickering AGN jets: travelling shocks and hotspot brightening
› MARVEL Analysis of the Measured High-resolution Spectra of CO Isotopologues
› Forecasting Continuum Intensity for Solar Active Region Emergence Prediction using Transformers
› SolARED: Solar Active Region Emergence Dataset for Machine Learning Aided Predictions
› Time variations of the mean magnetic flux in active regions of different magneto-morphological classes
› Toward Reliable Interpretations of Small Exoplanet Compositions: Comparisons and Considerations of Equations of State and Materials Used in Common Rocky Planet Models
› Broadband Variability Analysis of FSRQ PKS\,0402-362 with Indications of Quasi-Periodic Modulation
› Timescales diagnostics for saving viscous and MHD-driven dusty discs from external photoevaporation
› Optomechanical design of the DragonCam microscopic camera
› An efficient model of cosmology dependence in the covariance matrix of the matter power spectrum
› A Newly Identified Degeneracy Keeps the Planetary Interpretation Viable for OGLE-2011-BLG-0950
› The Occurrence Rate of Nearby Planetary Companions to Hot Jupiters
› Testing the Physical Parameter Constraining Power of HCN and HNC with Neural Networks
› Signatures of Black Hole Spin and Plasma Acceleration in Jet Polarimetry II: Off-Axis Jets
› Galaxy transformation across the cosmic web: The influence zone of filaments
› Variability as a new discovery channel for Intermediate-Mass Black Holes in the Time Domain Era
› Multi-Tracer Cross-Correlations of the Unresolved $\gamma$-Ray Sky
› Combined LOFAR-uGMRT analysis of the diffuse radio emission in the massive clusters Abell 773 and Abell 1351
› The ESA Meerkat Asteroid Guard: a monitoring service for imminent impactors
› The DESIRED temperature-metallicity relations in star-forming regions: probing the Galactic radial and azimuthal metallicity distributions
› Locating the missing large-scale emission in the jet of M87* with short EHT baselines
› The odyssey of the black hole low mass X-ray binary GX339-4: Five years of dense multi-wavelength monitoring
› Environment and Gas Fraction in Type-2 AGN versus Non-AGN Galaxies
› Neutrinos from hidden ultraluminous X-ray sources in the Galaxy
› Probing the kinematics of the Local Group with chemically enriched gas in the Hestia simulations
› Turbulence Can Persist in the Inner Regions of Weakly-Ionized Planet Forming Disks
› Discovery of 1H-cyclopent[cd]indene (c-C11H8) in TMC-1 with the QUIJOTE line survey: A new three-ringed polycyclic aromatic hydrocarbon
› Mass density structuring around galaxy formation sites: impact on galaxy basic properties
› A dual tunnel structure for the Einstein Telescope
› Observations with the Southern Connecticut Stellar Interferometer. II. First Three-Telescope Observations and a New Diameter Measurement of Arcturus
› Four Cold Super-Jupiters Revealed by Extended and Complex Microlensing Signals
› The Relationship between Accretion and Ionised Ejection among Young Stellar Objects in the Coronet Cluster
› Magnetic field morphological diagnostics with ALMA in the G327.29 protocluster: VGT versus dust polarization
› Architectures of Exoplanetary Systems. IV: A Multi-planet Model for Reproducing the Radius Valley and Intra-system Size Similarity of Planets around Kepler's FGK Dwarfs
› Initial Investigations of the Outskirts of XLSSC 122
› c-C3H2 deuteration towards prestellar and starless cores in the Perseus Molecular Cloud
› MIU2Net: weak-lensing mass inversion using deep learning with nested U-structures
› Observational Relationship between Spectral Properties of Gamma-ray and X-ray Emissions from Pulsars
› Dynamical Origin of (469219) Kamo`oalewa of Tianwen-2 Mission from the Main-Belt: $\nu_6$ Secular Resonance, Flora Family or 3:1 Resonance with Jupiter
› The R2Pub Telescopes for Surveying: An Overview and Performance Evaluation of the System
› The Structure of an 80 pc Long Massive Filament
› Joint constraints on cosmic birefringence and early dark energy from ACT, Planck, DESI, and PantheonPlus
› HD 26172: an active solar-type subgiant in a close binary system
› Possible time-variable iron-K$\alpha$ emission in the circum-nuclear region of the Circinus galaxy
› The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) II. The radial structure of debris discs
› Three-dimensional properties of a coronal shock and the longitudinal distribution of its related solar energetic particles
› XPE and VLT /FORS2 polarimetry challenge the Seyfert-1.9 classification of MCG-05-23-16
› A jet-gas interaction beyond the host galaxy: detection of a neutral hydrogen outflow at cosmic noon
› SIRIUS: Dark matter cusp evolution in dense dwarf galaxies
› Still Accelerating: Type Ia supernova cosmology is robust to host galaxy age evolution
› Tracing Cosmological Signature with Doppler Lensing: Insights from Cosmological Simulations
› Examination of frequency and scale dependence of CMB hemispherical power asymmetry
› Follow-up of three exocomet-host candidates
› The Characteristic Mass and Energy Conversion Efficiency in the Cusp-Core Transition of Dark Matter Haloes: Implications for Scaling Relations and Supernova feedbacks
› Boxy/Peanut Bulges: Comparative Analysis of EGIPS Galaxies and TNG50 Models
› Prospecting MeerKAT Continuum Data for Enigmatic Radio Sources with Unsupervised Vector-Quantised Variational Autoencoders
› Frequency shift and viewing direction variations in gravitational lensing
› Primitive asteroids in the main belt, Cybele, and Hilda populations from Gaia DR3
› Secular Evolution of PSR J2021+4026: Long-Term {\gamma}-Ray Flux and Spin-Down Variability Beyond State Transitions
› Rotational enhancement and stability of protoquark stars during thermal evolution
› Optimising gravitational-wave sky maps for pulsar timing arrays
› X-ray Analysis and Photon-transport Simulations of SMC X-1: A Warped-disc Origin of the Superorbital Modulation
› Evaluating state-of-the-art cloud quantum computers for quantum neural networks in gravitational waves data analysis
› Discovery and characterisation of two exoplanets orbiting the metal-poor, solar-type star TOI-5788 with TESS, CHEOPS, and HARPS-N
› Unveiling Hidden Clustering: An Unsupervised Machine Learning Study of Repeating FRB 20220912A
› RV$\times$TESS I: Modeling Asteroseismic Signals with Simultaneous Photometry and RVs
› The JEM-EUSO Collaboration: Contributions to the 39th International Cosmic Ray Conference (ICRC2025)
› Accretion flow around Kerr metric in the infra-red limit of asymptotically safe gravity
› Minutes-long soft X-ray prompt emission from a compact object merger
› A multi-wavelength study of the 2025 low state of the intermediate polar BG CMi
› Pre-computed aerosol extinction, scattering and asymmetry grids for scalable atmospheric retrievals
› Dynamical mass of a solar-like oscillator at the main-sequence turnoff from Gaia astrometry & ground-based spectroscopy
› The PAIRS project: a global formation model for planets in binaries. I. Effect of disc truncation on the growth of S-type planets
› The PAIRS project: a global formation model for planets in binaries. II. Gravitational perturbation effects from secondary stars
› The [Fe XIII] Infrared 10747 Angstrom and 10798 Angstrom Lines in Novae
› Probing AGN duty cycle and cluster-driven morphology in a giant episodic radio galaxy
› Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension
› Decoupling of large-scale, adiabatic inflationary perturbations from enhanced small-scale modes at one-loop
› Opportunities in AI/ML for the Rubin LSST Dark Energy Science Collaboration
› A Quenched and Relatively Isolated Dwarf Galaxy in the Local Volume
› Using observations of escaping H/He to constrain the atmospheric composition of sub-Neptunes
› A self-consistent explanation of the MeV line in GRB 221009A unveils a dense circum-stellar medium
› Probing super-heavy dark matter with ultra-high-energy gamma rays
› Stimulated radiation from superradiant scalar cloud in scalar-tensor theory
› The gravitational energy-momentum pseudo-tensor in $f(Q)$ non-metric gravity
› Forbidden dark matter assisted by first-order phase transition and associated gravitational waves
› Revisiting $^7$Be Weak and Radiative Transition Rates in Big Bang Nucleosynthesis: Implications for the Primordial Lithium Problem
› Plasmoid formation via competing lower-hybrid drift and Kelvin-Helmholtz instabilities: A hybrid kinetic-gyrokinetic simulation study
› Lessons Learned from Structural Design and Vibration Testing of 50-kg Microsatellites Deployed from the International Space Station
› Anisotropic Collective Excitations of Bose Gases in Modified Newtonian Dynamics
› System Analysis and Pre-Flight Evaluation of Deployable Solar Panels for 3U CubeSat HOKUSHIN-1
› Report on Earth Observation Missions and Ground Station Management using On-Demand Satellite Operation System
› Baryon-dark matter coincidence in Randall-Sundrum Model
› AMACA: Astronomy education with a Multi-sensory, Accessible, and Circular Approach
› Universal Dense-Matter Trace Anomaly Inferred from Collective Flow in Heavy-Ion Collisions and Global Properties of Neutron Stars
› An upper limit on cosmological chiral gravitational wave background
› AAFIYA: Antenna Analysis in Frequency-domain for Impedance and Yield Assessment
› Cosmological Budget of Entropy from Merging Black Holes
› RNLE: Residual neural likelihood estimation and its application to gravitational-wave astronomy
› Quasi-linear approach of bi-Kappa distributed electrons with dynamic $\kappa$ parameter. EMEC instability
› Influence of Finite-Nuclei Constraints on High-Density Transitions and Neutron Star Properties
› The Cosmic Expansion History from Line-Intensity Mapping
› A User's Guide to Extracting Cosmological Information from Line-Intensity Maps
› JEM-EUSO Collaboration contributions to the 37th International Cosmic Ray Conference
› JEM-EUSO Collaboration contributions to the 38th International Cosmic Ray Conference
› JADES: Rest-frame UV-to-NIR Size Evolution of Massive Quiescent Galaxies from Redshift z=5 to z=0.5
› On the importance of geometry in exoplanet irradiation : Implications for the day-night contrast
› Cosmoglobe DR2. III. Improved modelling of zodiacal light with COBE-DIRBE through global Bayesian analysis
› The compact object of HESS J1731-347 and its implication on neutron star matter
› Halo Spin Depends on The Distance to Large-scale Filament
› The non-linear dynamics of axion inflation: a detailed lattice study
› Bumblebee cosmology: Tests using distance- and time-redshift probes
› Searching for New Physics in Ultradense Environment: a Review on Dark Matter Admixed Neutron Stars
› Revisiting the Galactic Winds in M82 I: the recent starburst and launch of outflow in simulations
› Angular bispectrum of matter number counts in cosmic structures
› Impact of multi-messenger spectral modelling on blazar-neutrino associations
› Galaxies in the Epoch of Reionization Are All Bark and No Bite -- Plenty of Ionizing Photons, Low Escape Fractions
› A black hole in a near-pristine galaxy 700 million years after the Big Bang
› Shape Shifting Light Dark Matter Solitons
› Distinguishing Orbiting and Infalling Dark Matter Particles with Machine Learning
› Hawking Radiation Signatures from Primordial Black Holes Transiting the Inner Solar System: Prospects for Detection
› Euclid: An emulator for baryonic effects on the matter bispectrum
› An Accretion Flare Interpretation for the Ultra-High-Energy Neutrino Event KM3-230213A
› REBELS-MOSFIRE: Weak CIII] Emission is Typical Among Extremely UV-bright, Massive Galaxies at $z\sim7$
› Multimessenger Emission from Very-High-Energy Black Hole-Jet Systems in the Milky Way
› The diffuse supernova neutrino background: an update with modern population synthesis and core-collapse simulations
› Gravitational lensing rarely produces high-mass outliers to the compact binary population
› MIRACLE II: Unveiling the multi-phase gas interplay in the circumnuclear region of NGC 1365 via multi-cloud modeling
› Simulation-based inference with deep ensembles: Evaluating calibration uncertainty and detecting model misspecification
› Optical and near-infrared nebular-phase spectroscopy of SN 2024ggi: constraints on the structure of the inner ejecta, progenitor mass, and dust
› On frequentist confidence intervals in a non-Gaussian regime
› Three-Dimensional Numerical Simulations of Magnetar Crust Quakes
› SISSI: Supernovae in a stratified, shearing interstellar medium. II. Star formation near the Sun is quenched by expansion of the Local Bubble
› A multiwavelength study of the new Galactic center black hole candidate MAXI J1744-294
› A HyperFlash and \'ECLAT view of the local environment and energetics of the repeating FRB 20240619D
› Light curves of time-dependent accretion disk in tidal disruption events
› The impact of cosmic filaments on the abundance of satellite galaxies
› BAO miscalibration cannot rescue late-time solutions to the Hubble tension
› Improved Radiative Transfer Corrections in Helium Emission Lines
› Vision-Based CNN Prediction of Sunspot Numbers from SDO/HMI Images
› Is the high-energy environment of K2-18b special?
› Cavendish experiment with fast radio bursts on cosmological scales
› Strong Evidence for Cosmic Ray-Supported $\sim$L$^{\ast}$ Galaxy Halos via X-ray \& tSZ Constraints
› The selection function of the Gaia DR3 open cluster census
› Binding energy of compact stars and their non-radial oscillations
› Galactic bars and active galactic nucleus fuelling in the second half of cosmic history
› Polarization Diagnostics Applied to Coronal Mass Ejections and the Background Solar Wind
› Limits of self-interacting neutrinos from the BAO and CMB phase shift
› Uncertainties in the production of iron-group nuclides in core-collapse supernovae from Monte Carlo variations of reaction rates
› Euclid Quick Data Release (Q1). Quenching precedes bulge formation in dense environments but follows it in the field
› Artificial Precision Polarization Array: Sensitivity for the axion-like dark matter with clock satellites
› Historical Surveys to Rubin First Look: Absolute Colors of trans-Neptunian objects
› Electron Cyclotron Maser Emission as the Driving Mechanism in Long-Period Radio Transients
› Explosions in the Empty: A Survey of Transients in Local Void Galaxies
› Absorption effects in the expanding Universe: spectral transmittance functions of intergalactic medium for distant sources
› JWST COMPASS: Insights into the Systematic Noise Properties of NIRSpec/G395H From a Uniform Reanalysis of Seven Transmission Spectra
› Connecting Star Formation in the Milky Way and Nearby Galaxies -II. An Observationally Driven Analytical Model for Predicting Cloud-Scale Star Formation Rates
› The Kinematic Properties of T\.ZO Candidate HV 11417 with Gaia DR3
› The art of simulating the early Universe. Part II. Non-canonical cases & gravitational waves
› An Improved Machine Learning Approach for Radio Frequency Interference Mitigation in FAST-SETI Survey Archival Data
› Machine-learning approaches to dispersion measure estimation for fast radio bursts
› A spectroscopically confirmed, strongly lensed, metal-poor Type II supernova at z = 5.13
› Nitrogen enhancement of GN-z11 by metal pollution from supermassive stars
› Triaxial Magnetars as Sources of Fast Radio Bursts
› Constraining the Primordial Black Hole Abundance with Space-Based Detectors
› An eclipsing 8.56 minute orbital period mass-transferring binary
› The drastic impact of Eddington-limit induced mass ejections on massive star populations
› Using 23 Years of ACS/SBC Data to Understand Backgrounds: Explaining & Predicting Background Variations
› The impact of disc photoevaporation on the long-term evolution of giant planets in mean motion resonances
› Radiative Cooling Effects on Plasmoid Formation in Black Hole Accretion Flows with Multiple Magnetic Loops
› KiDS-Legacy: WIMP dark matter constraints from the cross-correlation of weak lensing and Fermi-LAT gamma rays
› Determination of varying speed of light from Black hole
› Strongly Interacting Dark Matter admixed Neutron Stars
› Deflection angle in the strong deflection limit for static and axisymmetric spacetimes: Local curvature, matter fields, and quasinormal modes
› Bumblebee cosmology: The FLRW solution and the CMB temperature anisotropy
› Indirect searches for realistic sub-GeV Dark Matter models
› Discrete Chi-Square Method can model and forecast complex time series
› Bouncing Cosmologies in modified gravity with space time torsion
› Hyperons in Neutron Stars across the observed mass range: Insights from realistic $\Lambda$-N and $\Lambda$-$\Lambda$ interactions within a Microscopic Framework
› Charged particle dynamics in singular spacetimes: hydrogenic mapping and curvature-corrected thermodynamics
› The Nature of Turbulence at Sub-Electron Scales in the Solar Wind
› Anderson self-localization of light in pair plasmas
› Automating Sensor Characterization with Bayesian Optimization
› High Reheating Temperature without Axion Domain Walls
› Implications of $f(R)$ gravity on late-time cosmic structure growth through a complete description of density perturbations
› Conserved Quantities in Expanding G\"odel Cosmology
› Time-dependent flux backgrounds in type IIB supergravity
› Taxonomy of periodic orbits and gravitational waves in a deformed Schwarzschild black hole spacetime
› From the Wavefunction of the Universe to In-In-Correlators: A Perturbative Map to All Orders
› Symmetries of cosmological perturbations: The residual low-multipole ambiguity
› DC response of an interferometer topology with an L-shaped cavity: a tabletop study
› Effects of spontaneous Lorentz Symmetry breaking on Letelier-AdS charged black holes within Kalb-Ramond gravity

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