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Moon and Jupiter over the small dome
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RSS  Latest preprints on astro-ph:

› Advanced System Engineering Approaches to Emerging Challenges in Planetary and Deep-Space Exploration
› Velocity Reconstruction from KSZ: Measuring $f_{NL}$ with ACT and DESILS
› Synergies between Euclid, Roman and JWST Could Reveal Quasars at up to $z \sim$ 15
› Optical Strong Line Ratios Cannot Distinguish Between Stellar Populations and Accreting Black Holes at High Ionization Parameters and Low Metallicities
› TDCOSMO XXIII. First spatially resolved kinematics of the lens galaxy obtained using JWST-NIRSpec to improve time-delay cosmography
› A Demonstration of Interstellar Navigation Using New Horizons
› Resupplying planetary debris to old white dwarfs with supernova blast waves
› REBELS-MOSFIRE: Weak CIII] Emission is Typical Among Extremely UV-bright, Massive Galaxies at $z\sim7$
› Lensing Without Borders: Measurements of galaxy-galaxy lensing and projected galaxy clustering in DESI DR1
› Spectral evolution of GX 17+2 using AstroSat and NICER observations
› KSZ Velocity Reconstruction with ACT and DESI-LS using a Tomographic QML Power Spectrum Estimator
› CANUCS/Technicolor Data Release 1: Imaging, Photometry, Slit Spectroscopy, and Stellar Population Parameters
› Impact of magnetic field-driven anisotropies on the equation of state probed in neutron star mergers
› The Growth and Decay of Individual Sunspots and Pores
› A Statistical Approach to Quantifying Uncertainty in Meteoroid Physical Properties
› AGN with massive black holes have closer galactic neighbors: k-Nearest-Neighbor statistics of an unbiased sample of AGN at z~0.03
› Kinematic misalignment as a driver of black hole activity in galaxies with external interactions
› Constraining the Faint-End Slope of the FRB Energy Function Using CHIME/FRB Catalog-1 and Local Volume Galaxies
› Apache Point Observatory follow-up of ACcelerating Candidate ExopLanet host Stars (APO ACCELS): Ages for 166 Accelerating Stars in the Northern Hemisphere
› Astrometric Accelerations of Provisional Targets for the Habitable Worlds Observatory
› Detecting Land with Reflected Light Spectroscopy to Rule Out Waterworld O2 Biosignature False Positives
› BASS. XLIV. Morphological preferences of local hard X-ray selected AGN
› Towards an Observational Detection of Halo Spin Bias using Spin-Orbit Coherence
› A Comprehensive Multiwavelength Study of the OH Megamaser galaxy IRAS 09320+6134
› Spectroscopic Analysis of Pictor II: a very low metallicity ultra-faint dwarf galaxy bound to the Large Magellanic Cloud
› Decoding AGN Feedback with X-arithmetic: From Morphology to Physical Mechanisms
› Probing the peak of star formation with the stochastic background of binary black hole mergers
› Quantifying Radio Source Morphology
› A Statistical Analysis of Magnetic Parameters in Solar Source Regions of Halo-CMEs with and without SEP events
› Filters for NIR astronomical photometry: comparison of commercial IRWG filters and designs using OpenFilters
› A search of periodic variable stars in the LMC by JWST photometry
› Updated constraints on Regge-Teitelboim gravity
› Jet precession in gamma-ray bursts: The roles of fallback accretion and disk dynamics
› The NIKA2 cosmological legacy survey at 2 mm: catalogs, colors, redshift distributions, and implications for deep surveys
› Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys
› The dynamical lineage of ultra-diffuse galaxies from TNG50-1
› HOLISMOKES XVIII: Detecting strongly lensed SNe Ia from time series of multi-band LSST-like imaging data
› Infrared Variability of Carbon Stars in the LMC Observed with NEOWISE-R
› Stationary quasi-periodic pulsations in 20-second cadence TESS flares
› JADES reveals a large population of low mass black holes at high redshift
› Stretch to stretch, dust to dust: low-value local $H_{0}$ measurement from two-population modelling of type Ia supernovae
› Spins of SMBHs in distant low luminosity AGNs
› Requirements on bandpass resolution and measurement precision for LiteBIRD
› Euclid preparation. Full-shape modelling of 2-point and 3-point correlation functions in real space
› A pipeline to search for signatures of line-of-sight acceleration in gravitational wave signals produced by compact binary coalescences
› Revision of conservative lower bound on intergalactic magnetic field from Fermi and Cherenkov telescope observations of extreme blazars
› Cool Gas in the Circumgalactic Medium of Massive Post Starburst Galaxies
› Constraining the Stellar-to-Halo Mass Relation with Galaxy Clustering and Weak Lensing from DES Year 3 Data
› Cosmography with DESI DR2 and SN data
› Modeling the Mass Distribution and Gravitational Potential of Nearby Disk Galaxies: Implications for the ISM Dynamical Equilibrium
› MeerKAT radio continuum imaging of nearby star-forming spirals in the NGC 6221, NGC 3256/3263, and NGC 2434 galaxy groups
› Forecasting constraints on quintessential inflation from future generation of galaxy and CMB surveys
› Cost Effective Designs For Next-Generation Radio Telescopes
› A high stellar multiplicity rate amongst TESS planet candidates in the Neptunian desert using Gaia DR3 astrometry
› NuSTAR and XMM-Newton Observations of PSR J1930+1852 and Its Pulsar Wind Nebula
› Cosmology from Planck CMB Lensing and DESI DR1 Quasar Tomography
› Gravitational redshift from large-scale structure: nonlinearities, anti-symmetries, and the dipole
› Glitches far from transient gravitational-wave events do not bias inference
› Energetic ($< 2$ MeV) Ion Environment of the Magnetosphere as measured by ASPEX-STEPS on board Aditya-L1 during its earth-bound phase
› Constraint on the Deviation of Kerr Metric via Bumpy Parameterization and Particle Swarm Optimization in Extreme Mass-Ratio Inspirals
› A Common Origin of Asymmetric Self-interacting Dark Matter and Dirac Leptogenesis
› The eROSITA DR1 variability catalogue
› Structural response of neutron stars to rapid rotation and its impact on the braking index
› The Atacama Cosmology Telescope: A census of bridges between galaxy clusters
› Characterising the z $\sim$ 7.66 Type-II AGN candidate SMACS S06355 using BEAGLE-AGN and JWST NIRSpec/NIRCam
› A revisited Correction to the Halo Mass Function for local-type Primordial non-Gaussianity
› Phase Space of Binary Black Holes from Gravitational Wave Observations to Unveil its Formation History
› The Dependence of Dark Matter Halo Properties on the Morphology of Their Central Galaxies from Weak Lensing
› The [C II] line emission as an interstellar medium probe in the MARIGOLD galaxies
› Is the formation of primordial black holes from single-field inflation compatible with standard cosmology?
› Rapid follow-up observations of infant supernovae with the Gran Telescopio Canarias
› Deep source separation of overlapping gravitational-wave signals and non-stationary noise artifacts
› Multiwavelength Analysis of GRB 250101A: From Gamma-ray Prompt Emission to Optical Afterglow
› To detect strong nugget with an acoustic array
› Rapid inference and comparison of gravitational-wave population models with neural variational posteriors
› Millimeter emission from supermassive black hole coronae
› On the Efficacy of Ocean Formation with a Primordial Hydrogen Atmosphere
› The Orbit of WASP-4 b is in Decay
› The Vela pulsar and its pulsar wind nebula Vela-X using 13 years of Fermi-LAT Observations
› Systematic Biases from ARM-Based Sensitivity and Imaging in Compton Cameras
› Understanding the Drag Torque in Common Envelope Evolution
› Non-Gaussian statistics in galaxy weak lensing: compressed three-point correlations and cosmological forecasts
› The MALATANG survey: Dense gas distribution on sub-kiloparsec scales across the disk of M82
› Blowing star formation away in AGN Hosts (BAH) -- III: Feeding and feedback in 3C 293 observed with JWST NIRSpec
› Deterministic and Stochastic Study of the X-ray Emission from the TeV Blazar Mrk~421
› The Kaleidoscope Survey: Strong Gravitational Lensing in Galaxy Clusters with Radial Arcs
› Triple-$\alpha$ reaction rates below $T_9=3$ by a non-adiabatic three-body model
› Null Stream Based Third-generation-ready Glitch Mitigation for Gravitational Wave Measurements
› Two simple photon gauges in inflation

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