Imagen de Portada

Astrophysics Wrapped 2025: Year-in-Review of Every Astrophysics arXiv Paper from 2025

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Lewis, Rommulus Francis, Shah, Hetansh, Alfred, Amruth
Formato:	Preprint
Publicado:	2026
Materias:	Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics Earth and Planetary Astrophysics Astrophysics of Galaxies Solar and Stellar Astrophysics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Nemesis: A Multi-Scale, Multi-Physics Algorithm for Astrophysics
por: Hochart, Erwan, et al.
Publicado: (2026)

The Wide-field Spectroscopic Telescope (WST) Science White Paper
por: Mainieri, Vincenzo, et al.
Publicado: (2024)

The Space-Based Time-Domain Revolution in Astrophysics
por: Huber, Daniel
Publicado: (2025)

KMT-2025-BLG-1314 and KMT-2025-BLG-1392: two microlensing planetary/brown-dwarf candidates analyzed with differentiable code
por: Ren, Haibin, et al.
Publicado: (2026)

Cl+ and HCl+ in Reaction with H2 and Isotopologues: A Glance into H Abstraction and Indirect Exchange at Astrophysical Conditions
por: Jiménez-Redondo, Miguel, et al.
Publicado: (2025)

AtLAST Science Overview Report
por: Booth, Mark, et al.
Publicado: (2024)

The key science drivers for the Atacama Large Aperture Submillimeter Telescope (AtLAST)
por: Booth, Mark, et al.
Publicado: (2024)

The Sound of the Universe: A Resonant Gravitational Instability Driven by Baryon-Dark Matter Relative Drift
por: Shalaby, Mohamad, et al.
Publicado: (2026)

Towards ALMA2040: An update from the European community and invitation to contribute
por: Facchini, Stefano, et al.
Publicado: (2025)

Compilation of Technical Papers on ALMA Receivers
por: Bakx, Tom, et al.
Publicado: (2024)

Hubble Science in the 2030s White Paper: High-Contrast Optical and UV Spectroscopy with HST/STIS
por: Ward-Duong, K., et al.
Publicado: (2026)

Comission Femmes et Astronomie de la SF2A : Women participation in french astronomy 2025
por: Lagarde, N., et al.
Publicado: (2025)

Systematic Reanalysis of KMTNet microlensing events, Paper I: Updates of the Photometry Pipeline and a New Planet Candidate
por: Yang, Hongjing, et al.
Publicado: (2023)

Written in the Stars: How your (pens and) papers decide the fate of the arXiverse
por: Tan, Joanne
Publicado: (2025)

Gaia22dkvLb: A Microlensing Planet Potentially Accessible to Radial-Velocity Characterization
por: Wu, Zexuan, et al.
Publicado: (2023)

High-temperature dust formation in carbon-rich astrophysical environments
por: Libourel, Guy, et al.
Publicado: (2024)

Probing the origins. I. Generalised Additive Model inference of birth radii for Milky Way stars in the solar vicinity
por: Dantas, M. L. L., et al.
Publicado: (2025)

A Fast, Analytic Empirical Model of the Gaia Data Release 3 Astrometric Orbit Catalog Selection Function
por: Lam, Casey Y., et al.
Publicado: (2024)

Ariel stellar characterisation III. Fast rotators and new FGK stars in the Ariel Mission Candidate Sample
por: Tsantaki, M., et al.
Publicado: (2025)

Dynamical Constraints on a Population of Massive Interstellar Objects
por: Trivedi, Oem, et al.
Publicado: (2025)

The Prime Focus Infrared Microlensing Experiment (PRIME): First Results
por: Sumi, Takahiro, et al.
Publicado: (2025)

Searching for Extragalactic Exoplanets: A Survey of the Sagittarius Dwarf Galaxy Stream with TESS
por: Schap, William, et al.
Publicado: (2026)

Astrometric Radial Velocities from the Hipparcos-Gaia Catalog of Accelerations and Implications for Astrometric Acceleration Measurements
por: Brandt, Timothy D
Publicado: (2026)

Closeby Habitable Exoplanet Survey (CHES). II. An Observation Strategy for the Target Stars
por: Tan, Dongjie, et al.
Publicado: (2024)

Searching for Exoplanets Born Outside the Milky Way: VOYAGERS Survey Design
por: Aloisi, Robert, et al.
Publicado: (2025)

Planet-Host Stars Across the Galaxy in the 2040s
por: Tsantaki, M., et al.
Publicado: (2026)

The HITRAN2024 methane update
por: Bertin, T., et al.
Publicado: (2025)

Mining the Kepler Field: Atmospheric Parameters, Bolometric Corrections, and Luminosities
por: Godoy-Rivera, Diego, et al.
Publicado: (2026)

A Characterization of JWST MIRI Detector Persistence and Implications for High-Contrast Imaging
por: Vasan, Alisha, et al.
Publicado: (2025)

Twinkle: A GPU-based binary-lens microlensing code with contour integration method
por: Wang, Suwei, et al.
Publicado: (2025)

First Calculations of Starspot Spectra based on 3D Radiative Magnetohydrodynamics Simulations
por: Smitha, H. N., et al.
Publicado: (2024)

Identifying new high-confidence polluted white dwarf candidates using Gaia XP spectra and Self-Organizing Maps
por: Pérez-Couto, Xabier, et al.
Publicado: (2024)

Contour Analysis Tool: an interactive tool for background and morphology analysis
por: Hutchison, Mark A., et al.
Publicado: (2024)

paired: A Statistical Framework for Detecting Stellar Binarity with Gaia RVs. I. Sensitivity to Unresolved Binaries
por: Chance, Quadry, et al.
Publicado: (2022)

The Basic Iterative Deconvolution: A fast instrumental point-spread function deconvolution method that corrects for light that is scattered out of the field of view of a detector
por: Hofmeister, Stefan Johann
Publicado: (2023)

The UV Legacy Library of Young Stars as Essential Standards (ULLYSES) Large Director's Discretionary Program with Hubble. I. Goals, Design, and Initial Results
por: Roman-Duval, Julia, et al.
Publicado: (2025)

Multidimensional half-moment multigroup radiative transfer. Improving moment-based thermal models of circumstellar disks
por: Fuksman, David Melon, et al.
Publicado: (2025)

microJAX: A Differentiable Framework for Microlensing Modeling with GPU-Accelerated Image-Centered Ray Shooting
por: Miyazaki, Shota, et al.
Publicado: (2025)

Identification of new nearby white dwarfs using Gaia DR3
por: Golovin, Alex, et al.
Publicado: (2023)

Verification of astrometrically accelerating stars from Hipparcos and Gaia: I. Methodology and application to HIP 44842
por: Makarov, Valeri V., et al.
Publicado: (2024)