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Every paper Pith has read. Search by title, abstract, or pith.
1109 papers in astro-ph.SR · page 1
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Seismic radius from SOHO and SDO best matches solar size
Sharper Than Ever: Do Modern Observations Pin Down the Solar Radius to Converge on New Standards?
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Gaia benchmark stars gain neutron-capture abundances
Gaia FGK benchmark stars: abundances of \textit{n}-capture elements of the third version
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Low-frequency radio luminosity scales with magnetic field and rotation
GMRT Survey of Radio Emission from Magnetic Massive Stars -- I: Emission from Single Stars at sub-GHz Frequencies
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SEP flux shifts expose magnetic flux tubes in solar wind
Probing Solar Wind Structures with Solar Energetic Particle Observations from Solar Orbiter
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Deep learning finds 13 new substellar candidates in SHINE F150 sample
New substellar candidates identified through deep learning in the F150 sample of the large-scale SHINE direct imaging survey
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Review separates solar abundances into s- and r-process parts
The s- and r- components of the proto-solar composition
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SN 2019vxm light curve traces extreme pre-explosion mass loss
Long-term optical and near-infrared photometric evolution of SN 2019vxm, an interacting Type IIn supernova
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Coronal wave speeds differ over 40% by direction
Investigation of the Two-Dimensional Velocity Field of the Large-Scale Coronal Wave from September 6, 2011 using the SOLERwave Tool
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Stacking detects K-dwarf oscillations with PLATO
Ensemble asteroseismology: An ensemble approach to detecting signatures of solar-like oscillations in K-dwarfs
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Solar radio burst pairs are turbulent echoes
Imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona
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Eccentric brown dwarf near star boundary keeps tilt in old system
TOI-7154b: A Close-in Massive Brown Dwarf in an Eccentric Orbit
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Evolving starspot distorts radial velocities in binary giant
Nature of HD 251108: an RS CVn binary with a long-term evolving spot
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Photon reprocessing boosts stellar dark photon production
Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades
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Most extreme helium stars show stochastic low-frequency variability
TESS Observations of Stochastic Low-frequency Variability in Extreme Helium Stars
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HDBSCAN detects solar active regions with higher sensitivity
An Improved HDBSCAN-based Detection and Tracking Method for Solar Active Regions in Magnetograms
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Little to no mass-ratio reversal in 10 solar mass BBH peak
A Strongly Parametrized Mass Ratio Model for the Stable Mass Transfer Channel: a Case Study of the $10 \, \rm{M}_{\odot}$ Peak
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Gaia plus RV data fix orbits of three wide companions
Gaia Exoplanet Orbits, Demographics, and Evolution Survey (GEODES): Characteristics of Three Long-Period Companions Accelerating their Host Stars
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SDO data lets solar atmosphere be modeled as dynamical system
The Solar Dynamics Observatory in the Living With a Star Era: From Solar Observations to Predictive Heliophysics
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HST UV spectroscopy key to stellar mass loss
The unique capabilities of HST for stellar physics Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars
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3D evolution reshapes rotation and magnetism in pre-collapse stars
The first 3D MHD core-collapse progenitors II: Rotation, magnetic-field amplification, and magnetic topology
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Accretion enlarges water emitting area in planet-forming disks
JWST-DECO: The Impact of Accretion on Mid-Infrared Observable Water in Planet-forming Disks
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3D models show doubled turbulence in pre-supernova oxygen shells
The first 3D MHD core-collapse progenitors I: General properties, convection and nuclear burning
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Phase-locked flares give 16-gauss field on Proxima d
Star-planet interaction in the Proxima system
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3D RT matches Mg II h&k cores to observations better than 1.5D
Mg II h&k spectral line properties computed using 3D radiative transfer in an enhanced network region simulated with the MURaM-ChE code
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Failed common envelopes yield 6-14 solar mass stripped stars
Mergers via failed common envelope as a route towards intermediate-mass stripped stars
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White dwarf in nova YZ Ret spins every 37.7 seconds
A very rapidly rotating white dwarf in nova YZ Reticuli
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Magnetosonic polarization gives field lines (δB/B)^4 diffusion scaling
Polarized 3D Synthetic Turbulence I: Magnetic Field Line Random Walk
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Brown dwarfs 9 percent larger than models predict
Evidence of Radius Inflation Based on 50 Transiting Brown Dwarfs and Low-mass Stellar Companions
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Activity known for 70% of HWO targets but cycles for under 20%
HWO Target Stars and Systems: Activity and Rotation Catalog (ARC) of Potential Target Stars for the Habitable Worlds Observatory
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No polarization detected in radio emission from two wind-colliding binaries
Search for radio polarization in the particle-accelerating colliding-wind binaries WR 147 and HD 167971
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Faculae flip radial velocity from redshift to blueshift past 60 degrees
Decoding the Radial Velocity Signatures of Solar Faculae with 3D MHD Simulations
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X-class flares show iron fluorescence varying by viewing angle
Iron Fluorescence in X-class Solar Flares: Aditya-L1/SoLEXS Observations
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ξ Tau needs 100 s tidal lag and outer binary for best fit
Configuration of the $\xi$ Tau system constrained by multi-technique observations
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Magnetic field of ~4 kG inferred in gamma Doradus star KIC 2309579
Seismic signature of a magnetic field in the $\gamma$ Doradus star KIC 2309579
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Non-equilibrium galaxies top habitability proxy rankings
The habitability trade-off: Chemical decoupling and quenching in massive galaxies
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Reconstruction shows solar irradiance varied by only 1 W/m² over 3000 years
Reconstruction of annual solar irradiance over the last three millennia
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Magnetar fireball models forecast high polarization in short bursts
Magnetar Fireballs and Short Bursts: Curved Spacetime Lensing, QED Effects, High-Energy Spectra and Polarization, and Energy-Time Impulse Responses
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Composite images boost solar prominence detection to 78% recall
A Robust Deep Learning Framework for Prominence Detection through Composite Feature Representations
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LLMs treat stellar spectra as language sequences to estimate parameters
Spectra as Language: Large Language Models for Scalable Stellar Parameter and Abundance Inference
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Language models treat star spectra as text to estimate parameters
Spectra as Language: Large Language Models for Scalable Stellar Parameter and Abundance Inference
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Altair shows normal abundances but slightly subsolar metallicity
Photospheric abundances of the rapidly-rotating A-type star Altair
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Hot subdwarf matches i-process nucleosynthesis
Evidence for neutron capture in heavy-metal hot subdwarfs: Far-UV spectroscopy of EC22536-5304 and LSIV-14 116
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NGC 6791 Dated to 8.46 Billion Years Old
The Absolute Age of the Open Cluster NGC 6791 and Its Implications for Galactic Archaeology and Asteroseismic Calibration
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Low turbulence plus third dredge-up produces rare isotopologue-dominated SiO masers
29SiO and 30SiO J=1--0 maser signatures in Galactic AGB stars: the impact of third dredge up and turbulence velocity
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Iso-dom spectra mark third dredge-up plus low turbulence in AGB stars
29SiO and 30SiO J=1--0 maser signatures in Galactic AGB stars: the impact of third dredge up and turbulence velocity
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Magnetized envelopes around black holes explain little red dots
A Magnetized Black Hole Envelope Model for Little Red Dots
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Mass reversals let lighter stars form heavier black holes
Massquerade: Impacts of Mass Ratio Reversals on Binary Black Hole Merger Rates and Mass Distributions
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Turbulence criterion unifies detonation outcomes in white dwarf explosions
First-Principles Turbulence-Driven Deflagration-to-Detonation Transition Mechanism for Near-Chandrasekhar Mass White Dwarf Progenitors
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Subgiant lithium excess matches planet of 9-95 Earth masses
Lithium Enrichment in a Subgiant Star with a Brown Dwarf Companion: A Planetary Engulfment Candidate
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Icy bodies fission outside white dwarf Roche radii in under 10 years
Producing planetary debris exterior to white dwarf Roche radii through sublimative rotational fission