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Every paper Pith has read. Search by title, abstract, or pith.
1731 papers in astro-ph.GA · page 1
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Uniform parameters derived for 5056 open clusters from Gaia
Astrophysical Parameters of 5056 Open Star Clusters from Bayesian Nested Sampling with PARSEC Isochrones
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Clustering reveals five new inner-halo substructures
Unsupervised Chemo-Dynamical Dissection of the Inner Galactic Halo: Discovery of Five Accreted Substructures with SDSS-V and Gaia
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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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FRIIs rarer in clusters than FRIs at high luminosity
Probing the environments of FRI and FRII radio galaxies in LoTSS DR2 with galaxy clusters
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Li plateaus appear in GSE main-sequence and giant stars
Gaia-Sausage-Enceladus: Lithium evolution from early red-giant-branch and main-sequence stars
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Rayleigh-Taylor instabilities accelerate electrons in Fermi Bubbles
Hydrodynamic model of nonthermal emission from the Fermi bubbles
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Pilot FAST survey detects 34 HI sources per square degree
The FAST Hundred-Deg$^2$ HI Deep (HD$^2$) Survey: Early Results from the Pilot Survey
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Gas fraction and depletion time each drive half the main-sequence scatter at z~1.5
Gas Fraction and Depletion Time Drive the Main-Sequence Scatter in Massive Galaxies at $z\sim1.5$
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GAMA data splits galaxy bimodality into quenching sub-groups
Multi-layered model-based characterisation of the local-Universe galaxy data from the GAMA survey
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Three supernova types share atomic gas preferences
Atomic gas properties at the positions of supernovae Type Ia, II, and Ib/c
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Two-parameter PDFs fit SN Ia extinction better than exponential in 3D simulations
Examining extinction distributions for type Ia supernovae in simulated 3D galaxies
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Local structures shape most polarized microwave sky
A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz
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Spectroscopy traces ω Centauri tidal tails to 3.2 degrees
Disruption of a Giant: Spectroscopic Identification of Members in the Periphery and Tidal Tails of $\omega$ Centauri
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Filaments shrink and distort cold gas discs of low-mass galaxies
Cosmic web stripping and starvation of low-mass filament galaxies in TNG50
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Pressure and quadrupole set disk eccentricity regimes around binaries
Insights from Analytical Theory of Eccentric Circumbinary Disks II. Forced Modes and Resonance for Precessing Binaries
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Void galaxies match denser regions in molecular gas relations
ALMA CO-CAVITY I. Resolved Molecular Gas in Void Galaxies
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Gaia DR4 classifiers reach 88% completeness for bright quasars
Performance analysis of extragalactic classifications in Gaia Data Release 4
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Groups pre-process then protect galaxies from cluster quenching
The dual effect of group-scale environments on galaxy quenching during cluster infall: pre-processing and protection
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Rotation-curve residuals split into mass-dependent linear branches
Rotation-curve residuals reveal a suppressed acceleration branch in dwarf galaxies
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AGN feedback quenches star formation in barred galaxy centers
Suppression of star formation at the centre of barred AGN galaxies
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Dust attenuation stays constant at fixed galaxy mass from z=0 to 7
SDSS+JWST Census of Stellar and Nebular Dust Attenuation at $z \sim 0$-7: Mass Dependence and Redshift Evolution
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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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Clumpy winds drive X-ray variability in I Zwicky 1
Strong X-ray Variability of I Zwicky 1: Obscuration from Clumpy Accretion-Disk Winds
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Outflows turn early galaxies from red to blue
No Blue without Red: Evolutionary Properties of Super-Early Galaxies
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Simulations trace Milky Way's shift from sloshing gas to thick then thin disk
From protogalaxy through thick and thin: Why did the Milky Way evolve in three kinematic phases?
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Solitons cannot have mass-radius index Γ in [0
A No-Go Theorem for the Mass-Radius Relation of Solitons
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Only five of 17 CMZ clouds show mass segregation
Mass Segregation in the CMZoom Survey
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3D map shows cosmic-ray protons with inner Galaxy enhancement
A Three-Dimensional Tomographic Reconstruction of the Galactic Cosmic-Ray Proton Density
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Dwarf galaxies set fermion dark matter mass to 100-300 eV
Dwarf Galaxy Constraints on Interacting Fermionic Dark Matter
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This paper reports a mean velocity difference of about 0.05 km/s between ions traced by…
Probing the ion-neutral drift velocity towards the L1544 prestellar core: Detection of ambipolar diffusion using N$_2$D$^+$ and para-NH$_2$D
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Eccentric binaries near black holes show step-like vZLK shifts
Dynamics of Binary System around a Supermassive Black Hole :Binary Scattering and Eccentric vZLK Oscillations
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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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Shocks link feedback and feeding in Centaurus A nucleus
MICONIC: The multiphase circumnuclear region of Centaurus A as seen with JWST/MIRI MRS observations. I. Spectral inventory and properties of the warm molecular disk
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Weak Fe K beta line in 3C 111 suggests ionized wind absorption
A Weak Fe K$\beta$ Emission Line in the Broad-Line Radio Galaxy 3C 111 Observed with XRISM: An Ionized Wind Absorption Feature?
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Silicate dust shatters at 6 km/s
Silicate cosmic dust grain collisions in the interstellar medium: A molecular dynamics study
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Unified database merges HI curves for 129 dwarf galaxies
A Unified H i Rotation Curve Database for 129 Local Volume Dwarf and Irregular Galaxies
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Blue-tilted running resolves JWST galaxy tension at 1σ
Blue-tilted Runnings and the JWST Early Galaxy Tension
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13-day changes at 100 GHz flag hidden AGN in Antennae
An AGN in the Antennae galaxies ?
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ASKAP maps show jets in 173 of 264 bright southern sources
Powerful Radio Sources in the Southern Sky. IV. Observations of the G4Jy-3CRE Catalog with the Australian Square Kilometre Array Pathfinder
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Four patterns turn Milky Way abundances into continuous paths
Milky Way Mapper decoded abundances -- II: From patterns to paths
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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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Colliding plasma flows form persistent isothermal turbulent layer
Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas
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JADES DR5 supplies stellar parameters for half a million galaxies
JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: stellar population catalogue for galaxies in GOODS-N and GOODS-S
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New tool doubles ultra-diffuse galaxies known in Hydra I
Advancing the detection of low surface brightness galaxies. I. ATTILA: multi-tAsking deTecTIon tool for Lsb gAlaxies
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ML models predict globular clusters rarely host black holes above 100 solar masses
Predicting intermediate-mass black hole formation in star clusters with machine learning
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Group central galaxies deplete molecular gas in under 1.5 Gyr at z~0.3
Molecular gas properties of star-forming brightest group galaxies at $z \sim 0.3$
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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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Pixel variations expose variable stars and carbon stars in galaxy bulges
Decomposing cool stellar populations with H-band spectral fluctuations: Long-period variable stars in NGC 5128 and carbon stars in NGC 5102
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Age-bias correction in supernovae holds after age mapping changes
Still non-accelerating: age-bias correction in supernova cosmology is robust to host-progenitor age mapping
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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