Quantitative Bayesian inference using a deep-learning emulator detects 0.018-0.020 M_sun of helium in the Type Ic supernova 2014L.
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18 Pith papers cite this work. Polarity classification is still indexing.
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A low-redshift-agnostic BAO compression applied to DESI data yields binned constraints on dark-energy density evolution X(z) that are consistent with a constant value.
Retrievals on 22 cool brown dwarfs from JWST data yield VMRs for H2O, CH4, CO and other species, metallicities, masses, radii, and ages of 0.4-10 Gyr, with systematic differences from Elf-Owl thermal profiles.
New upper limits on gravitational-wave amplitude, ellipticity below 4e-7 for fast spins, and crustal anisotropy below 5e-3 for 1.3-100 ms periods from Cas A, Vela Jr., and G347.3-0.5, plus one surviving candidate.
Multi-epoch ALMA data on 22 massive protoclusters show five variable sources out of 383 condensations (1.3% lower limit), including one hypercompact H II region with a 68% peak intensity rise over one year.
Dynamical traceback of 16 low-mass associations shows most originated from larger complexes or feedback-driven bubbles, with one possibly from an intermediate-velocity cloud collision in Orion.
XRISM Resolve data on NGC 4151 favor relativistic reflection from an inner disk at r ~ 3 GM/c², Compton scattering from dust in the BLR/torus, and a spectrum of warm, fast, and ultra-fast outflows with constraints on their properties and potential feedback.
Inverse velocity arrival in solar energetic particle events results from magnetic connectivity shifting from weak flanks to stronger apex regions of evolving CME-driven shocks.
JWST data on ISO-Oph 37 show hydrocarbon-enhanced molecular absorption in a stratified disk wind, attributed to early pebble drift and soot-line processing of carbonaceous grains.
Hybrid FLI-SBI framework maps shear fields directly to cosmological parameters, achieving ~2x FoM versus convergence-based inference and 36.4% gain over shear two-point statistics on mock catalogs.
XSNAP provides a unified pipeline for X-ray supernova analysis and derives a progenitor mass-loss rate of (6.2±0.2)×10^{-5} solar masses per year for SN 2024ggi assuming a 20 km/s wind.
NOEMA CO(2-1) data show a nuclear molecular outflow in NGC 3079 offset by 14 pc with velocities -350 to -450 km/s, mass outflow rate 8.82 M_sun/yr, kinetic power 3.8e41 erg/s, and momentum rate 15 times the AGN radiation momentum, indicating an energy-driven jet-powered outflow.
Convolutional neural networks can infer galaxy cluster virial masses and scale radii from 2D projected position and line-of-sight velocity distributions with nearly unbiased results and reduced scatter when richness is added or training is limited to relaxed systems.
Hybrid neural network predicts eruptive versus confined solar flares from SDO/HMI magnetogram sequences, reports good performance, and links results to magnetic flux cancellation in polarity inversion lines.
LightCurveLynx is a flexible forward-modeling tool that produces supernova light-curve simulations matching ZTF observations with low KL divergence and consistent completeness limits.
Observations of Snake III demonstrate that molecular cloud density and early feedback jointly regulate the sequence of star formation, with older clusters in cavities and young stars forming in dense regions.
Systematic search of ZTF DR23 data yields catalogs of 28,504 coarse and 1,984 refined AGN flares with public release.
Simulations indicate LISA could statistically distinguish CDM from SIDM (constant 1 cm²/g cross-section) with at least ~70 high-SNR massive black hole merger detections.
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Molecular Outflows in the Nucleus of the Nearby Compton-thick AGN NGC 3079
NOEMA CO(2-1) data show a nuclear molecular outflow in NGC 3079 offset by 14 pc with velocities -350 to -450 km/s, mass outflow rate 8.82 M_sun/yr, kinetic power 3.8e41 erg/s, and momentum rate 15 times the AGN radiation momentum, indicating an energy-driven jet-powered outflow.