JWST spectra of SN 2024abup show CO, C, O, and Mg features plus possible dust emission, with no clear r-process signatures identified via SUMO modeling.
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J., Hilker M., Baumgardt H., C \^o t \'e P., Grebel E
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- background provide an internal consistency test of GR through independent waveform reconstruction and binary parameter estimation. Future work could extend the LILA selection function presented in this paper to make astrophysical predictions, such as expected LILA detection rates and redshift evolution of black hole merger rates, using semi-analytical models (e.g., Volonteri et al. 2008; Barausse 2012; Pacucci & Ferrara 2015; Valiante et al. 2018; Dayal et al. 2019; Sassano et al. 2021; Trinca et al. 2023;
- background 2020, 2021a; Pellejero Ibañez et al. 2023; Zennaro et al. 2023; Contreras et al. 2023a; Ortega- Martinez et al. 2024). Each emulator can vary the SHAMe-SF parameters, cosmological parameters (σ8,Ω m,Ω b,n s,handM ν), redshift, and number density simultaneously within the follow- ing ranges for the SHAMe-SF parameters: β∈[0,20] γ∈[−10,25] ∆γ∈[−10,10] V1 ∈[10 1.2,10 3.5] (km/s) ∆V1 ∈[10 0.2,10 1.9] (km/s) σ∈[0,1.7] fk,(cen+sat)/2 ∈[−1,1] fk,(cen−sat)/2 ∈[−1,1] α0 ∈[0,8] αexp ∈[−8,8] (4) Mcrit ∈[9,
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FRTSearch: Unified Detection and Parameter Inference of Fast Radio Transients using Instance Segmentation
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The Milky Way Tomography with Subaru Hyper Suprime-Cam: Implications for the past orbit of the Large Magellanic Cloud
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Tracing Active Galactic Nuclei Properties Through a Changing-look Event
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The Role of Baryonic and Dark Matter in Bar Kinematics
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Something Bright at the Edge of Everything: A Uniquely JWST-Dark Radio Source in COSMOS
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The Structure and Evolution of LRDs: Insights from JWST NIRSpec Medium and High Resolution Spectroscopy at $z\sim4$
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The MASSIVE SURVEY XXI: Local Variations in the Stellar Initial Mass Function of MASSIVE Early-Type Galaxies
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Planet-Planet Secular Migration Predicts a Stellar Obliquity-Period Anti-Correlation
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Dynamical Tides during High-Eccentricity Migration produces the Hot Jupiter Pile-up, Neptune Ridge, and Neptune Desert
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A Consistent Comparison of Intracluster Light Assembly in Simulations I. Redshift Evolution and Progenitor Galaxies
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The impact of evolving cosmic filaments on mass and spin evolution of dark matter halos
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A New Methodology for Classifying Eclipsing Binaries with Kepler Data and Deep Learning
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PHANTOM: A MATLAB and Octave Toolbox Connecting Linear Field Statistics to Dark Matter Halo Observables
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Direct Optical Evidence of Late-Stage Infall in AB Aurigae: A Stagnant [O I] Reservoir and a Crushed Magnetosphere
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The Contribution of Disrupted Dense Star Clusters to Gaia's Compact Object Binaries
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Consistency of DES and DESI distances and the Standard Cosmological Model
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MeV Gamma-Ray Lines from Radioactive Nuclei in Magnetar Giant Flares
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Tracing the very early disruption of the Sagittarius dwarf galaxy in the distant Milky Way halo
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A fast spectral-multigrid Poisson solver in non-Cartesian geometries
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