TOI-2195 A b is an inflated hot Neptune that likely originated as a Jovian planet losing ~90% mass through Roche lobe overflow during EKL-driven high-eccentricity migration triggered by a wide binary companion.
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9 Pith papers cite this work, alongside 34 external citations. Polarity classification is still indexing.
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A Pop III.1-driven early ionization phase at z=20 yields τ=0.087 consistent with pkSZ and Lyα constraints, potentially resolving BAO-CMB tensions on neutrino mass.
DiStash extends FoundationDB into a disaggregated multi-stash transactional KV store supporting inclusive or exclusive configurations across ephemeral and durable storage pools.
Mass-ratio reversal in isolated binaries offers a viable formation path for GW241011-like events under specific stellar-evolution and interaction conditions.
Hardware-software architecture for drone swarms illuminating line drawings mid-air, including Blender add-on, SVG import, and user study validating misalignment tolerance.
Simulated GW–FRB associations show Cosmic Explorer can constrain cosmology and host DM without redshifts, while current LIGO-Virgo cannot.
Evaluation finds Random Subset (RS) superior for small groups (G ≤ 5) and Closest Available Neighbor First (CANF) superior for large groups (G ≥ 10) using synthetic and real point clouds.
Swarical provides a hierarchical localization technique for swarms of Flying Light Specks that achieves state-of-the-art accuracy while running more than twice as fast.
Reproducibility companion paper that supplies artifacts and instructions for replicating the Swarical localization technique for Flying Light Specks drones.
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Discovery of an Inflated Hot Neptune and Its Formation from Jovian Mass Loss
TOI-2195 A b is an inflated hot Neptune that likely originated as a Jovian planet losing ~90% mass through Roche lobe overflow during EKL-driven high-eccentricity migration triggered by a wide binary companion.