The Role of Stellar Spin in Repeating Partial Tidal Disruption Events

Kavli Affiliate: Dheeraj Pasham | Summary:The repeated tidal stripping of a star by a supermassive black hole, known as a repeating partial tidal disruption event (rpTDE), can give rise to a transient that rebrightens months to years after the first outburst. Among the rpTDE candidates so far observed, some exhibit dimmer peak luminosities during each […]


Continue.. The Role of Stellar Spin in Repeating Partial Tidal Disruption Events

Mergers Matter: Gravothermal Collapse in Dwarf Halos with Self-Interacting Dark Matter

Kavli Affiliate: Lina Necib | Summary:Self-Interacting Dark Matter (SIDM) models with large cross sections at relative velocities below $sim100,rm km , s^-1$ can be tested with dwarf galaxy observations. We analyze six dark-matter-only zoom-in $sim10^10,rm M_odot$ halos with diverse assembly histories, adopting a cross section over mass of $σ/m = 70,cm^2 , g^-1$. We find […]


Continue.. Mergers Matter: Gravothermal Collapse in Dwarf Halos with Self-Interacting Dark Matter

The Pan-Pacific Planet Search — IX. A menagerie of companions orbiting evolved stars

Kavli Affiliate: Avi Shporer | Summary:We present resolutions as to the nature of six speculative candidate companions proposed in the final data release of the Pan-Pacific Planet Search, a 6-year radial-velocity survey of 164 southern evolved stars using the now-decommissioned UCLES spectrograph on the 3.9m Anglo-Australian Telescope. New radial-velocity observations, TESS asteroseismology, and Hipparcos-Gaia astrometry […]


Continue.. The Pan-Pacific Planet Search — IX. A menagerie of companions orbiting evolved stars

A Consistent Implementation of Cluster Strong Lensing in Cosmological Simulation Light Cones

Kavli Affiliate: Michael McDonald | Summary:Galaxy cluster strong gravitational lensing plays a central role in precision cosmology, yet robust theoretical predictions have lagged behind an abundance of high-quality strong lensing observations. This shortfall reflects both a mismatch between the geometry of the strong-lensing problem and standard cubic simulation boxes, and the fundamental tension between simulation […]


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The Lumina Project: The Demographics of Active Galactic Nuclei from Quasars to Little Red Dots at $zgeq 3$

Kavli Affiliate: Mark Vogelsberger | Summary:High-redshift active galactic nuclei (AGN) serve as powerful probes of early black-hole growth, galaxy formation, and the evolving intergalactic medium (IGM). In this work, we use Lumina, a cosmological radiation-hydrodynamic simulation spanning the epochs of hydrogen and helium reionization, which combines a large $(500,rm cMpc)^3$ volume with $2times 6000^3$ resolution […]


Continue.. The Lumina Project: The Demographics of Active Galactic Nuclei from Quasars to Little Red Dots at $zgeq 3$

OncoTriad-QA: A Patient-Level Radiology-Pathology-Genomics Benchmark for Pan-Cancer Reasoning

Kavli Affiliate: Michael McDonald | Summary:Cancer diagnosis and characterization require integrating complementary evidence from radiology, pathology, genomics, and clinical metadata. However, most medical large language model (LLM) and vision-language model (VLM) benchmarks focus on isolated modalities or narrow image-text tasks, leaving patient-level oncology assessment across multiple evidence streams largely untested. We introduce OncoTriad-QA, a patient-level […]


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Lithium Enrichment in a Subgiant Star with a Brown Dwarf Companion: A Planetary Engulfment Candidate

Kavli Affiliate: Andrew Vanderburg | Summary:Theoretical models predict that subgiants within a narrow mass regime can retain detectable lithium enrichment signatures from planetary engulfment. We test this prediction using TOI-5882, selected because it occupies this favorable subgiant parameter space and hosts a massive brown dwarf ($22 , M_ rm J$, $P=7.1 ,rm d$) companion capable […]


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Optical Super-orbital Modulation of SMC X-1: Disk Precession and a Revised Pulsar Mass

Kavli Affiliate: Michael Fausnaugh | Summary:The observational determination of the lower limit of neutron star masses is crucial for the physics of core-collapse supernovae. In this light, SMC X-1 is an important object because of its estimated pulsar mass lying near or potentially below the theoretical lower limit. SMC X-1 exhibits a double peaked optical […]


Continue.. Optical Super-orbital Modulation of SMC X-1: Disk Precession and a Revised Pulsar Mass

The emphR-process Alliance: A Bright, Strongly emphR-process-enhanced Extremely Metal-poor Star Observed with GHOST

Kavli Affiliate: Anna Frebel | Summary:We present a detailed chemical-abundance and kinematic analysis of four extremely metal-poor (EMP; [Fe/H] $leq -3.0$) stars identified from textitGaia BP/RP data in our ongoing search for the most primitive stars. This includes a primary target, textitGaia~DR3~2563539603865382656 (hereafter G256353), a strongly $r$-process-enhanced star with [Eu/Fe]~$= +1.20$ and [Ba/Eu]~$= -0.64$. Our […]


Continue.. The emphR-process Alliance: A Bright, Strongly emphR-process-enhanced Extremely Metal-poor Star Observed with GHOST