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 $zgeq 3$

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 […]


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

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

TIC 295741342: A Triply-Eclipsing Triple Star System with a Giant Tertiary

Kavli Affiliate: Saul Rappaport | Summary:We present the discovery and characterization of TIC 295741342, a triply-eclipsing triple star system with a giant tertiary. The eclipsing binary consists of two similar main-sequence stars in a 4.75-day orbit. The binary is in a 412.8-day orbit with the giant tertiary. We found two degenerate solutions for the system: […]


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Optimal mitigation of random telegraph noise for improved photometry at high frame rates

Kavli Affiliate: Gabor Furesz | Summary:Random telegraph noise (RTN) is a major contributor to read noise in many CMOS image sensors considered for astronomical use. While scientific CMOS image sensors deliver lower read noise than traditional charge-coupled devices, mitigating RTN would widen this gap and enable more precise photometry when using the fast readout rates […]


Continue.. Optimal mitigation of random telegraph noise for improved photometry at high frame rates

The Lumina Project: CMB Optical Depth Fluctuations from Patchy Reionization

Kavli Affiliate: Mark Vogelsberger | Summary:Patchy reionization couples the ionized-bubble morphology to the underlying density field, making the CMB Thomson optical depth sensitive to both the global ionization history and anisotropic fluctuations on the sky. Using the large-volume radiation-hydrodynamical Lumina simulation, we compute $τ_rm CMB$ in two ways: (i) from global volume- and mass-weighted ionization […]


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A Wafer-Scale Heterogeneous III-V-on-Silicon Nitride Quantum Photonic Platform

Kavli Affiliate: Nergis Mavalvala | Summary:Heterogeneous integration of gain and strongly nonlinear materials with ultra-low-loss silicon nitride (SiN) photonics offers a route to scalable quantum circuits, but concurrent wafer-scale manufacturability, low interlayer loss, and high performance have been challenging to realize. Here we demonstrate a wafer-scale III-V-on-SiN quantum photonic platform that directly integrates III-V layers […]


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High-Frequency Thermal Noise in Michelson Interferometers

Kavli Affiliate: Lee McCuller | Summary:New experiments are being developed without the background of quantum shot noise to look for weak, high-frequency signals using Michelson interferometers. Since shot noise is no longer the dominant noise source with these readout schemes, it is important to accurately model thermal noise to characterize signals and design more sensitive […]


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Bidirectional Internal Squeezing for Gravitational-Wave Detectors

Kavli Affiliate: Lee McCuller | Summary:We present a bidirectional internal squeezing scheme for gravitational-wave detectors and show that it saturates the lowest known lower bounds on quantum noise from internal optical dissipation. The scheme uses two optical parametric amplification stages inside the signal-extraction cavity that act on intra-cavity fields propagating in opposite directions. Thereby, most […]


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