A Physically Motivated Compact Parameterization of Neutron Star Atmosphere Emission for Thermal X-ray Pulse-Profile Modeling

Kavli Affiliate: Renxin Xu | Summary:Thermal X-ray pulse-profile modeling depends on the angular and spectral properties of neutron star atmosphere emission. We construct a compact empirical approximation to the specific intensity using eight coefficients for the angular dependence and five for a normalized spectral kernel. The angular prescription is motivated by the formal solution of […]


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Cauchy-Combined Hettmansperger-Randles Location Tests in High Dimensions

Kavli Affiliate: Feng Long| Summary: High-dimensional mean testing is challenging under strong dependence and heavy tails, since classical Hotelling statistics are ill posed and regularized versions based on sample moments remain sensitive to outliers. This paper develops a robust regularized Hotelling framework for one-sample mean inference under elliptical distributions. The proposed HRST statistic combines a […]


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PyCC: A Reference Quantum Chemistry Python Package for Education, Validation, and Rapid Prototyping

Kavli Affiliate: Thomas Crawford | Summary:PyCC is a Python-based quantum chemistry package that emphasizes coupled cluster and related methods. Developed over the last five years, PyCC’s purpose is to provide a clear reference implementation that will serve as a validation suite for production code, a platform for rapid prototyping and testing of new methods, and […]


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SCALES. II. The Internal Composition of Giant Star-Forming Clumps at $z = 1 – 4$

Kavli Affiliate: Luis Ho | Summary:Star-forming structures of scale $sim0.5-1,mathrmkpc$, dubbed ‘giant’ star-forming clumps, are routinely detected in unlensed surveys of $z > 1$ galaxies. Two scenarios are usually invoked to explain their existence — genuine physical structures or resolution-driven artifacts — yet distinguishing between them requires characterizing their internal structure. In this work, part […]


Continue.. SCALES. II. The Internal Composition of Giant Star-Forming Clumps at $z = 1 – 4$

SCALES. I. Bridging Lensed Clump – Giant Clump Scales in Lensed Galaxies at $z=1-4$

Kavli Affiliate: Luis Ho | Summary:Dense star-forming regions in $z>1$ galaxies, often termed ‘clumps’, have been studied across two distinct regimes of telescope resolution, each motivating interpretations in tension with the other. In the SCALES series (Star-Forming Clumps As Layered Emergent Structures), we aim to connect star-forming structures across scales, from the $sim100,mathrmpc$ clumps in […]


Continue.. SCALES. I. Bridging Lensed Clump – Giant Clump Scales in Lensed Galaxies at $z=1-4$

Distinguishing the origin of cosmic birefringence: dark energy, dark matter, and neutrino asymmetry

Kavli Affiliate: Eiichiro Komatsu | Summary:Cosmic birefringence, the isotropic rotation of the plane of linear polarization of photons from sources at cosmological distances, can be generated by different parity-violating mechanisms. While the net rotation angle of a single polarized source carries little information about its physical origin, sources at various redshifts $z$ can be used […]


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A Refined Analytic Oblate–Schwarzschild Model for Thermal X-Ray Pulse Profiles of Rotating Neutron Stars

Kavli Affiliate: Renxin Xu | Summary:Thermal X-ray pulse profiles constrain neutron-star masses and radii through the effects of gravitational light bending and rotation on surface emission. The precision anticipated from the enhanced X-ray Timing and Polarimetry (eXTP) mission motivates more accurate analytic light-bending formulae that retain the efficiency needed for repeated model evaluations. We derive […]


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Which Milky Way Streams Make the Best Dark Matter Detectors?

Kavli Affiliate: Risa Wechsler | Summary:The abundance and properties of low-mass dark matter subhalos can be inferred by measuring the density and velocity structure of stellar streams, testing physical models of dark matter. Which streams make the most promising dark matter detectors, and which subhalos would they encounter? We use the semi-analytic model galacticus to […]


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Interpreting the High-Recoil LUX-ZEPLIN Event with Bino-/Singlino-like and Higgsino Dark Matter

Kavli Affiliate: Carlos Wagner | Summary:The LUX-ZEPLIN (LZ) experiment has recently reported a nuclear-recoil candidate at $E_Rsimeq248$ keV. We study two supersymmetric interpretations based on distinct neutralino couplings to the $Z$ boson. In the elastic case, a bino- or singlino-like neutralino scatters through a diagonal axial $Z$ coupling set by the Higgsino asymmetry $X=|N_13|^2-|N_14|^2$ rather […]


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Improved Constraints on Cosmic Microwave Background Circular Polarization with CLASS

Kavli Affiliate: Jeffrey McMahon | Summary:We present improved constraints on circular polarization in the cosmic microwave background (CMB) from the Cosmology Large Angular Scale Surveyor (CLASS) experiment using data at 90, 150, and 220 GHz to complement previous results based on 40 GHz data alone. We extend constraints on circular polarization from the atmosphere to […]


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