Search arXiv⌕ Search

arXiv · 2610.35998

A High Precision Metacalibration Response Correction

Abstract

In Metacalibration the shear response of a weak lensing measurement is estimated by applying an artificial shear to the image, but the shear operation imprints a spin-2 modulation on the image noise power, which biases the measured response. The standard fix adds a sheared noise field that symmetrizes the anisotropy, at the cost of doubling the noise variance ($\sqrt2$ in the noise). The fusion correction presented in this note reaches the same unbiased response while adding only the minimum power needed. It measures the noise power transfer by passing an impulse through the Metacal process, forms the common-level azimuthal deficit that equalizes the spin-2 ($m{=}2$) and spin-6 ($m{=}6$) modulations across the metacal types, and adds just that deficit by filtering the rotated noise field. The fusion correction raises the per-pixel noise by only $\sim2\%$ for a round PSF (versus $\sqrt2$ for the standard correction), rising toward the $\sqrt2$ level only for highly elliptical PSFs.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Erin S. Sheldon. 2026-10-26. A High Precision Metacalibration Response Correction. https://arxiv.org/abs/2610.35998

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

High-frequency water megamasers as precision probes of black holes, galaxies and cosmology: A case for a next-generation sub-mm/mm interferometer

Water megamasers in the circumnuclear disks of active galactic nuclei are among the most precise probes of supermassive black holes. VLBI imaging of 22 GHz disk masers has provided geometric distances to independently constrain $H_0$, accurate black hole mass measurements, and sub-parsec views of accretion disk geometry. ALMA has opened a new window into water maser transitions in the sub-mm/mm regime, which trace temperatures, densities and disk regions that are inaccessible at 22 GHz, and can be observed at higher spatial resolution and with less free-free absorption. However, current detections are limited to a few bright extragalactic masers in nearby galaxies. We present the case for a next-generation sub-mm/mm interferometer - ALMA2040 - that would open a new parameter space for maser studies. We show that a 10-fold increase in line sensitivity and three times longer baselines compared to ALMA would transform sub-mm maser studies from a few bright detections into a population-level probe, delivering black hole masses and geometric distances from sub-mm masers alone, independent of and complementary to 22 GHz measurements. Integrated into a VLBI array, ALMA2040 would resolve maser disks out to $>$160 Mpc, extend maser black hole masses into the largely untested intermediate-mass regime, reveal magnetic field structure in accretion disks through polarization studies, and test systematics in $H_0$ measurements.

astro-ph.IM↗

von Neumann Stability Analysis of Braginskii MHD: Thermal Conduction, Viscosity, Magnetic Diffusion, and Thermoelectric Effects; and an Implementation in Athena++

Athena++ is a finite-volume astrophysical magnetohydrodynamics (MHD) code. As of writing, isotropic thermal conduction and kinematic viscosity, Ohmic resistivity, and ambipolar diffusion are present in the main branch. Here we present a fork of Athena++, ``Athena-Aniso''. It implements fully anisotropic thermal conduction (parallel, perpendicular, and the Righi--Leduc effect); anisotropic viscosity (all five Braginskii viscosity tensors); the Hall effect; and several thermoelectric effects (Peltier, Seebeck, Nernst, and Ettingshausen). These effects can be weighted by ionisation fraction in a partially ionised gas, with the neutral part diffusing isotropically. We have also added isotropic bulk viscosity. The Biermann battery is not implemented here. The dissipative terms have super-time-stepping support, while the non-dissipative terms are combined with the ideal MHD flux. A CFL condition for all terms is derived and implemented using von Neumann stability analysis. The dissipative terms are found to be stable under first-order time integration. The non-dissipative terms are found to be stable under third-order time integration. We additionally derive new signal speeds for a modified HLLE Riemann solver. These suppress grid-scale non-linear instabilities still present in the non-dissipative terms. The Nernst/Ettingshausen system is found to be ill-posed unless it is stabilised by both perpendicular thermal conduction and perpendicular magnetic diffusion. We derive a well-posedness criterion for this. We provide numerical tests of each implemented effect against derived analytical solutions.

astro-ph.IM↗

Preliminary Goniopolarimetric Simulations for Space Weather Radio (SWARA) Polarimeter

Goniopolarimetry is a technique that measures the direction-of-arrival (DoA) using the polarization properties of the incident electromagnetic (EM) waves. This study aims to incorporate the technique of Goniopolarimetry for our proposed polarimeter, Space Weather Radio (SWARA) Polarimeter, to provide early warnings for space weather or solar events. We have performed preliminary simulations for a tri-monopole antenna configuration. The behaviour of the tri-monopole antenna with varying signal-to-noise (SNR) ratios along the field-of-view (FOV) was investigated using simulations. The angular localization error (ALE) variations, along with SNRs, were simulated to quantify the sensitivity of the Goniopolarimetric algorithm to galactic background noise. Future work will focus on determining the optimum effective length of the individual monopoles to maximize sensitivity and localization accuracy while ensuring efficient impedance matching with the receiver. The optimized antenna will be evaluated under realistic plasma environments through electromagnetic and plasma simulations to investigate the influence of plasma parameters.

astro-ph.IM↗