Searcharxiv⌕ Search

arXiv · 2610.41586

HWP-synchronous signal induced by misalignment of the sapphire crystal axis

Abstract

We investigate the optical response of a rotating sapphire half-wave plate (HWP) with optic axis misalignment, defined as a deviation of the optic axis from the ideal a-cut orientation. We extend the transfer-matrix formalism for calculating the modulated transmittance of multi-layer wave plates with optic axis misalignment and oblique incidence. Using this formalism, we compute the modulated response of a rotating HWP with an optic axis misalignment to linearly polarized incident light. We experimentally validate the model at 90 GHz using sapphire wave plates with intentionally introduced optic axis misalignments of up to 30 degrees. Additional even harmonics are observed for oblique incidence and optic axis misalignment, with odd harmonics appearing when both effects are present. The measured modulation signals are in good agreement with the model predictions. We also evaluate the potential impact of a illustrative small optic axis misalignment of 3 degrees on precision polarimetry. For the configuration considered, the model predicts odd-harmonic amplitudes at the percent level for a single-layer HWP and up to 8% at individual frequencies for a five-layer achromatic HWP.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Yurika Hoshino, Ryota Takaku, Tomotake Matsumura, Yuki Sakurai, Nobuhiko Katayama, Makoto Tashiro, Yukikatsu Terada, Kosuke Sato, Satoru Katsuda, Tommaso Ghigna, Kunimoto Komatsu, Shinya Sugiyama. 2026-10-30. HWP-synchronous signal induced by misalignment of the sapphire crystal axis. https://arxiv.org/abs/2610.41586

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

KEEP EXPLORING

Related papers

Geometrical and Optical Design of the GUEST Laser-Ranged Test Masses for the Detection of Gravitational Waves in the $μ$Hz range

The GUEST (Gravitational Universe Exploration with Satellite Tracking) mission aims at detecting gravitational waves in the yet almost unexplored $μ$Hz frequency range through high-precision orbital tracking. The unprecedented scientific objectives of this experiment demand equally advanced optical solutions: the highly eccentric orbit imposes dual measurement regimes; a low-velocity, long-range scenario at apogee and a high-velocity, short-range scenario at perigee. The substantial disparity between these conditions is addressed through a novel optical architecture incorporating two distinct types of Corner-Cube Retroreflectors (CCRs) with 1" and 2" apertures (CCR1 and CCR2, respectively). The proposed layout has been designed to ensure isotropy and homogeneity of the optical response while maintaining efficient packing over the spherical surface of the spacecraft. The resulting Optical Cross-Section (OCS) has been evaluated using a custom reduced-order model, which captures the behavior of individual CCRs under varying illumination conditions. This model has been calibrated by reconstructing the optical response of the LARES-2 satellite and has enabled a detailed assessment of the contributions of each CCR type along the GUEST orbit. Finally, sensitivity analyses have been conducted to investigate the impact of key design parameters, including the ratio between CCR types, laser wavelength, spacecraft diameter, Dihedral Angle Offsets (DAOs), and mechanical configurations.

astro-ph.IM↗

COSMIO: A Benchmark for Cross-Survey Modality Imputation

Large-scale astronomical surveys define a heterogeneous, partially observed multi-survey learning setting: each object is observed by only a subset of surveys, while survey observations differ in resolutions, wavelength coverage, noise characteristics, and footprints. This setting gives rise to a natural machine learning problem: given observations of an object in some surveys, how to infer its appearance in other surveys. We formalize this as the problem of cross-survey modality imputation and introduce COSMIO, a multi-survey benchmark of aligned observations obtained by forward-rendered shared astrophysical scenes across LSST, Euclid, and Roman under survey-specific instrument characteristics. The benchmark enables systematic evaluation of imputation across source-target survey combinations and missing-survey patterns. We evaluate a broad range of machine learning methods for imputation, which reveal a clear domain gap: methods developed for existing imputation settings transfer poorly to the survey setting. We identify rare-event imputation as a central challenge. This regime arises in the early stages of new surveys, when rare but scientifically valuable phenomena may be available only from prior surveys. We use strong gravitational lensing, where light from a background galaxy is gravitationally deflected by a foreground galaxy, as a representative rare-event setting. We evaluate model performance on zero-shot imputation of gravitational lenses and on downstream scientific tasks using the imputed lens observations. On our constructed evaluation set of galaxy-galaxy strong lenses, performance degrades under rare-event distribution shift, and this degradation further propagates to the downstream lens-detection task. Code: https://github.com/fw-ic/COSMIO.

astro-ph.IM↗

Photometric calibration of the 4m ILMT data

The International Liquid Mirror Telescope (ILMT) is a 4-meter survey telescope continuously observing towards the zenith in the SDSS g', r', and i' bands. This survey telescope is designed to detect various astrophysical transients (for example, supernovae) and very faint objects like multiply-imaged quasars and low surface brightness galaxies. Ensuring accurate and stable calibration of supernova (SN) and quasar measurements is essential for studying their intrinsic variability and long-term brightness evolution. In this work, we present a dedicated calibration approach tailored for ILMT point-like object observations obtained in Time Delayed Integration (TDI) mode. Using ZTF reference sources cross-matched with the Pan-STARRS1 catalog, we derive robust photometric zero-points along the ILMT scan. This calibration procedure enables the production of consistent, high-precision SN and quasar light curves, suitable for variability studies, structure-function analysis, and future reverberation-mapping applications.

astro-ph.IM↗