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From the 14 of 280 papers with an AI index.

most citedSPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field

55 citations

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11 papers · 1 filter

astro-ph.IM2026

Instrumental artifacts in photonic lantern spectroastrometry and their mitigation with PLred

Yoo Jung Kim, Michael P. Fitzgerald, Malena Bloom +10

Spectroastrometry is a powerful spectral-differential technique for probing angular scales below the resolution limit, but it is also well known to be susceptible to instrumental a…

astro-ph.IM2026

Early Exploration of the Scientific Discovery Space for the Habitable Worlds Observatory

Courtney D. Dressing, Danica Adams, Evelyne Alecian +324

The paper summarizes 70 science cases for the proposed NASA Habitable Worlds Observatory, outlining the observational needs across four scientific pillars and detailing required ca…

astro-ph.IM2026

GRAVITY+: reducing non-common-path aberrations for sub-10 μas astrometric accuracy

Quentin Fournier, Guillaume Bourdarot, Frank Eisenhauer +26

GRAVITY is a state-of-the-art instrument for near-infrared astrometric interferometry that routinely achieves astrometric accuracy of 30-100 microarcsecond in its phase-referenced…

astro-ph.IM20263 cited

The MICADO first-light imager for the ELT: first steps of the SCAO system MAIT

Yann Clénet, Eric Gendron, Fabrice Vidal +39

The paper reports on the early manufacturing and integration steps of the single-conjugate adaptive optics (SCAO) module for MICADO, the first-light imager of the Extremely Large T…

astro-ph.IM2026

Thermal Deformation Reduction in High-Power Interferometry with Higher-Order Laser Modes

Liu Tao, Yuhang Zhao, Zong-Hong Zhu +1

Test-mass thermal noise is a limiting noise source for current and next-generation ground-based gravitational-wave observatories. Uniform-intensity higher-order laser beams, includ…

astro-ph.IM2026

Differentiable Forward Modeling for Efficient and Accurate Shear Inference

Ismael Mendoza, Axel Guinot, Matthew R. Becker +6

Forthcoming Stage-IV dark energy optical surveys, such as LSST, have the ambitious goal of measuring cosmological parameters at sub-percent precision. Realizing their full scientif…