SPT-3G D1: Foreground-Robust Lensing Templates for Primordial Gravitational Wave Searches
astro-ph.CO
Submitted: 2026-08-06
Updated: 2026-09-30
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Planck 2018 results. VI. Cosmological parameters
- SPT-3G D1: Maps of the millimeter-wave sky from 2019 and 2020 observations of the SPT-3G Main field
- Cosmic Microwave Background Delensing Revisited: Residual Biases and a Simple Fix
- Internal delensing of Planck CMB temperature and polarization
- Impact of internal-delensing biases on searches for primordial B-modes of CMB polarisation
- The Spectrum of the Extragalactic Far Infrared Background from the COBE Firas Observations
- Large-scale Maps of the Cosmic Infrared Background from Planck
- Large-scale galactic-dust-cleaned cosmic infrared background maps from \textit{Planck} PR4 and HI4PI with \texttt{pyilc}
- Efficient Computation of CMB anisotropies in closed FRW models
- A Measurement of Gravitational Lensing of the Cosmic Microwave Background Using SPT-3G 2018 Data
- A Measurement of the Cosmic Microwave Background Lensing Potential and Power Spectrum from 500 deg$^2$ of SPTpol Temperature and Polarization Data
- Delensing the CMB with the cosmic infrared background: the impact of foregrounds
- CMB-S4: Iterative Internal Delensing and $r$ Constraints
- The Simons Observatory: forecasted constraints on primordial gravitational waves with the expanded array of Small Aperture Telescopes
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