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astro-ph.IM2024

The Simons Observatory: Design, Integration, and Current Status of Small Aperture Telescopes

Aashrita Mangu, Lance Corbett, Sanah Bhimani +14

The Simons Observatory (SO) is a cosmic microwave background (CMB) survey experiment located in the Atacama Desert in Chile at an elevation of 5200 meters, nominally consisting of…

astro-ph.CO2024

Absolute reference for microwave polarization experiments -- The COSMOCal project and its proof of concept

A. Ritacco, L. Bizzarri, S. Savorgnano +25

The cosmic microwave background (CMB), a remnant of the Big Bang, provides unparalleled insights into the primordial universe, its energy content, and the origin of cosmic structur…

astro-ph.CO2024

Pixel domain implementation of the Minimally Informed CMB MAp foreground Cleaning method

Magdy Morshed, Arianna Rizzieri, Clément Leloup +2

High fidelity separation of astrophysical foreground contributions from the cosmic microwave background (CMB) signal has been recognized as one of the main challenges of modern CMB…

astro-ph.CO2024

Exploration of the polarization angle variability of the Crab Nebula with POLARBEAR and its application to the search for axion-like particles

Shunsuke Adachi, Tylor Adkins, Carlo Baccigalupi +23

The Crab Nebula, also known as Tau A, is a polarized astronomical source at millimeter wavelengths. It has been used as a stable light source for polarization angle calibration in…

astro-ph.CO2024

The Simons Observatory: Combining cross-spectral foreground cleaning with multitracer -mode delensing for improved constraints on inflation

Emilie Hertig, Kevin Wolz, Toshiya Namikawa +16

The Simons Observatory (SO), due to start full science operations in early 2025, aims to set tight constraints on inflationary physics by inferring the tensor-to-scalar ratio f…

astro-ph.CO2024

The Simons Observatory: impact of bandpass, polarization angle and calibration uncertainties on small-scale power spectrum analysis

S. Giardiello, M. Gerbino, L. Pagano +17

We study the effects due to mismatches in passbands, polarization angles, and temperature and polarization calibrations in the context of the upcoming cosmic microwave background e…