PROTOCALC, a W-band Polarized Calibrator for Cosmic Microwave Background Telescopes: Application to Simons Observatory and CLASS

Gabriele Coppi, Nadia Dachlythra, Federico Nati, Rolando Dünner-Planella, Alexandre E. Adler, Josquin Errard, Nicholas Galitzki, Yunyang Li, Matthew A. Petroff, Sara M. Simon, Ema Tsang King Sang, Amalia Villarrubia Aguilar, Edward J. Wollack, Mario Zannoni
The Astrophysical Journal Supplement Series
279,
30
(2025)
Open access
Protocalc paper first page
Coppi et al. (2025)
The Astrophysical Journal Supplement Series 279, 30

Research overview

This paper presents PROTOCALC, a drone-borne polarized calibration source operating in the W-band (~90 GHz) to address the scarcity of bright, naturally polarized celestial calibrators. High-precision polarization angle calibration is essential for cosmic microwave background (CMB) telescopes searching for primordial B-modes and cosmic birefringence. The 1.75 kg payload—mounted on a DJI Matrice 600 Pro drone—integrates an RF synthesizer and multiplier chain, a wire-grid polarizer, and a photogrammetry camera tracking ground targets for attitude determination. Laboratory characterization demonstrated optical alignment accuracy better than 0.01°, while field deployments in the Atacama Desert targeting the CLASS and Simons Observatory telescopes achieved a mean roll-angle reconstruction accuracy of 0.045°, validating the system’s potential for next-generation CMB experiments such as CMB-S4.

Key findings

  • W-band source
  • ~90 GHz operating region
  • drone deployment
  • optical alignment accuracy better than 0.01°

Role of the Purewavepolarizers wire-grid polarizer in PROTOCALC

A calibrated, linearly polarized W-band source for cosmic background telescopes

PROTOCALC Layout Schematic

In the instrument

Why it was needed

PROTOCALC uses a controlled linearly polarized W-band source to calibrate the polarization angle of cosmic microwave background telescopes. The wire-grid polarizer defines the polarization state of the emitted radiation, providing the known polarization reference required for the calibration measurement.

Coppi et al.,
2025

Publication details

Journal

The Astrophysical Journal Supplement Series

Volume

279

Issue

1

Article

30

Published

2025

Research area

Space Sensing and Astrophysics

Application

W-band polarization calibration for CMB telescopes

Licence

CC BY 4.0

Institution

University of Milano-Bicocca / INFN

DOI