Ground diode and on-sky calibration of QUIJOTE-TFGI confirms phase-switch errors near zero and yields Moon refraction index 1.209 at 31 GHz with consistent responsivity results.
L., Larson, D., Weiland, J
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2025 2representative citing papers
Simulations show that combining QUIJOTE-MFI2 with WMAP and Planck reduces synchrotron spectral index uncertainty by a factor of ~10, curvature uncertainty by ~5, and polarization amplitude uncertainty by ~43 in bright regions while cutting 100 GHz residuals by a factor of 6.
citing papers explorer
-
QUIJOTE-TFGI polarization calibration -- Ground characterization and on-sky validation with Tau A and the Moon
Ground diode and on-sky calibration of QUIJOTE-TFGI confirms phase-switch errors near zero and yields Moon refraction index 1.209 at 31 GHz with consistent responsivity results.
-
Forecasting synchrotron spectral parameters with QUIJOTE-MFI2 in combination with Planck and WMAP
Simulations show that combining QUIJOTE-MFI2 with WMAP and Planck reduces synchrotron spectral index uncertainty by a factor of ~10, curvature uncertainty by ~5, and polarization amplitude uncertainty by ~43 in bright regions while cutting 100 GHz residuals by a factor of 6.