Revised planet brightness temperatures using the Planck/LFI 2018 data release
Michele Maris, Erik Romelli, Maurizio Tomasi, Anna Gregorio, Maura, Sandri, Samuele Galeotta, Daniele Tavagnacco, Marco Frailis, Gianmarco, Maggio, Andrea Zacchei

TL;DR
This paper provides revised brightness temperature estimates for planets Jupiter, Saturn, Uranus, and Neptune using Planck/LFI 2018 data, improving previous measurements and comparing results with other observations and models.
Contribution
It introduces new, more accurate brightness temperature measurements for planets based on Planck/LFI 2018 data, extending prior work and systematic analysis methods.
Findings
Jupiter's brightness temperatures at 30, 44, 70 GHz are 144.9, 159.8, 170.5 K.
Saturn's disc brightness temperatures are approximately 140-150 K across frequencies.
Results are consistent with WMAP and existing planetary microwave emission models.
Abstract
We present new estimates of the brightness temperatures of Jupiter, Saturn, Uranus, and Neptune based on the measurements carried in 2009--2013 by PLANCK/LFI at 30, 44, and 70 GHz and released to the public in 2018. This work extends the results presented in the 2013 and 2015 PLANCK/LFI Calibration Papers, based on the data acquired in 2009--2011. PLANCK observed each planet up to eight times during the nominal mission. We processed time-ordered data from the 22 LFI radiometers to derive planet antenna temperatures for each planet and transit. We accounted for the beam shape, radiometer bandpasses, and several systematic effects. We compared our results with the results from the ninth year of WMAP, PLANCK/HFI observations, and existing data and models for planetary microwave emissivity. For Jupiter, we obtain Tb = 144.9, 159.8, 170.5 K (+/- 0.2 K at 1 sigma, with temperatures expressed…
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