We report on the disk-averaged absolute brightness temperatures of Venus measured at four microwave frequency bands with the Cosmology Large Angular Scale Surveyor (CLASS). We measure temperatures of
Additional file 1. Figure S1. Five model spectra including white noise with the RMS of 0.5 erg/s/cm2/sr/cm−1. Other symbols are the same as those in Fig. 1. Figure S2. Standard deviations for the (a)
Data Set Overview The Mars Express (MEX) Radio Science (MaRS) Data Archive is a timeordered collection of raw and partially processed data collected during the MEX Mission to Mars. For more informatio
The ACS-MIR_profiles_reff_kext folder contains the retrieved water ice clouds effective radii (reff) along with the atmospheric extinction (kext) at 3.2μm and 3.4μm below the haze top, retrieved from
With the advent of direct-imaging spectroscopy, the number of spectra from brown dwarfs and extrasolar gas giants is growing rapidly. Many brown dwarfs and extrasolar gas giants...
