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On the first day of CMBmas, the observatory Had a low PWV Telescopes like us are inconvenienced by water in the atmosphere emitting/blocking microwaves (same reason why a microwave heats food well). Luckily, the #Atacama desert has one of the lowest Precipitable Water Vapour amounts Earth.

On the second day of CMBmas, my telescope gave to me: Two optical designs 🔭🧪 and a low PWV We are fielding both refractors and a reflector in the Atacama Desert, (see our two previous threads for explainers!) bsky.app/profile/simo... bsky.app/profile/simo... Image credit: Elle Shaw

Simons Observatory@simonsobservatory.org

As we are putting the finishing touches on our Large Aperture Telescope 🔭, now might be a good time to explain what science goals it serves. The problem is that there are many to choose from! (Image credit: Mark Devlin) 1/8

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On the third day of CMBmas, my telescope gave to me: Three working SATs 🔭 Two optical designs and a low PWV Last winter, we fixed a cracked lens in one of our Small Aperture Telescopes. We put it back on its' platform and it's now scanning the sky again. (Timelapse made by Josh Borrow, UPenn)

On the fourth day of CMBmas, my telescope gave to me: Four Stokes components Three working SATs 🔭 Two optics designs and a low PWV Any light can be decomposed into the four so-called Stokes parameters: total intensity I, two linear polarizations Q and U, and circular V. SO measures I, Q and U.