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<blockquote style="position: relative; padding-left: 55px;"><section><a href="https://astrodon.social/users/kellylepo/statuses/113853738127238484">Kelly Lepo (kellylepo@astrodon.social)'s status on Tuesday, 21-Jan-2025 01:35:06 JST</a><a href="https://astrodon.social/@kellylepo" title="kellylepo@astrodon.social"><img src="https://gnusocial.jp/avatar/28639-48-20221116180105.webp" width="48" height="48" alt="Kelly Lepo" style="position: absolute; left: 0; top: 0;">Kelly Lepo</a><div><a href="https://astrodon.social/@kellylepo/113853113397103289" rel="in-reply-to">in reply to</a></div></section><article><p>Next up the Heineman Prize Lecture at <a href="https://astrodon.social/tags/AAS245" rel="tag">#AAS245</a> by John Carlstrom: Past, Present, and Future Cosmic Microwave Background Surveys.</p><p>I took an intro astronomy course from Carlstrom as an undergrad, so it was cool to see him up on the stage!</p></article><footer><a rel="bookmark" href="https://gnusocial.jp/conversation/4411031#notice-8629063">In conversation</a><time datetime="2025-01-21T01:35:06+09:00" title="Tuesday, 21-Jan-2025 01:35:06 JST">about 4 months ago</time> <span>from <span><a href="https://astrodon.social/@kellylepo/113853738127238484" rel="external" title="Sent from astrodon.social via ActivityPub">astrodon.social</a></span></span><a href="https://astrodon.social/@kellylepo/113853738127238484">permalink</a><h4>Attachments</h4><ol><li><label><a rel="external" href="https://gnusocial.jp/attachment/3968302">A bit about this talk and me
About talk: Want to give you a sense of the trajectory of Cosmic Microwave Background (CMB) measurements and results, from one experimentalist's (mine) perspective. So, biased towards my past, present and future.
About me: Started by helping to build and
using Hat Creek mm-wave interferometer to study star formation. Then to Caltech using the OVRO interferometer and linking CSO and JCMT telescopes as a submm interferometer to measure protostellar disks, but I was a closet cosmologist...
Was intrigued with exploiting the stability of interferometry to study the CMB.</a></label><br><a href="https://media.astrodon.social/media_attachments/files/113/853/192/444/374/922/original/29b0526de3de8bff.png" rel="external">https://media.astrodon.social/media_attachments/files/113/853/192/444/374/922/original/29b0526de3de8bff.png</a></li></ol></footer></blockquote>

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Kelly Lepo (kellylepo@astrodon.social)'s status on Tuesday, 21-Jan-2025 01:35:06 JST Kelly Lepo
in reply to
Next up the Heineman Prize Lecture at #AAS245 by John Carlstrom: Past, Present, and Future Cosmic Microwave Background Surveys.
I took an intro astronomy course from Carlstrom as an undergrad, so it was cool to see him up on the stage!
In conversationabout 4 months ago from astrodon.socialpermalink
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1. A bit about this talk and me About talk: Want to give you a sense of the trajectory of Cosmic Microwave Background (CMB) measurements and results, from one experimentalist's (mine) perspective. So, biased towards my past, present and future. About me: Started by helping to build and using Hat Creek mm-wave interferometer to study star formation. Then to Caltech using the OVRO interferometer and linking CSO and JCMT telescopes as a submm interferometer to measure protostellar disks, but I was a closet cosmologist... Was intrigued with exploiting the stability of interferometry to study the CMB.
  https://media.astrodon.social/media_attachments/files/113/853/192/444/374/922/original/29b0526de3de8bff.png

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