{"id":2,"date":"2013-09-10T12:19:15","date_gmt":"2013-09-10T12:19:15","guid":{"rendered":"https:\/\/sites.krieger.jhu.edu\/template-research\/?page_id=2"},"modified":"2026-04-22T13:57:45","modified_gmt":"2026-04-22T17:57:45","slug":"sample-page","status":"publish","type":"page","link":"https:\/\/sites.krieger.jhu.edu\/class\/","title":{"rendered":"CLASS"},"content":{"rendered":"\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-8f761849 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\" style=\"flex-basis:52%\">\n<h3 class=\"wp-block-heading\">A Unique View of the Heavens<\/h3>\n\n\n\n<p class=\"wp-block-paragraph\">Welcome to the public website of the Cosmology Large Angular Scale Surveyor (CLASS)! From high atop a mountain in Northern Chile, CLASS uses polarized light from the Big Bang, the cosmic microwave background (CMB), to measure when the first stars lit up the universe, an epoch called cosmic dawn or reionization. Additionally with CLASS we can study our solar system and galaxy as well as better understand results on neutrinos and dark energy. The measurement requires cutting-edge technology and data analysis to detect the faint signal. Students and early-career researchers are the core of the CLASS team and go on to exciting careers in science and technology. This site is a clearinghouse for popular media and professional publications on CLASS as well as data, code, student theses, and educational materials. You can also check out the CLASS team and follow us on&nbsp;<a href=\"https:\/\/x.com\/CLASS_telescope\" target=\"_blank\" rel=\"noreferrer noopener\">X<\/a>&nbsp;or&nbsp;<a href=\"https:\/\/bsky.app\/profile\/classtelescope.org\" target=\"_blank\" rel=\"noreferrer noopener\">Bluesky<\/a>!<\/p>\n<\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\" style=\"flex-basis:48%\">\n<figure class=\"wp-block-image size-large\"><img decoding=\"async\" width=\"1024\" height=\"100\" data-src=\"https:\/\/sites.krieger.jhu.edu\/class\/files\/2025\/06\/white-1024x100.jpg\" alt=\"white space\" class=\"wp-image-1532 lazyload\" data-srcset=\"https:\/\/sites.krieger.jhu.edu\/class\/files\/2025\/06\/white-1024x100.jpg 1024w, https:\/\/sites.krieger.jhu.edu\/class\/files\/2025\/06\/white-300x29.jpg 300w, https:\/\/sites.krieger.jhu.edu\/class\/files\/2025\/06\/white-768x75.jpg 768w, https:\/\/sites.krieger.jhu.edu\/class\/files\/2025\/06\/white.jpg 1190w\" data-sizes=\"(max-width: 1024px) 100vw, 1024px\" src=\"data:image\/svg+xml;base64,PHN2ZyB3aWR0aD0iMSIgaGVpZ2h0PSIxIiB4bWxucz0iaHR0cDovL3d3dy53My5vcmcvMjAwMC9zdmciPjwvc3ZnPg==\" style=\"--smush-placeholder-width: 1024px; --smush-placeholder-aspect-ratio: 1024\/100;\" \/><\/figure>\n\n\n\n<figure class=\"wp-block-image\"><img decoding=\"async\" width=\"1024\" height=\"683\" data-src=\"https:\/\/sites.krieger.jhu.edu\/class\/files\/2025\/06\/class-site-at-night_2019-09-20-Bright1-1024x683.jpeg\" alt=\"CLASS telescopes at night\" class=\"wp-image-1425 lazyload\" data-srcset=\"https:\/\/sites.krieger.jhu.edu\/class\/files\/2025\/06\/class-site-at-night_2019-09-20-Bright1-1024x683.jpeg 1024w, https:\/\/sites.krieger.jhu.edu\/class\/files\/2025\/06\/class-site-at-night_2019-09-20-Bright1-300x200.jpeg 300w, https:\/\/sites.krieger.jhu.edu\/class\/files\/2025\/06\/class-site-at-night_2019-09-20-Bright1-768x512.jpeg 768w, https:\/\/sites.krieger.jhu.edu\/class\/files\/2025\/06\/class-site-at-night_2019-09-20-Bright1-1536x1024.jpeg 1536w, https:\/\/sites.krieger.jhu.edu\/class\/files\/2025\/06\/class-site-at-night_2019-09-20-Bright1-2048x1365.jpeg 2048w\" data-sizes=\"(max-width: 1024px) 100vw, 1024px\" src=\"data:image\/svg+xml;base64,PHN2ZyB3aWR0aD0iMSIgaGVpZ2h0PSIxIiB4bWxucz0iaHR0cDovL3d3dy53My5vcmcvMjAwMC9zdmciPjwvc3ZnPg==\" style=\"--smush-placeholder-width: 1024px; --smush-placeholder-aspect-ratio: 1024\/683;\" \/><figcaption class=\"wp-element-caption\">CLASS telescopes in Chile. Credit Matthew Petroff<\/figcaption><\/figure>\n<\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-8f761849 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\" style=\"flex-basis:50%\">\n<figure class=\"wp-block-image\"><img decoding=\"async\" width=\"1024\" height=\"553\" data-src=\"https:\/\/sites.krieger.jhu.edu\/class\/files\/2025\/06\/xqml_clee_proposal-1024x553.jpg\" alt=\"XQML CEE\" class=\"wp-image-1426 lazyload\" data-srcset=\"https:\/\/sites.krieger.jhu.edu\/class\/files\/2025\/06\/xqml_clee_proposal-1024x553.jpg 1024w, https:\/\/sites.krieger.jhu.edu\/class\/files\/2025\/06\/xqml_clee_proposal-300x162.jpg 300w, https:\/\/sites.krieger.jhu.edu\/class\/files\/2025\/06\/xqml_clee_proposal-768x415.jpg 768w, https:\/\/sites.krieger.jhu.edu\/class\/files\/2025\/06\/xqml_clee_proposal-1536x830.jpg 1536w, https:\/\/sites.krieger.jhu.edu\/class\/files\/2025\/06\/xqml_clee_proposal-2048x1106.jpg 2048w\" data-sizes=\"(max-width: 1024px) 100vw, 1024px\" src=\"data:image\/svg+xml;base64,PHN2ZyB3aWR0aD0iMSIgaGVpZ2h0PSIxIiB4bWxucz0iaHR0cDovL3d3dy53My5vcmcvMjAwMC9zdmciPjwvc3ZnPg==\" style=\"--smush-placeholder-width: 1024px; --smush-placeholder-aspect-ratio: 1024\/553;\" \/><figcaption class=\"wp-element-caption\">CLASS Optical Depth Measurement. Li et al. 2025\u200b<\/figcaption><\/figure>\n<\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\" style=\"flex-basis:50%\">\n<h3 class=\"wp-block-heading\">First CLASS Results on Optical Depth<\/h3>\n\n\n\n<p class=\"wp-block-paragraph\">In early 2025, <a href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/1538-4357\/adc723\" target=\"_blank\" rel=\"noreferrer noopener\">CLASS announced a new measurement<\/a> of the so-called \u201coptical depth to reionization,\u201d the probability that a CMB photon interacts with electrons freed from intergalactic gas by starlight. CLASS data, in combination with data from the Planck and WMAP telescopes, implies an optical depth of \ud835\udf49=0.053+0.018-0.019, consistent with previous measurements. This result will improve with more CLASS data and upgrades to the telescopes!&nbsp;&nbsp;<\/p>\n<\/div>\n<\/div>\n\n\n\n<hr class=\"wp-block-separator has-alpha-channel-opacity\"\/>\n\n\n\n<h2 class=\"wp-block-heading\">Acknowledgments<\/h2>\n\n\n\n<p class=\"wp-block-paragraph\">We acknowledge the National Science Foundation Division of Astronomical Sciences for their support of CLASS under Grant Numbers 0959349, 1429236, 1636634, 1654494, 2034400, 2109311, and 2442928. The CLASS project employs detector technology developed under several NASA grants. Detector development work at JHU was funded by NASA cooperative agreement 80NSSC19M0005. Data analysis for CLASS is conducted at the Advanced Research Computing at Hopkins (ARCH) core facility (rockfish.jhu.edu), which is supported by the National Science Foundation (NSF) grant number OAC1920103. We further acknowledge the very generous support of Jim Murren and Heather Miller (JHU A&amp;S \u201988), Matthew Polk (JHU A&amp;S Physics BS \u201971), David Nicholson, and Michael Bloomberg (JHU Engineering \u201964). CLASS is located in the Parque Astron\u00f3mico Atacama in northern Chile under the auspices of the Agencia Nacional de Investigaci\u00f3n y Desarrollo (ANID).<\/p>\n\n\n\n<p class=\"wp-block-paragraph\"><\/p>\n","protected":false},"excerpt":{"rendered":"<p>A Unique View of the Heavens Welcome to the public website of the Cosmology Large Angular Scale Surveyor (CLASS)! From high atop a mountain in Northern Chile, CLASS uses polarized light from the Big Bang, the cosmic microwave background (CMB), to measure when the first stars lit up the universe, an epoch called cosmic dawn [&hellip;]<\/p>\n","protected":false},"author":47,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_acf_changed":false,"footnotes":""},"class_list":["post-2","page","type-page","status-publish","hentry"],"acf":[],"_links":{"self":[{"href":"https:\/\/sites.krieger.jhu.edu\/class\/wp-json\/wp\/v2\/pages\/2","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/sites.krieger.jhu.edu\/class\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/sites.krieger.jhu.edu\/class\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/sites.krieger.jhu.edu\/class\/wp-json\/wp\/v2\/users\/47"}],"replies":[{"embeddable":true,"href":"https:\/\/sites.krieger.jhu.edu\/class\/wp-json\/wp\/v2\/comments?post=2"}],"version-history":[{"count":5,"href":"https:\/\/sites.krieger.jhu.edu\/class\/wp-json\/wp\/v2\/pages\/2\/revisions"}],"predecessor-version":[{"id":1615,"href":"https:\/\/sites.krieger.jhu.edu\/class\/wp-json\/wp\/v2\/pages\/2\/revisions\/1615"}],"wp:attachment":[{"href":"https:\/\/sites.krieger.jhu.edu\/class\/wp-json\/wp\/v2\/media?parent=2"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}