{"id":1008,"date":"2020-05-19T12:48:07","date_gmt":"2020-05-19T16:48:07","guid":{"rendered":"https:\/\/sites.krieger.jhu.edu\/class\/?page_id=1008"},"modified":"2025-06-13T09:11:37","modified_gmt":"2025-06-13T13:11:37","slug":"code","status":"publish","type":"page","link":"https:\/\/sites.krieger.jhu.edu\/class\/more\/code\/","title":{"rendered":"Code"},"content":{"rendered":"\n<ul class=\"wp-block-list\">\n<li><strong><a href=\"https:\/\/doi.org\/10.5281\/zenodo.15579119\" target=\"_blank\" rel=\"noreferrer noopener\">CMB large scale anomalies code<\/a><\/strong>: A Python package for computing various large-scale anomaly estimators in Cosmic Microwave Background (CMB) data as described in\u00a0<a href=\"https:\/\/doi.org\/10.3847\/1538-4357\/acb339\" target=\"_blank\" rel=\"noreferrer noopener\">Testing Cosmic Microwave Background Anomalies in E-mode Polarization with Current and Future Data (Shi et al. 2023)<\/a>. It includes tools for analyzing (1) Lack of correlation, (2) Quadrupole-Octupole alignment, (3) Odd-parity asymmetry, and (4) Hemispherical power asymmetry.<br><\/li>\n\n\n\n<li><strong><a href=\"https:\/\/doi.org\/10.5281\/zenodo.3526651\">Polarized millimeter-wave atmospheric emission model code<\/a><\/strong>: This code serves as a supplement to the paper titled <em><a href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/1538-4357\/ab64e2\" target=\"_blank\" rel=\"noreferrer noopener\">Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: A First Detection of Atmospheric Circular Polarization at Q Band<\/a><\/em>. It simulates millimeter-wave atmospheric emission, including polarization. This emission is primarily from molecular oxygen, with emission by water vapor and the dry continuum also considered.<br><\/li>\n\n\n\n<li><strong><a href=\"https:\/\/zenodo.org\/record\/1066548#.XsVL5sZ7n6B\">Clee-fast code<\/a><\/strong>: First release of code that allows for quick interpolation between Cosmic Microwave Background polarized power spectra as a function of scalar fluctuations, tensor fluctuations, and the optical depth to reionization. This code serves as a supplement to the paper titled <em><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2018ApJ...863..121W\/abstract\" target=\"_blank\" rel=\"noreferrer noopener\">A Projected Estimate of the Reionization Optical Depth Using the CLASS Experiment\u2019s Sample Variance Limited E-mode Measurement<\/a><\/em>.  Note: <a href=\"https:\/\/github.com\/pqrs6\/clee_fast\"><strong>clee_fast is also available on Github<\/strong><\/a>.<\/li>\n<\/ul>\n\n\n\n\n","protected":false},"excerpt":{"rendered":"","protected":false},"author":47,"featured_media":0,"parent":1491,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_acf_changed":false,"footnotes":""},"class_list":["post-1008","page","type-page","status-publish","hentry"],"acf":[],"_links":{"self":[{"href":"https:\/\/sites.krieger.jhu.edu\/class\/wp-json\/wp\/v2\/pages\/1008","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=1008"}],"version-history":[{"count":4,"href":"https:\/\/sites.krieger.jhu.edu\/class\/wp-json\/wp\/v2\/pages\/1008\/revisions"}],"predecessor-version":[{"id":1540,"href":"https:\/\/sites.krieger.jhu.edu\/class\/wp-json\/wp\/v2\/pages\/1008\/revisions\/1540"}],"up":[{"embeddable":true,"href":"https:\/\/sites.krieger.jhu.edu\/class\/wp-json\/wp\/v2\/pages\/1491"}],"wp:attachment":[{"href":"https:\/\/sites.krieger.jhu.edu\/class\/wp-json\/wp\/v2\/media?parent=1008"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}