Campuses:
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| Both sides previous revisionPrevious revisionNext revision | Previous revision | ||
| datachallenge [2018/01/31 13:22] – [Mission Model] borrill | datachallenge [2018/02/14 17:27] (current) – [Subscribing to this Group's Mailing List] borrill | ||
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| A sky model comprises four elements: | A sky model comprises four elements: | ||
| * Scalar, tensor and non-Gaussian CMB | * Scalar, tensor and non-Gaussian CMB | ||
| - | * Extragalactic foregrounds | + | * Extragalactic foregrounds, including their lensing. |
| * Galactic foregrounds | * Galactic foregrounds | ||
| * Zodiacal emission | * Zodiacal emission | ||
| - | ==Sky Model 0== | ||
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| - | * Unlensed scalar and tensor CMB with zero and non-zero r | ||
| - | * PySM galactic foregrounds including AME, thermal dust, free-free & synchrotron (a2d7f1s3) | ||
| - | * No extragalactic foregrounds or lensing | ||
| - | * No zodiacal emission | ||
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| - | ===== Subscribing to this Group' | ||
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| - | Send e-mail to: \\ | ||
| - | probedatachallenge+subscribe@umn.edu | ||
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| - | The subject and body of the e-mail can be empty. Within minutes you will receive an automated e-mail response asking you to click on a radio button to subscribe. The group' | ||
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| - | __**Important: | ||