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| 20180815_sevem_model90 [2018/08/15 11:30] – barreiro | 20180815_sevem_model90 [2018/08/15 11:34] (current) – barreiro | ||
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| SEVEM results on model 90.00, no delensing | SEVEM results on model 90.00, no delensing | ||
| - | We have produced cleaned frequency maps at 62, 75, 90, 108, 155 and 186 GHz for the simple 90.00 model (homogeneous foregrounds over the sky) using template fitting. We have considered the simulation number 0000, with no delensing. | + | We have produced cleaned frequency maps at 62, 75, 90, 108, 155 and 186 GHz for the simple 90.00 model (homogeneous foregrounds over the sky) produced by Clem using template fitting. We have considered the simulation number 0000, with no delensing. |
| The different frequency maps can be used to obtain directly the auto-spectrum or for cross-correlation between them. | The different frequency maps can be used to obtain directly the auto-spectrum or for cross-correlation between them. | ||
| The noise, synchrotron and dust components have also been propagated through the pipeline. We have also propagated the tensor component provided with the simulations. | The noise, synchrotron and dust components have also been propagated through the pipeline. We have also propagated the tensor component provided with the simulations. | ||