ASCL.net

Astrophysics Source Code Library

Making codes discoverable since 1999

ASCL Code Record

[ascl:2106.023] so_noise_models: Simons Observatory N(ell) noise models

so_noise_models is the N(ell) noise curve projection code for the Simons Observatory. The code, written in pure Python, consists of several independent sub-modules, representing each version of the noise code. The usage of the models can vary substantially from version to version. The package also includes demo code that that demonstrates usage of the noise models, such as by producing noise curve plots, effective noise power spectra for SO LAT component-separated CMB T, E, B, and Compton-y maps, and lensing noise curves from SO LAT component-separated CMB T, E, B maps.

Code site:
https://github.com/simonsobs/so_noise_models
Used in:
https://ui.adsabs.harvard.edu/abs/2021arXiv210603846S
Described in:
https://ui.adsabs.harvard.edu/abs/2019JCAP...02..056A
Bibcode:
2021ascl.soft06023S

Views: 332

ascl:2106.023
Add this shield to your page
Copy the above HTML to add this shield to your code's website.