CAMB: Code for Anisotropies in the Microwave Background

By A. Lewis, A. Challinor. 2011

240 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/c6fc523685fb8b3a776cb4b81b442b5d55cc1073

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

1. O. Philcox
2. Mikhail Ivanov
3. A. Mead
4. M. Simonovi'c
5. Catherine Heymans
6. S. Brieden
7. T. Troster
8. M. Zaldarriaga

Citations in the corpus

• Combining full-shape and BAO analyses of galaxy power spectra: a 1.6% CMB-independent constraint on H0 (2020, methodology): “Plin is the linear power spectrum computable via CAMB [69] or CLASS [70].”
• hmcode-2020: improved modelling of non-linear cosmological power spectra with baryonic feedback (2020, methodology): “When fluctuations are small, linear theory allows the power spectrum and its evolution to be calculated analytically – an inflationary powerlaw spectrum of fluctuations is processed by linear electromagnetic and gravitational evolution (e.g., using CAMB of Lewis & Challinor 2011).”