Planck 2015 results: XI. CMB power spectra, likelihoods, and robustness of parameters
- Submitting institution
-
Cardiff University / Prifysgol Caerdydd
- Unit of assessment
- 9 - Physics
- Output identifier
- 96929556
- Type
- D - Journal article
- DOI
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10.1051/0004-6361/201526926
- Title of journal
- Astronomy and Astrophysics
- Article number
- A11
- First page
- -
- Volume
- 594
- Issue
- -
- ISSN
- 0004-6361
- Open access status
- Technical exception
- Month of publication
- September
- Year of publication
- 2016
- URL
-
http://dx.doi.org/10.1051/0004-6361/201526926
- Supplementary information
-
-
- Request cross-referral to
- -
- Output has been delayed by COVID-19
- No
- COVID-19 affected output statement
- -
- Forensic science
- No
- Criminology
- No
- Interdisciplinary
- No
- Number of additional authors
-
222
- Research group(s)
-
I - Astronomy Instrumentation
- Citation count
- 480
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- -
- Author contribution statement
- I led the development and testing of Planck high-multipole likelihoods, and personally developed the Plik_lite code (now standard software used by the community to investigate Planck data, and by Planck to generate simulations for robustness and consistency tests). The comparison between Planck, ACT and SPT in the paper was made using this methodology. I contributed text and plots for Sections 5.6, 5.7.2 and Appendix C6, and generated Fig. 49, one of the key results showing the state-of-the-art of CMB temperature data. I also made Fig. 15, and Plik_lite results are shown in two other figures and reported in the conclusions.
- Non-English
- No
- English abstract
- -
