Cosmic microwave background lensing reconstruction on the full sky
By T. Okamoto, Wayne Hu. 2003
261 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/c445e1b60d32f9755588cec2eda618027da7ea86
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
- S. Vagnozzi
- D. Baumann
- V. Poulin
- Julien Lesgourgues
- M. Zaldarriaga
- Juan García-Bellido
- E. di Valentino
- Guido D'Amico
Citations in the corpus
- A MEASUREMENT OF GRAVITATIONAL LENSING OF THE MICROWAVE BACKGROUND USING SOUTH POLE TELESCOPE DATA (2012, methodology): “However, Feng et al. (2011) recently applied the optimal quadratic estimator of Hu (2001b); Okamoto & Hu (2003) to the WMAP7 maps, finding no significant signal.”
- Robust forecasts on fundamental physics from the foreground-obscured, gravitationally-lensed CMB polarization (2015, background): “In the CMB×CMB case, the noise on this estimate is [28]”
- Exploring cosmic origins with CORE: Inflation (2016, methodology): “As an estimate for the noise spectrum NPP ` of the CMB lensing potential, we consider the EB estimator [192] as in [168].”
- SIMULATIONS OF THE MICROWAVE SKY (2009, background): “By studying the lensing distortions in the microwave sky, we should also be able to reconstruct the projected matter distribution or the deflection field in the Universe (Hu & Okamoto 2002; Okamoto & Hu 2003; Hirata & Seljak 2003; Yoo & Zaldarriaga 2008).”