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researcher

D. Larson

6 papers hereh-index 44k citations6 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author3

Across the 4 of 6 papers where every author was matched, so the position is known.

fields
  • astro-ph3
  • astro-ph.CO2
  • astro-ph.GA1
same name
  • D. Larson — 36 papers, h 50
  • D. Larson — 27 papers, h 28
  • D. Larson — 23 papers, h 22
  • D. Larson — 22 papers, h 18
  • D. Larson — 15 papers, h 27
  • D. Larson — 11 papers, h 3

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20082014
most citedFive-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation

5.7k citations · 8.5k across the 6 of their papers we have counts for

collaborators
Showing 2008Show all

3 papers · 1 filter

astro-ph2008★ 125 cited

Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Bayesian Estimation of CMB Polarization Maps

J. Dunkley, D. N. Spergel, E. Komatsu +17

We describe a sampling method to estimate the polarized CMB signal from observed maps of the sky. We use a Metropolis-within-Gibbs algorithm to estimate the polarized CMB map, cont…

astro-ph2008★ 1.8k cited

Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results

G. Hinshaw, J. L. Weiland, R. S. Hill +18

We present new full-sky temperature and polarization maps in five frequency bands from 23 to 94 GHz, based on data from the first five years of the WMAP sky survey. The five-year m…

astro-ph2008★ 5.7k cited

Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation

E. Komatsu, J. Dunkley, M. R. Nolta +16

(Abridged) The WMAP 5-year data strongly limit deviations from the minimal LCDM model. We constrain the physics of inflation via Gaussianity, adiabaticity, the power spectrum shape…

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