Research profile
Eiichiro Komatsu
Garching, Max Planck Inst.
arXiv endorsement eligibility
arXiv requires established authors to endorse first-time submitters in a subject area. Eligibility depends on papers submitted between three months and five years ago, so it changes over time. These are estimates computed from public arXiv metadata — arXiv does not publish its exact thresholds, and endorsement decisions are private.
Selected publications
First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Determination of cosmological parameters
2003astro-ph10744 citationsarXiv:astro-ph/0302209
Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
2010astro-ph.CO8363 citationsarXiv:1001.4538
Wilkinson Microwave Anisotropy Probe (WMAP) three year results: implications for cosmology
2006astro-ph7573 citationsarXiv:astro-ph/0603449
Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
2012astro-ph.CO5763 citationsarXiv:1212.5226
Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
2008astro-ph5735 citationsarXiv:0803.0547
First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Preliminary maps and basic results
2003astro-ph5027 citationsarXiv:astro-ph/0302207
Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
2012astro-ph.CO2822 citationsarXiv:1212.5225
Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
2008astro-ph1888 citationsarXiv:0803.0586
Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results
2008astro-ph1804 citationsarXiv:0803.0732
Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology associated with the cosmological tensions and anomalies
2022astro-ph.CO · hep-ph1583 citationsarXiv:2203.06142
Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived Parameters
2010astro-ph.CO1571 citationsarXiv:1001.4635
Non-Gaussianity from inflation: Theory and observations
2004astro-ph1359 citationsarXiv:astro-ph/0406398
H0LiCOW – XIII. A 2.4 per cent measurement of H0 from lensed quasars: 5.3σ tension between early- and late-Universe probes
2019astro-ph.CO · astro-ph.GA1354 citationsarXiv:1907.04869
Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Sky Maps, Systematic Errors, and Basic Results
2010astro-ph.CO1315 citationsarXiv:1001.4744
First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Implications for inflation
2003astro-ph1293 citationsarXiv:astro-ph/0302225
Acoustic signatures in the primary microwave background bispectrum
2001astro-ph1144 citationsarXiv:astro-ph/0005036
Three-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: temperature analysis
2006astro-ph1100 citationsarXiv:astro-ph/0603451
Three year Wilkinson Microwave Anisotropy Probe (WMAP) observations: polarization analysis
2006astro-ph1020 citationsarXiv:astro-ph/0603450
First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: The Angular power spectrum
2003astro-ph891 citationsarXiv:astro-ph/0302217
First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: tests of gaussianity
2003astro-ph628 citationsarXiv:astro-ph/0302223
Sources
Identity, affiliation and publication record: INSPIRE-HEP
ORCID: 0000-0002-0136-2404
Endorsement eligibility computed from public arXiv submission metadata.
Last refreshed July 27, 2026.
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