The DOI matches its Crossref record; 101 of the 101 references it cites were found in a registry or an index.
First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Preliminary Maps and Basic Results
Open accessAbstract
We present full sky microwave maps in five frequency bands (23 to 94 GHz) from the WMAP first year sky survey. Calibration errors are less than 0.5% and the low systematic error level is well specified. The cosmic microwave background (CMB) is separated from the foregrounds using multifrequency data. The sky maps are consistent with the 7 in. full-width at half-maximum (FWHM) Cosmic Background Explorer (COBE) maps. We report more precise, but consistent, dipole and quadrupole values. The CMB anisotropy obeys Gaussian statistics with -58 less than f(sub NL) less than 134 (95% CL). The 2 less than or = l less than or = 900 anisotropy power spectrum is cosmic variance limited for l less than 354 with a signal-to-noise ratio greater than 1 per mode to l = 658. The temperature-polarization cross-power spectrum reveals both acoustic features and a large angle correlation from reionization. The optical depth of reionization is tau = 0.17 +/- 0.04, which implies a reionization epoch of t(sub r) = 180(sup +220, sub -80) Myr (95% CL) after the Big Bang at a redshift of z(sub r) = 20(sup +10, sub -9) (95% CL) for a range of ionization scenarios. This early reionization is incompatible with the presence of a significant warm dark matter density. A best-fit cosmological model to the CMB and other measures of large scale structure works remarkably well with only a few parameters. The age of the best-fit universe is t(sub 0) = 13.7 +/- 0.2 Gyr old. Decoupling was t(sub dec) = 379(sup +8, sub -7)kyr after the Big Bang at a redshift of z(sub dec) = 1089 +/- 1. The thickness of the decoupling surface was Delta(sub z(sub dec)) = 195 +/- 2. The matter density of the universe is Omega(sub m)h(sup 2) = 0.135(sup +0.008, sub -0.009) the baryon density is Omega(sub b)h(sup 2) = 0.0224 +/- 0.0009, and the total mass-energy of the universe is Omega(sub tot) = 1.02 +/- 0.02. There is progressively less fluctuation power on smaller scales, from WMAP to fine scale CMB measurements to galaxies and finally to the Ly-alpha forest. This is accounted for with a running spectral index, significant at the approx. 2(sigma) level. The spectral index of scalar fluctuations is fit as n(sub s) = 0.93 +/-0.03 at wavenumber k(sub o) = 0.05/Mpc ((sub eff) approx. = 700), with a slope of dn(sub s)/d I(sub nk) = -0.031(sup + 0.016, sub -0.018) in the best-fit model.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
The source backs part of the claim, not all of it — or backs it for a different population, condition or comparison.
In the citing paper
“This is the only free input parameter that enters in nucleosynthesis calculations of the primordial abundance of light elements[12, 13].”
From Phase Transitions in the Early and Present Universe (2006) · cites this paper as [12]
Experimental — accuracy not yet measuredThe cited source says what the claim attributes to it.
In the citing paper
“This is in good agreement with observations [12, 13].”
From Phase Transitions in the Early and Present Universe (2006) · cites this paper as [12]
The check wasn’t confident either way, so it gives no verdict — never disputed.
In the citing paper
“These quark nuggets could contribute to the dark matter today [95] or affect BBN [12, 13].”
From Phase Transitions in the Early and Present Universe (2006) · cites this paper as [12]
Experimental — accuracy not yet measured
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
Schlegel, D. J., Finkbeiner, D. P., & Davis, M. (1998) · The Astrophysical Journal · doi:10.1086/305772 · Cited by 15,126
Spergel, D. N., Verde, L., Peiris, H. V., Komatsu, E., Nolta, M. R., Bennett, C. L., Halpern, M., Hinshaw, G., Jarosik, N., Kogut, A., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377226 · Cited by 10,976
Self-citationFinal Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
Freedman, W. L., Madore, B. F., Gibson, B. K., Ferrarese, L., Kelson, D. D., Sakai, S., Mould, J. R., Robert C. Kennicutt, Jr., Ford, H. C., Graham, J. A., et al. (2001) · The Astrophysical Journal · doi:10.1086/320638 · Cited by 3,543
A Measurement of Excess Antenna Temperature at 4080 Mc/s.
Penzias, A. A., & Wilson, R. W. (1965) · The Astrophysical Journal · doi:10.1086/148307 · Cited by 2,606
Structure in the COBE differential microwave radiometer first-year maps
Smoot, G. F., Bennett, C. L., Kogut, A., WRIGHT, E. L., Aymon, J., Boggess, N. W., Cheng, E. S., Amici, G. D., Gulkis, S. L., Hauser, M. G., et al. (1992) · The Astrophysical Journal · doi:10.1086/186504 · Cited by 2,595
Self-citationObservational Evidence for Self-Interacting Cold Dark Matter
Spergel, D. N., & Steinhardt, P. J. (2000) · Physical Review Letters · doi:10.1103/physrevlett.84.3760 · Cited by 2,097
Self-citationHanany, S., Ade, P. A. R., Balbi, A., Bock, J. J., Borrill, J., Boscaleri, A., de Bernardis, P., Ferreira, P. G., Hristov, V. V., Jaffe, A. H., et al. (2000) · The Astrophysical Journal · doi:10.1086/317322 · Cited by 1,317
Four-Year [ITAL]COBE[/ITAL] DMR Cosmic Microwave Background Observations: Maps and Basic Results
Bennett, C. L., Banday, A. J., Gorski, K. M., Hinshaw, G. F., Jackson, P., Keegstra, P., Kogut, A., Smoot, G. F., Wilkinson, D. T., & WRIGHT, E. L. (1996) · The Astrophysical Journal · doi:10.1086/310075 · Cited by 1,255
Self-citationFirst‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Implications For Inflation
Peiris, H. V., Komatsu, E., Verde, L., Spergel, D. N., Bennett, C. L., Halpern, M., Hinshaw, G. F., Jarosik, N., Kogut, A., Limon, M., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377228 · Cited by 1,247
Self-citationThe Cosmic Triangle: Revealing the State of the Universe
Bahcall, N. A., Ostriker, J. P., Perlmutter, S., & Steinhardt, P. J. (1999) · Science · doi:10.1126/science.284.5419.1481 · Cited by 1,190
Flagged first, then by citations
Research works printed but not linked: 6
- Haslam C. G. T., 1981, A&A, 100, 209
- Kuo, C. L., etal 2002, ApJ, submitted (astro-ph/0212289) · arXiv
- Reynolds, R. J., Haffner, L. M. & Madsen, G. J. 2002, in ASP Conf. Ser. 282, Galaxies: The Third Dimension, ed. M. Rosado, L. Binette, & L. Arias (San Francisco: ASP), 31
- Ricotti, M. 2002, MNRAS, submitted (astro-ph/0212146) · arXiv
- 10.1086/322348 · DOI
- Ruhl, J. E., etal 2003, ApJ, submitted (astro-ph/0212229) · arXiv
Cited by
Sorted by citations
Planck 2018 results: VI. Cosmological parameters
Planck Collaboration, Aghanim, N., Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., et al. (2020) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201833910 · Cited by 14,258
Spergel, D. N., Verde, L., Peiris, H. V., Komatsu, E., Nolta, M. R., Bennett, C. L., Halpern, M., Hinshaw, G., Jarosik, N., Kogut, A., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377226 · Cited by 10,976
Self-citationAde, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Bartolo, N., et al. (2016) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201525830 · Cited by 10,685
SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE(WMAP) OBSERVATIONS: COSMOLOGICAL INTERPRETATION
Komatsu, E., Smith, K. M., Dunkley, J., Bennett, C. L., Gold, B., Hinshaw, G., Jarosik, N., Larson, D., Nolta, M. R., Page, L., et al. (2011) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/192/2/18 · Cited by 8,802
Self-citationPlanck 2013 results. XVI. Cosmological parameters
Ade, P. A. R., Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., et al. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201321591 · Cited by 6,875
Three‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Implications for Cosmology
Spergel, D. N., Bean, R., Dore, O., Nolta, M. R., Bennett, C. L., Dunkley, J., Hinshaw, G., Jarosik, N., Komatsu, E., Page, L., et al. (2007) · The Astrophysical Journal Supplement Series · doi:10.1086/513700 · Cited by 6,778
Self-citationGórski, K., Hivon, E., Banday, A., Wandelt, B. D., Hansen, F., Reinecke, M., & Bartelmann, M. (2004) · The Astrophysical Journal · doi:10.1086/427976 · Cited by 5,217
FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: COSMOLOGICAL INTERPRETATION
Komatsu, E., Dunkley, J., Nolta, M. R., Bennett, C. L., Gold, B., Hinshaw, G., Jarosik, N., Larson, D., Limon, M., Page, L., et al. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/180/2/330 · Cited by 5,786
Self-citationAde, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Bartolo, N., et al. (2016) · Research at the University of Copenhagen (University of Copenhagen) · doi:10.17863/cam.32861 · Cited by 5,299
Simulations of the formation, evolution and clustering of galaxies and quasars
Springel, V., White, S. D. M., Jenkins, A. R., Frenk, C. S., Yoshida, N., Gao, L., Navarro, J. F., Thacker, R. J., Croton, D., Helly, J. C., et al. (2005) · Nature · doi:10.1038/nature03597 · Cited by 5,060
Eisenstein, D. J., Zehavi, I., Hogg, D. W., Scoccimarro, R., Blanton, M. R., Nichol, R. C., Scranton, R., Seo, H., Tegmark, M., Zheng, Z., et al. (2005) · The Astrophysical Journal · doi:10.1086/466512 · Cited by 4,641
Riess, A. G., Strolger, L., Tonry, J., Casertano, S., Ferguson, H. C., Mobasher, B., Challis, P., Filippenko, A. V., Jha, S., Li, W., et al. (2004) · The Astrophysical Journal · doi:10.1086/383612 · Cited by 4,315
“We find w ¼ 1:02 0:130:19 and w ¼ 1:08 0:200:18 with the use of an M prior and from WMAPext+ 2dFGRS, respectively.”
Cosmological parameters from SDSS and WMAP
Tegmark, M., Strauss, M. A., Blanton, M. R., Abazajian, K. N., Dodelson, S., Sandvik, H. B., Wang, X., Weinberg, D. H., Zehavi, I., Bahcall, N. A., et al. (2004) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.69.103501 · Cited by 3,977
Planck 2018 results. VI. Cosmological parametersPreprint
Planck Collaboration, Aghanim, N., Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., et al. (2018) · arXiv (Cornell University) · doi:10.48550/arxiv.1807.06209 · Cited by 3,364
Scolnic, D. M., Jones, D. O., Rest, A., Pan, Y. C., Chornock, R., Foley, R. J., Huber, M. E., Kessler, R., Narayan, G., Riess, A. G., et al. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aab9bb · Cited by 2,700
NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: FINAL MAPS AND RESULTS
Bennett, C. L., Larson, D., Weiland, J. L., Jarosik, N., Hinshaw, G., Odegard, N., Smith, K. M., Hill, R. S., Gold, B., Halpern, M., et al. (2013) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/208/2/20 · Cited by 2,639
Self-citationEisenstein, D. J., Zehavi, I., Hogg, D. W., Scoccimarro, R., Blanton, M. R., Nichol, R. C., Scranton, R., Seo, H., Tegmark, M., Zheng, Z., et al. (2005) · Cited by 2,568
Is cosmic speed-up due to new gravitational physics?
Carroll, S. M., Duvvuri, V., Trodden, M., & Turner, M. S. (2004) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.70.043528 · Cited by 2,438
How do galaxies get their gas?
Kere, D., Katz, N. S., Weinberg, D. H., & Davé, R. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09451.x · Cited by 2,267
Nojiri, S., & Odintsov, S. D. (2003) · Physical Review D · doi:10.1103/physrevd.68.123512 · Cited by 2,183
The Three‐Dimensional Power Spectrum of Galaxies from the Sloan Digital Sky Survey
Tegmark, M., Blanton, M. R., Strauss, M. A., Hoyle, F., Schlegel, D. J., Scoccimarro, R., Vogeley, M. S., Weinberg, D. H., Zehavi, I., Berlind, A. A., et al. (2004) · The Astrophysical Journal · doi:10.1086/382125 · Cited by 1,790
Self-citationThe clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at z=0.15
Ross, A. J., Samushia, L., Howlett, C., Percival, W. J., Burden, A., & Manera, M. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv154 · Cited by 1,745
Planck2013 results. I. Overview of products and scientific results
Ade, P. A. R., Aghanim, N., Alves, M. I. R., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Aussel, H., Baccigalupi, C., et al. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201321529 · Cited by 1,738
Aghanim, N., Akrami, Y., Arroja, F. M. A., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., et al. (2019) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201833880 · Cited by 2,386
The Simons Observatory: science goals and forecasts
Ade, P. A. R., Aguirre, J., Ahmed, Z., Aiola, S., Ali, A., Alonso, D., Alvarez, M. A., Arnold, K., Ashton, P., Austermann, J. E., et al. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/02/056 · Cited by 1,524
f ( T ) teleparallel gravity and cosmology
Cai, Y.-F., Capozzıello, S., Laurentis, M. D., & Saridakis, E. N. (2016) · Reports on Progress in Physics · doi:10.1088/0034-4885/79/10/106901 · Cited by 1,647
Observational probes of cosmic acceleration
Weinberg, D. H., Mortonson, M. J., Eisenstein, D. J., Hirata, C. M., Riess, A. G., & Rozo, E. (2013) · Physics Reports · doi:10.1016/j.physrep.2013.05.001 · Cited by 1,520
Larson, D., Dunkley, J., Hinshaw, G., Komatsu, E., Nolta, M. R., Bennett, C. L., Gold, B., Halpern, M., Hill, R. S., Jarosik, N., et al. (2011) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/192/2/16 · Cited by 1,358
Self-citationTowards inflation in string theory
Shamit Kachru, A., Каллош, Р., Linde, A. D., MALDACENA, J. M., McAllister, L., & Trivedi, S. P. (2003) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2003/10/013 · Cited by 1,439
The Discovery and Analysis of Very Metal-Poor Stars in the Galaxy
Beers, T. C., & Christlieb, N. (2005) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.42.053102.134057 · Cited by 1,223
Jarosik, N., Bennett, C. L., Dunkley, J., Gold, B., Greason, M. R., Halpern, M., Hill, R. S., Hinshaw, G., Kogut, A., Komatsu, E., et al. (2011) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/192/2/14 · Cited by 1,115
Self-citationJegerlehner, F., & Nyffeler, A. (2009) · Physics Reports · doi:10.1016/j.physrep.2009.04.003 · Cited by 1,217
The 6dF Galaxy Survey: final redshift release (DR3) and southern large-scale structures
Jones, D. H. P., Read, M., Saunders, W., Colless, M., Jarrett, T. H., Parker, Q. A., Fairall, A. P., Mauch, T., Sadler, E. M., Watson, F. G., et al. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15338.x · Cited by 1,052
Cosmology and fundamental physics with the Euclid satellite
The Euclid Theory Working Group, Amendola, L., Appleby, S. A., Avgoustidis, A., Bacon, D., Baker, T., Baldi, M., Bartolo, N., Blanchard, A., Bonvin, C., et al. (2018) · Living Reviews in Relativity · doi:10.1007/s41114-017-0010-3 · Cited by 1,095
Self-citationWRIGHT, E. L. (2016) · Texas ScholarWorks (Texas Digital Library) · doi:10.15781/t2rn30970 · Cited by 992
Self-citationTests of the Gravitational Inverse-Square Law below the Dark-Energy Length Scale
Kapner, D. J., Cook, T. S., Adelberger, E. G., Gundlach, J. H., Heckel, B. R., Hoyle, C. D., & Swanson, H. E. (2007) · Physical Review Letters · doi:10.1103/physrevlett.98.021101 · Cited by 984
Three‐YearWilkinson Microwave Anisotropy Probe(WMAP) Observations: Temperature Analysis
Hinshaw, G. F., Nolta, M. R., Bennett, C. L., Bean, R., Doré, O., Greason, M. R., Halpern, M., Hill, R., Jarosik, N., Kogut, A., et al. (2007) · The Astrophysical Journal Supplement Series · doi:10.1086/513698 · Cited by 972
Self-citationCMS Physics Technical Design Report, Volume II: Physics Performance
The CMS Collaboration (2007) · Journal of Physics G Nuclear and Particle Physics · doi:10.1088/0954-3899/34/6/s01 · Cited by 940
Kogut, A., Spergel, D. N., Barnes, C., Bennett, C. L., Halpern, M., Hinshaw, G., Jarosik, N., Limon, M., Meyer, S. S., Page, L., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377219 · Cited by 938
Self-citationChallenges for Λ CDM: An update
Perivolaropoulos, L., & Skara, F. (2022) · New Astronomy Reviews · doi:10.1016/j.newar.2022.101659 · Cited by 1,130
Cosmology and Fundamental Physics with the Euclid Satellite
The Euclid Theory Working Group, Amendola, L., Appleby, S., Bacon, D., Baker, T., Baldi, M., Bartolo, N., Blanchard, A., Bonvin, C., Borgani, S., et al. (2013) · Living Reviews in Relativity · doi:10.12942/lrr-2013-6 · Cited by 899
Self-citationDarkSUSY: computing supersymmetric dark matter properties numerically
Paolo Gondolo, A., Edsjö, J., Ullio, P., Bergström, L., Schelke, M., & Baltz, E. A. (2004) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2004/07/008 · Cited by 898
First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: The Angular Power Spectrum
Hinshaw, G. F., Spergel, D. N., Verde, L., Hill, R., Meyer, S. S., Barnes, C., Bennett, C. L., Halpern, M., Jarosik, N., Kogut, A., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377225 · Cited by 882
Self-citationLi, M., Li, X.-D., Wang, S., & Wang, Y. (2011) · Communications in Theoretical Physics · doi:10.1088/0253-6102/56/3/24 · Cited by 896
Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys
Seo, H., & Eisenstein, D. J. (2003) · The Astrophysical Journal · doi:10.1086/379122 · Cited by 797
Giudice, G. F., & Romanino, A. (2004) · Nuclear Physics B · doi:10.1016/j.nuclphysb.2004.08.001 · Cited by 793
Wollack, E. J., & WRIGHT, E. L. (2016) · Cited by 764
Self-citationObservational evidence for AGN feedback in early-type galaxies
Schawinski, K., Thomas, D., Sarzi, M., Maraston, C., Kaviraj, S., Joo, S.-J., Yi, S. K., & Silk, J. I. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.12487.x · Cited by 761
Asymmetries in the Cosmic Microwave Background Anisotropy Field
Eriksen, H. K., Hansen, F. K., Banday, A. J., Gorski, K. M., & Lilje, P. B. (2004) · The Astrophysical Journal · doi:10.1086/382267 · Cited by 767
Wolfe, A. M., Gawiser, E., & Prochaska, J. X. (2005) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.42.053102.133950 · Cited by 727
Gamma‐Ray Burst Formation Rate Inferred from the Spectral Peak Energy–Peak Luminosity Relation
Yonetoku, D., Murakami, T., Nakamura, T., Yamazaki, R., Inoue, A. K., & Ioka, K. (2004) · The Astrophysical Journal · doi:10.1086/421285 · Cited by 714
First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Tests of Gaussianity
Komatsu, E., Kogut, A., Nolta, M. R., Bennett, C. L., Halpern, M., Hinshaw, G. F., Jarosik, N., Limon, M., Meyer, S. S., Page, L. A., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377220 · Cited by 693
Self-citationThe phantom menaced: Constraints on low-energy effective ghosts
Cline, J. M., Jeon, S., & Moore, G. D. (2004) · Physical Review D · doi:10.1103/physrevd.70.043543 · Cited by 677
Can dark energy evolve to the phantom?
Vikman, A. (2005) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.71.023515 · Cited by 671
LEPTOGENESIS AS THE ORIGIN OF MATTER
Buchmüller, W., Peccei, R. D., & Yanagida, T. (2005) · Annual Review of Nuclear and Particle Science · doi:10.1146/annurev.nucl.55.090704.151558 · Cited by 642
High resolution foreground cleaned CMB map from WMAP
Tegmark, M., Angélica De Oliveira-costa, A., & Hamilton, A. J. S. (2003) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.68.123523 · Cited by 616
Significance of the largest scale CMB fluctuations in WMAP
de Oliveira-Costa, A., Tegmark, M., Zaldarriaga, M., & Hamilton, A. (2004) · Physical Review D · doi:10.1103/physrevd.69.063516 · Cited by 651
Cosmology of generalized modified gravity models
Carroll, S. M., De Felice, A., Duvvuri, V., Easson, D. A., Trodden, M., & Turner, M. S. (2005) · Physical Review D · doi:10.1103/physrevd.71.063513 · Cited by 604
Wormhole geometries in f ( R ) modified theories of gravity
Lobo, F. S. N., & Oliveira, M. A. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.80.104012 · Cited by 593
Tri-bimaximal neutrino mixing from discrete symmetry in extra dimensions
Altarelli, G., & Ferruccio Feruglio, A. (2005) · Nuclear Physics B · doi:10.1016/j.nuclphysb.2005.05.005 · Cited by 587
Bennett, C. L., Hill, R., Hinshaw, G. F., Larson, D., Smith, K. M., Dunkley, J., Gold, B., Halpern, M., Jarosik, N., Kogut, A., et al. (2011) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/192/2/17 · Cited by 569
Self-citationNonperturbative effect on dark matter annihilation and gamma ray signature from the galactic center
Hisano, J., Matsumoto, S., Nojiri, M. M., & Saito, O. (2005) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.71.063528 · Cited by 659
Planck 2013 results. XXIII. Isotropy and statistics of the CMB
Ade, P. A. R., Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., et al. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201321534 · Cited by 559
Fukugita, M., & Peebles, P. J. E. (2004) · The Astrophysical Journal · doi:10.1086/425155 · Cited by 550
Phantom energy traversable wormholes
Lobo, F. S. N. (2005) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.71.084011 · Cited by 550
What is the lowest possible reheating temperature?
Hannestad, S. (2004) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.70.043506 · Cited by 530
Detection methods for stochastic gravitational-wave backgrounds: a unified treatment
Romano, J. D., & Cornish, N. J. (2017) · Living Reviews in Relativity · doi:10.1007/s41114-017-0004-1 · Cited by 604
The WiggleZ Dark Energy Survey: survey design and first data release
Drinkwater, M. J., Jurek, R. J., Blake, C., Woods, D., Pimbblet, K. A., Glazebrook, K., Sharp, R., Pracy, M., Brough, S., Colless, M., et al. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15754.x · Cited by 517
Examination of Evidence for a Preferred Axis in the Cosmic Radiation Anisotropy
Land, K., & Magueijo, J. (2005) · Physical Review Letters · doi:10.1103/physrevlett.95.071301 · Cited by 521
K‐band Properties of Galaxy Clusters and Groups: Brightest Cluster Galaxies and Intracluster Light
Lin, Y., & Mohr, J. J. (2004) · The Astrophysical Journal · doi:10.1086/425412 · Cited by 496
Vielva, P., Martínez-González, E., Barreiro, R. B., Sanz, J. L., & Cayón, L. (2004) · The Astrophysical Journal · doi:10.1086/421007 · Cited by 494
Theory of neutrinos: a white paper
Mohapatra, R. N., Antusch, S., Babu, K. S., Barenboim, G., Chen, M.-C., de Gouvêa, A., de Holanda, P. C., Dutta, B., Grossman, Y., Joshipura, A. S., et al. (2007) · Reports on Progress in Physics · doi:10.1088/0034-4885/70/11/r02 · Cited by 599
The shape of non-Gaussianities
Babich, D., Creminelli, P., & Zaldarriaga, M. (2004) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2004/08/009 · Cited by 492
Longair, M. S. (2011) · Cambridge University Press eBooks · doi:10.1017/cbo9780511778346 · Cited by 536
Interacting Dark Matter and Dark Energy
Farrar, G. R., & Peebles, P. J. E. (2004) · The Astrophysical Journal · doi:10.1086/381728 · Cited by 491
Matsubara, T. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.77.063530 · Cited by 491
Black Hole Mass Decreasing due to Phantom Energy Accretion
Babichev, E., Dokuchaev, V. I., & Eroshenko, Y. (2004) · Physical Review Letters · doi:10.1103/physrevlett.93.021102 · Cited by 505
Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Basak, S., Benabed, K., et al. (2019) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201935201 · Cited by 485
The holographic dark energy in a non-flat universe
Huang, Q.-G., & Li, M. (2004) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2004/08/013 · Cited by 480
How many cosmological parameters?
Liddle, A. R. (2004) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2004.08033.x · Cited by 475
The XMM-Newton view of PG quasars
Piconcelli, E., Jimenez‐Bailon, E., Guainazzi, M., Schartel, N., Rodriguez, P., & Santos‐Lleó, M. (2005) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20041621 · Cited by 473
Non-perturbative effect on thermal relic abundance of dark matter
Hisano, J., Matsumot, S., Nagai, M., Saito, O., & Senami, M. (2007) · Physics Letters B · doi:10.1016/j.physletb.2007.01.012 · Cited by 469
Is the Low-ℓMicrowave Background Cosmic?
Schwarz, D. J., Starkman, G. D., Huterer, D., & Copi, C. J. (2004) · Physical Review Letters · doi:10.1103/physrevlett.93.221301 · Cited by 488
Explosive Dark Matter Annihilation
Hisano, J., Matsumoto, S., & Nojiri, M. M. (2004) · Physical Review Letters · doi:10.1103/physrevlett.92.031303 · Cited by 521
On the Robustness of the Acoustic Scale in the Low‐Redshift Clustering of Matter
Eisenstein, D. J., Seo, H., & White, M. J. (2007) · The Astrophysical Journal · doi:10.1086/518755 · Cited by 460
Sullivan, M., Guy, J., Conley, A., Regnault, N., Astier, P., Balland, C., Basa, S., Carlberg, R. G., Fouchez, D., Hardin, D., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/737/2/102 · Cited by 455
MeV Dark Matter: Has It Been Detected?
Bœhm, C., Hooper, D., Silk, J. I., Cassé, M., & Paul, J. (2004) · Physical Review Letters · doi:10.1103/physrevlett.92.101301 · Cited by 495
Gott, J. R., III, Jurić, M., Schlegel, D., Hoyle, F., Vogeley, M., Tegmark, M., Bahcall, N., & Brinkmann, J. (2005) · The Astrophysical Journal · doi:10.1086/428890 · Cited by 448
Constraints on holographic dark energy from type Ia supernova observations
Zhang, X., & Wu, F. (2005) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.72.043524 · Cited by 446
Wyithe, J. S. B., & Loeb, A. (2003) · The Astrophysical Journal · doi:10.1086/377475 · Cited by 440
Bélanger, G., Boudjema, F., Pukhov, A., & Semenov, A. (2006) · Computer Physics Communications · doi:10.1016/j.cpc.2005.12.005 · Cited by 436
Ade, P. A. R., Aghanim, N., Akrami, Y., Aluri, P. K., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., et al. (2015) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201526681 · Cited by 428
Luminet, J.-P., Weeks, J. R., Riazuelo, A., Lehoucq, R., & Uzan, J.-P. (2003) · Nature · doi:10.1038/nature01944 · Cited by 424
Cosmological perturbations in f(T) gravity
Chen, S.-H., Dent, J. B., Dutta, S., & Saridakis, E. N. (2011) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.83.023508 · Cited by 420
Dark energy from mass varying neutrinos
Fardon, R., Nelson, A. E., & Weiner, N. (2004) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2004/10/005 · Cited by 414
Estimation of the XUV radiation onto close planets and their evaporation
Sanz-Forcada, J., Micela, G., Ribas, I., Pollock, A. M. T., Eiroa, C., Velasco, A., Solano, E., & García-Álvarez, D. (2011) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201116594 · Cited by 410
Proton stability in grand unified theories, in strings and in branes
Nath, P., & Perez, P. (2007) · Physics Reports · doi:10.1016/j.physrep.2007.02.010 · Cited by 449
Early galaxy formation and its large-scale effects
Dayal, P., & Ferrara, A. (2018) · Physics Reports · doi:10.1016/j.physrep.2018.10.002 · Cited by 438
New BBN limits on physics beyond the standard model from 4He
Cyburt, R. H., Fields, B. D., Olive, K. A., & Skillman, E. D. (2005) · Astroparticle Physics · doi:10.1016/j.astropartphys.2005.01.005 · Cited by 403
Ulrich Ellwanger, A., & Hugonie, C. (2006) · Computer Physics Communications · doi:10.1016/j.cpc.2006.04.004 · Cited by 403
Metadata
- Authors
- Bennett, C. L., Halpern, M., Hinshaw, G., Jarosik, N., Kogut, A., Limon, M., Meyer, S. S., Page, L., Spergel, D. N., Tucker, G. S., Wollack, E., Wright, E. L., Barnes, C., Greason, M. R., Hill, R. S., Komatsu, E., Nolta, M. R., Odegard, N., Peiris, H. V., Verde, L., & Weiland, J. L.
- Affiliations
- Goddard Space Flight Center (US)
- University of British Columbia (CA)
- Princeton University (US)
- University of Chicago (US)
- University of California, Los Angeles (US)
- Science Systems and Applications (United States) (US)
- ORCID
- Venue
- The Astrophysical Journal Supplement Series
- Publisher
- American Astronomical Society
- Published
- 2003-09
- Volume
- 148
- Issue
- 1
- Pages
- 1-27
- ISSN
- 0067-0049 (ISSN-L)
- 1538-4365
- OpenAlex
- W2075884494
- Cited by
- 4,860
- References
- 99
- Citations by year
- 2026: 73 · 2025: 109 · 2024: 115 · 2023: 115 · 2022: 90 · 2021: 100 · 2020: 122 · 2019: 115 · 2018: 119 · 2017: 90 · 2016: 143 · 2015: 101 · 2014: 132 · 2013: 171 · 2012: 185
- FWCI
- 354.79
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- The Astrophysical Journal Supplement Series (publishedVersion)
- arXiv (Cornell University) (acceptedVersion)
- NASA STI Repository (National Aeronautics and Space Administration) (submittedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- UCL Discovery (University College London) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Keywords
- WMAP, cosmic microwave background anisotropies, reionization optical depth, cosmic reionization, matter density, baryon density, dark energy equation of state, dark energy, scalar spectral index, running of the spectral index, isocurvature modes, tensor-to-scalar ratio, inflation (cosmology), warm dark matter, acoustic features
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
