Reference health
Baryonic Features in the Matter Transfer Function
35/35 checkable references clean · checked 2026-09-05
Every reference with a DOI in the deposited reference list resolved to a known work in Crossref or DataCite at the dated check, and none carried a retraction, withdrawal, or removal notice.
4 without a DOI — not checked. A reference deposited without a DOI is never matched by title or guessed at; it stays outside the checked set, and this line discloses that.
The 35 checked references that resolve
resolves10.1093/mnras/265.1.145
The three-dimensional power spectrum measured from the APM Galaxy Survey - I. Use of the angular correlation function
resolves10.1086/310075
Four-Year [ITAL]COBE[/ITAL] DMR Cosmic Microwave Background Observations: Maps and Basic Results
resolves10.1086/184362
Cosmic background radiation anisotropies in universes dominated by nonbaryonic dark matter
resolves10.1086/175722
Cosmological implications of ROSAT observations of groups and clusters of galaxies
resolves10.1086/178173
The Cosmic Microwave Background Spectrum from the Full<i>COBE</i>FIRAS Data Set
resolves10.1086/191362
Microwave background anisotropies and large-scale structure in universes with cold dark matter, baryons, radiation, and massive and massless neutrinos
resolves10.1103/PhysRevD.52.5498
Effect of physical assumptions on the calculation of microwave background anisotropies
resolves10.1093/mnras/267.4.1020
Reconstructing the linear power spectrum of cosmological mass fluctuations
resolves10.1086/183911
Large-scale background temperature and mass fluctuations due to scale-invariant primeval perturbations
resolves10.1086/157749
Propagation of adiabatic cosmological perturbations through the ERA of matter-radiation decoupling
resolves10.1086/177793
A Line-of-Sight Integration Approach to Cosmic Microwave Background Anisotropies
resolves10.1103/RevModPhys.61.185
The large-scale structure of the universe: Turbulence, intermittency, structures in a self-gravitating medium
resolves10.1038/381207a0
Cosmological baryon density derived from the deuterium abundance at redshift z = 3.57
resolves10.1038/366429a0
The baryon content of galaxy clusters: a challenge to cosmological orthodoxy
The 4 references without a DOI — listed, not checked
no DOI — not checkedFreedman, W. L. 1996, in Critical Dialogues in Cosmology, ed. N. Turok (Cambridge: Cambridge Univ. Press), 92
no DOI — not checkedGoldberg, D. M. & Strauss, M. 1997, preprint (astro-ph/9707209)
no DOI — not checkedGunn, J. E. & Weinberg, D. H. 1995, in Wide-Field Spectroscopy and the Distant Universe, ed. S. J. Maddox & A. Aragon-Salamanca (Singapore: World Scientific), 3
no DOI — not checkedTaylor, K. 1995, in Wide-Field Spectroscopy and the Distant Universe, ed. S. J. Maddox & A. Aragon-Salamanca (Singapore: World Scientific), 15
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