The DOI matches its Crossref record; 53 of the 53 references it cites were found in a registry or an index.
Radial Acceleration Relation in Rotationally Supported Galaxies
Open accessAbstract
We report a correlation between the radial acceleration traced by rotation curves and that predicted by the observed distribution of baryons. The same relation is followed by 2693 points in 153 galaxies with very different morphologies, masses, sizes, and gas fractions. The correlation persists even when dark matter dominates. Consequently, the dark matter contribution is fully specified by that of the baryons. The observed scatter is small and largely dominated by observational uncertainties. This radial acceleration relation is tantamount to a natural law for rotating galaxies.
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.
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
A Universal Density Profile from Hierarchical Clustering
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1997) · The Astrophysical Journal · doi:10.1086/304888 · Cited by 9,917
A Universal Density Profile from Hierarchical ClusteringPreprint
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1996) · Cited by 6,275
Stellar Mass‐to‐Light Ratios and the Tully‐Fisher Relation
Bell, E. F., & de Jong, R. S. (2001) · The Astrophysical Journal · doi:10.1086/319728 · Cited by 1,806
Physics of the Interstellar and Intergalactic Medium
Draine, B. T. (2011) · doi:10.1515/9781400839087 · Cited by 1,787
Stellar mass-to-light ratios and the Tully-Fisher relation
Bell, E. F., & De Jong, R. S. (2000) · CERN Document Server (European Organization for Nuclear Research) · Cited by 1,077
A modification of the Newtonian dynamics - Implications for galaxies
Milgrom, M. (1983) · The Astrophysical Journal · doi:10.1086/161131 · Cited by 1,072
de Blok, W. J. G. (2009) · Advances in Astronomy · doi:10.1155/2010/789293 · Cited by 934
The Baryonic Tully-Fisher Relation
McGaugh, S., Schombert, J. M., Bothun, G. D., & de Blok, W. J. G. (2000) · The Astrophysical Journal · doi:10.1086/312628 · Cited by 836
Self-citationRubin, V. C., Thonnard, N., & K., J. F. W. (1978) · The Astrophysical Journal · doi:10.1086/182804 · Cited by 594
A New Method of Determining Distances to Galaxies
Tully, R., de Marseille, O., & Fisher, J. R. (1975) · Bulletin of the American Astronomical Society · Cited by 491
Research works printed but not linked: 3
- R. B. Tully, 1977, Astron. Astrophys., 54, 661
- J. Binney, 1987, Galactic Dynamics
- J. M. van der Hulst, 1992, Proceedings of the Astronomical Society of the Pacific Conference
Cited by
Sorted by citations
Items 401–500 of 661
Pressure-regulated formation of molecular clouds and stars: the case of the Milky Way
Franco, J., Rodríguez-Puebla, A., Ballesteros‐Paredes, J., & Zamora-Avilés, M. (2025) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staf1572 · Cited by 2
Dado, D., Oman, K. A., Harborne, K. E., Fragkoudi, F., Schaye, J., Schaller, M., Benítez-Llambay, A., Chaikin, E., Frenk, C. S., Huško, F., et al. (2026) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stag356 · Cited by 2
Dalui, S. K., & Desai, S. (2026) · Physics of the Dark Universe · doi:10.1016/j.dark.2026.102265 · Cited by 2
MONDian predictions for Newtonian mass-to-light ratios for ultrafaint dSphs
Cortés, R. A. M., & Hernández, X. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx1233 · Cited by 2
Dark matter fluid constraints from galaxy rotation curves
Perković, D., & Štefančić, H. (2023) · The European Physical Journal C · doi:10.1140/epjc/s10052-023-11457-3 · Cited by 2
Formation of collisional ring galaxies in Milgromian dynamics
Ma, L., & Wu, X. (2024) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stae021 · Cited by 2
McGruder, C. H. (2024) · Journal of Modern Physics · doi:10.4236/jmp.2024.158048 · Cited by 2
Bílek, M. (2024) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202450154 · Cited by 2
Phenomenology of renormalization group improved gravity from the kinematics of SPARC galaxies
Bhatia, E., Chakrabarti, S. K., & Chakraborty, S. (2024) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.110.124014 · Cited by 2
Beordo, W., Crosta, M., & Lattanzi, M. G. (2024) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2024/12/024 · Cited by 2
Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA
Lee, G.-M., & van Putten, M. H. P. M. (2025) · New Astronomy · doi:10.1016/j.newast.2025.102360 · Cited by 2
On a Critical Acceleration Scale of Dark Matter in ΛCDM and Dynamical Dark Energy
Xu, Z. (2025) · The Astrophysical Journal · doi:10.3847/1538-4357/adaeb3 · Cited by 2
Perković, D., & Štefančić, H. (2025) · Classical and Quantum Gravity · doi:10.1088/1361-6382/adbeb3 · Cited by 2
Zhu, Y. (2021) · International Journal of Astronomy and Astrophysics · doi:10.4236/ijaa.2021.113016 · Cited by 2
Dark Matter without New Matter Is Compliant with General Relativity
Corre, S. L. (2017) · OALib · doi:10.4236/oalib.1103877 · Cited by 2
The dark-baryonic matter mass relation for observational verification in Verlinde’s emergent gravity
Shen, J. Q. (2018) · General Relativity and Gravitation · doi:10.1007/s10714-018-2382-4 · Cited by 2
On Nonlinear Schrödinger Equation as a Model for Dark Matter
Paredes, Á., & Michinel, H. (2018) · Understanding complex systems · doi:10.1007/978-3-319-66766-9_5 · Cited by 2
MOUND: An Alternative to Milgrom’s MOND
Tonin, P. G. (2021) · International Journal of Astronomy and Astrophysics · doi:10.4236/ijaa.2021.111006 · Cited by 2
Dynamics of Disk and Elliptical Galaxies in Refracted Gravity
Cesare, V. (2021) · Electronic Conference on Universe (ECU) · doi:10.3390/ecu2021-09292 · Cited by 2
Characterization of the GRB prompt fundamental plane using Fermi-GBM data
Pradyumna, S., & Desai, S. (2022) · Journal of High Energy Astrophysics · doi:10.1016/j.jheap.2022.06.003 · Cited by 2
A test of linearity of the ratio of dark matter to baryonic matter in galaxy clusters
Upadhyaya, V., & Desai, S. (2023) · Physics of the Dark Universe · doi:10.1016/j.dark.2023.101182 · Cited by 2
Square-torsion gravity: a geometric candidate for dark matter
Mégier, E. A. S. (2019) · Classical and Quantum Gravity · doi:10.1088/1361-6382/ab4bf8 · Cited by 2
On the radial acceleration of disc galaxies
Wilhelm, K., & Dwivedi, B. N. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa967 · Cited by 2
Dark matter, dark energy and fundamental acceleration
Edmonds, D., Minić, D., & Takeuchi, T. (2020) · International Journal of Modern Physics D · doi:10.1142/s0218271820430300 · Cited by 2
Modified inertia as nonconservative Newtonian dynamics
Shariati, A., & Jafari, N. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.104.084070 · Cited by 2
A test of galaxy cluster fundamental plane for the X-COP sample
Pradyumna, S., & Desai, S. (2022) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2022/01/058 · Cited by 2
Statistical description of galaxy clusters in Finzi model of gravity
Khanday, A. W., Upadhyay, S., Iqbal, N., & Ganai, P. A. (2023) · Physica Scripta · doi:10.1088/1402-4896/acd5cd · Cited by 2
A new perspective on galactic dynamicsPreprint
Tuveri, M., & Cadoni, M. (2019) · arXiv (Cornell University) · doi:10.48550/arxiv.1904.08209 · Cited by 2
Information Dark Energy can resolve Hubble tension and is falsifiable by experiment.Preprint
Gough, M. P. (2022) · Preprints.org · doi:10.20944/preprints202102.0052.v2 · Cited by 2
Sigtermans, D. (2025) · Preprints.org · doi:10.20944/preprints202506.0665.v1 · Cited by 2
Cosmological Background and Linear Perturbations in Quantum Vacuum Polarization GravityPreprint
Đulović, D. (2025) · Zenodo (CERN European Organization for Nuclear Research) · doi:10.5281/zenodo.17753038 · Cited by 2
Facchinetti, G. (2021) · theses.fr (ABES) · doi:10.70675/84e471a2z44fcz4c6bz8bd7z07bf94031b23 · Cited by 2
Understanding galaxy rotation curves with Verlinde’s emergent gravity
Yoon, Y., Park, J.-C., & Hwang, H. S. (2022) · Classical and Quantum Gravity · doi:10.1088/1361-6382/acaae6 · Cited by 1
Corre, S. L. (2018) · OALib · doi:10.4236/oalib.1105028 · Cited by 1
Galaxies with fuzzy dark matter
Lee, J. W. (2021) · Journal of the Korean Physical Society · doi:10.1007/s40042-021-00077-3 · Cited by 1
Vorticity of Matter or Vorticity of Space?
Benedetto, E., Iovane, G., & Laserra, E. (2021) · Gravitation and Cosmology · doi:10.1134/s0202289321010059 · Cited by 1
Thater, S., Krajnović, D., Weilbacher, P. M., Nguyen, D. D., Bureau, M., Cappellari, M., Davis, T. A., Iguchi, S., McDermid, R. M., Onishi, K., et al. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab3210 · Cited by 1
Velocity relationships of isolated galaxy pairs in support of MOND-type theories
Penner, A. R. (2023) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stad1116 · Cited by 1
Relativistic tensorial model for fractional interaction between dark matter and gravity
Benetti, F., Lapi, A., Silveravalle, S., Liberati, S., Haridasu, B. S., Boumechta, Y., Butt, M. A., & Baccigalupi, C. (2025) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.111.024026 · Cited by 1
Comparison of HMG and Flat Rotation Velocities Inferred from Galaxy–Galaxy Weak Lensing
Monjo, R. (2025) · The Astrophysical Journal · doi:10.3847/1538-4357/adb8d7 · Cited by 1
Negligible MOND effects on the orbits of planets
Yoon, Y. (2025) · Classical and Quantum Gravity · doi:10.1088/1361-6382/ae085b · Cited by 1
Renzo’s rule revisited: a statistical study of galaxies’ baryon–dark matter coupling
Ko, E., Yasin, T., Desmond, H., Stiskalek, R., & Jarvis, M. J. (2025) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staf2004 · Cited by 1
Cusp-to-core transition of dark matter halos across galaxy mass scales
Hayashi, K., Kaneda, Y., Mori, M., & Shinozaki, M. (2026) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/psag016 · Cited by 1
Stålhammar, G. (2026) · Results in Physics · doi:10.1016/j.rinp.2026.108649 · Cited by 1
Jeanneau, A., Richard, J., Bouché, N., Krajnović, D., Ciocan, B. I., Freundlich, J., Épinat, B., & Contini, T. (2026) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202659953 · Cited by 1
On the Residual Missing Mass of the Bullet Cluster
Famaey, B. (2026) · Research Notes of the AAS · doi:10.3847/2515-5172/ae9f45 · Cited by 1
Singh, A., & Desai, S. (2026) · Astrophysics and Space Science · doi:10.1007/s10509-026-04589-x · Cited by 1
Cavedon, M. (2026) · IPI Letters · doi:10.59973/ipil.380 · Cited by 1
Symbolic Discovery of a Non-Linear Acceleration Scaling Relation in Galaxy Rotation Data
Santos, R., & Felizardo, M. (2026) · Particles · doi:10.3390/particles9030070 · Cited by 1
A Detailed MOND Modelling of the Bullet Cluster
Hernández, X. (2026) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ae9d4c · Cited by 1
1-D harmonic oscillator in MONDified inertia
Bonetto, R. (2018) · Physics Letters A · doi:10.1016/j.physleta.2018.06.003 · Cited by 1
Probing the universality of acceleration scale in modified Newtonian dynamics with SPARC galaxies *
Li, X., Zhao, S.-P., Lin, H.-N., & Zhou, Y. (2020) · Chinese Physics C · doi:10.1088/1674-1137/abce53 · Cited by 1
Revisiting two well studied galaxy samples using alternative gravity
O’Brien, J. G., Chiarelli, T. L., Kerin, W. M., & Belanger, J. (2021) · Journal of Physics Conference Series · doi:10.1088/1742-6596/1956/1/012003 · Cited by 1
Weyl Conformal Symmetry Model of the Dark Galactic Halo
NESBET, R. K. (2022) · Galaxies · doi:10.3390/galaxies10020049 · Cited by 1
Modeling the Rotation Curve of Disk Galaxies
Meza, A., & Lipovka, A. A. (2022) · Astrophysical Bulletin · doi:10.1134/s1990341322020055 · Cited by 1
Conformal gravity: Newton's constant is not universal
NESBET, R. K. (2022) · Europhysics Letters (EPL) · doi:10.1209/0295-5075/ac8d28 · Cited by 1
General Relativity and the Tully-Fisher Relation for Rotating Galaxies
Srivastava, Y. N., Immirzi, G., Swain, J., Panella, O., & Pacetti, S. (2022) · Journal of Modern Physics · doi:10.4236/jmp.2022.1311090 · Cited by 1
Ultra faint edge on galaxies: standard and alternative gravity explorations
O'Brien, J. G., Kerin, W. M., & Chiarelli, T. L. (2023) · Journal of Physics Conference Series · doi:10.1088/1742-6596/2482/1/012004 · Cited by 1
Quadratic gravity potentials in de Sitter spacetime from Feynman diagrams
Ferrero, R., & Ripken, C. (2023) · Journal of High Energy Physics · doi:10.1007/jhep08(2023)199 · Cited by 1
Derivation of MOND from Hossenfelder–Verlinde gravity
Yoon, Y. (2023) · Classical and Quantum Gravity · doi:10.1088/1361-6382/acf8aa · Cited by 1
Bílek, M., Hilker, M., Renaud, F., Richtler, T., Chaturvedi, A., & Samurović, S. (2023) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202244093 · Cited by 1
Explanation of Two Important Empirical Relations for Galaxies
Gu, Y.-Q. (2024) · Journal of Applied Mathematics and Physics · doi:10.4236/jamp.2024.121023 · Cited by 1
Refracted Gravity Solutions from Small to Large Scales
Cesare, V. (2024) · Astronomy · doi:10.3390/astronomy3020006 · Cited by 1
Hubble tension and gravitational self-interaction
Sargent, C., Clark, W., DEUR, A., & Terzić, B. (2024) · Physica Scripta · doi:10.1088/1402-4896/ad570f · Cited by 1
Probing the Nonlinear Density Wave Theory of Spiral Galaxies by Baryonic Tully–Fisher Relation
Vukčević, M., Savić, Đ., & Jovanović, P. (2024) · Universe · doi:10.3390/universe10090359 · Cited by 1
Many body gravity and the galaxy rotation curves
Ganesh, S. (2024) · The European Physical Journal C · doi:10.1140/epjc/s10052-024-13310-7 · Cited by 1
Comparing radial migration in dark matter and MOND regimes
Nagy, R., Janák, F., Šturc, M., Jurčík, M., & Puha, E. (2024) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202452112 · Cited by 1
Luo, M. J. (2024) · Annals of Physics · doi:10.1016/j.aop.2024.169899 · Cited by 1
Evidence for Dark Energy Driven by Star Formation: Information Dark Energy?
Gough, M. P. (2025) · Entropy · doi:10.3390/e27020110 · Cited by 1
Kambe, T. (2025) · WSEAS TRANSACTIONS on SYSTEMS archive · doi:10.37394/23202.2025.24.58 · Cited by 1
On the scaling properties of excited stationary states of the Schrödinger-Poisson model
Marangon, G., Ponno, A., & Zanelli, L. (2025) · Communications in Nonlinear Science and Numerical Simulation · doi:10.1016/j.cnsns.2025.109486 · Cited by 1
Cosmic rays and galactic rotation curves
Clark, M. J. (2018) · Astrophysics and Space Science · doi:10.1007/s10509-018-3434-7 · Cited by 1
Conformal gravity and the radial acceleration relation
O'Brien, J. G., Chiarelli, T. L., Falcone, M. A., & AlQurashi, M. H. (2019) · Astronomische Nachrichten · doi:10.1002/asna.201913568 · Cited by 1
Fifth forces and discrete symmetry breaking
Millington, P. (2020) · Journal of Physics Conference Series · doi:10.1088/1742-6596/1586/1/012024 · Cited by 1
A toy model for the dynamical discrepancies on galactic scales
Petersen, J., & Rosenlyst, M. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz2625 · Cited by 1
Can the Standard Model Predict a Minimum Acceleration That Gets Rid of Dark Matter?
Haug, E. G. (2021) · Journal of High Energy Physics Gravitation and Cosmology · doi:10.4236/jhepgc.2021.72035 · Cited by 1
Modeling dark matter halos with nonlinear field theories
Correa, R. A. C., Moraes, P. H. R. S., DUTRA, A. D. S., Dors, O. L., de Paula, W., & Frederico, T. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.103.103519 · Cited by 1
Lutephy, M. (2020) · Physics International · doi:10.3844/pisp.2020.4.35 · Cited by 1
Pattern dark matter and galaxy scaling relations
Venkataramani, S. C., & Newell, A. C. (2021) · The European Physical Journal Special Topics · doi:10.1140/epjs/s11734-021-00196-9 · Cited by 1
Theory Variant T2: A Relativistic Theory
Merritt, D. R. (2020) · Cambridge University Press eBooks · doi:10.1017/9781108610926.007 · Cited by 1
Dark Matter as a Metric PerturbationPreprint
Stuckey, W. M., McDevitt, T. J., Sten, A. K., & Silberstein, M. (2016) · Preprints.org · doi:10.20944/preprints201611.0080.v1 · Cited by 1
Alternative approach to gravity and MONDPreprint
Klačka, J. (2019) · arXiv (Cornell University) · doi:10.48550/arxiv.1904.04074 · Cited by 1
A local Lagrangian for MOND as modified inertiaPreprint
Costa, R., Franzmann, G., & Pereira, J. P. (2019) · arXiv (Cornell University) · doi:10.48550/arxiv.1904.07321 · Cited by 1
Information Energy Mimics Ʌ and CDMPreprint
Gough, M. P. (2019) · Preprints.org · doi:10.20944/preprints201910.0019.v1 · Cited by 1
A Physical Interpretation of Milky Way Galaxy Dynamics from Precision AstrometricsPreprint
Fortune, J. M. L. (2020) · arXiv (Cornell University) · doi:10.48550/arxiv.2008.10445 · Cited by 1
Mining the SPARC Galaxy Database: Finding "Hidden Variables" in the Baryonic Tully-Fisher RelationPreprint
Fortune, J. M. L. (2021) · arXiv (Cornell University) · doi:10.48550/arxiv.2101.01537 · Cited by 1
Could Information Energy resolve Hubble Tension?Preprint
Gough, M. P. (2021) · Preprints.org · doi:10.20944/preprints202102.0052.v1 · Cited by 1
On a Generalized Mass-Velocity Relation for Disk Galaxies and Galaxy ClustersPreprint
Fortune, J. M. L. (2021) · arXiv (Cornell University) · doi:10.48550/arxiv.2110.02684 · Cited by 1
Verlinde, E. (2017) · SciPost Physics · doi:10.21468/scipost.report.76 · Cited by 1
Zhu, Y. (2024) · Preprints.org · doi:10.20944/preprints202402.1765.v2 · Cited by 1
A Conjecture on the Possible Another Supermassive Black Hole in the Bar of Our Milky WayPreprint
Zhu, Y. (2024) · Preprints.org · doi:10.20944/preprints202406.1730.v1 · Cited by 1
Galactic SymmetryPreprint
Oldani, R. J. (2024) · Preprints.org · doi:10.20944/preprints202009.0215.v8 · Cited by 1
Optics Effect on the Observed Image about Sgr A* and Orbits of S-StarsPreprint
Zhu, Y. (2024) · Preprints.org · doi:10.20944/preprints202407.2142.v1 · Cited by 1
Яковчиц, В. (2025) · doi:10.24108/preprints-3113879 · Cited by 1
Теория Универсального Поля: Квантовая космология перерождения и программа предсказания (Уровень 3)Preprint
Яковчиц, В. (2025) · doi:10.24108/preprints-3113878 · Cited by 1
On the Dynamics of Rotationally Supported GalaxiesPreprint
Suleiman, R. (2019) · Preprints.org · doi:10.20944/preprints201903.0107.v1 · Cited by 1
Đulović, D. (2025) · Zenodo (CERN European Organization for Nuclear Research) · doi:10.5281/zenodo.17778864 · Cited by 1
Kobayashi, M. (2026) · Zenodo (CERN European Organization for Nuclear Research) · doi:10.5281/zenodo.18139449 · Cited by 1
The a0(z) tests: does the MOND acceleration scale track the cosmic horizon? A preregistered record
Maggio, J. (2026) · Zenodo (CERN European Organization for Nuclear Research) · doi:10.5281/zenodo.23280955 · Cited by 1
Melchiorri, A., & Ruchika (2026) · New Astronomy Reviews · doi:10.1016/j.newar.2026.101758
Metadata
- Authors
- McGaugh, S. S., Lelli, F., & Schombert, J. M.
- Affiliations
- Case Western Reserve University (US)
- University of Oregon (US)
- Venue
- Physical Review Letters
- Publisher
- American Physical Society (APS)
- Published
- 2016-11-09
- Volume
- 117
- Issue
- 20
- Pages
- 201101-201101
- ISSN
- 0031-9007 (ISSN-L)
- 1079-7114
- OpenAlex
- W2523266658
- Cited by
- 665
- References
- 53
- Citations by year
- 2026: 71 · 2025: 49 · 2024: 53 · 2023: 66 · 2022: 69 · 2021: 67 · 2020: 78 · 2019: 69 · 2018: 64 · 2017: 67 · 2016: 12
- FWCI
- 33.79
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Licence
- Locations
- Physical Review Letters (publishedVersion)
- PubMed (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- Scholarly Commons @ Case Western Reserve University (submittedVersion)
- arXiv (Cornell University)
- Funders
- Jet Propulsion Laboratory
- California Institute of Technology
- National Aeronautics and Space Administration (NNX13AH32G)
- John Templeton Foundation
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Keywords
- radial acceleration relation, rotation curves, baryonic Tully-Fisher relation, dark matter, baryon distribution, galaxy morphology, galaxy mass, void fraction
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
