Detection of the Keplerian decline in the Milky Way rotation curve
Open accessAbstract
Our position inside the Galactic disc has previously prevented us from establishing an accurate rotation curve (RC). The advent of Gaia and its third data release ( Gaia DR3) made it possible to specify the RC up to twice the optical radius. We aim to establish a new RC of the Galaxy from the Gaia DR3 by drastically reducing systematic uncertainties. Our goal is to provide a new estimate of the mass of the Galaxy. We compared different estimates, established a robust assessment of the systematic uncertainties, and addressed differences in methodologies, particularly regarding distance estimates. We find a sharply decreasing RC for the Milky Way; the decrease in velocity between 19.5 and 26.5 kpc is approximately 30 km s −1 . We identify, for the first time, a Keplerian decline of the RC, starting at ∼19 kpc and ending at ∼26.5 kpc from the Galaxy centre, while a flat RC is rejected with a significance of 3 σ . The total mass is revised downwards to 2.06 −0.13 +0.24 × 10 11 M ⊙ , which is in agreement with the absence of a significant mass increase at radii larger than 19 kpc. We evaluated the upper limit on the total mass by considering the upper values of velocity measurements, which leads to a strict, unsurpassable limit of 5.4 × 10 11 M ⊙ .
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The exclusion of Zhou et al. (2023) by Jiao et al. rests on a comparison with distance scales that are somewhat shorter than the Zhou et al. scale for R > 10 kpc; since all are spectrophotometric distances, the offset is more naturally read as a difference among calibrations than as proof that one is biased.
“Regarding the exclusion of Zhou et al. (2023), we note that the argument of Jiao et al. (their Fig. B1) rests on a comparison with the distance scales of Wang et al. (2016, as updated with Gaia EDR3 priors), Hogg et al. (2019) and StarHorse (Queiroz et al. 2023), all of which are somewhat shorter than the Zhou et al. scale for R > 10 kpc. Since all of these are spectrophotometric distances, the”
From The rotation curve of the Milky Way: State of the art, the Keplerian decline debate, and implications for dark matter (2026) · cites this paper as Jiao et al. (2023)
Split into 2 atoms — 1 confirmed, 0 partially supported, 1 disputed, 0 misattributed, 0 unverifiable. Expand the claim to see per-atom verdicts.
Checked by a reasoning model — may be wrong.
Experimental — accuracy not yet measuredJiao et al. (2023) fit a power-law model vc ∝ R^γ to the data at R > 19 kpc, finding γ = -0.47 ± 0.15 for their RC and γ = -0.56 +0.23 -0.22 for the Ou et al. (2024) RC, both consistent with Keplerian (γ = -0.5) at 1σ; a flat RC (γ = 0) is excluded at the 3σ level.
“They then fit a power-law model vc ∝ R γ to the data at R > 19 kpc, finding γ = -0 . 47 ± 0 . 15 for their RC and γ = -0 . 56 + 0 . 23 -0 . 22 for the Ou et al. (2024) RC, both consistent with Keplerian ( γ = -0 . 5) at 1 σ . A flat RC ( γ = 0) is excluded at the 3 σ level.”
From The rotation curve of the Milky Way: State of the art, the Keplerian decline debate, and implications for dark matter (2026) · cites this paper as Jiao et al. (2023)
Split into 2 atoms — 1 confirmed, 1 partially supported, 0 disputed, 0 misattributed, 0 unverifiable. Expand the claim to see per-atom verdicts.
Experimental — accuracy not yet measuredOu et al. (2024) used an axisymmetric Jeans analysis but neglected the vertical cross-term in equation (22), estimating its omission as one contribution to their systematic error budget; their quoted systematic uncertainties remain small out to about 20 kpc and grow rapidly beyond 22 kpc, where the asymmetric-drift contribution alone reaches the ∼15% level (Jiao et al., 2023).
“Ou et al. (2024) used an axisymmetric Jeans analysis but neglected the vertical cross-term in equation (22), estimating its omission as one contribution to their systematic error budget. Their quoted systematic uncertainties remain small out to about 20 kpc and grow rapidly beyond 22 kpc, where the asymmetric-drift contribution alone reaches the ∼ 15% level (Jiao et al., 2023)”
From The rotation curve of the Milky Way: State of the art, the Keplerian decline debate, and implications for dark matter (2026) · cites this paper as Jiao et al., 2023
Split into 2 atoms — 0 confirmed, 2 partially supported, 0 disputed, 0 misattributed, 0 unverifiable. Expand the claim to see per-atom verdicts.
Experimental — accuracy not yet measuredBoth RCs decline with a very similar linear slope, β = -(2.18 ± 0.23) km s^-1 kpc^-1 for Jiao et al. (2023) and β = -(2.22 ± 0.20) km s^-1 kpc^-1 for Ou et al. (2024).
“Both RCs decline with a very similar linear slope, β = -(2 . 18 ± 0 . 23) km s -1 kpc -1 for their own measurement and β = -(2 . 22 ± 0 . 20) km s -1 kpc -1 for that of Ou et al. (2024).”
From The rotation curve of the Milky Way: State of the art, the Keplerian decline debate, and implications for dark matter (2026) · cites this paper as Jiao et al. (2023)
Section 4.1 reports both slopes exactly as quoted and says the two rotation curves decline similarly. It attributes the second slope to Ou et al. (2023), however, not Ou et al. (2024). (LLM, conf=0.90)
Experimental — accuracy not yet measuredJiao et al. (2023) re-derived the RC of Wang et al. (2023) with a revised binning and a full systematic error budget, and compared it with a preliminary version of Ou et al. (2024) after reconciling their different distance scales.
“Jiao et al. (2023) re-derived the RC of Wang et al. (2023) with a revised binning and a full systematic error budget, and compared it with a preliminary version of Ou et al. (2024) (circulated as Ou et al. 2023 on arXiv at the time of submission), after carefully reconciling their different distance scales;”
From The rotation curve of the Milky Way: State of the art, the Keplerian decline debate, and implications for dark matter (2026) · cites this paper as Jiao et al. (2023)
Section 2.1 describes recalculating Wang et al.’s rotation curve with adjusted binning, and §2.2.5 describes error bars incorporating systematic uncertainties. The paper compares its curve with Ou et al. (2023), listed in its references as an arXiv preprint. But Appendix B’s distance correction concerns Zhou et al. (2023), not a reconciliation of Wang’s and Ou’s distance scales; it also calls that correction very rough. (LLM, conf=0.88)
Experimental — accuracy not yet measured
The Keplerian behaviour is not a feature of the Jiao et al. reanalysis alone: although neither Wang et al. (2023) nor Ou et al. (2024) explicitly claim a Keplerian decline, the outer slopes of their own RCs, taken at face value, are consistent with one.
“It is worth stressing that the Keplerian behaviour is not a feature of the Jiao et al. reanalysis alone: although neither Wang et al. (2023) nor Ou et al. (2024) explicitly claim a Keplerian decline, the outer slopes of their own RCs, taken at face value, are consistent with one”
From The rotation curve of the Milky Way: State of the art, the Keplerian decline debate, and implications for dark matter (2026) · cites this paper as Jiao et al. (2023)
Split into 2 atoms — 0 confirmed, 1 partially supported, 0 disputed, 0 misattributed, 1 unverifiable. Expand the claim to see per-atom verdicts.
Experimental — accuracy not yet measuredThe inferred spherical-equivalent mass within 30 kpc, Msph,30 approximately 2.6 × 10^11 solar masses, exceeds the strict Keplerian spherical-equivalent total of 2.06 × 10^11 solar masses (Jiao et al., 2023).
“The inferred spherical-equivalent mass within 30 kpc, M sph , 30 ≈ 2 . 6 × 10 11 M ⊙ , exceeds the strict Keplerian sphericalequivalent total of 2 . 06 × 10 11 M ⊙ (Jiao et al., 2023).”
From The rotation curve of the Milky Way: State of the art, the Keplerian decline debate, and implications for dark matter (2026) · cites this paper as Jiao et al. (2023)
The Conclusions report an average total Milky Way mass of 2.06 × 10^11 solar masses, supporting that number. But §5.3 gives approximately 1.95 × 10^11 solar masses for the Keplerian-decline fit and 1.9–2.0 × 10^11 solar masses for the enclosed mass beyond 19 kpc. The cited paper does not identify 2.06 × 10^11 as a strict Keplerian spherical-equivalent total or report the claimed 2.6 × 10^11 within 30 kpc. (LLM, conf=0.87)
Experimental — accuracy not yet measuredThe lower inner-plateau velocity reflects the weight of the Jiao et al. (2023) points in the compilation, which lie about 5 km/s below the RGB-based curves at R < 13 kpc and are referred to R⊙ = 8.34 kpc.
“this reflects the weight of the Jiao et al. (2023) points in the compilation, which lie ∼ 5 km s -1 below the RGBbased curves at R < 13 kpc and are referred to R ⊙ = 8 . 34 kpc.”
From The rotation curve of the Milky Way: State of the art, the Keplerian decline debate, and implications for dark matter (2026) · cites this paper as Jiao et al. (2023)
Section 4.1 says the paper’s rotation-curve points are slightly lower than Ou et al.’s RGB-based curve at R = 9–13 kpc. A note on p. 5 gives R⊙ = 8.34 kpc for this curve. The paper does not quantify the difference as approximately 5 km/s or establish it for all R < 13 kpc; the compilation’s weighting is the citing authors’ own explanation. (LLM, conf=0.86)
Experimental — accuracy not yet measuredThe equilibrium assumption is less problematic for the Milky Way disc than for many external spirals because the Milky Way's last major merger was about 10 Gyr ago, whereas a typical spiral of comparable mass had its last major merger on average about 6 Gyr ago.
“The last major merger experienced by the MW (Gaia-Sausage-Enceladus) dates back to ∼ 10 Gyr ago, whereas a typical spiral of comparable mass experienced its last major merger more recently, on average ∼ 6 Gyr ago (see Jiao et al., 2023, and references therein). The equilibrium assumption is therefore less problematic for the MWdisc than for many external spirals, and in particular than for M31.”
From The rotation curve of the Milky Way: State of the art, the Keplerian decline debate, and implications for dark matter (2026) · cites this paper as Jiao et al. (2023)
Split into 2 atoms — 1 confirmed, 1 partially supported, 0 disputed, 0 misattributed, 0 unverifiable. Expand the claim to see per-atom verdicts.
Experimental — accuracy not yet measuredSeveral analyses now find a velocity decline in the Milky Way rotation curve beyond R ≈ 15 kpc.
“Gaia DR3 has changed the picture: several analyses now find a velocity decline beyond R ≈ 15 kpc”
From The rotation curve of the Milky Way: State of the art, the Keplerian decline debate, and implications for dark matter (2026) · cites this paper as Jiao et al., 2023
For plausible outer-disc tracer profiles the quadratic asymmetric drift correction is va ∼ 30-55 km s^-1, and even a 30% error in va shifts vc by only ∼1-4 km s^-1, below the ∼30 km s^-1 outer-disc decline claimed by Jiao et al. (2023).
“For plausible outer-disc tracer profiles the quadratic correction is va ∼ 30-55 km s -1 (the toy value above lies at the upper end), it propagates into the inferred circular speed weakly, since v 2 c = ⟨ v ϕ ⟩ 2 + v 2 a implies δ vc ≈ ( va / vc ) δ va . For this range of va and vc ≈ 230 km s -1 , even a 30% error in va shifts vc by only ∼ 1-4 km s -1 , below the ∼ 30 km s -1 outer-disc decline”
From The rotation curve of the Milky Way: State of the art, the Keplerian decline debate, and implications for dark matter (2026) · cites this paper as Jiao et al. (2023)
The subsequent DR3-based analyses of Wang et al. (2023), Jiao et al. (2023), and Ou et al. (2024) all find a steeper decline at R > 15 kpc.
“The subsequent DR3-based analyses of Wang et al. (2023), Jiao et al. (2023), and Ou et al. (2024) all find a steeper decline at R > 15 kpc, with the extreme interpretation of Jiao et al. (2023) claiming a Keplerian decline and a total mass nearly five times lower.”
From The rotation curve of the Milky Way: State of the art, the Keplerian decline debate, and implications for dark matter (2026) · cites this paper as Jiao et al., 2023
Jiao et al. (2023) quote 2.06 +0.24 -0.13 × 10^11 M⊙ for their preferred total mass and a strict upper limit of 5.4 × 10^11 M⊙.
“Jiao et al. (2023) quote 2 . 06 + 0 . 24 -0 13 × 10 11 M ⊙ for their preferred total mass and a strict upper limit of 5 . 4 × 10 11 M ⊙ .”
From The rotation curve of the Milky Way: State of the art, the Keplerian decline debate, and implications for dark matter (2026) · cites this paper as Jiao et al. (2023)
Klačka & Šturc (2025) showed that in the best-fit mass models of Jiao et al. (2023) and Ou et al. (2024), the spherically distributed dark matter halo accounts for at least 88% of the total radial gravitational acceleration at R = 27 kpc.
“Klaˇ cka & Šturc (2025) showed that in the best-fit mass models of Jiao et al. (2023) and Ou et al. (2024), the spherically distributed DM halo accounts for ≳ 88% of the total radial gravitational acceleration at R = 27 kpc”
From The rotation curve of the Milky Way: State of the art, the Keplerian decline debate, and implications for dark matter (2026) · cites this paper as Jiao et al. (2023)
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Cites
<i>Planck</i> 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 · see citing works
Foreman-Mackey, D., Hogg, D. W., Lang, D., & Goodman, J. (2013) · Publications of the Astronomical Society of the Pacific · doi:10.1086/670067 · Cited by 13,362 · see citing works
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 · see citing works
Hinshaw, G., Larson, D., Komatsu, E., Spergel, D. N., Bennett, C. L., Dunkley, J., Nolta, M. R., Halpern, M., Hill, R. S., Odegard, N., et al. (2013) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/208/2/19 · Cited by 5,121 · see citing works
Galactic Dynamics: Second Edition
Binney, J., & Tremaine, S. (2008) · doi:10.1515/9781400828722 · Cited by 4,375 · see citing works
Vallenari, A., Brown, A. G. A., Prusti, T., de Bruijne, J. H. J., Arenou, F., Babusiaux, C., Biermann, M., Creevey, O. L., Ducourant, C., Evans, D. W., et al. (2022) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202243940 · Cited by 4,225 · see citing works
An iterative technique for the rectification of observed distributions
Lucy, L. B. (1974) · The Astronomical Journal · doi:10.1086/111605 · Cited by 3,866 · see citing works
The Milky Way Tomography with SDSS. I. Stellar Number Density Distribution
Jurić, M., Ivezić, Ž., Brooks, A. M., Lupton, R. H., Schlegel, D. J., Finkbeiner, D. P., Padmanabhan, N., Bond, N., Sesar, B., Rockosi, C. M., et al. (2008) · The Astrophysical Journal · doi:10.1086/523619 · Cited by 1,318 · see citing works
The merger that led to the formation of the Milky Way’s inner stellar halo and thick disk
Helmi, A., Babusiaux, C., Koppelman, H. H., Massari, D., Veljanoski, J., & Brown, A. G. A. (2018) · Nature · doi:10.1038/s41586-018-0625-x · Cited by 1,235 · see citing works
Lindegren, L., Klioner, S. A., Hernández, J., Bombrun, A., Ramos-Lerate, M., Steidelmüller, H., Bastian, U., Biermann, M., de Torres, A., Gerlach, E., et al. (2020) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202039709 · Cited by 1,200 · see citing works
Lindegren, L., Bastian, U., Biermann, M., Bombrun, A., de Torres, A., Gerlach, E., Geyer, R., Hernández, J., Hilger, T., Hobbs, D., et al. (2020) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202039653 · Cited by 1,037 · see citing works
Co-formation of the disc and the stellar halo★
Belokurov, V, Erkal, D., Evans, N. W., Koposov, S. E., & Deason, A. J. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty982 · Cited by 1,020 · see citing works
HIGH-RESOLUTION ROTATION CURVES AND GALAXY MASS MODELS FROM THINGS
de Blok, W. J. G., Walter, F., Brinks, E., Trachternach, C., Oh, S.-H., & Kennicutt, R. C. (2008) · The Astronomical Journal · doi:10.1088/0004-6256/136/6/2648 · Cited by 940 · see citing works
The Ghost of Sagittarius and Lumps in the Halo of the Milky Way
Newberg, H. J., Yanny, B., Rockosi, C., Grebel, E. K., Rix, H., Brinkmann, J., Csabai, I., Hennessy, G., Hindsley, R. B., Ibata, R., et al. (2002) · The Astrophysical Journal · doi:10.1086/338983 · Cited by 760 · see citing works
Rubin, V. C., Thonnard, N., & K., J. F. W. (1978) · The Astrophysical Journal · doi:10.1086/182804 · Cited by 594 · see citing works
Bovy, J., & Rix, H.-W. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/779/2/115 · Cited by 523 · see citing works
The Circular Velocity Curve of the Milky Way from 5 to 25 kpc
Eilers, A.-C., Hogg, D. W., Rix, H.-W., & Ness, M. K. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/aaf648 · Cited by 404 · see citing works
Koposov, S. E., Rix, H.-W., & Hogg, D. W. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/712/1/260 · Cited by 403 · see citing works
Besla, G., Kallivayalil, N., Hernquist, L., van der Marel, R. P., Cox, T. J., & Kereš, D. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.20466.x · Cited by 400 · see citing works
Haywood, M., Di Matteo, P., Lehnert, M. D., Snaith, O., Khoperskov, S., & Gómez, A. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aad235 · Cited by 360 · see citing works
The Milky Way total mass profile as inferred from Gaia DR2
Cautun, M., Benitez-Llambay, A., Deason, A. J., Frenk, C. S., Fattahi, A., Gómez, F. A., Grand, R. J. J., Oman, K. A., Navarro, J. F., & Simpson, C. M. (2019) · arXiv · doi:10.48550/arxiv.1911.04557 · Cited by 335
The milky way total mass profile as inferred from Gaia DR2
Cautun, M., Benítez-Llambay, A., Deason, A. J., Frenk, C. S., Fattahi, A., Gómez, F. A., Grand, R. J. J., Oman, K. A., Navarro, J. F., & Simpson, C. M. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa1017 · Cited by 332 · see citing works
Sofue, Y., Honma, M., & Omodaka, T. (2009) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/61.2.227 · Cited by 314 · see citing works
The Circular Velocity Curve of the Milky Way from 5 to 25 kpc
Eilers, A., Hogg, D., Rix, H., & Ness, M. (2019) · MPG.PuRe (Max Planck Society) · Cited by 303 · see citing works
Tango for three: Sagittarius, LMC, and the Milky Way
Vasiliev, E., Belokurov, V., & Erkal, D. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa3673 · Cited by 285 · see citing works
van der Kruit, P. C., & Freeman, K. C. (2011) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-083109-153241 · Cited by 283 · see citing works
Does the Milky Way Have a Maximal Disk?
Sackett, P. D. (1997) · The Astrophysical Journal · doi:10.1086/304223 · Cited by 273 · see citing works
One ring to encompass them all: a giant stellar structure that surrounds the Galaxy
Ibata, R., Irwin, M. J., Lewis, G. F., Ferguson, A. M. N., & Tanvir, N. R. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06545.x · Cited by 269 · see citing works
The Milky Way, an Exceptionally Quiet Galaxy: Implications for the Formation of Spiral Galaxies
Hammer, F., Puech, M., Chemin, L., Flores, H., & Lehnert, M. D. (2007) · The Astrophysical Journal · doi:10.1086/516727 · Cited by 261 · see citing works
Self-citationDid most present-day spirals form during the last 8 Gyr?
Hammer, F., Flores, H., Elbaz, D., Zheng, X., Liang, Y. C., & Cesarsky, C. J. (2005) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20041471 · Cited by 243 · see citing works
Self-citationModeling the Galactic Bar Using Red Clump Giants
Stanek, K. Z., Udalski, A., Szymański, M. K., Kałużny, J., Kubiak, Z. M., Mateo, M. L., & Krzeminski, W. (1997) · The Astrophysical Journal · doi:10.1086/303702 · Cited by 240 · see citing works
RINGS AND RADIAL WAVES IN THE DISK OF THE MILKY WAY
Xu, Y., Newberg, H. J., Carlin, J. L., Liu, C., Deng, L., Li, J., Schönrich, R. A., & Yanny, B. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/801/2/105 · Cited by 235 · see citing works
Posti, L., & Helmi, A. (2019) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201833355 · Cited by 233 · see citing works
MAPPING THE STELLAR STRUCTURE OF THE MILKY WAY THICK DISK AND HALO USING SEGUE PHOTOMETRY
de Jong, J. T. A., Yanny, B., Rix, H.-W., Dolphin, A. E., Martin, N. F., & Beers, T. C. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/714/1/663 · Cited by 231 · see citing works
Laporte, C. F. P., Johnston, K. V., Gómez, F. A., Garavito-Camargo, N., & Besla, G. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty1574 · Cited by 230 · see citing works
GLOBULAR CLUSTER STREAMS AS GALACTIC HIGH-PRECISION SCALES—THE POSTER CHILD PALOMAR 5
Küpper, A. H. W., Balbinot, E., Bonaca, A., Johnston, K. V., Hogg, D. W., Kroupa, P., & Santiago, B. X. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/803/2/80 · Cited by 209 · see citing works
THE SPACE MOTION OF LEO I: THE MASS OF THE MILKY WAY'S DARK MATTER HALO
Boylan-Kolchin, M., Bullock, J. S., Sohn, S. T., Besla, G., & van der Marel, R. P. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/768/2/140 · Cited by 204 · see citing works
Evidence for dark matter in the inner Milky Way
Iocco, F., Pato, M., & Bertone, G. (2015) · Nature Physics · doi:10.1038/nphys3237 · Cited by 192 · see citing works
On the estimation of the local dark matter density using the rotation curve of the Milky Way
de Salas, P. F., Malhan, K., Freese, K., Hattori, K., & Valluri, M. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/10/037 · Cited by 176 · see citing works
Noordermeer, E., van der Hulst, J. M., Sancisi, R., Swaters, R. A., & van Albada, T. S. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.11533.x · Cited by 171 · see citing works
Rotation Curve of the Milky Way from Classical Cepheids
Mróz, P., Udalski, A., Skowron, D. M., Skowron, J., Soszyński, I., Pietrukowicz, P., Szymański, M. K., Poleski, R., Kozłowski, S., & Ulaczyk, K. (2019) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/aaf73f · Cited by 153 · see citing works
Drimmel, R., Romero-Gómez, M., Chemin, L., Ramos, P., Poggio, E., Ripepi, V., Andrae, R., Blomme, R., Cantat-Gaudin, T., Castro-Ginard, A., et al. (2022) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202243797 · Cited by 149 · see citing works
Self-citationAnalytical properties of Einasto dark matter haloes
Retana-Montenegro, E., Hese, E. V., Gentile, G., Baes, M., & Frutos─Alfaro, F. (2012) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201118543 · Cited by 148 · see citing works
The dark matter profile of the Milky Way inferred from its circular velocity curve
Ou, X., Eilers, A., Necib, L., & Frebel, A. (2024) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stae034 · Cited by 132 · see citing works
Infall times for Milky Way satellites from their present-day kinematics
Rocha, M., Peter, A. H. G., & Bullock, J. S. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21432.x · Cited by 125 · see citing works
On the Self‐consistent Response of Stellar Systems to Gravitational Shocks
Gnedin, O. Y., & Ostriker, J. P. (1999) · The Astrophysical Journal · doi:10.1086/306864 · Cited by 121 · see citing works
All-sky dynamical response of the galactic halo to the large magellanic cloud
Conroy, C., Naidu, R. P., Garavito-Camargo, N., Besla, G., Zaritsky, D., Bonaca, A., & Johnson, B. D. (2021) · Nature · doi:10.1038/s41586-021-03385-7 · Cited by 120 · see citing works
Queiroz, A. B. A., Anders, F., Chiappini, C., Khalatyan, A., Santiago, B. X., Nepal, S., Steinmetz, M., Gallart, C., Valentini, M., Ponte, M. D., et al. (2023) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202245399 · Cited by 114 · see citing works
The Galactic warp revealed by Gaia DR2 kinematics
Poggio, E., Drimmel, R., Lattanzi, M. G., Smart, R. L., Spagna, A., Andrae, R., Bailer‐Jones, C. A. L., Fouesneau, M., Antoja, T., Babusiaux, C., et al. (2018) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1093/mnrasl/sly148 · Cited by 111 · see citing works
The Hubble sequence: just a vestige of merger events?
Hammer, F., Flores, H., Puech, M., Yang, Y., Athanassoula, E., Rodrigues, M., & Delgado-Serrano, R. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200912115 · Cited by 109 · see citing works
Self-citationKoposov, S. E., Erkal, D., Li, T. S., Da Costa, G. S., Cullinane, L. R., Ji, A. P., Kuehn, K., Lewis, G. F., Pace, A. B., Shipp, N., et al. (2023) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stad551 · Cited by 109 · see citing works
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Self-citationPuech, M., Hammer, F., Hopkins, P. F., Athanassoula, E., Flores, H., Rodrigues, M., Wang, J., & Yang, Y. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/753/2/128 · Cited by 69 · see citing works
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Wang, J., Hammer, F., Yang, Y., Ripepi, V., Cioni, M.-R. L., Puech, M., & Flores, H. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz1274 · Cited by 55 · see citing works
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Bergemann, M., Sesar, B., Cohen, J., Serenelli, A., Sheffield, A., Li, T. S., Casagrande, L., Johnston, K., Laporte, C., Price-Whelan, A., et al. (2018) · Nature · doi:10.1038/nature25490 · Cited by 52 · see citing works
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Karukes, E., Benito, M., Fabio Iocco, A., Trotta, R., & Geringer-Sameth, A. (2019) · Spiral (Imperial College London) · Cited by 52 · see citing works
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Wang, H.-F., López-Corredoira, M., Huang, Y., Chang, J., Zhang, H.-W., Carlin, J. L., Chen, X.-D., Chrobáková, Ž., & Chen, B. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/ab93ad · Cited by 43 · see citing works
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Dicaire, I., Claude Carignan, A., Amram, P., Marcelin, M., Hlavacek-Larrondo, J., de Denus‐Baillargeon, M., Olivier Daigle, A., & Hernandez, O. (2008) · The Astronomical Journal · doi:10.1088/0004-6256/135/6/2038 · Cited by 40 · see citing works
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Self-citationThe dark matter profile of the Milky Way inferred from its circular velocity curvePreprint
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Research works printed but not linked: 95
- Babcock, H. W. 1939, Lick Obs. Bull., 498, 41 · DOI
- Bailin, J. 2003, ApJ, 583, L79 · DOI
- Belokurov, V., Erkal, D., Evans, N. W., Koposov, S. E., & Deason, A. J. 2018, MNRAS, 478, 611 · DOI
- Bergemann, M., Sesar, B., Cohen, J. G., et al. 2018, Nature, 555, 334 · DOI
- Besla, G., Kallivayalil, N., Hernquist, L., et al. 2012, MNRAS, 421, 2109 · DOI
- Bosma, A. 1978, PhD Thesis, University of Groningen, The Netherlands
- Bovy, J., & Rix, H.-W. 2013, ApJ, 779, 115 · DOI
- Boylan-Kolchin, M., Bullock, J. S., Sohn, S. T., Besla, G., & van der Marel, R. P. 2013, ApJ, 768, 140 · DOI
- Calchi Novati, S., & Mancini, L. 2011, MNRAS, 416, 1292 · DOI
- Cautun, M., Benítez-Llambay, A., Deason, A. J., et al. 2020, MNRAS, 494, 4291 · DOI
- Chemin, L., de Blok, W. J. G., & Mamon, G. A. 2011, AJ, 142, 109 · DOI
- Chrobáková, Ž., Nagy, R., & López-Corredoira, M. 2020a, A&A, 637, A96 · DOI
- Chrobáková, Ž., López-Corredoira, M., Sylos Labini, F., Wang, H. F., & Nagy, R. 2020b, A&A, 642, A95 · DOI
- Conn, B. C., Lane, R. R., Lewis, G. F., et al. 2007, MNRAS, 376, 939 · DOI
- Conn, B. C., Noël, N. E. D., Rix, H.-W., et al. 2012, ApJ, 754, 101 · DOI
- Conroy, C., Naidu, R. P., Garavito-Camargo, N., et al. 2021, Nature, 592, 534 · DOI
- Correa Magnus, L., & Vasiliev, E. 2022, MNRAS, 511, 2610 · DOI
- de Blok, W. J. G., Walter, F., Brinks, E., et al. 2008, AJ, 136, 2648 · DOI
- de Jong, J. T. A., Yanny, B., Rix, H.-W., et al. 2010, ApJ, 714, 663 · DOI
- de Salas, P. F., Malhan, K., Freese, K., Hattori, K., & Valluri, M. 2019, JCAP, 2019, 037 · DOI
- Dicaire, I., Carignan, C., Amram, P., et al. 2008, AJ, 135, 2038 · DOI
- Eadie, G., & Jurić, M. 2019, ApJ, 875, 159 · DOI
- Eilers, A.-C., Hogg, D. W., Rix, H.-W., & Ness, M. K. 2019, ApJ, 871, 120 · DOI
- Einasto, J. 1965, Trudy Astrofizicheskogo Instituta Alma-Ata, 5, 87 · DOI
- Erkal, D., Deason, A. J., Belokurov, V., et al. 2021, MNRAS, 506, 2677 · DOI
- Foreman-Mackey, D., Hogg, D. W., Lang, D., & Goodman, J. 2013, PASP, 125, 306 · DOI
- Gaia Collaboration (Drimmel, R., et al.) 2023a, A&A, 674, A37 · DOI
- Gaia Collaboration (Vallenari, A., et al.) 2023b, A&A, 674, A1 · DOI
- Georgelin, Y. M., & Georgelin, Y. P. 1976, A&A, 49, 57 · DOI
- Gnedin, O. Y., & Ostriker, J. P. 1999, ApJ, 513, 626 · DOI
- Goodwin, S. P., Gribbin, J., & Hendry, M. A. 1998, The Observatory, 118, 201 · DOI
- Hammer, F., Flores, H., Elbaz, D., et al. 2005, A&A, 430, 115 · DOI
- Hammer, F., Puech, M., Chemin, L., Flores, H., & Lehnert, M. D. 2007, ApJ, 662, 322 · DOI
- Hammer, F., Flores, H., Puech, M., et al. 2009, A&A, 507, 1313 · DOI
- Hammer, F., Yang, Y. B., Flores, H., Puech, M., & Fouquet, S. 2015, ApJ, 813, 110 · DOI
- Hammer, F., Li, H., Mamon, G. A., et al. 2023, MNRAS, 519, 5059 · DOI
- Haywood, M., Di Matteo, P., Lehnert, M. D., et al. 2018, ApJ, 863, 113 · DOI
- Helmi, A., Babusiaux, C., Koppelman, H. H., et al. 2018, Nature, 563, 85 · DOI
- Hinshaw, G., Larson, D., Komatsu, E., et al. 2013, ApJS, 208, 19 · DOI
- Hogg, D. W., Eilers, A.-C., & Rix, H.-W. 2019, AJ, 158, 147 · DOI
- Ibata, R. A., Irwin, M. J., Lewis, G. F., Ferguson, A. M. N., & Tanvir, N. 2003, MNRAS, 340, L21 A208, page 10 of 13 · DOI
- Jiao, Y., et al.: A&A 678, A208 (2023)
- Iocco, F., Pato, M., & Bertone, G. 2015, Nat. Phys., 11, 245 · DOI
- Jiao, Y., Hammer, F., Wang, J. L., & Yang, Y. B. 2021, A&A, 654, A25 · DOI
- Johnston, K. V., Price-Whelan, A. M., Bergemann, M., et al. 2017, Galaxies, 5, 44 · DOI
- Jurić, M., Ivezić, Ž., Brooks, A., et al. 2008, ApJ, 673, 864 · DOI
- Karukes, E. V., Benito, M., Iocco, F., Trotta, R., & Geringer-Sameth, A. 2020, JCAP, 2020, 033 · DOI
- Koposov, S. E., Rix, H.-W., & Hogg, D. W. 2010, ApJ, 712, 260 · DOI
- Koposov, S. E., Erkal, D., Li, T. S., et al. 2023, MNRAS, 521, 4936 · DOI
- Küpper, A. H. W., Balbinot, E., Bonaca, A., et al. 2015, ApJ, 803, 80 · DOI
- Laporte, C. F. P., Johnston, K. V., Gómez, F. A., Garavito-Camargo, N., & Besla, G. 2018, MNRAS, 481, 286 · DOI
- Li, Z.-Z., Qian, Y.-Z., Han, J., et al. 2020, ApJ, 894, 10 · DOI
- Li, H., Hammer, F., Babusiaux, C., et al. 2021, ApJ, 916, 8 · DOI
- Li, X., Wang, H.-F., Luo, Y.-P., et al. 2023, ApJ, 943, 88 · DOI
- Lindegren, L., Bastian, U., Biermann, M., et al. 2021a, A&A, 649, A4 · DOI
- Lindegren, L., Klioner, S. A., Hernández, J., et al. 2021b, A&A, 649, A2 · DOI
- Lucchini, S., D'Onghia, E., Fox, A. J., et al. 2020, Nature, 585, 203 · DOI
- Lucchini, S., D'Onghia, E., & Fox, A. J. 2021, ApJ, 921, L36 · DOI
- Lucy, L. B. 1974, AJ, 79, 745 · DOI
- Lundmark, K. 1925, MNRAS, 85, 865 · DOI
- Mayall, N. U. 1951, Pub. Mich. Obs., 10, 19 · DOI
- Mróz, P., Udalski, A., Skowron, D. M., et al. 2019, ApJ, 870, L10 · DOI
- Navarro, J. F., Frenk, C. S., & White, S. D. M. 1997, ApJ, 490, 493 · DOI
- Newberg, H. J., Yanny, B., Rockosi, C., et al. 2002, ApJ, 569, 245 · DOI
- Noordermeer, E., van der Hulst, J. M., Sancisi, R., Swaters, R. S., & van Albada, T. S. 2007, MNRAS, 376, 1513 · DOI
- Planck Collaboration VI. 2020, A&A, 641, A6 · DOI
- Poggio, E., Drimmel, R., Lattanzi, M. G., et al. 2018, MNRAS, 481, L21 · DOI
- Posti, L., & Helmi, A. 2019, A&A, 621, A56 · DOI
- Pouliasis, E., Di Matteo, P., & Haywood, M. 2017, A&A, 598, A66 · DOI
- Puech, M., Hammer, F., Hopkins, P. F., et al. 2012, ApJ, 753, 128 · DOI
- Queiroz, A. B. A., Anders, F., Chiappini, C., et al. 2023, A&A, 673, A155 · DOI
- Retana-Montenegro, E., van Hese, E., Gentile, G., Baes, M., & Frutos-Alfaro, F. 2012, A&A, 540, A70 · DOI
- Rocha, M., Peter, A. H. G., & Bullock, J. 2012, MNRAS, 425, 231 · DOI
- Rubin, V. C., Ford, W. K., Jr., & Thonnard, N. 1978, ApJ, 225, L107 · DOI
- Sackett, P. D. 1997, ApJ, 483, 103 · DOI
- Schmidt, M. 1965, in Galactic Structure, eds. A. Blaauw, & M. Schmidt (Chicago: University of Chicago Press), 513 · DOI
- Slizewski, A., Dufresne, X., Murdock, K., et al. 2022, ApJ, 924, 131 · DOI
- Sofue, Y., Honma, M., & Omodaka, T. 2009, PASJ, 61, 227 · DOI
- Stanek, K. Z., Udalski, A., Szyma Ński, M., et al. 1997, ApJ, 477, 163 · DOI
- Sylos Labini, F., Chrobáková, Ž., Capuzzo-Dolcetta, R., & López-Corredoira, M. 2023, ApJ, 945, 3 · DOI
- Urrejola-Mora, C., Gómez, F. A., Torres-Flores, S., et al. 2022, ApJ, 935, 20 · DOI
- van der Kruit, P. C., & Freeman, K. C. 2011, ARA&A, 49, 301 · DOI
- Vasiliev, E., Belokurov, V., & Erkal, D. 2021, MNRAS, 501, 2279 · DOI
- Wang, J., Shi, J., Pan, K., et al. 2016, MNRAS, 460, 3179 · DOI
- Wang, H.-F., Liu, C., Xu, Y., Wan, J.-C., & Deng, L. 2018, MNRAS, 478, 3367 · DOI
- Wang, J., Hammer, F., Yang, Y., et al. 2019, MNRAS, 486, 5907 · DOI
- Wang, H. F., López-Corredoira, M., Huang, Y., et al. 2020, ApJ, 897, 119 · DOI
- Wang, J., Hammer, F., & Yang, Y. 2022a, MNRAS, 515, 940 · DOI
- Wang, J., Hammer, F., & Yang, Y. 2022b, MNRAS, 510, 2242 · DOI
- Wang, H.-F., Chrobáková, Ž., López-Corredoira, M., & Sylos Labini, F. 2023a, ApJ, 942, 12 · DOI
- Wang, J., Cao, Z., Huang, Y., & Yuan, H. 2023b, Res. Astron. Astrophys., 23, 025020 · DOI
- Wegg, C., Gerhard, O., & Portail, M. 2016, MNRAS, 463, 557 · DOI
- Xu, Y., Newberg, H. J., Carlin, J. L., et al. 2015, ApJ, 801, 105 · DOI
- Zhou, Y., Li, X., Huang, Y., & Zhang, H. 2023, ApJ, 946, 73 · DOI
- Zobnina, D. I., & Zasov, A. V. 2020, Astron. Rep., 64, 295 A208, page 11 of 13 · DOI
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García-Bellido, J., & Hawkins, M. (2024) · Universe · doi:10.3390/universe10120449 · Cited by 19 · see citing works
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Kroupa, P., Pflamm-Altenburg, J., Mazurenko, S., Wu, W., Thies, I., Jadhav, V. V., & Jeřábková, T. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad4c66 · Cited by 19 · see citing works
Vitral, E., van der Marel, R. P., Sohn, S. T., Libralato, M., del Pino, A., Watkins, L. L., Bellini, A., Walker, M. G., Besla, G., Pawlowski, M. S., et al. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad571c · Cited by 18 · see citing works
The Escape Velocity Profile of the Milky Way from Gaia DR3
Roche, C., Necib, L., Lin, T., Ou, X., & Nguyên, T. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad58d7 · Cited by 17 · see citing works
A review of basic results on the Bose–Einstein condensate dark matter model
Chavanis, P.-H. (2025) · Frontiers in Astronomy and Space Sciences · doi:10.3389/fspas.2025.1538434 · Cited by 16 · see citing works
Entering the window of primordial black hole dark matter with x-ray microlensing
Tamta, M., Raj, N., & Sharma, P. (2025) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.111.043043 · Cited by 21 · see citing works
Koop, O., Antoja, T., Helmi, A., Callingham, T. M., & Laporte, C. F. P. (2024) · Astronomy & Astrophysics · doi:10.1051/0004-6361/202450911 · Cited by 14 · see citing works
Murase, K., Narita, Y., & Yin, W. (2025) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2025/10/109 · Cited by 13 · see citing works
Mróz, P., Udalski, A., Szymański, M. K., Soszyński, I., Pietrukowicz, P., Kozłowski, S., Poleski, R., Skowron, J., Skowron, D. M., Ulaczyk, K., et al. (2025) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/adf842 · Cited by 13 · see citing works
A non-axisymmetric potential for the Milky Way disk
Khalil, Y. R., Famaey, B., Monari, G., Bernet, M., Siebert, A., Ibata, R., Thomas, G. F., Ramos, P., Antoja, T., Li, C., et al. (2025) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202453077 · Cited by 11 · see citing works
Generalized Rotation Curves of the Milky Way from the GAIA DR3 Data Set: Constraints on Mass Models
Sylos Labini, F. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad88f1 · Cited by 9 · see citing works
emPDF : inferring the Milky Way mass with data-driven distribution function in phase space
Li, Z., Han, J., Wang, W., Qian, Y.-Z., Li, Q., Jing, Y., & Li, T. S. (2025) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staf358 · Cited by 9 · see citing works
The inner rotation curve of the Milky Way
Sofue, Y., & Kohno, M. (2025) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/psaf114 · Cited by 9 · see citing works
Space astrometry with Gaia: Advances in understanding our Galaxy
Perryman, M. A. C. (2025) · Physics Reports · doi:10.1016/j.physrep.2025.09.004 · Cited by 8 · see citing works
Mestre, M. F., Argüelles, C. R., Carpintero, D. D., Crespi, V., & Krut, A. (2024) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202348626 · Cited by 7 · see citing works
An overlooked source of uncertainty in the mass of the Milky Way
Oman, K. A., & Riley, A. H. (2024) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1093/mnrasl/slae042 · Cited by 7 · see citing works
Dark matter fraction derived from the m31 rotation curve
Hammer, F., Yang, Y. B., Amram, P., Chemin, L., Mamon, G. A., Wang, J. L., Akib, I., Jiao, Y. J., & Wang, H. F. (2025) · Astronomy & Astrophysics · doi:10.1051/0004-6361/202452753 · Cited by 6 · see citing works
Self-citationFirst measurement of the triaxiality of the inner dark matter halo of the Milky Way
Woudenberg, H. C., & Helmi, A. (2024) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202451743 · Cited by 6 · see citing works
Halim, A. A., Abreu, P., Aglietta, M., Allekotte, I., Cheminant, K. A., Almela, A., Aloisio, R., Álvarez-Muñiz, J., Yebra, J. A., Anastasi, G. A., et al. (2024) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.109.l081101 · Cited by 6 · see citing works
Shimoda, J., Inutsuka, S., & Nagashima, M. (2024) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/psad081 · Cited by 6 · see citing works
Bar-driven Streaming Motions Mimic a Massive Bulge in the Inner Milky Way
Baba, J. (2025) · The Astrophysical Journal · doi:10.3847/1538-4357/adf2a3 · Cited by 5 · see citing works
Exploring sub-GeV dark matter physics with cosmic ray and future telescopes
Wang, G.-S., Su, B., Zu, L., & Feng, L. (2025) · The European Physical Journal C · doi:10.1140/epjc/s10052-025-14998-x · Cited by 5 · see citing works
The Milky Way accretion history compared to cosmological simulations
Hammer, F., Jiao, Y., Mamon, G. A., Yang, Y., Akib, I., Amram, P., Wang, H. F., Wang, J., & Chemin, L. (2024) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202451381 · Cited by 5 · see citing works
Self-citationThe accretion history of the Milky Way
Yang, Y., Caffau, E., Bonifacio, P., Hammer, F., Wang, J., & Mamon, G. A. (2024) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202451233 · Cited by 5 · see citing works
Self-citationIcarus Revisited: An Ancient, Metal-poor Accreted Stellar Stream in the Disk of the Milky Way
Fiorentin, P. R., Spagna, A., Lattanzi, M. G., Cignoni, M., & Vitali, S. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad8887 · Cited by 5 · see citing works
Yang, S., Lu, J., Li, W., Xu, M., & Xu, J. (2025) · The European Physical Journal C · doi:10.1140/epjc/s10052-025-14640-w · Cited by 4 · see citing works
Radio-frequency WIMP search with the MeerKAT galaxy cluster legacy survey
Lavis, N., Sarkis, M., Beck, G., & Knowles, K. (2023) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.108.123536 · Cited by 4 · see citing works
Milky Way Dark Matter Distribution or MOND Test from Vertical Stellar Kinematics with Gaia DR3
López-Corredoira, M. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad94f5 · Cited by 4 · see citing works
Cosmological implications of the <i>Gaia</i> Milky Way declining rotation curve
Coquery, E., & Blanchard, A. (2025) · Astronomy & Astrophysics · doi:10.1051/0004-6361/202556337 · Cited by 3 · see citing works
On the baryon budget in the X-ray-emitting circumgalactic medium of Milky Way-mass galaxies
Zhang, Y., Shreeram, S., Ponti, G., Comparat, J., Merloni, A., Qu, Z., Li, J., Bregman, J. N., & Fang, T. (2025) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202556835 · Cited by 3 · see citing works
Akib, I., Hammer, F., Yang, Y., Pawlowski, M. S., & Wang, J. (2025) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202452131 · Cited by 3 · see citing works
Self-citationWilliams, L. L. R., Hjorth, J., & Skillman, E. D. (2025) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2025/08/052 · Cited by 3 · see citing works
Krut, A., Argüelles, C. R., & Chavanis, P.-H. (2025) · Physical review. D/Physical review. D. · doi:10.1103/346d-d17c · Cited by 3 · see citing works
Asymmetric warm dark matter: from cosmological asymmetry to chirality of life
Yin, W., Nakagawa, S., Murokoshi, T., & Hattori, M. (2025) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2025/02/063 · Cited by 3 · see citing works
Zhu, Y. (2024) · Preprints.org · doi:10.20944/preprints202402.1765.v3 · Cited by 3 · see citing works
Implications of the Milky Way declining rotation curve
Moffat, J. W., Sharron, H., & Toth, V. T. (2025) · International Journal of Modern Physics D · doi:10.1142/s0218271825500348 · Cited by 2 · see citing works
A Strong Falsification of the Universal Radial Acceleration Relation in Galaxies
Chan, M. H. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad1e60 · Cited by 2 · see citing works
Dark matter: what is it, and can quantum sensors help find it?
Devlin, J. A. (2024) · Contemporary Physics · doi:10.1080/00107514.2025.2513120 · Cited by 2 · see citing works
Constraints on superheavy dark matter decaying into $$h\nu $$, $$Z\nu $$ and $$W\ell $$
Deligny, O. (2025) · The European Physical Journal C · doi:10.1140/epjc/s10052-025-14736-3 · Cited by 2 · see citing works
A Low-mass Model of the Milky Way: The Disk Warp Resulting from a Galaxy Merger
Deng, M., Du, C., Zhang, J., Liu, H., & Li, Z. (2026) · The Astrophysical Journal · doi:10.3847/1538-4357/ae3bd3 · Cited by 2 · see citing works
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 · see citing works
Nagao, K. I., Naka, T., & Nomura, T. (2025) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2025/04/030 · Cited by 2 · see citing works
Ou, X., Necib, L., Wetzel, A. R., Frebel, A., Bailin, J., & Oeur, M. (2025) · The Astrophysical Journal · doi:10.3847/1538-4357/ae0b63 · Cited by 2 · see citing works
Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections
Li, Q., Iminniyaz, H., & Liu, F. (2025) · Fortschritte der Physik · doi:10.1002/prop.70026 · Cited by 1 · see citing works
Milky Way Mass Through Escape Velocity Curve from LAMOST K Giants
Wu, Y., Li, H., Huang, Y., Xue, X.-X., & Zhao, G. (2025) · The Astrophysical Journal · doi:10.3847/1538-4357/adf2a4 · Cited by 1 · see citing works
Crespi, V., Argüelles, C. R., Becerra‐Vergara, E. A., Mestre, M. F., Peißker, F., Rueda, J. A., & RUFFINI, R. J. (2025) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staf1854 · Cited by 1 · see citing works
Stellar kinematics of the Milky Way Galaxy in post-Newtonian gravity
Biswas, S. (2025) · New Astronomy · doi:10.1016/j.newast.2025.102499 · Cited by 1 · see citing works
The rotation curve of the Milky Way measured by classical Cepheids from <i>Gaia</i> DR3
Feng, Q., Huang, Y., Zhang, H., & Liu, J. (2026) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stag011 · Cited by 2 · see citing works
Singh, A., & Desai, S. (2026) · Astrophysics and Space Science · doi:10.1007/s10509-026-04589-x · Cited by 1 · see citing works
Updated Constraints on the Injection Energy of Positrons Generating the Galactic 511 keV γ -Ray Line
Anonymous, Krumholz, M. R., Crocker, R. M., Siegert, T., & Eisenberger, L. (2026) · Physical Review Letters · doi:10.1103/7v14-g7tf · Cited by 1 · see citing works
General Relativity Can Explain Dark Matter without Exotic Matter
Corre, S. L. (2024) · OALib · doi:10.4236/oalib.1111149 · Cited by 1 · see citing works
The Schwarzschild–de Sitter Metric of Nonlocal dS Gravity
Dimitrijević, I., Dragovich, B. G., Rakić, Z., & Stanković, J. (2024) · Symmetry · doi:10.3390/sym16050544 · Cited by 1 · see citing works
Keplerian Rotation Curve of the Milky Way
Colenbrander, B. G., & Hulscher, W. S. (2024) · American Journal of Modern Physics · doi:10.11648/j.ajmp.20241304.11 · Cited by 1 · see citing works
Zhu, Y. (2024) · Preprints.org · doi:10.20944/preprints202402.1765.v2 · Cited by 1 · see citing works
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 · see citing works
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.v2 · Cited by 1 · see citing works
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 · see citing works
Melchiorri, A., & Ruchika (2026) · New Astronomy Reviews · doi:10.1016/j.newar.2026.101758
“The choice of Jeans formalism at large radii Klaˇcka & Šturc (2025) showed that in the best-fit mass models of Jiao et al. (2023) and Ou et al. (2024), the spherically distributed DM halo accounts for ≳ 88% of the total radial gravitational acceleration at R = 27 kpc, and argued on this basis that…”
InfluentialHigh-energy emission from the Galactic Center
Goldwurm, A., Clavel, M., Stefano Gabici, A., & Terrier, R. (2025) · Reviews of Modern Physics · doi:10.1103/9nww-fclb · Cited by 1 · see citing works
A Possible Explanation for the Flat Curve Paradox
Haraux, A. (2024) · Lobachevskii Journal of Mathematics · doi:10.1134/s1995080224604259
Relativity CosmologyPreprint
Choi, J. (2023) · SSRN Electronic Journal · doi:10.2139/ssrn.4643365
Relativity CosmologyPreprint
Choi, J. (2023) · Preprints.org · doi:10.20944/preprints202312.2215.v1
Relativity CosmologyPreprint
Choi, J. (2024) · doi:10.31219/osf.io/j8tb3
Relativity CosmologyPreprint
Choi, J. (2024) · Preprints.org · doi:10.20944/preprints202312.2215.v2
A New Dark Matter and Dark Energy Theory Based on the Assumption of Mass VectorizationPreprint
Zhou, F. (2024) · SSRN Electronic Journal · doi:10.2139/ssrn.4692093
(2024) · International Journal of Fundamental Physical Sciences · doi:10.14331/ijfps.2024.330166
Deligny, O. (2025) · Journal of Physics Conference Series · doi:10.1088/1742-6596/3053/1/012016
The DR3 Milky Way Rotation Curve within the Framework of General Relativity Without Dark Matter
Canac, M. (2024) · Reports in Advances of Physical Sciences · doi:10.1142/s2424942424500087
A Survey of Dynamical and Gravitational Lensing Tests in Scale Invariance: The Fall of Dark Matter?
Maeder, A., & Courbin, F. (2024) · Symmetry · doi:10.3390/sym16111420
Impact of merger histories on the timing argument estimate of the Local Group mass
Akib, I., Hammer, F., & Yang, Y. (2025) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202553769
Self-citationGravitational Waves and Gravitational Lensing According to Particle Based Gravity
Hulscher, W. S. (2025) · American Journal of Modern Physics · doi:10.11648/j.ajmp.20251401.14
The Solar System: Nature and mechanicsPreprint
Ljubičić, M. (2025) · doi:10.31219/osf.io/7dpvw_v2
Newtonian Field Interaction Hypothesis and Equilibrium Potential Theory
Leportier, P. A. L. (2025) · Journal of High Energy Physics Gravitation and Cosmology · doi:10.4236/jhepgc.2025.112032
Hawkins, M. R. S. (2025) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staf736
Nonlocal de Sitter $$\sqrt{dS}$$ Gravity Model and Its Applications
Dimitrijević, I., Dragovich, B. G., Rakić, Z., & Stanković, J. (2025) · Russian Journal of Mathematical Physics · doi:10.1134/s1061920824601824
Relativity CosmologyPreprint
Choi, J. (2025) · doi:10.31219/osf.io/j8tb3_v3
Investigating the origin of the Milky Way streams
Asencio, E., Kroupa, P., & Thies, I. (2025) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202451179
On the presence of angular-velocity offsets in disc galaxies
Zimmerman, T., Tal-Or, L., & Gomel, R. (2025) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staf2170
Mkrtchyan, A., & Horns, D. (2026) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202555415
No evidence for Keplerian taper of far-out galactic rotation in the SPARC galaxy database
Bariego-Quintana, A., & Llanes–Estrada, F. J. (2026) · New Astronomy · doi:10.1016/j.newast.2026.102537
The odd primordial halo of the Milky Way implied by Gaia : A shallow core, but a steep decline
Li, P., McGaugh, S., Pawlowski, M. S., Hammer, F., & Sellwood, J. A. (2025) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202557021
Self-citationThree Models of the Gravitational Potential of the Milky Way
Бобылев, В. В., Bajkova, A. T., & Smirnov, A. A. (2025) · Astronomy Reports · doi:10.1134/s1063772925702178
Local Jeans estimates of the Galaxy’s circular velocity, based on RGB stars from the Gaia catalogue
Fedorov, P. N., Dmytrenko, A., Akhmetov, V. S., Velichko, A. B., Железняк, А. П., Khramtsov, V., Denyshchenko, S. I., Vavilova, I. B., Dobrycheva, D. V., Sergijenko, O., et al. (2026) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stag1310
The Baryonic Mass and Size of the Milky Way Galaxy from the Local Static Cosmological PerturbationsPreprint
Biswas, S. (2025) · SSRN Electronic Journal · doi:10.2139/ssrn.5520813
Dark matter in galactic structure: From the milky way to the high redshift universe
Argüelles, C. R., Becerra‐Vergara, E. A., Collazo, S., Crespi, V., Deluca, A., Krut, A., Mestre, M. F., Pelle, J., Rueda, J. A., RUFFINI, R. J., et al. (2026) · International Journal of Modern Physics D · doi:10.1142/s0218271825400188
Biswas, S. (2026) · SSRN Electronic Journal · doi:10.2139/ssrn.6193881
Role of Dark Matter in the Dynamics of Compact-Object Binaries
Argüelles, C. R., Crespi, V., Rodriguez-Ruiz, J. F., & Rueda, J. A. (2026) · Symmetry · doi:10.3390/sym18030484
Axisymmetric Jeans modelling systematically overestimates the circular speed in the inner Milky Way
Yamaguchi, T., & Baba, J. (2026) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/psag066
Rotation Curves of Galaxies: A New Theoretical Approach and Comparison With Observations
Klačka, J. (2026) · Advances in Astronomy · doi:10.1155/aa/8364318
Constraining the Geometry of Galactic Dark Matter with Gaia Data Release 3
Labini, F. S., & Capuzzo-Dolcetta, R. (2026) · The Astrophysical Journal · doi:10.3847/1538-4357/ae7be7
Synchrotron self-Compton process for constraining sub-GeV dark matter in Omega Centauri via SKA
Anonymous, Su, B., Yang, Y., Zhang, B., & Feng, L. (2026) · Physical review. D/Physical review. D. · doi:10.1103/99qh-v2fy
Self-citationInvestigation of high-quality spectra of a sample of high-radial-velocity stars
Alazzawi, J., Caffau, E., Bonifacio, P., Çal, S., Monaco, L., Sbordone, L., & Lombardo, L. (2026) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202659789
- Authors
- Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., & Yang, Y.
- Affiliations
- Centre National de la Recherche Scientifique (FR)
- Centro Ricerche Enrico Fermi (IT)
- Universidad Andrés Bello (CL)
- ORCID
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2023-10
- Volume
- 678
- Pages
- A208
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W4386437529
- Cited by
- 107
- References
- 94
- Citations by year
- 2026: 24 · 2025: 42 · 2024: 38 · 2023: 3
- FWCI
- 12.46
- Type
- journal article
- Language
- en
- Open access
- gold
- doi.org
- Licence
- Locations
- Astronomy and Astrophysics (publishedVersion, cc-by)
- arXiv (Cornell University) (submittedVersion)
- HAL (submittedVersion, cc-by)
- Springer Link (Chiba Institute of Technology) (submittedVersion)
- Repositorio Institucional Académico , Sistema de Bibliotecas Universidad Andrés Bello (UNAB) (Universidad Andrés Bello (UNAB)) (submittedVersion, cc-by)
- arXiv (Cornell University)
- Funders
- China Scholarship Council
- Centre National de la Recherche Scientifique
- Institute of High Energy Physics
- National Astronomical Observatories, Chinese Academy of Sciences
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysical Phenomena and Observations
- Keywords
- Milky Way rotation curve, galaxy mass, Gaia DR3, systematic uncertainties, distance estimates, flat rotation curves, Galactic disc
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