The DOI matches its Crossref record; 230 of the 230 references it cites were found in a registry or an index.
The Adequacy of Stellar Evolution Models for the Interpretation of the Color-Magnitude Diagrams of Resolved Stellar Populations
Abstract
▪ Abstract Most of what we know about the stellar population of nearby, resolved galaxies comes from the interpretation of their color-magnitude diagrams, by comparison with stellar evolutionary models. We review how well current stellar evolution models reproduce the properties of simple stellar populations. Emphasis is given to the regions of the color-magnitude diagram which are most useful for deriving age, metallicity, or distance of a population. Extensive comparison is made between the predictions of the most-used stellar evolution libraries, in order to estimate how model dependent the results are. The present review, written from a user perspective, aims at emphasizing the strengths and weaknesses of the models, and is intended both for observers and theoreticians. We hope to encourage observers to provide stronger observational constraints where they are needed, and to stimulate theoreticians to isolate the input physics responsible for the different behavior between models and the reasons for the discrepancies with data.
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
On the variation of the initial mass function
Kroupa, P. (2001) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2001.04022.x · Cited by 7,499
Final 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., Kennicutt, Jr., Ford, H. C., Graham, J. A., et al. (2001) · The Astrophysical Journal · doi:10.1086/320638 · Cited by 3,298
Girardi, L., Bressan, A., Bertelli, G., & Chiosi, C. (2000) · Astronomy and Astrophysics Supplement Series · doi:10.1051/aas:2000126 · Cited by 2,553
DWARF GALAXIES OF THE LOCAL GROUP
Mateo, M. (1998) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.36.1.435 · Cited by 2,362
A compilation of charged-particle induced thermonuclear reaction rates
Angulo, C., Arnould, M., Rayet, M., Descouvemont, P., Baye, D., Leclercq-Willain, C., Coc, A., Barhoumi, S., Aguer, P., Rolfs, C., et al. (1999) · Nuclear Physics A · doi:10.1016/s0375-9474(99)00030-5 · Cited by 2,265
Thermonuclear reaction rates V
Caughlan, G. R., & Fowler, W. A. (1988) · Atomic Data and Nuclear Data Tables · doi:10.1016/0092-640x(88)90009-5 · Cited by 1,465
Pietrinferni, A., Cassisi, S., Salaris, M., & Castelli, F. (2004) · The Astrophysical Journal · doi:10.1086/422498 · Cited by 1,418
Asymptotic Giant Branch Evolution and Beyond
Iben, I., & Renzini, A. (1983) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.aa.21.090183.001415 · Cited by 1,290
Girardi, L., Bertelli, G., Bressan, A., Chiosi, C., Groenewegen, M. A. T., Marigo, P., Salasnich, B., & Weiss, A. (2002) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20020612 · Cited by 1,263
Low-temperature Rosseland opacities
Alexander, D. R., & Ferguson, J. W. (1994) · The Astrophysical Journal · doi:10.1086/175039 · Cited by 1,161
Cited by
Conroy, C., Gunn, J. E., & White, M. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/699/1/486 · Cited by 1,891
Star-Formation Histories, Abundances, and Kinematics of Dwarf Galaxies in the Local Group
Tolstoy, E., Hill, V., & Tosi, M. (2009) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082708-101650 · Cited by 1,179
Weisz, D. R., Dolphin, A. E., Skillman, E. D., Holtzman, J., Gilbert, K. M., Dalcanton, J. J., & Williams, B. F. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/789/2/147 · Cited by 499
Girardi, L., Williams, B. F., Gilbert, K. M., Rosenfield, P., Dalcanton, J. J., Marigo, P., Boyer, M. L., Dolphin, A., Weisz, D. R., Melbourne, J., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/724/2/1030 · Cited by 335
Uncovering the birth of the Milky Way through accurate stellar ages with Gaia
Gallart, C., Bernard, E. J., Brook, C. B., Ruiz-Lara, T., Cassisi, S., Hill, V., & Monelli, M. (2019) · Nature Astronomy · doi:10.1038/s41550-019-0829-5 · Cited by 262
Self-citation
Metadata
- Authors
- Gallart, C., Zoccali, M., & Aparicio, A.
- Venue
- Annual Review of Astronomy and Astrophysics
- Publisher
- Annual Reviews
- Published
- 2005-09-01
- Volume
- 43
- Issue
- 1
- Pages
- 387-434
- ISSN
- 0066-4146 (ISSN-L)
- 1545-4282
- OpenAlex
- W2168664302
- Cited by
- 293
- References
- 230
- FWCI
- 1.48
- Type
- journal article
- Language
- en
- Open access
- closed
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
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: The Adequacy of Stellar Evolution Models for the Interpretation of the Color-Magnitude Diagrams of Resolved Stellar Populations. https://app.cochat.ai/papers/10.1146/annurev.astro.43.072103.150608
- The paper
- Gallart, C., Zoccali, M., & Aparicio, A. (2005). The Adequacy of Stellar Evolution Models for the Interpretation of the Color-Magnitude Diagrams of Resolved Stellar Populations. Annual Review of Astronomy and Astrophysics. https://doi.org/10.1146/annurev.astro.43.072103.150608
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.