The DOI matches its Crossref record; 35 of the 35 references it cites were found in a registry or an index.
A standard stellar library for evolutionary synthesis: III. Metallicity calibration
Open accessAbstract
We extend the colour calibration of the widely used BaSeL standard stellar library (Lejeune et al. 1997, 1998) to non-solar metallicities, down to dex. Surprisingly, we find that at the present epoch it is virtually impossible to establish a unique calibration ofUBVRIJHKL colours in terms of stellar metallicity which is consistent simultaneously with both colour-temperature relations and colour-absolute magnitude diagrams (CMDs) based on observed globular cluster photometry data and on published, currently popular standard stellar evolutionary tracks and isochrones. The problem appears to be related to the long-standing incompleteness in our understanding of convection in late-type stellar evolution, but is also due to a serious lack of relevant observational calibration data that would help resolve, or at least further significant progress towards resolving this issue. In view of the most important applications of the BaSeL library, we here propose two different metallicity calibration versions: (1) the “WLBC 99” library, which consistently matches empirical colour-temperature relations and which, therefore, should make an ideal tool for the study of individual stars; and (2), the “PADOVA 2000” library, which provides isochrones from the Padova 2000 grid (Girardi et al. [CITE]) that successfully reproduce Galactic globular-cluster colour-absolute magnitude diagrams and which thus should prove particularly useful for studies of collective phenomena in stellar populations in clusters and 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 Catalog of Parameters for Globular Clusters in the Milky Way
Harris, W. E. (1996) · The Astronomical Journal · doi:10.1086/118116 · Cited by 4,500 · cited 1×
“In order to put these colour-magnitude diagrams onto the intrinsic system, the EB−V and (m-M)V values from the Harris online catalog of globular cluster parameters (Harris, 1996) were used.”
MethodStarburst99: Synthesis Models for Galaxies with Active Star Formation
Leitherer, C., Schaerer, D., Goldader, J. D., Delgado, R. M. G., Robert, C., Kune, D. F., de Mello, D. F., Devost, D., & Heckman, T. M. (1999) · The Astrophysical Journal Supplement Series · doi:10.1086/313233 · Cited by 4,126
Girardi, L., Bressan, A., Bertelli, G., & Chiosi, C. (2000) · Astronomy and Astrophysics Supplement Series · doi:10.1051/aas:2000126 · Cited by 2,553
The interstellar extinction law from 1 to 13 microns
Rieke, G. H., & Lebofsky, M. J. (1985) · The Astrophysical Journal · doi:10.1086/162827 · Cited by 2,365
JHKLM photometry - Standard systems, passbands, and intrinsic colors
Bessell, M. S., & Brett, J. M. (1988) · Publications of the Astronomical Society of the Pacific · doi:10.1086/132281 · Cited by 2,070
Spectral evolution of stellar populations using isochrone synthesis
Bruzual A., G., & Charlot, S. (1993) · The Astrophysical Journal · doi:10.1086/172385 · Cited by 1,808
Alonso, A., Arribas, S., & Martínez-Roger, C. (1999) · Astronomy and Astrophysics Supplement Series · doi:10.1051/aas:1999521 · Cited by 1,019
A standard stellar library for evolutionary synthesis: I. Calibration of theoretical spectra
Lejeune, T., Cuisinier, F., & Buser, R. (1997) · Astronomy and Astrophysics Supplement Series · doi:10.1051/aas:1997373 · Cited by 785
Self-citationBessell, M. S. (1979) · Publications of the Astronomical Society of the Pacific · doi:10.1086/130542 · Cited by 720
Abundances for globular cluster giants. I. Homogeneous metallicities for 24 clusters
Carretta, E., & Gratton, R. G. (1997) · Astronomy and Astrophysics Supplement Series · doi:10.1051/aas:1997116 · Cited by 634
Cited by
Stellar population synthesis at the resolution of 2003
Bruzual, G., & Charlot, S. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06897.x · Cited by 10,500
Self-citationConroy, C., Gunn, J. E., & White, M. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/699/1/486 · Cited by 1,891
Modeling the Panchromatic Spectral Energy Distributions of Galaxies
Conroy, C. (2013) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082812-141017 · Cited by 959
Moustakas, J., Coil, A. L., Aird, J., Blanton, M. R., Cool, R. J., Eisenstein, D. J., Mendez, A. J., Wong, K. C., Zhu, G., & Arnouts, S. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/767/1/50 · Cited by 542
STELIB: A library of stellar spectra at ${\vec R}\sim2000$
Le Borgne, J.-F., Bruzual, G., Pelló, R., Lançon, A., Rocca-Volmerange, B., Sanahuja, B., Schaerer, D., Soubiran, C., & Vílchez-Gómez, R. (2003) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20030243 · Cited by 502
Self-citation
Metadata
- Authors
- Westera, P., Lejeune, T., Buser, R., Cuisinier, F., & Bruzual, G.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2002-01
- Volume
- 381
- Issue
- 2
- Pages
- 524-538
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W4297889187
- Cited by
- 259
- References
- 35
- FWCI
- 6.35
- Type
- journal article
- Language
- en
- Open access
- bronze
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: A standard stellar library for evolutionary synthesis: III. Metallicity calibration. https://app.cochat.ai/papers/10.1051/0004-6361:20011493
- The paper
- Westera, P., Lejeune, T., Buser, R., Cuisinier, F., & Bruzual, G. (2002). A standard stellar library for evolutionary synthesis: III. Metallicity calibration. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361%3A20011493
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.