The DOI matches its Crossref record; 52 of the 52 references it cites were found in a registry or an index.
A library of high resolution synthetic stellar spectra from 300 nm to 1.8 ${\rm \mu}$m with solar and α-enhanced composition
Open accessAbstract
Libraries of stellar spectra are fundamental tools for the study of stellar populations, and both empirical and synthetic libraries have been used for this purpose. In this paper, a new library of high resolution synthetic spectra is presented, ranging from the near-ultraviolet (300 nm) to the near-infrared (1.8 m). The library spans all the stellar types that are relevant to the integrated light of old and intermediate-age stellar populations in the involved spectral region (spectral types F through M and all luminosity classes). The grid was computed for metallicities ranging from [Fe/H] = –2.5 to +0.5, including both solar and α-enhanced ([ α/Fe] = 0.4) chemical compositions. The synthetic spectra are a good match to observations of stars throughout the stellar parameter space encompassed by the library and over the whole spectral region covered by the computations.
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
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
Constants of diatomic molecules
Huber, K. P., & Herzberg, G. (1979) · Molecular Spectra and Molecular Structure · doi:10.1007/978-1-4757-0961-2_2 · Cited by 5,113
Starburst99: 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
Grevesse, N., & Sauval, A. J. (1998) · Space Science Reviews · doi:10.1023/a:1005161325181 · Cited by 3,480
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
VALD–2: Progress of the Vienna Atomic Line Data Base
Kupka, F., Piskunov, N., Ryabchikova, T. A., Stempels, H. C., & Weiss, W. W. (1999) · Astronomy and Astrophysics Supplement Series · doi:10.1051/aas:1999267 · Cited by 1,579
A Stellar Spectral Flux Library: 1150–25000 Å
Pickles, A. J. (1998) · Publications of the Astronomical Society of the Pacific · doi:10.1086/316197 · Cited by 1,488
Valenti, J. A., & Fischer, D. A. (2005) · The Astrophysical Journal Supplement Series · doi:10.1086/430500 · Cited by 1,460
The Observation and Analysis of Stellar Photospheres
Gray, D. F. (2005) · Cambridge University Press eBooks · doi:10.1017/cbo9781316036570 · Cited by 1,404
Old stellar populations. 5: Absorption feature indices for the complete LICK/IDS sample of stars
Worthey, G., Faber, S. M., Gonzalez, J. J., & Burstein, D. (1994) · The Astrophysical Journal Supplement Series · doi:10.1086/192087 · Cited by 1,045
Cited by
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
Vazdekis, A., Sánchez-Blázquez, P., Falcón-Barroso, J., Cenarro, A. J., Beasley, M. A., Cardiel, N., Gorgas, J., & Peletier, R. F. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.16407.x · Cited by 802
UV-extended E-MILES stellar population models: young components in massive early-type galaxies
Vazdekis, A., Koleva, M., Ricciardelli, E., Röck, B., & Falcón-Barroso, J. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2231 · Cited by 518
Zoccali, M., Hill, V., Lecureur, A., Barbuy, B., Renzini, A., Minniti, D., Gómez, A., & Ortolani, S. (2008) · Astronomy & Astrophysics · doi:10.1051/0004-6361:200809394 · Cited by 346
Self-citationFitting the integrated spectral energy distributions of galaxies
Walcher, J., Groves, B., Budavári, T., & Dale, D. (2011) · Astrophysics and Space Science · doi:10.1007/s10509-010-0458-z · Cited by 344
Metadata
- Authors
- Coelho, P., Barbuy, B., Meléndez, J., Schiavon, R. P., & Castilho, B. V.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2005-11
- Volume
- 443
- Issue
- 2
- Pages
- 735-746
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W2051879158
- Cited by
- 411
- References
- 52
- FWCI
- 4.29
- 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 library of high resolution synthetic stellar spectra from 300 nm to 1.8 ${\rm \mu}$m with solar and α-enhanced composition. https://app.cochat.ai/papers/10.1051/0004-6361:20053511
- The paper
- Coelho, P., Barbuy, B., Meléndez, J., Schiavon, R. P., & Castilho, B. V. (2005). A library of high resolution synthetic stellar spectra from 300 nm to 1.8 ${\rm \mu}$m with solar and α-enhanced composition. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361%3A20053511
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.
