The DOI matches its Crossref record; 68 of the 68 references it cites were found in a registry or an index.
Evolutionary stellar population synthesis at high spectral resolution: optical wavelengths
Open accessAbstract
We present the single stellar population (SSP) synthesis Results of our new synthetic stellar atmosphere models library with a spectral sampling of 0.3 Å, covering the wavelength range from 3000 to 7000 Å for a wide range of metallicities (twice solar, solar, half solar and 1/10 solar). The stellar library is composed of 1650 spectra computed with the latest improvements in stellar atmospheres. In particular, it incorporates non-local thermodynamic equilibrium (LTE) line-blanketed models for hot (Teff≥ 27 500 K), and LTE line-blanketed models (Phoenix) for cool (3000 ≤Teff≤ 4500 K) stars. Because of the high spectral resolution of this library, evolutionary synthesis models can be used to predict the strength of numerous weak absorption lines and the evolution of the profiles of the strongest lines over a wide range of ages. The SSP Results have been calculated for ages from 1 Myr to 17 Gyr using the stellar evolutionary tracks provided by the Geneva and Padova groups. For young stellar populations, our Results have a very detailed coverage of high-temperature stars with similar Results for the Padova and Geneva isochrones. For intermediate and old stellar populations, our Results, once degraded to a lower resolution, are similar to the ones obtained by other groups (limitations imposed by the stellar evolutionary physics notwidthstanding). The limitations and advantages of our models for the analysis of integrated populations are described. The full set of the stellar library and the evolutionary models are available for retrieval at the websites http://www.iaa.csic.es/~rosa and http://www.iaa.csic.es/~/sed@, or on request from the first two authors.
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
The Luminosity Function and Stellar Evolution.
Salpeter, E. E. (1955) · The Astrophysical Journal · doi:10.1086/145971 · Cited by 8,697
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
Self-citationThe host galaxies of active galactic nuclei
Kauffmann, G., Heckman, T. M., Tremonti, C., Brinchmann, J., Charlot, S., White, S. D. M., Ridgway, S. E., Brinkmann, J., Fukugita, M., Hall, P. B., et al. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2003.07154.x · Cited by 3,978
The physical properties of star-forming galaxies in the low-redshift Universe
Brinchmann, J., Charlot, S., White, S. D. M., Tremonti, C., Kauffmann, G., Heckman, T., & Brinkmann, J. (2004) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2004.07881.x · Cited by 3,290
Girardi, L., Bressan, A., Bertelli, G., & Chiosi, C. (2000) · Astronomy and Astrophysics Supplement Series · doi:10.1051/aas:2000126 · Cited by 2,553
Stellar masses and star formation histories for 105galaxies from the Sloan Digital Sky Survey
Kauffmann, G., Heckman, T. M., Simon White, D. M., Charlot, S., Tremonti, C., Brinchmann, J., Bruzual, G., Peng, E. W., Seibert, M., Bernardi, M., et al. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06291.x · Cited by 2,417
Kauffmann, G., Heckman, T. M., Tremonti, C., Brinchmann, J., Charlot, S., White, S. D. M., Ridgway, S. E., Brinkmann, J., Fukugita, M., Hall, P. B., et al. (2003) · doi:10.48550/arxiv.astro-ph/0304239 · Cited by 1,845
Kauffmann, G., Heckman, T. M., White, S. D. M., Charlot, S., Tremonti, C., Peng, E. W., Seibert, M., Brinkmann, J., Nichol, R. C., SubbaRao, M., et al. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06292.x · Cited by 1,358
Spectroscopic Confirmation of a Population of Normal Star-forming Galaxies at Redshifts z > 3
Steidel, C. C., Giavalisco, M., Pettini, M., Dickinson, M., & Adelberger, K. L. (1996) · The Astrophysical Journal · doi:10.1086/310029 · Cited by 1,309
Cited by
SDSS IV MaNGA – spatially resolved diagnostic diagrams: a proof that many galaxies are LIERs
Belfiore, F., Maiolino, R., Maraston, C., Emsellem, E., Bershady, M. A., Masters, K. L., Yan, R., Bizyaev, D., Boquien, M., Brownstein, J. R., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw1234 · Cited by 363
Fitting 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
Izotov, Y. I., Thuan, T. X., & Guseva, N. G. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu1771 · Cited by 248
Metadata
- Authors
- Delgado, R. M. G., Cerviño, M., Martins, L. P., Leitherer, C., & Hauschildt, P. H.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2005-03
- Volume
- 357
- Issue
- 3
- Pages
- 945-960
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2028207989
- Cited by
- 337
- References
- 68
- FWCI
- 11.71
- Type
- journal article
- Language
- en
- Open access
- green
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: Evolutionary stellar population synthesis at high spectral resolution: optical wavelengths. https://app.cochat.ai/papers/10.1111/j.1365-2966.2005.08692.x
- The paper
- Delgado, R. M. G., Cerviño, M., Martins, L. P., Leitherer, C., & Hauschildt, P. H. (2005). Evolutionary stellar population synthesis at high spectral resolution: optical wavelengths. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1111/j.1365-2966.2005.08692.x
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.
