The DOI matches its Crossref record; 28 of the 28 references it cites were found in a registry or an index.
Recovering galaxy star formation and metallicity histories from spectra using VESPA: Recovering galaxy histories using VESPA
Open accessAbstract
We introduce versatile spectral analysis (VESPA): a new method which aims to recover robust star formation and metallicity histories from galactic spectra. VESPA uses the full spectral range to construct a galaxy history from synthetic models. We investigate the use of an adaptative parametrization grid to recover reliable star formation histories on a galaxy‐by‐galaxy basis. Our goal is robustness as opposed to high‐resolution histories, and the method is designed to return high time resolution only where the data demand it. In this paper we detail the method and we present our findings when we apply VESPA to synthetic and real Sloan Digital Sky Survey (SDSS) spectroscopic data. We show that the number of parameters that can be recovered from a spectrum depends strongly on the signal‐to‐noise ratio, wavelength coverage and presence or absence of a young population. For a typical SDSS sample of galaxies, we can normally recover between two and five stellar populations. We find very good agreement between VESPA and our previous analysis of the SDSS sample with MOPED.
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
Spergel, D. N., Verde, L., Peiris, H. V., Komatsu, E., Nolta, M. R., Bennett, C. L., Halpern, M., Hinshaw, G., Jarosik, N., Kogut, A., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377226 · Cited by 10,976
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 Sloan Digital Sky Survey: Technical Summary
York, D. G., Adelman, J., Anderson, Jr., Anderson, S. F., Annis, J., Bahcall, N. A., Bakken, J. A., Barkhouser, R., Bastian, S., Berman, E., et al. (2000) · The Astronomical Journal · doi:10.1086/301513 · Cited by 10,366
Galactic Stellar and Substellar Initial Mass Function
Chabrier, G. (2003) · Publications of the Astronomical Society of the Pacific · doi:10.1086/376392 · Cited by 9,071
Solving Least Squares Problems
Lawson, C. L., & Hanson, R. J. (1995) · doi:10.1137/1.9781611971217 · Cited by 7,103
The Global Schmidt Law in Star‐forming Galaxies
Kennicutt, Jr. (1998) · The Astrophysical Journal · doi:10.1086/305588 · Cited by 5,202
Tremonti, C. A., Heckman, T. M., Kauffmann, G., Brinchmann, J., Charlot, S., White, S. D. M., Seibert, M., Peng, E. W., Schlegel, D. J., Uomoto, A., et al. (2004) · The Astrophysical Journal · doi:10.1086/423264 · Cited by 3,608
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
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
High-redshift galaxies in the Hubble Deep Field: colour selection and star formation history to z 4
Madau, P., Ferguson, H. C., Dickinson, M. E., Giavalisco, M., Steidel, C. C., & Fruchter, A. (1996) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/283.4.1388 · Cited by 2,055
Cited by
Moresco, M., Pozzetti, L., Cimatti, A., Jimenez, R., Maraston, C., Verde, L., Thomas, D., Citro, A., Tojeiro, R., & Wilkinson, D. (2016) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2016/05/014 · Cited by 1,182
Self-citationCosmology and Fundamental Physics with the Euclid Satellite
The Euclid Theory Working Group, Amendola, L., Appleby, S., Bacon, D., Baker, T., Baldi, M., Bartolo, N., Blanchard, A., Bonvin, C., Borgani, S., et al. (2013) · Living Reviews in Relativity · doi:10.12942/lrr-2013-6 · Cited by 899
Self-citationStellar Population Inference with Prospector
Johnson, B. D., Leja, J., Conroy, C., & Speagle, J. S. (2021) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/abef67 · Cited by 678
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
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
Metadata
- Authors
- Tojeiro, R., Heavens, A. F., Jimenez, R., & Panter, B.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2007-09-26
- Volume
- 381
- Issue
- 3
- Pages
- 1252-1266
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2098830799
- Cited by
- 256
- References
- 28
- FWCI
- 6.84
- 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: Recovering galaxy star formation and metallicity histories from spectra using VESPA: Recovering galaxy histories using VESPA. https://app.cochat.ai/papers/10.1111/j.1365-2966.2007.12323.x
- The paper
- Tojeiro, R., Heavens, A. F., Jimenez, R., & Panter, B. (2007). Recovering galaxy star formation and metallicity histories from spectra using VESPA: Recovering galaxy histories using VESPA. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1111/j.1365-2966.2007.12323.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.