The DOI matches its Crossref record; 257 of the 257 references it cites were found in a registry or an index.
Fitting the integrated spectral energy distributions of galaxies
Open accessAbstract
Fitting the spectral energy distributions (SEDs) of galaxies is an almost universally used technique that has matured significantly in the last decade. Model predictions and fitting procedures have improved significantly over this time, attempting to keep up with the vastly increased volume and quality of available data. We review here the field of SED fitting, describing the modelling of ultraviolet to infrared galaxy SEDs, the creation of multiwavelength data sets, and the methods used to fit model SEDs to observed galaxy data sets. We touch upon the achievements and challenges in the major ingredients of SED fitting, with a special emphasis on describing the interplay between the quality of the available data, the quality of the available models, and the best fitting technique to use in order to obtain a realistic measurement as well as realistic uncertainties. We conclude that SED fitting can be used effectively to derive a range of physical properties of galaxies, such as redshift, stellar masses, star formation rates, dust masses, and metallicities, with care taken not to over-interpret the available data. Yet there still exist many issues such as estimating the age of the oldest stars in a galaxy, finer details of dust properties and dust-star geometry, and the influences of poorly understood, luminous stellar types and phases. The challenge for the coming years will be to improve both the models and the observational data sets to resolve these uncertainties. The present review will be made available on an interactive, moderated web page (sedfitting.org), where the community can access and change the text. The intention is to expand the text and keep it up to date over the coming years.
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Cites
The relationship between infrared, optical, and ultraviolet extinction
Cardelli, J. A., Clayton, G. C., & Mathis, J. S. (1989) · The Astrophysical Journal · doi:10.1086/167900 · Cited by 11,795
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
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
The Luminosity Function and Stellar Evolution.
Salpeter, E. E. (1955) · The Astrophysical Journal · doi:10.1086/145971 · Cited by 8,697
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
STAR FORMATION IN GALAXIES ALONG THE HUBBLE SEQUENCE
Kennicutt, R. C. (1998) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.36.1.189 · Cited by 6,578
The cosmological simulation code gadget-2
Springel, V. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09655.x · Cited by 6,368
The Dust Content and Opacity of Actively Star‐forming Galaxies
Calzetti, D., Armus, L., Bohlin, R. C., Kinney, A. L., Koornneef, J., & Storchi‐Bergmann, T. (2000) · The Astrophysical Journal · doi:10.1086/308692 · Cited by 5,717
THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY
Abazajian, K. N., Adelman-McCarthy, J. K., Agüeros, M. A., Allam, S. S., Prieto, C. A., An, D., Anderson, K. S. J., Anderson, S. F., Annis, J., Bahcall, N. A., et al. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/182/2/543 · Cited by 5,341
Self-citationClassification parameters for the emission-line spectra of extragalactic objects
Baldwin, J. A., Phillips, M. M., & Terlevich, R. (1981) · Publications of the Astronomical Society of the Pacific · doi:10.1086/130766 · Cited by 5,132
Cited by
A HIGHLY CONSISTENT FRAMEWORK FOR THE EVOLUTION OF THE STAR-FORMING “MAIN SEQUENCE” FROM z ∼ 0-6
Speagle, J. S., Steinhardt, C. L., Capak, P. L., & Silverman, J. D. (2014) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/214/2/15 · Cited by 1,646
CALIFA, the Calar Alto Legacy Integral Field Area survey: I. Survey presentation⋆
Sánchez, S. F., Kennicutt, R. C., Gil de Paz, A., van de Ven, G., Vílchez, J. M., Wisotzki, L., Walcher, C. J., Mast, D., Aguerri, J. A. L., Albiol-Pérez, S., et al. (2012) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201117353 · Cited by 1,254
Colours and luminosities of z = 0.1 galaxies in the eagle simulation
Trayford, J. W., Theuns, T., Bower, R. G., Schaye, J., Furlong, M., Schaller, M., Frenk, C. S., Crain, R. A., Vecchia, C. D., & McCarthy, I. G. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1461 · Cited by 251
Huang, S., Leauthaud, A., Greene, J. E., Bundy, K., Lin, Y.-T., Tanaka, M., Miyazaki, S., & Komiyama, Y. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx3200 · Cited by 113
Johnson, B. D., Weisz, D. R., Dalcanton, J. J., Johnson, L. C., Dale, D. A., Dolphin, A. E., Gil de Paz, A., Kennicutt, R. C., Lee, J. C., Skillman, E. D., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/772/1/8 · Cited by 57
Self-citation
Metadata
- Authors
- Walcher, J., Groves, B., Budavári, T., & Dale, D.
- Venue
- Astrophysics and Space Science
- Published
- 2010-08-17
- Volume
- 331
- Issue
- 1
- Pages
- 1-51
- ISSN
- 0004-640X (ISSN-L)
- 1572-946X
- OpenAlex
- W2076666823
- Cited by
- 344
- References
- 257
- FWCI
- 7.66
- Type
- journal article
- Language
- en
- Open access
- green
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