Survey design for spectral energy distribution fitting: A fisher matrix approach

Viviana Acquaviva, Eric Gawiser, Steven J. Bickerton, Norman A. Grogin, Yicheng Guo, Seong Kook Lee

Research output: Contribution to journalArticle

3 Citations (Scopus)

Abstract

The spectral energy distribution (SED) of a galaxy contains information on the galaxy's physical properties, and multi-wavelength observations are needed in order to measure these properties via SED fitting. In planning these surveys, optimization of the resources is essential. The Fisher Matrix (FM) formalism can be used to quickly determine the best possible experimental setup to achieve the desired constraints on the SED-fitting parameters. However, because it relies on the assumption of a Gaussian likelihood function, it is in general less accurate than other slower techniques that reconstruct the probability distribution function (PDF) from the direct comparison between models and data. We compare the uncertainties on SED-fitting parameters predicted by the FM to the ones obtained using the more thorough PDF-fitting techniques. We use both simulated spectra and real data, and consider a large variety of target galaxies differing in redshift, mass, age, star formation history, dust content, and wavelength coverage. We find that the uncertainties reported by the two methods agree within a factor of two in the vast majority (∼90%) of cases. If the age determination is uncertain, the top-hat prior in age used in PDF fitting to prevent each galaxy from being older than the universe needs to be incorporated in the FM, at least approximately, before the two methods can be properly compared. We conclude that the FM is a useful tool for astronomical survey design.

Original languageEnglish (US)
Article number72
JournalAstrophysical Journal
Volume749
Issue number1
DOIs
StatePublished - Apr 10 2012

Fingerprint

survey design
spectral energy distribution
probability distribution functions
matrix
galaxies
matrices
energy
chronology
wavelengths
wavelength
planning
star formation
resources
universe
physical properties
dust
age determination
distribution
histories
formalism

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • galaxies: evolution
  • methods: statistical
  • surveys

Cite this

Acquaviva, Viviana ; Gawiser, Eric ; Bickerton, Steven J. ; Grogin, Norman A. ; Guo, Yicheng ; Lee, Seong Kook. / Survey design for spectral energy distribution fitting : A fisher matrix approach. In: Astrophysical Journal. 2012 ; Vol. 749, No. 1.
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Survey design for spectral energy distribution fitting : A fisher matrix approach. / Acquaviva, Viviana; Gawiser, Eric; Bickerton, Steven J.; Grogin, Norman A.; Guo, Yicheng; Lee, Seong Kook.

In: Astrophysical Journal, Vol. 749, No. 1, 72, 10.04.2012.

Research output: Contribution to journalArticle

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AU - Acquaviva, Viviana

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