The spectral appearance of primeval galaxies
The current and forthcoming observations of large samples of high-redshift galaxies selected according to various photometric and spectroscopic criteria can be interpreted in the context of galaxy formation, by means of models of evolving spectral energy distributions (SEDs). We hereafter present ST...
Prif Awduron: | Guiderdoni, B, Devriendt, J |
---|---|
Fformat: | Conference item |
Cyhoeddwyd: |
1999
|
Eitemau Tebyg
-
Spectroscopic analysis of primeval galaxy candidates
gan: Caruana, J
Cyhoeddwyd: (2013) -
Galaxy Modelling -- I. Spectral Energy Distributions from Far-UV to
Sub-mm Wavelengths
gan: Devriendt, J, et al.
Cyhoeddwyd: (1999) -
Galaxy Modelling - II. Multi-Wavelength Faint Counts from a
Semi-Analytic Model of Galaxy Formation
gan: Devriendt, J, et al.
Cyhoeddwyd: (2000) -
Modelling high-z galaxies from the far-UV to the far-IR
gan: Devriendt, J, et al.
Cyhoeddwyd: (1998) -
Contribution of galaxies to the background hydrogen-ionizing flux
gan: Devriendt, J, et al.
Cyhoeddwyd: (1998)