A code computing consistently the evolution of stars, gas and dust, as well as the energy they radiate, is required to derive reliably the history of galaxies by fitting synthetic spectral energy distributions (SEDs) to multiwavelength observations. The new code PÉGAS
We have developed a new evolutionary synthesis code, which incorporates the output from chemical ev...
We provide here the documentation of the new version of the spectral evolution model PEGASE. PEGASE ...
A key issue in galaxy formation and evolution is to deepen our understanding of the complex (astro)p...
A code computing consistently the evolution of stars, gas and dust, as well as the energy they radia...
International audienceA code computing consistently the evolution of stars, gas and dust, as well as...
We present models of photometric evolution of galaxies in which the effects of a dusty interstellar ...
We present models of photometric evolution of galaxies in which the effects of a dusty interstellar ...
We present photometric evolution models of galaxies, in which, in addition to the stellar component,...
Context. Measuring how the physical properties of galaxies change across cosmic times is essential t...
(abridged) We present STARDUST, a new self-consistent modelling of the spectral energy distributions...
Aims. The Herschel Extragalactic Legacy Project (HELP) focuses on the data from ESA’s Herschel missi...
This thesis project involves the improvement of existing computer code, which is used in modeling th...
The galaxy spectral energy distributions (SEDs) from far-UV to far-IR are very important source of i...
We have fit the far-ultraviolet (FUV) to sub-millimeter (850 μm) spectral energy distributions (SEDs...
An updated version of the dust radiation transfer code sunrise, including mod-els for star-forming r...
We have developed a new evolutionary synthesis code, which incorporates the output from chemical ev...
We provide here the documentation of the new version of the spectral evolution model PEGASE. PEGASE ...
A key issue in galaxy formation and evolution is to deepen our understanding of the complex (astro)p...
A code computing consistently the evolution of stars, gas and dust, as well as the energy they radia...
International audienceA code computing consistently the evolution of stars, gas and dust, as well as...
We present models of photometric evolution of galaxies in which the effects of a dusty interstellar ...
We present models of photometric evolution of galaxies in which the effects of a dusty interstellar ...
We present photometric evolution models of galaxies, in which, in addition to the stellar component,...
Context. Measuring how the physical properties of galaxies change across cosmic times is essential t...
(abridged) We present STARDUST, a new self-consistent modelling of the spectral energy distributions...
Aims. The Herschel Extragalactic Legacy Project (HELP) focuses on the data from ESA’s Herschel missi...
This thesis project involves the improvement of existing computer code, which is used in modeling th...
The galaxy spectral energy distributions (SEDs) from far-UV to far-IR are very important source of i...
We have fit the far-ultraviolet (FUV) to sub-millimeter (850 μm) spectral energy distributions (SEDs...
An updated version of the dust radiation transfer code sunrise, including mod-els for star-forming r...
We have developed a new evolutionary synthesis code, which incorporates the output from chemical ev...
We provide here the documentation of the new version of the spectral evolution model PEGASE. PEGASE ...
A key issue in galaxy formation and evolution is to deepen our understanding of the complex (astro)p...
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