Construction of spectral libraries of star-forming galaxies at 0.3 ≤ z ≤ 2.5
November 28, 2022
June 15, 2023
Spectral energy distribution (SED) models of galaxies at 0.3 ≤ z ≤ 2.5 were constructed to be processed by the Euclid spectroscopic channel simulator in order to investigate the Euclid Near-Infrared Spectrometer and Photometer (NISP) capabilities.
We developed a solid methodology to build a realistic and epresentative synthetic SED library of star-forming galaxies, including reliable emission line fluxes and widths. The construction of the SEDs consists in computing the continuum using the Bruzual & Charlot (2003) models, calling out SED fitting parameters available in publicly released multi-wavelength catalogues. Emission lines were added using empirical and theoretical relations.
How to cite
Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating
very compact bibliographies which can be beneficial to authors and
readers, and in "proceeding" format
which is more detailed and complete.