Spectro-Imaging Forward Model of Red and Blue Galaxies

For the next generation of spectroscopic galaxy surveys, it is important to forecast their performances and to accurately interpret their large data sets. For this purpose, it is necessary to consistently simulate different populations of galaxies, in particular Emission Line Galaxies (ELGs), less u...

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Veröffentlicht in:	arXiv.org 2020-06
Hauptverfasser:	Fagioli, Martina, Tortorelli, Luca, Herbel, Jörg, Zürcher, Dominik, Refregier, Alexandre, Amara, Adam
Format:	Artikel
Sprache:	eng
Schlagworte:	Accuracy Astronomical models Computer simulation Cosmology Digital imaging Galactic evolution Photometry Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Principal components analysis Properties (attributes) Sky surveys (astronomy) Spectroscopy Star & galaxy formation Stars & galaxies Statistical methods Stellar age
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