This will provide an unparalleled resource to study the physical processes that shape galaxy evolution and will determine the key relations between stellar mass, star-formation, metallicity and the role of feedback. Hα, OIII, Ca HK).Įxploiting the large multiplex and wavelength coverage of MOONS will provide high-quality spectra for a statistically significant number of galaxies (∼1 M) at z>1 for the first time, matching a similar rest-frame wavelength, volume, range of environments and stellar masses as the successful Sloan Digital Sky Survey (SDSS) in the local Universe. In fact, at these redshifts almost all the main spectral features used to determine the physical, chemical and dynamical properties of galaxies are shifted to λ > 1μm (e.g. In recent years, large spectroscopic surveys at optical wavelengths (0.3 μm – 1 μm) have provided important information on the formation and evolution of galaxies, but near-IR spectroscopy is now required to extend our knowledge beyond z∼1. In the past we put countless of hours into this including the galacticraft dev. This has been part of a recurring issue with the worlds. Tracing the assembly history of galaxies over cosmic time remains a primary goal for observational and theoretical studies of the Universe. We decided to reset Galactic Science for these reasons: Tardis Dimensions are currently broken and after days of debugging we were not able to resolve this issue.
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