The End of Galaxy Surveys

TL;DR

This paper explores the concept of a final, comprehensive galaxy survey at NIR wavelengths, outlining technological requirements and potential survey parameters to maximize scientific information on dark energy, galaxy evolution, and supernovae.

Contribution

It defines the concept of a final galaxy survey, proposes scaling relations for survey design, and discusses technological advances needed to achieve this goal.

Findings

A 280m telescope could exhaust cosmological information in 10 years.

Scaling relations link sky background, aperture, and focal plane size for survey optimization.

Technological advances are essential for realizing the last galaxy survey.

Abstract

For nearly a century, imaging and spectroscopic surveys of galaxies have given us information about the contents of the universe. We attempt to define the logical endpoint of such surveys by defining not the next galaxy survey, but the final galaxy survey at NIR wavelengths; this would be the galaxy survey that exhausts the information content useful for addressing extant questions. Such a survey would require incredible advances in a number of technologies and the survey details will depend on the as yet poorly constrained properties of the earliest galaxies. Using an exposure time calculator, we define nominal surveys for extracting the useful information for three science cases: dark energy cosmology, galaxy evolution, and supernovae. We define scaling relations that trade off sky background, telescope aperture, and focal plane size to allow for a survey of a given depth over a given area. For optimistic assumptions, a 280m telescope with a marginally resolved focal plane of 20 deg$^2$ operating at L2 could potentially exhaust the cosmological information content of galaxies in a 10 year survey. For galaxy evolution (making use of gravitational lensing to magnify the earliest galaxies) and SN, the same telescope would suffice. We discuss the technological advances needed to complete the last galaxy survey. While the final galaxy survey remains well outside of our technical reach today, we present scaling relations that show how we can progress toward the goal of exhausting the information content encoded in the shapes, positions, and colors of galaxies.