Dark Energy Spectroscopic Instrument (DESI) starts 5-year survey


A small section of the DESI focal plane, showing the one-of-a-kind robotic positioners. The optical fibers, which are installed in the robotic positioners, are backlit with blue light in this image. Credit: DESI collaboration
A small section of the DESI focal plane, showing the one-of-a-kind robotic positioners. The optical fibers, which are installed in the robotic positioners, are backlit with blue light in this image. Credit: DESI collaboration

A five-year quest to map the universe and unravel the mysteries of dark energy is beginning officially on May 17, at Kitt Peak National Observatory near Tucson, Arizona. To complete its quest, the Dark Energy Spectroscopic Instrument (DESI) will capture and study the light from tens of millions of galaxies and other distant objects in the universe.


DESI is an international science collaboration managed by the Department of Energy's Lawrence Berkeley National Laboratory, or Berkeley Lab, with primary funding from DOE's Office of Science.


By gathering light from some 30-million galaxies, project scientists say DESI will help them construct a 3D map of the universe with unprecedented detail. The data will help them better understand the repulsive force associated with dark energy that drives the acceleration of the expansion of the universe across vast cosmic distances.


Jim Siegrist, associate director for High Energy Physics at DOE, says we are excited to see the start of DESI, the first next-generation dark energy project to begin its science survey. Along with its primary mission of dark energy studies, the data set will be of use by the wider scientific community for a multitude of astrophysics studies.


What sets DESI apart from previous sky surveys? The project director, Berkeley Lab's Michael Levi, said, We will measure 10 times more galaxy spectra than ever obtained. These spectra get us a third dimension. Instead of two-dimensional images of galaxies, quasars, and other distant objects, the instrument collects light, or spectra, from the cosmos such that it "becomes a time machine where we place those objects on a timeline that reaches as far back as 11-billion years ago.


Project co-spokesperson Nathalie Palanque-Delabrouille, a cosmologist at France's Alternative Energies and Atomic Energy Commission, or CEA said, DESI is the most ambitious of a new generation of instruments aimed at better understanding the cosmos in particular, its dark energy component. The scientific program including her own interest in quasars will allow researchers to address with precision two primary questions: what is dark energy; and the degree to which gravity follows the laws of general relativity, which form the basis of our understanding of the cosmos. It's been a long journey from the first steps that we took almost a decade ago to design the survey, then to decide which targets to observe, and now to have the instruments so that we can achieve those science goals. It's very exciting to see where we stand today.

The formal start of DESI's five-year survey follows a four-month trial run of its custom instrumentation that captured 4-million spectra of galaxies more than the combined output of all previous spectroscopic surveys.


The DESI instrument resides at the retrofitted Nicholas U. Mayall 4-meter Telescope at Kitt Peak National Observatory, a program of the National Science Foundation's NOIRLab. The instrument includes new optics that increase the field of view of the telescope and includes 5,000 robotically controlled optical fibers to gather spectroscopic data from an equal number of objects in the telescope's field of view.


Berkeley Lab's David Schlegel, who is DESI project scientist said, We're not using the biggest telescopes. It's that the instruments are better and very highly multiplexed, meaning that we can capture the light from many different objects at once. In fact, the telescope is literally pointing at 5,000 different galaxies simultaneously. On any given night as the telescope is moved into a target position, the optical fibers align to collect light from galaxies as it is reflected off the telescope mirror. From there, the light is fed into a bank of spectrographs and CCD cameras for further processing and study.


Survey validation lead, Christophe Yeche, also a cosmologist at CEA said, It's really a factory that we have, a spectra factory. We can collect 5,000 spectra every 20 minutes. On a good night, we collect spectra from some 150,000 objects.


Klaus Honscheid, a professor of physics at Ohio State University who directed the design of the DESI instrument control and monitoring systems said, But it's not just the instrument hardware that got us to this point, it's also the instrument software, DESI's central nervous system.


He credits scores of people in his group and around the world who have built and tested thousands of DESI's component parts, most of which are unique to the instrument.


Spectra collected by DESI are the components of light corresponding to the colors of the rainbow. Their characteristics, including wavelength, reveal information such as the chemical composition of objects being observed as well as information about their relative distance and velocity.


As the universe expands, galaxies move away from each other, and their light is shifted to longer, redder wavelengths. The more distant the galaxy, the greater its redshift. By measuring galaxy redshifts, DESI researchers will create a 3D map of the universe. The detailed distribution of galaxies in the map is expected to yield new insights into the influence and nature of dark energy.


Project co-spokesperson Kyle Dawson, a professor of physics and astronomy at the University of Utah. The goal is not so much to find out how much there is, we know that about 70% of the energy in the universe today is dark energy but to study its properties. Dark energy is one of the key science drivers for DESI.


The universe is expanding at a rate determined by its total energy contents, Dawson explains. As the DESI instrument looks out in space and time, we can literally take snapshots today, yesterday, 1-billion years ago, 2-billion years ago as far back in time as possible. We can then figure out the energy content in these snapshots and see how it is evolving.

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