Researchers capture direct high-definition image of the “Cosmic Web”

Simulation of a vast region of the Universe based on the current cosmological model and performed using supercomputers. In the image, the faint glow of the gas within the cosmic filaments, forming a dense cosmic web, is shown in white. At the intersections of these filaments, the gas within galaxies, which fuels the formation of new stars, is highlighted in red. © Alejandro Benitez-Llambay/Universität Mailand-Bicocca/MPA

The image shows the diffuse gas (yellow to purple) contained within the cosmic filament connecting two galaxies (yellow stars), extending across a vast distance of 3 million light-years. © Davide Tornotti/University of Milano-Bicocca

A twin of the cosmic filament observed in the MUDF as seen in a supercomputer simulation describing the large-scale distribution of gas in the Universe. The gas flowing within the cosmic web, feeding galaxy formation at filament intersections, is shown in purple. Davide Tornotti/University of Milano-Bicocca/MPA

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Matter in intergalactic space is distributed in a vast network of interconnected filamentary structures, collectively referred to as the cosmic web. With hundreds of hours of observations, an international team of researchers has now obtained an unprecedented high-definition image of a cosmic filament inside this web, connecting two active forming galaxies – dating back to when the Universe was about 2 billion years old.

A pillar of modern cosmology is the existence of dark matter, which constitutes about 85% of all matter in the Universe. Under the influence of gravity, dark matter forms an intricate cosmic web composed of filaments, at whose intersections the brightest galaxies emerge. This cosmic web acts as the scaffolding on which all visible structures in the Universe are built: within the filaments, gas flows to fuel star formation in galaxies. Direct observations of the fuel supply of such galaxies would advance our understanding of galaxy formation and evolution

. However, studying the gas within this cosmic web is incredibly challenging. Intergalactic gas has been detected mainly indirectly through its absorption of light from bright background sources. But the observed results do not elucidate the distribution of this gas. Even the most abundant element, hydrogen, emits only a faint glow, making it basically impossible for instruments of the previous generation to directly observe such gas.

In this new study, an international team led by researchers at the University of Milano-Bicocca and including scientists at the Max Planck Institute for Astrophysics (MPA) obtained an unprecedented high-definition image of a cosmic filament using MUSE (Multi-Unit Spectroscopic Explorer), an innovative spectrograph installed on the Very Large Telescope at the European Southern Observatory in Chile. Even with the advanced capabilities of this sophisticated instrument, the research group had to carry out one of the most ambitious MUSE observation campaigns ever completed in a single region of the sky, acquiring data over hundreds of hours to detect the filament at high significance.

The study, led by Davide Tornotti, PhD student at the University of Milano-Bicocca, used this ultrasensitive data to produce the sharpest image ever obtained of a cosmic filament spanning 3 million light-years and connecting two galaxies, each hosting an active supermassive black hole. The discovery, recently published in Nature Astronomy opens new avenues to directly constrain gas properties within intergalactic filaments and to refine our understanding of galaxy formation and evolution.

“By capturing the faint light emitted by this filament, which travelled for just under 12 billion years to reach Earth, we were able to precisely characterize its shape, explains Davide Tornotti. “For the first time, we could trace the boundary between the gas residing in galaxies and the material contained within the cosmic web through direct measurements.” The researchers took advantage of supercomputer simulations of the Universe run at MPA to calculate predictions of the expected filamentary emission given the current cosmological model. “When comparing to the novel high-definition image of the cosmic web, we find substantial agreement between current theory and observations,” Tornotti adds.

This discovery and the encouraging agreement with supercomputer simulations are key to understanding the tenuous gas environment around galaxies and open up novel possibilities to pin down the galaxies’ fuel supply. Fabrizio Arrigoni Battaia, MPA staff scientist involved in the study, concludes: “We are thrilled by this direct, high-definition observation of a cosmic filament. But as people say in Bavaria: ‘Eine ist keine’ – one doesn’t count. So we are gathering further data to uncover more such structures, with the ultimate goal to have a comprehensive vision of how gas is distributed and flows in the cosmic web.”

Source: Max Planck Institute for Astrophysics/Press Releases

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Contact:

Fabrizio Arrigoni Battaia
Scientific Staff
tel:2288
arrigoni@mpa-garching.mpg.de

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Original publication

Davide Tornotti et al.
High-definition imaging of a filamentary connection between a close quasar pair at z=
Nature Astronomy, 29 January 2025

Source

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More Information

Revealing a filament from the cosmic web
ESO Press Release

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Cosmic Web Lights Up in the Darkness of Space

A mosaic of images captured using W. M. keck Observatory's keck cosmic web imager showing the filaments of gas that make up the cosmic web. the green dots mark known galaxies the filaments connect to. Credit: C. Martin et al./Caltech/W. M. Keck Observatory

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Keck Cosmic Web Imager Offers Best Glimpse Yet of the Filamentous Network That Connects Galaxies

Maunakea, Hawaiʻi Like rivers feeding oceans, streams of gas nourish galaxies throughout the cosmos. But these streams, which make up a part of the so-called cosmic web, are very faint and hard to see. While astronomers have known about the cosmic web for decades, and even glimpsed the glow of its filaments around bright cosmic objects called quasars, they have not directly imaged the extended structure in the darkest portions of space—until now.

New results from the Keck Cosmic Web Imager, or KCWI, which was designed by Caltech’s Edward C. Stone Professor of Physics Christopher Martin and his team, are the first to show direct light emitted by the largest and most hidden portion of the cosmic web: the crisscrossing wispy filaments that stretch across the darkest corners of space between galaxies. The KCWI instrument is based at the W. M. Keck Observatory atop Maunakea in Hawaiʻi.

“We chose the name Keck Cosmic Web Imager for our instrument because we were hoping it would directly detect the cosmic web,” says Martin, who is also the director of the Caltech Optical Observatories, which includes Caltech’s portion of Keck Observatory; other Keck Observatory partners are the University of California and NASA. “I’m very happy it worked out.”

Galaxies in our universe condense out of swirling clouds of gas. That gas then further condenses into stars that light up the galaxies, making them visible to telescopes in a range of wavelengths of light. Astronomers think that cold, dark filaments in deep space snake their way to the galaxies, supplying them with gas, which is fuel for making more stars. In 2015, Martin and his colleagues found “smoking-gun evidence,” as Martin describes it, for this so-called cold-flow model of galaxy formation: a long filament funneling gas into a large galaxy. For this work, they used a prototype instrument to KCWI, the Cosmic Web Imager, which was based at Caltech’s Palomar Observatory.

In that case, the filament was being lit up by a nearby quasar, the bright nucleus of a young galaxy. But most of the cosmic web lies in the desolate territory between galaxies and is hard to image.

“Before this latest finding, we saw the filamentary structures under the equivalent of a lamppost,” says Martin. “Now we can see them without a lamp.”

The new findings appear in a paper published in Nature Astronomy on September 28.

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Detecting the Cosmic Web

This animation reveals a 3-D slice through a network of hydrogen gas filaments that crisscross the spaces between galaxies. The data were collected by the Keck Cosmic Web Imager, or KCWI, which was designed to reveal the structure of this previously hidden component of the universe. The region covered in this observation is about 10.5 billion light-years away. The volume depicted here spans an area of 2.3 by 3.2 million light-years and extends across a depth of 600 million light-years (50 million per segment). Credit: Caltech/R. Hurt (IPAC)

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Martin has been driven to reveal the cosmic web in its full glory ever since he was a graduate student. This detailed imaging of the web, he says, will provide astronomers with missing information they need to understand the details of how galaxies form and evolve. It can also help astronomers map the distribution of dark matter in our universe (dark matter makes up about 85 percent of all matter in the universe, but scientists still don’t know what it is made of).

“The cosmic web delineates the architecture of our universe,” he says. “It’s where most of the normal, or baryonic, matter in our galaxy resides and directly traces the location of dark matter.”

The Feeble Glow of Filaments

The best way to see the cosmic web directly is to pick up signatures of its main component, hydrogen gas, using instruments called spectrometers, which spread light out into a multitude of wavelengths, also known as a spectrum. Hydrogen gas can be identified within these spectra via its strongest emission line, called the Lyman alpha line. Martin and his colleagues designed KCWI to find these faint Lyman alpha signatures across a two-dimensional (2D) image of the cosmos (hence KCWI is known as an imaging spectrometer). The instrument’s first installment covers the “blue” portion of the visible-light spectrum, spanning wavelength ranges from 350 to 560 nanometers. (The second part of the instrument, called the Keck Cosmic Reionization Mapper, or KCRM, which sees the red, or longer-wavelength portion, of the visible spectrum, was recently installed at Keck Observatory).

KCWI’s precise spectrometers can look for the Lyman alpha signatures of the cosmic web across a range of wavelengths. Because of the expansion of the universe, which stretches light to longer wavelengths, gas that is located farther away from Earth has a redder Lyman alpha signature. The 2D images captured by KCWI at each wavelength of light can be stacked together to make a three-dimensional (3D) map of the emission from the cosmic web. For this observation, KCWI observed a region of space between 10 and 12 billion light-years away.

“We are basically creating a 3D map of the cosmic web,” Martin explains. “We take spectra for every point in an image at range of wavelengths, and the wavelengths translate to distance.”

Confusion with the Diffuse Light of Space

One challenge in detecting the cosmic web is that its dim light can be confused with nearby background light that suffuses the skies above Maunakea, including the glow from the atmosphere, zodiacal light from the solar system (generated when sunlight scatters off interplanetary dust), and even our own galaxy’s light.

To solve this problem, Martin came up with a new strategy to subtract this background light from the images of interest.

“We look at two different patches of sky, A and B. The filament structures will be at distinct distances in the two directions in the patches, so you can take the background light from image B and subtract it from A, and vice versa, leaving just the structures. I ran detailed simulations of this in 2019 to convince myself that this method would work,” he says.

The result is that astronomers now have “a whole new way to study the universe,” as Martin says.

“With KCRM, the newly deployed red channel of KCWI, we can see even farther into the past,” says senior instrument scientist Mateusz Matuszewski. “We are very excited about what this new tool will help us learn about the more distant filaments and the era when the first stars and black holes formed.”

Speaking of new ways to view the universe, Martin teamed up with artist Matt Schumaker to translate data from the cosmic web into music for a project called “Spiral, supercluster, filament, wall (after Michael Anderson).” The project celebrates the life of Anderson, who perished along with his fellow astronauts in the Space Shuttle Columbia accident in 2003. Martin, who “pretended the filaments were giant violin strings,” translated the filaments’ masses to frequencies based around the note middle C. The piece can be heard here.

The Nature Astronomy study, titled “Extensive diffuse Lyman alpha emission correlated with cosmic structure,” was funded by the National Science Foundation and Caltech.

Source: W.M.Keck Observatory

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About KCWI

The Keck Cosmic Web Imager (KCWI) is designed to provide visible band, integral field spectroscopy with moderate to high spectral resolution formats and excellent sky-subtraction. The astronomical seeing and large aperture of the telescope enables studies of the connection between galaxies and the gas in their dark matter halos, stellar relics, star clusters, and lensed galaxies. KCWI covers the blue side of the visible spectrum; the instrument also features the Keck Cosmic Reionization Mapper (KCRM), extending KCWI’s coverage to the red side of the visible spectrum. The combination of KCWI-blue and KCRM provides simultaneous high-efficiency spectral coverage across the entire visible spectrum. Support for KCWI was provided by the National Science Foundation, Heising-Simons Foundation, and Mt. Cuba Astronomical Foundation. Support for KCRM was provided by the National Science Foundation and Mt. Cuba Astronomical Foundation.

About W. M. Keck Observatory

The W. M. Keck Observatory telescopes are among the most scientifically productive on Earth. The two 10-meter optical/infrared telescopes atop Maunakea on the Island of Hawaii feature a suite of advanced instruments including imagers, multi-object spectrographs, high-resolution spectrographs, integral-field spectrometers, and world-leading laser guide star adaptive optics systems. Some of the data presented herein were obtained at Keck Observatory, which is a private 501(c) 3 non-profit organization operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the Native Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain..

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