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CHANCES: A New Look at Galaxy Clusters

A project studying galaxy clusters to reveal their evolution and interactions.

Cristóbal Sifón, Alexis Finoguenov, Christopher P. Haines, Yara Jaffé, B. M. Amrutha, Ricardo Demarco, E. V. R. Lima, Ciria Lima-Dias, Hugo Méndez-Hernández, Paola Merluzzi, Antonela Monachesi, Gabriel S. M. Teixeira, Nicolas Tejos, Pablo Araya-Araya, Maria Argudo-Fernández, Raúl Baier-Soto, Lawrence E. Bilton, C. R. Bom, Juan Pablo Calderón, Letizia P. Cassarà, Johan Comparat, H. M. Courtois, Giuseppe D'Ago, Alexandra Dupuy, Alexander Fritz, Rodrigo F. Haack, Fabio R. Herpich, E. Ibar, Ulrike Kuchner, Amanda R. Lopes, Sebastian Lopez, Elismar Lösch, Sean McGee, C. Mendes de Oliveira, Lorenzo Morelli, Alessia Moretti, Diego Pallero, Franco Piraino-Cerda, Emanuela Pompei, U. Rescigno, Rory Smith, Analía V. Smith Castelli, Laerte Sodré, Elmo Tempel

― 7 min read


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Table of Contents

Let’s talk about the universe and some big groups of galaxies called clusters. If you've ever thought about how galaxies come together and change over time, you’re in luck! A new project called CHANCES, which stands for CHilean Cluster Galaxy Evolution Survey, is on a mission to find out more about these clusters and their surroundings. Think of it as the universe's version of a long-running reality show, but instead of drama and romance, we have galaxies and their life stories.

CHANCES aims to study 150 Massive Galaxy clusters, zooming in from our local area to the far reaches of the universe. The team will use some fancy equipment at a telescope in Chile to get a good look at 500,000 galaxies. Sounds like a cosmic shopping spree, right? Well, they’re just gathering data instead of picking out shoes!

The Plan

The CHANCES project has a cool plan. It’s like a two-part adventure: the Low-z subsurvey and the Evolution subsurvey.

Low-z Subsurvey

In this part, the focus is on 50 clusters of galaxies that are not too far away from us. They are known as "low redshift" clusters. The team will look closely at these clusters because they want to see how they differ in mass-much like how some people have heavier wallets than others. They will also peek into two superclusters, which are like the VIP sections of the cosmic club, where many clusters hang out together.

Evolution Subsurvey

Now, this is where things get really exciting. The Evolution subsurvey will explore some of the biggest Galaxy Clusters, searching for the biggest and baddest out there. The goal is to see how these massive clusters have changed over time. Imagine trying to keep tabs on your friends as they grow up, except your friends are gigantic groups of stars and planets!

The Equipment

To carry out this ambitious plan, the team will use a special instrument called the 4MOST (Four Meter Multi-Object Spectroscopic Telescope). This big telescope can capture the light from many galaxies at once, which is super handy. Picture it like a huge cosmic camera that can take a group photo of galaxies all at once-no awkward poses required!

With 2436 science fibers (think of them as high-tech straws), 4MOST can observe galaxies in a wide field. It’s like having all the friends in one shot instead of taking individual selfies. With this tech, the researchers will take a closer look at how these galaxies interact, what causes them to change, and how they affect each other. No pressure!

Galaxy Clusters: What Are They?

You might be wondering, "What’s a galaxy cluster anyway?" Well, imagine a party where everyone knows each other. A galaxy cluster is a group of galaxies that are close enough to interact and influence one another. They often share a lot of gas and dark matter, which sounds like a complicated relationship, but that’s the nature of the cosmic game!

Clusters can come in different sizes. Some are huge and contain thousands of galaxies, while others are smaller. It’s kind of like comparing a massive shopping mall to a small boutique. Both are great, just different sizes!

The Importance of Study

You might be thinking, “Why study these clusters?” Well, looking at them helps scientists understand the bigger picture of how galaxies evolve. It’s like piecing together a giant jigsaw puzzle. The researchers hope to learn what drives changes in galaxies-why some stay young and vibrant while others become more old and settled down.

They want to see how the environment affects these galaxies. Some might be influenced by their luxurious cosmic surroundings, while others might be struggling in a less favorable neighborhood. Understanding these dynamics can provide insights into the life cycles of galaxies and the forces at play in the universe.

What’s Happening Around the Clusters?

While scientists will be focusing on the clusters themselves, they will also take a close look at what's happening nearby. Think of a cluster as a bustling city, and the surrounding area as the suburbs. The researchers want to figure out how galaxies that live in clusters differ from those that live a bit further away. Do they lead different lives? Are they hanging out with different crowds?

By studying the environment around the clusters, they can see if galaxies are getting influenced by their neighbors. Some galaxies may lose or gain gas, depending on their social circle. If you’ve ever changed your style because of your friends, you’ll get the idea!

Massive Clusters and Galaxy Evolution

Focusing on massive clusters is critical because they can provide insights into galaxy evolution. It’s like getting an exclusive backstage pass to understand the bigger picture. The researchers have found that many galaxies in rich clusters have lost their gas and morphed into quiescent, starless relics. Meanwhile, their less fortunate cousins in looser clusters might still be forming stars and shining bright.

So, what causes this transformation? Researchers suspect that both internal forces (like supernova explosions) and external forces (like interactions with other galaxies) play key roles. The more they delve into these aspects, the clearer the picture of galaxy evolution will become.

Cluster Density and Its Effects

One of the exciting parts of the study will be how the density of the cluster affects the galaxies. Imagine two friends going to parties: one is at an intimate dinner, and the other is at a huge concert. Their experiences will likely differ significantly!

In dense clusters, the level of star formation tends to drop as galaxies become more settled. On the other hand, in less crowded environments, galaxies may continue to flourish. The researchers want to see how far this pattern extends, possibly leading to new discoveries about how galaxies thrive or struggle based on their surroundings.

Connecting the Dots

The researchers will not only study individual clusters but also connect the dots between them. They will look at the relationship between clusters and the larger cosmic web, which consists of filaments and sheets of galaxies. It’s like connecting the stars to see constellations in the night sky, revealing the structure of the universe itself.

What Data Will Be Collected?

Throughout the five years of the CHANCES survey, the team will collect tons of data. They will focus not only on the clusters themselves but also on the surrounding regions and any interesting anomalies. By looking at various details, such as galaxy types and masses, they will get a more extensive understanding of how clusters and their inhabitants evolve.

The Future of CHANCES

As the CHANCES survey moves forward, researchers will continue to analyze and interpret the data they collect. They will work tirelessly to connect individual stories of galaxies to the larger narrative of cosmic evolution. Who knows what discoveries lie ahead? Perhaps a new understanding of how galaxies evolve or what makes them tick!

Conclusion

In a nutshell, the CHANCES project is set to embark on a cosmic quest to uncover the secrets of galaxy clusters and their environments. With advanced technology, a solid plan, and a team of bright minds, this survey could bring new insights into the life stories of galaxies. It’s like reading a page-turner full of twists and turns, where every chapter dives deeper into the mysteries of the universe. So buckle up and get ready; this will be one stellar ride!

Original Source

Title: CHANCES, The Chilean Cluster Galaxy Evolution Survey: selection and initial characterization of clusters and superclusters

Abstract: CHANCES, the CHileAN Cluster galaxy Evolution Survey, will study the evolution of galaxies in and around ${\sim}$150 massive galaxy clusters, from the local universe out to z=0.45. CHANCES will use the new 4MOST Spectroscopic Survey Facility on the VISTA 4m telescope to obtain spectra for ${\sim}$500,000 galaxies with magnitudes $r_\mathrm{AB} < 20.5$, providing comprehensive spectroscopic coverage of each cluster out to $5r_{200}$. Its wide and deep scope will trace massive and dwarf galaxies from the surrounding filaments and groups to the cores of galaxy clusters, enabling the study of galaxy pre-processing and the role of the evolving environment on galaxy evolution. In this paper we present and characterize the sample of clusters and superclusters to be targeted by CHANCES. We used literature catalogues based on X-ray emission and Sunyaev-Zel'dovich effect to define the cluster sample in a homogeneous way, with attention to cluster mass and redshift, as well as the availability of ancillary data. We calibrated literature mass estimates from various surveys against each other and provide an initial mass estimate for each cluster, which we used to define the radial extent of the 4MOST coverage. We also present an initial assessment of the structure surrounding these clusters based on the redMaPPer red-sequence algorithm as a preview of some of the science CHANCES will enable.

Authors: Cristóbal Sifón, Alexis Finoguenov, Christopher P. Haines, Yara Jaffé, B. M. Amrutha, Ricardo Demarco, E. V. R. Lima, Ciria Lima-Dias, Hugo Méndez-Hernández, Paola Merluzzi, Antonela Monachesi, Gabriel S. M. Teixeira, Nicolas Tejos, Pablo Araya-Araya, Maria Argudo-Fernández, Raúl Baier-Soto, Lawrence E. Bilton, C. R. Bom, Juan Pablo Calderón, Letizia P. Cassarà, Johan Comparat, H. M. Courtois, Giuseppe D'Ago, Alexandra Dupuy, Alexander Fritz, Rodrigo F. Haack, Fabio R. Herpich, E. Ibar, Ulrike Kuchner, Amanda R. Lopes, Sebastian Lopez, Elismar Lösch, Sean McGee, C. Mendes de Oliveira, Lorenzo Morelli, Alessia Moretti, Diego Pallero, Franco Piraino-Cerda, Emanuela Pompei, U. Rescigno, Rory Smith, Analía V. Smith Castelli, Laerte Sodré, Elmo Tempel

Last Update: 2024-11-20 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2411.13655

Source PDF: https://arxiv.org/pdf/2411.13655

Licence: https://creativecommons.org/licenses/by/4.0/

Changes: This summary was created with assistance from AI and may have inaccuracies. For accurate information, please refer to the original source documents linked here.

Thank you to arxiv for use of its open access interoperability.

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