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“5000 Eyes” Premieres in Mexico City

August 6, 2024 by joannajita

joannajita

At the premiere of “5000 Eyes” in Mexico City: (left to right) Axel de la Macorra, Andrea Muñoz-Gutiérrez, and Octavio Valenzuela (DESI scientists), and Wilder Chicana (IPN). (Credit: Aldebarán López @aldebaran.smith)

by Andrea Muñoz Gutiérrez

On 20 June 2024, the DESI planetarium show “5000 Eyes” premiered in Mexico City at the Luis Enrique Erro Planetarium. Previously shown in traveling planetariums across the country, it is now, for the first time, part of the regular programming at the oldest planetarium in the nation. Authorities from several DESI institutions attended the premiere, along with numerous DESI scientists, both senior and early-career.

Dr. Axel de la Macorra and I spoke at the event on behalf of the DESI survey. Also present on stage to introduce the film were Dr. Abdel Pérez Lorenzana, Academic Secretary of Cinvestav (a DESI institution), and Dr. Tonatiuh Matos (DESI scientist), along with Dr. Ana Lilia Coria Páez and Dr. Omar Matamoros representing the Luis Enrique Erro Planetarium. Approximately 260 people enjoyed this inaugural screening of “5000 Eyes.”

Our goal for the event was to convey the wonder of the DESI project to both the authorities and the general public, and we had a significant impact. With the event covered by science communicators and the media, we conducted interviews and spoke with representatives from magazines, social media platforms, and newspapers, and even appeared on TV!

Attendees were wowed by the scale of the DESI project and very happy and thrilled by its results.

During the event, I was incredibly happy to share with colleagues, authorities, and the general public what we do in the collaboration and how we do it. When people approached us with questions, you could see the amazement and joy in their eyes, which is one of the greatest rewards a science communicator can experience.

Now, “5000 Eyes” will be part of the regular film schedule at this planetarium and will be shown at least three times a week. But there’s much more to come! Two planetariums in Guadalajara are set to host premieres in the next few months, and many other planetariums across the country are already interested in screening “5000 Eyes” to share with the public how DESI scientists are creating the largest 3D map in human history.

Several speakers introduced the DESI project and the “5000 Eyes” film at the premiere: (left to right) Omar Matamoros (representing the Luis Enrique Erro Planetarium), Axel de la Macorra (DESI scientist), Ana Lilia Coria Páez (representing the Luis Enrique Erro Planetarium), Abdel Pérez Lorenzana (Academic Secretary of Cinvestav, a DESI institution), Andrea Muñoz-Gutiérrez (DESI scientist), and Tonatiuh Matos (DESI scientist). (Credit: Aldebarán López @aldebaran.smith)

Filed Under: blog, feature on homepage

Some of the 600 visitors who visited Kitt Peak National Observatory for the Tohono O’odham Nation Open Night on 25 May 2024. Credit: KPNO/NOIRLab/NSF/AURA/A. Kocz

Joan Najita (NOIRLab)

30 May 2024

This past weekend, Kitt Peak National Observatory (KPNO) hosted an Open Night for members of the Tohono O’odham Nation. KPNO, where the DESI project is underway, is located atop I’oligam Du’ag (Manzanita Shrub Mountain) in the Tohono O’odham homeland. KPNO Open Nights celebrate the relationship between the Nation and the Kitt Peak astronomy community and express the community’s appreciation for the privilege of carrying out research at a site that is of deep historical and cultural significance to the Nation.

For the 25 May 2024 event, KPNO opened its doors, welcoming 600 Tohono O’odham community members to the observatory. Tribal members of all ages joined in a wide variety of activities, including solar and night-time telescope viewing, Waila music, hands-on activities, and observatory tours.

Visitors to the 4m Mayall Telescope were greeted by volunteers — including DESI collaboration members Dick Joyce, Luke Tyas, Chris Brownewell, Bob Stupak, Yuanyuan Zhang, and Joan Najita — who described the DESI project, its amazing technology and goals, and how the observations are carried out. Elsewhere on the mountain, DESI collaboration member and Mid-Scale Observatories Director Lori Allen greeted visitors as they arrived and helped them view highlights of the night sky through a small telescope.

Visitors observing the Sun through telescopes at the Sunset Point during the Tohono O’odham Nation Open Night on 25 May 2024. DESI’s home, the 4m Mayall Telescope, is in the background. Credit: KPNO/NOIRLab/NSF/AURA/R. Sparks

BaoBan, DESI’s ambassador for Education and Public Outreach, made several guest appearances. A coyote from the wilds of Arizona, BaoBan appeared on DESI-themed souvenir postcards created for the event and in the inaugural KPNO Newsletter for the Tohono O’odham Nation, both of which were distributed to visitors. BaoBan has previously appeared at the Tohono O’odham Rodeo, in comic strips, and other DESI-related public engagement activities.

The 25 May Open Night was long anticipated, with the recent coronavirus pandemic and Contreras fire of 2022 having disrupted the usual 2-3 year cadence of these events. With the mountain now reopened and normal observatory operations resumed, the Kitt Peak astronomy community was eager to restart the series. More than 70 volunteers from NOIRLab and Kitt Peak facilities worked together with local Tucson community organizations in hosting the event.

For Bob Stupak, NOIRLab Electronics Technician and DESI collaboration member, welcoming visitors at the Mayall was “a great time,” an opportunity to share the excitement of DESI with the community, resulting in smiles all around. He noted, “I was working at the top of the visitor’s elevator and everyone leaving the building seemed to have been really impressed.”

Further details about the event are available in a NOIRLab press release.

Rare night-time view of the 4m Mayall Telescope, illuminated by lights from the Tohono O’odham Nation Open Night. Credit: Bob Stupak

Filed Under: blog, feature on homepage

Joan Najita (NOIRLab) and Luke Tyas (LBL)

Science communicators across the internet are discussing DESI’s Year 1 results and their implications for the fate of the Universe. Here are some of the highlights.

An artistic celebration of the Dark Energy Spectroscopic Instrument (DESI) Year 1 data, showing a slice of the larger 3D map that DESI is constructing during its five-year survey. DESI is mounted on the Nicholas U. Mayall 4-meter Telescope at Kitt Peak National Observatory. Credit:
DESI Collaboration/KPNO/NOIRLab/NSF/AURA/P. Horálek/R. Proctor

World Science Festival: Is Dark Energy Decaying? 

Brian Greene sits down with Michael Levi (LBL) to discuss DESI’s revolutionary observations that may upend our understanding of the cosmos. In an hour-long conversation that takes us from the discovery of dark energy to the birth of the DESI project and on to its Year 1 Key Project results, Greene and Levi highlight the cutting-edge nature of the story. That is, we’re finding an intriguing hint that dark energy is weakening (i.e., becoming “less pushy” over time), and but we’re not completely sure. Commenting on the uncertainty, and how we’ll know more soon, “This is why I love doing physics,” says Levi, “It’s detective novel that you get to read and discover, and it was written by the Universe!” As for the bigger picture meaning of the results, should they hold up, the weakening accelerated expansion of the universe seems reminiscent of the end of the inflationary expansion phase that marked the birth of the Universe. Levi finds it “appealing that we may be living in an epoch that ties back to the beginning of time.”

PBS Nova: New Map of the Universe Hints that Dark Energy May Be Evolving

This 3-minute video, which includes commentary from David Kaiser (MIT) and Priya Natarajan (Yale), describes how the DESI results could “fundamentally change what we know about the Universe and how it may come to an end.” Kaiser says the new DESI map of the Universe is more than a simple accounting where stuff is at any given moment. It also captures the Universe’s dynamics, creating something more like a movie that shows how fast space was stretching at different times over the Universe’s history. Natarajan emphasizes the possible cosmological implications of the results, noting that “If dark energy was a constant, the fate of the Universe would be grim.” Instead The DESI results appear to “open the door to the possibility of changing dark energy models”, which for Natarajan, “means that we have more exciting (possible) fates that await us.”

NPR: This week in science: Pompeiian frescoes, dark energy and the largest marine reptile  — NPR’s Mary Louise Kelly talks with Emily Kwong and Rachel Carson of Short Wave about how dark energy may be changing, with commentary from Priya Natarajan (Yale).

Dr Becky: Does the expansion rate of the Universe CHANGE over time?! DESI 1 year results — In this 12-minute video, astrophysicist Dr Becky Smethurst (Oxford) explains Baryon Acoustic Oscillations in words normal people can understand and walks the listener through the main plots and results from the Year 1 Key Project papers and press release.

Anton Petrov: Strange Expansion of the Universe Results from the Most Accurate Map — With a phenomenal 268,000 views as of this writing, this 12-minute video from scientist and educator Anton Petrov describes the use of Baryonic Acoustic Oscillations as a cosmological standard ruler and the implications of the DESI results for our understanding of what the universe “was doing billions of years ago, what it’s going to be doing in the future, and how all of this ends.”

AM24:First Year Results from the Dark Energy Spectroscopic Instrument (DESI) — Three talks by DESI scientists at the April 2024 meeting of the American Physical Society unveil DESI’s cutting-edge results. First, Hee-Jong Seo (Ohio University) presents the BAO results from galaxies and quasars at z < 2. Next, Julien Guy (Berkeley Lab) presents BAO results from the Lyman-alpha forest at z > 2. Finally, Mustapha Ishak (UT Dallas) presents the cosmology implications of the measurements.

Filed Under: blog, feature on homepage

Joan Najita (NOIRLab)

Articles in the media covering the 4 April 2024 press release, by location, as of 22 April 2024.

As described in a recent press release, DESI has found subtle hints that dark energy, once assumed to be constant in time, may instead be evolving. Spectra that probe the past 11 billion years of cosmic history suggest that dark energy appears to be weakening, becoming “less pushy” over time. That appears to be the message from the first year of DESI data when interpreted in combination with other data, i.e.,  supernovae and the cosmic microwave background. The news was covered in more than 1200 articles written in over 30 languages across the globe.

While DESI scientists caution that it’s too early to be certain, astronomers and physicists are excited by the news and the possibilities ahead. “If it holds up, this is a very big deal,” said Adam Riess, one of the discoverers of dark energy, speaking to New Scientist: “It may be the first real clue we have gotten about the nature of dark energy in 25 years.” Michael Turner, who coined the term “dark energy,” told the New York Times, “the possible evidence that dark energy is not constant is the best news I have heard since cosmic acceleration was firmly established 20-plus years ago.”

The original discovery, in 1998, that the expansion of the Universe is accelerating rather than slowing with time, could be understood as evidence that the vacuum of space possesses a tiny amount of energy of its own, i.e., a “dark energy.” That idea found an echo in an earlier proposal from Einstein of a “cosmological constant,” a concept that has been at the heart of our standard model of the Universe for the past two decades.

The model has been popular. In finding explanations for how the world and the Universe works, physicists sometimes use aesthetics as a guide and are drawn to explanations that have a simplicity or elegance, often of a mathematical kind. The standard model fits the bill. Explaining the attractiveness of the standard model and the role of the cosmological constant, Licia Verde told Quanta magazine: “It’s simple. It’s one number. It has some story you can attach to it. That’s why it’s believed to be constant.”

The new DESI results shake that foundation.

If dark energy isn’t a strict constant, who knows how it evolves. That uncertainty, and the potential unshackling from a cosmological constant, opens a richer set of potential futures for us. If dark energy continues to significantly weaken with time, it may become not only “less pushy,” but perhaps even “sucky,” causing the Universe to contract rather than expand. On the other hand, it may also grow stronger with time or possibly just fade away.

Commenting on these options, Durham University Professor Carlos Frenk told the Guardian that if DESI’s hints are right, our earlier understanding “goes out the window and essentially we have to start from scratch, and that means revising our understanding of basic physics, our understanding of the big bang itself, and our understanding of the long-range forecast for the Universe.”

The news may be soothing to some of us, at a human level.

In covering the DESI results, NPR characterized our current model of the Universe as painting a bleak picture of the future, i.e., that if dark energy is constant, it “will continue to push everything in the Universe apart. So much so that one day other galaxies won’t be visible from Earth. Even the stars in our own galaxy will die out, leaving behind a cold dark nothing…” Pretty depressing. But Priya Natarajan told NPR that the possibility of a changing dark energy opens the way to a happier ending: “Our fate may not be as lonely and desolate and grim as we imagine.”

Our understanding of exactly what the future holds depends on what we learn about whether and how dark energy is evolving. We should know more soon. The reported results are based on just the first year of data from the DESI survey, which is designed to extend over 5 years. So stay tuned!

Read other news reports on the recent DESI results here.

Filed Under: blog, feature on homepage

The Guardian, 4 April 2024

Filed Under: in the news

DESI’s map of the Universe is the largest to date. The delicate bubble-like structures in the distribution of galaxies—seen in the inset—record vital clues to the expansion history of the universe. Credit: Claire Lamman/DESI collaboration; custom colormap package by cmastro.

In its quest to study the effect of dark energy on the expansion history of the Universe, DESI has been charting the cosmos, creating the largest 3D map of the Universe ever made — a map that stretches back over 11 billion years of cosmic time.

In a press announcement today, the project made its initial report on the cosmological clues recorded in the map. The results make use of data from the first year of the DESI survey, which will be carried out over a total of five years.

DESI’s 3D map tracks the frozen-in imprint of baryon acoustic oscillations (BAO), as recorded two ways: in the spatial distributions of galaxies, and in the structure of intergalactic gas seen along the line of sight to distant quasars (the Lyman alpha forest). Using these data, DESI scientists have measured the BAO signal at 7 epochs (i.e., slices of cosmic time) from 3 billion to 11 billion years ago. Because the measured BAO signal is a so-called “standard ruler”, the scientists can infer how the Universe expanded over its history.

The results are amazingly precise. Because of DESI’s high efficiency and stability, combined with its ability to measure spectra for large numbers of galaxies and quasars, the Universe’s expansion history is now known to better than 1% precision, yielding the best picture yet of how the universe has evolved.

The results are in general agreement with the current best cosmological model (Lambda CDM), which takes into account the roles of dark energy and dark matter. But as noted by DESI Director Michael Levi, “we’re also seeing some potentially interesting differences that could indicate that dark energy is evolving over time. Those may or may not go away with more data, so we’re excited to start analyzing our three-year dataset soon.”

With 4 more years of DESI data to come, stay tuned to see how the story evolves as DESI’s map reaches completion!

DESI’s measurement of the BAO signal at 7 cosmic epochs (from 3 billion to 11 billion years ago) are in general agreement with our current best model (Lambda CDM). Credit: Arnaud de Mattia/DESI collaboration.

These results were reported in multiple papers posted on arXiv and in talks presented today at the American Physical Society meeting. A guide to the suite of papers presenting these results is available at the DESI blog.

Filed Under: announcements

Joan Najita (NOIRLab)

12 February 2024 was a spectacular night for DESI: it broke its own record and acquired nearly 200,000 redshifts in a single night. The figure is remarkable, especially in the context of history.

The Dark Energy Spectroscopic Instrument (DESI) observing the night sky on the Nicholas U. Mayall 4-meter Telescope at Kitt Peak National Observatory in Arizona. Credit: KPNO/NOIRLab/NSF/AURA/T. Slovinský

Forty years ago, the first and second CfA redshift surveys acquired spectra of 2200 and 15,000 galaxies respectively, giving us the first glimpses of the large scale structure of galaxies. Rather than being distributed randomly, galaxies were found to cluster in a froth-like structure, arranged on bubble-like surfaces surrounding large volumes mostly devoid of galaxies. In these pioneering surveys, redshifts were painstakingly acquired one at a time. As a result, the first CfA redshift survey took 5 years to acquire its 2200 redshifts (1977-1982). In comparison, on 12 February DESI acquired 100 times that number in a single night.

How does DESI do it?

Rather than taking spectra of galaxies one at a time, DESI can acquire 5000 spectra at once through its 5000 robotically positioned fibers. Tiny robots center each fiber on an object (galaxy, quasar, or star). After an exposure is done, the fibers are quickly repositioned, within 1-2 minutes, and DESI is ready to acquire spectra of another 5000 objects. On 12 February, the seeing at the Mayall Telescope was very good (0.65 arcseconds) and DESI was able to go through the setup process more than 40 times. (The gory details: DESI observed 41 dark tiles, 4 bright tiles, and 2 backup tiles that night.)

A spectacular night in a notable month

While February’s weather was relatively poor, DESI still managed to acquire 1.8 million spectra over the month. The quick progress keeps DESI on track to complete its planned survey of 30 million galaxies and quasars and 10 million stars within 5 years. By measuring the large scale structure of galaxies at high precision, the DESI survey will lend new insights into the expansion history of the Universe and the nature of dark matter and dark energy.

Comparison of the famous “CfA Stick Man” to DESI galaxies in the same region: a 6-degree slice in declination, spanning about a third of the sky. The CfA Stick Man was one of the first clear examples of large-scale structure in the Universe. Credit: Claire Lamman | The CfA Redshift Survey: Data for the NGP +30 Zone. Huchra, Geller, de Lapparent, Corwin 1990

Filed Under: blog, feature on homepage

Joan Najita (NOIRLab)

16 February 2024

BaoBan, DESI’s ambassador for Education and Public Outreach, made a recent appearance at the 85th Annual Tohono O’odham Nation Rodeo and Parade, featuring prominently in the parade entry from Kitt Peak National Observatory (KPNO). A coyote from the wilds of Arizona, BaoBan has previously appeared in comic strips and other DESI-related public engagement activities. The DESI project is being carried out at KPNO, which is located atop I’oligam Du’ag, in the homeland of the Tohono O’odham Nation.

BaoBan greeted spectators at the 2024 Tohono O’odham Rodeo parade (Credit: M. Edwards).

At this year’s rodeo parade, held 3 February 2024, KPNO entered a float decorated with images of BaoBan, planets, stars, and telescopes. Sarah Logsdon, one of the NOIRLab volunteers who accompanied the float along the parade route, was thrilled to see spectators drawing their grandchildren’s attention to the pictures on the float and connecting them to the written words for these, which were posted on the float in both O’odham and English.

Baoban’s name, which was selected by the Tohono O’odham Nation Youth Council, combines several ideas. “Bao” is reminiscent of the sound the coyote makes and is also the acronym for “baryon acoustic oscillations”, a technique DESI is using to study the nature of dark energy and the expansion history of the universe. “Ban” is the word for coyote in the Tohono O’odham language. “BaoBan” is also the short form of  “Ba: ‘o ñia g Ban” meaning “Where is coyote looking?”, which symbolizes our exploration of the wonders of the universe with DESI. Read the full story of BaoBan’s origins at https://www.desi.lbl.gov/2023/05/11/the-new-desi-ambassador-baoban/.

This was the first year Kitt Peak has entered a float in the rodeo parade. BaoBan brought good luck and the KPNO team was happy to learn that their float received first place in the business category. Congratulations to the team and thank you BaoBan!

NOIRLab volunteers who accompanied the KPNO float along the parade route included Jessica Harris, Jacelle Ramon-Sauberan, Alice Jacques, Pipa Fernandez, Sarah Logsdon, Michelle Edwards, and Lori Allen (Credit: L. Allen).

Filed Under: blog, feature on homepage

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