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Dark Energy Spectroscopic Instrument (DESI)

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Ting-Yun Cheng (Sunny)

September 18, 2023 by aberti

aberti

What is your position or role in the DESI project?
I am a postdoctoral researcher at Durham University and fairly new in DESI. I collaborate on projects in the Galaxy & QSO working group.

Where were you born?
I was born and raised at a harbor city called Kaohsiung in Taiwan.

Where do you live now?
I live in Durham, United Kingdom where I work as postdoc at the Centre for Extragalactic Astronomy, Durham University.

What do you do as part of DESI?
As a new member, I have not been involved with many projects yet. I just recently get involved with a project on the detection and characterization of absorption features in QSO spectra using visual inspection and machine learning techniques.

What is the most interesting or exciting thing about your job?
As an academic, our job is not just research. There are also many other works involved such as teaching, supervision, observation, meeting organizing, etc. Each of them attracts me for different reasons. For example, I found it’s really rewarding to support students and see their growth.

Any advice for an aspiring scientist?
Searching for your science questions, as it is the best motivation when feeling lost during this journey.

What do you do for fun?
I enjoy doing all kinds of sports and video games. In particular, I love volleyball and was playing in a team for many years. I also enjoy being a backpacker traveling to many places. Sometimes, I’d listen to music while walking and daydreaming, and it feels great.

If you weren’t a scientist, what would be your dream job?
I have been strongly fascinated by three mysterious things—Universe, history, and ocean—since I was a kid. If I were not an astrophysicist, I’d probably become either an archaeologist or an oceanographer.

What excites/interests you most about DESI?
DESI (will) produces over millions of quasar (QSO) spectra. This huge amount of data can not only provide a great constraint to cosmological parameters as well as be used to investigate the environmental impact in galaxy evolution and formation.

Filed Under: meet a DESI member

What is your position or role in the DESI project?
I work in the DESI lensing topical group and I co-chair the DESI-II working group.

Where were you born?
Australia

Where do you live now?
Santa Cruz, California

What do you do as part of DESI?
My DESI work focuses on two things. First, together with the DESI lensing group, I am working on getting cosmological constraints for the Y1 data using galaxy clustering and galaxy lensing. Second, I am working in the DESI-II working group where we think about what science projects we could carry out after the end of the DESI 5 year survey.

What is the most interesting or exciting thing about your job?
Learning about new things everyday. I love knowing that there is still so much to discover.

Any advice for an aspiring scientist?
During your PhD, and postdoc years, it is important to specialize, and to “dig deep”. But after, don’t forget to also look around and see what else is going on. Try going to some talks in other departments and in other fields. Don’t ignore the bigger picture of the world in which we live.

What do you do for fun?
Activities with my kids, swimming, and gardening.

If you weren’t a scientist, what would be your dream job?
I would be a permaculture farmer.

What excites/interests you most about DESI?
The fact that we have so much data! I did my PhD on a survey that was 2 square degrees, so I still marvel at how much data we have with DESI.

Filed Under: meet a DESI member

What is your position or role in the DESI project?
I’m the co-lead of the “DESI CMB cross correlation” topical group within the Clusters, Cosmology, and Cross-Correlation working group. I work on thinking about the relationship between DESI galaxies and the cosmic microwave background–the oldest light in the universe, which can be gravitationally lensed, scattered, Doppler-shifted, and gravitationally-redshifted by galaxies, their host dark matter halos, and the hot gas inside them.

Where were you born?
I was born in New York City and grew up in Irvine, California.

Where do you live now?
I live in Waterloo, Ontario, Canada, just outside of the Toronto metro area. I’m a postdoc at the Perimeter Institute of Theoretical Physics and the Waterloo Centre for Astrophysics.

What do you do as part of DESI?
Mainly, I think about how we can learn about cosmology from DESI galaxies and quasars gravitationally lensing the cosmic microwave background. Lately, I’ve been working on using the gravitational lensing of the CMB by DESI quasars as a clean probe of the largest scales of the Universe, where certain models for inflation can generate strong large-scale correlations. I’ve also worked on studying redshift failures and identifying bad fibers within the LSS Catalog/KP3 working group, and am involved in the DESI-weak lensing cross-correlations project.

What is the most interesting or exciting thing about your job?
Contributing to our scientific understanding of the cosmos. I enjoy the thought that our work today might help people in the future understand the universe better. Or it may not—that’s the nature of science! At the least, any paper adds (even if only very incrementally) to our vast corpus of knowledge of physics.

Any advice for an aspiring scientist?
Always try to maintain a skeptical attitude towards your own research work. There’s no answer key in research, so you always have to come up with tests to make sure that what you’re doing is correct!

What do you do for fun?
Running, hiking, following baseball, and classical music.

If you weren’t a scientist, what would be your dream job?
I like exploring landscapes, so maybe something with maps or geography.

What excites/interests you most about DESI?
40 million galaxy spectra! The operations of DESI have gone so well (observing running months ahead of schedule despite the Contreras Fire), so I feel like that sets the standard for the rest of the collaboration.

Filed Under: meet a DESI member


What is your position or role in the DESI project?
I am a Theoretical Cosmologist working on the nature of Dark Energy and Dark Matter, where I have proposed new ideas related with Primordial Black Holes (PBH) and General Relativistic Entropic Acceleration (GREA).

Where were you born?
In Madrid, Spain, a member of a large family of scientists that date back several generations.

Where do you live now?
Also in Madrid, where I have a family with two children, a girl and a boy, aged 25 and 20 respectively. My wife is also a scientist, working in the LIGO-Virgo-KAGRA Collaboration.

What do you do as part of DESI?
I am now a member of the Publication Board, where I act as Handler for DESI collaboration papers. A year ago I was co-chair of the Education and Public Outreach team, that strives to make DESI’s scientific projects understandable by the general public.

What is the most interesting or exciting thing about your job?
Making theoretical predictions that can be tested with present-day observations.

Any advice for an aspiring scientist?
Explore what you like and think out of the box!

What do you do for fun?
Thinking in Science is the real fun! Well, I also enjoy oil painting, but this is mostly for relaxation. I attach here one of my last paintings.

If you weren’t a scientist, what would be your dream job?
I can’t even imagine it…!

What excites/interests you most about DESI?
The shear volume of exquisite data and the far-reaching fundamental physics scientific products (DM/DE) that this data will give us access to.

Filed Under: meet a DESI member

What is your position or role in the DESI project?
I am the manager of the DESI focal plane system, consisting of 5000 fiber-positioning robots and 10 cameras for guiding and focusing the telescope.

Where were you born?
I was born in Cambridge, England, and spent my early years in Bristol, Leeds and London, all in the UK, as well as Iran and Mexico. I went to high school and university in Toronto, Canada.

Where do you live now?
I came to California for graduate school, spent five years in France at CERN, then returned to California for a postdoc and faculty position. I now live in Irvine, which is just south of Los Angeles.

What do you do as part of DESI?
Each morning, I check on the 5000 robots to look for any problems during the night. The focal plane is a unique and central part of the DESI instrument, so I work on outreach materials to share the excitement with my collaborators and the public, including a poster, animations and 3D-printed models. I also work with my students at UC Irvine to better understand our quasar sample and Lyman-alpha forest absorption, and look for novel ways to apply machine learning methods.

What is the most interesting or exciting thing about your job?
A large survey like DESI offers such a great variety of interesting topics to work on, from instrumentation and operations to simulation and cosmological inference. I am excited to learn new skills every day, working with my students, in diverse areas such as electronics, statistics, machine learning, and visualization.

Any advice for an aspiring scientist?
Doing science isn’t only about publishing papers. Take advantage of the many opportunities to learn new skills and don’t be afraid to explore new avenues and change directions a few times in your career.

What do you do for fun?
I enjoy cooking and eating good food, building things, taking photos, and being active (especially running, soccer, and pickleball).

If you weren’t a scientist, what would be your dream job?
A sheep farmer in the Shetland Islands.

What excites/interests you most about DESI?
My collaborators. Although the DESI collaboration probably feels large to many of us, it is one of the smaller groups I have worked with, and we have an amazing team.

Filed Under: meet a DESI member

Nature, 3 July 2023

Filed Under: in the news

Science News Wire, 14 June 2023

Filed Under: in the news

Innovation News Network, 14 June 2023

Filed Under: in the news

Cosmos, 15 June 2023

Filed Under: in the news

Physics, 16 June 2023

Filed Under: in the news

What is your position or role in the DESI project?
I am a PhD candidate at the University of Utah primarily involved with Lyman-alpha forest cosmology studies.

Where were you born? Where do you live now?
I am from Omaha, Nebraska, and I now live in Salt Lake City, Utah. SLC is easily the most incredible and beautiful place I have ever lived!

What do you do as part of DESI?
I work on developing spectroscopic models for the quasars observed by DESI. These models will help us maximize the cosmological information we can extract from the quasar sample.

What is the most interesting or exciting thing about your job?
The potential for DESI to discover things that no one was expecting or looking for.

Any advice for an aspiring scientist?
In the words of Alie Ward: “ask smart people stupid questions”. Because in reality, there are no stupid questions. Never let anyone discourage your curiosity.<

What do you do for fun?
I try to spend as much time as I can outdoors: hiking, long camping trips, skiing, roller skating, and any sort of wildlife watching. I also love communicating science to the public. I host Astronomy on Tap in Salt Lake City, am a science communicator with the Natural History Museum of Utah, and volunteer at the local zoo. Finally, I have 3 perfect cats who command the remainder of my time.

If you weren’t a scientist, what would be your dream job?
A wildlife or park ranger… maybe in Alaska 🙂

Filed Under: meet a DESI member

Dillon Brout, Harvard University
June 16, 2023

The universe (and especially Messier 101) never ceases to amaze us. Recently, a remarkable Type II supernova event unfolded in the nearby “Pinwheel galaxy” (M101), captivating astronomers worldwide. We are just 12 years removed from the famed supernova 2011fe residing in M101 and that sparked its own paradigm shift for studies of supernovae. The one that occurred this past week, dubbed SN2023ixf, promises to offer a wealth of new scientific insights due to its exceptional characteristics and close proximity. This presents a rare opportunity to delve deeper into the mysteries of stellar explosions and gain a better understanding of their relation, formation, and interaction with their environments; and the DESI is on the case!

Why is this rare event so useful?
Type II supernovae occur when massive stars exhaust their nuclear fuel and undergo a catastrophic collapse, resulting in a brilliant explosion. These colossal explosions release an enormous amount of energy and because this occurred in one of the closest galaxies to our own (M101 is a mere 21 million light-years away) it is extremely bright in astronomical standards. Furthermore, the proximity of this supernova offers an unprecedented opportunity for astronomers to study its evolution from start to finish in great detail, unlike many other supernovae that occur in more distant galaxies. We can see the star as it was before its death and eventually peer into the aftermath.

What is a Type II Supernova?
Type II supernovae, like SN2023ixf, have distinctive characteristics that set them apart from other types of supernovae. These explosions occur when the star’s core collapses under its own gravity, leading to a rebound that creates a powerful shockwave. This shockwave blasts away the outer layers of the star, generating a brilliant burst of light. As the ejected material interacts with the surrounding medium, it produces various elements, enriching the cosmos with carbon and oxygen, crucial for life itself. They are primarily identified by the presence of hydrogen lines in their spectra, which signifies the explosion of massive stars that still contain substantial amounts of this elemental gas. By analyzing the spectroscopic signatures of these supernovae in detail, astronomers can glean valuable information about the nature of the progenitor star, the explosion dynamics, and the elements synthesized during the event.

What is DESI’s Role?
DESI is uniquely positioned to witness and document the evolution of SN2023ixf through careful analysis of its spectrum. We can take advantage of the twilight time before the night sky is fully dark, because the supernova is so near and so exceptionally bright, DESI can gather crucial data without impacting the regular survey operations. So we will be monitoring the spectrum of SN2023ixf continuously, especially during all phases of the moon when other spectrographs around the world will in many cases be swapped out for infrared instruments (due to the optical brightness of the moon).

DESI Nightly Spectra showing the evolution of SN2023ixf. Top: Flux versus wavelength shown for each night. Bottom: Ratio of the flux for each night compared to the flux on the previous night.

The continuous, uniform, and highly calibrated data acquired by DESI during this remarkable event will provide one of the highest quality datasets ever acquired for a type II supernova. This can be seen in the included Figure (raw data). We have been taking data every night since May 23rd just before it peaked in brightness.  One can see different elements of the spectral features evolving over time. In the bottom panel is the ratio of the spectra which suggests that the supernova is getting redder over time. Such data will enable us to address outstanding scientific questions and explore intriguing possibilities. For instance, the extended observations of SN2023ixf over the next few days and weeks  may offer insights into the interaction between the supernova ejecta and the surrounding medium. This scenario could potentially yield observations of shock waves, collisions, or even the formation of exotic elements through nucleosynthesis. In addition, the exceptional quality of DESI’s flux calibration will significantly contribute to the accuracy and reliability of the dataset when comparing features of the spectrum across different nights and observing conditions.

By harnessing the power of DESI, we will be closely monitoring and will be ready should something unexpected happen with SN2023ixf!

Filed Under: blog, feature on homepage

The first public release of DESI data is now available! Taken during DESI’s Survey Validation phase, the Early Data Release (EDR) includes spectra and redshifts for 1.2 million galaxies and quasars, as well as observations of nearly half a million stars in our own Milky Way galaxy.

The DESI Early Data Release by the numbers:

  • Amount of data: 80 TB
  • Exposures taken: 2,480
  • Redshifts collected: 1.2 million extragalactic (galaxies and quasars)
  • Objects in the Milky Way imaged: 496,000
  • Quasars spotted: 90,000
  • Time spent observing: 6 months 
  • Size compared to full DESI dataset: 2%

Part of DESI’s Survey Validation included the One-Percent Survey, visualized in the video below. Researchers took detailed images in 20 different directions on the sky, creating a 3D map of 700,000 objects and covering roughly 1% of the total volume DESI will study. With the instrument and survey plan successfully tested, the main DESI survey is now filling in the gaps between those observations.


Credit: David Kirkby/DESI collaboration

Filed Under: announcements, blog, feature on homepage

Lawrence Berkeley National Laboratory, 13 June 2023

Filed Under: press releases

What is your position or role in the DESI project?
I have worked as a co-lead of the galaxy and quasar clustering working group in the past. Right now, I don’t have official managerial positions. I am supervising my students’ research and trying to figure out how to extract cosmology with higher-order clustering.

Where were you born?
I was born in the Black Sea port of Sokhumi in Georgia (the country).

Where do you live now?
I live in Manhattan, Kansas, USA

What do you do as part of DESI?
I am trying to come up with new ways of analyzing the clustering of DESI galaxies. Two directions that interest me right now are the usage of higher-order statistics and small (nonlinear) scales for cosmology. Both are very promising in terms of potential scientific yield but the methodology for dealing with them is currently not fully developed.

What is the most interesting or exciting thing about your job?
The most exciting part of my job is that I spend quite a lot of it trying to solve mathematical puzzles, something I would be willing to do for free. Another part of my job is teaching young scientists physics and math, also something that I really enjoy.

Any advice for an aspiring scientist?
When you are an undergraduate student you succeed by doing well what other people tell you to do (i.e. solving homework problems, preparing well for the test, etc.). As soon as you become a Ph.D. student, you have to realize that your professional development is now completely up to you. Take the initiative, identify things that you need in your career but don’t know well (programming? applied statistics?), and learn them. Choose research projects that you feel passionate about and work hard on completing them. Your supervisors and senior peers will be glad to advise you and help you along but you must be the one in the driver’s seat.

What do you do for fun?
I enjoy playing chess and reading history books.

If you weren’t a scientist, what would be your dream job?
If I weren’t a scientist I would probably end up being a teacher or a librarian. Or I may have chosen a career that utilizes math, e.g. actuary or an accountant.

What excites/interests you most about DESI?
What excites me most about DESI is the opportunity to work alongside the brightest minds in my field. I enjoy going to the collaboration meetings, asking questions, and coming back with the research ideas.

Filed Under: meet a DESI member

The story behind creating and naming our favorite coyote.
Samuel Brieden, The University of Edinburgh
May 12, 2023

Welcome our new DESI ambassador for Education and Public Outreach (EPO), BaoBan! You might have met him already, when he was presenting our powerful focal plane (see a virtual tour through it here) or wishing a happy new year. From now on, BaoBan is assisting us with science communications, as long as he is in the mood. Although BaoBan is very attracted to the Mayall telescope, he shows up at Kitt Peak quite rarely because, like other wild coyotes, BaoBan spends most of his time hunting in the Arizona mountains. But whenever we are lucky enough to be honored with his visit, an aura of ancient wisdom about life and the night sky surrounding him sparks new insights and creative ideas. It’s a bit magical!

Say Hi to BaoBan! He is our ambassador, and NOT a “mascot”! Being called a domesticated animal makes BaoBan so angry that anyone who dares to take such words in their mouth will eventually meet BaoBan’s mouth. And believe me, nobody wants to be bitten by BaoBan!

This article is a chronology of our common history with BaoBan. From the story of his ancestors, to how he was brought to life and given a name, and finally his meaning to us, to our roots as a scientific collaboration, and to our environment.

The Tohono O’odham Nation

DESI resides in the Mayall telescope at Kitt Peak National Observatory (KPNO), which sits atop I’oligam Du’ag (audio below) in the homeland of the Tohono O’odham (audio below) Nation (TON). Since time immemorial the Tohono O’odham (TO), meaning “desert people”, have lived in the Sonoran desert and preserved their rich culture. The nation is governed by the TON Tribal Government, organized into 11 districts. You can learn more about the history and culture of the TON here. We are deeply grateful for their permission to undertake observations of the night sky within the TON homeland at KPNO, and we cannot emphasize enough that the success of our scientific mission would not be possible without the TON’s generosity.

Pronunciation of “I’oligam Du’ag”
Pronunciation of “Tohono O’odham”
The DESI logo
The DESI logo

It is this relation to the TON that must have inspired Berkeley Lab engineer (and artist!) Robin Lafever when he created the DESI logo in 2013, and in particular the detail in the lower right corner: the profile of a howling coyote. In fact, the coyote plays an important role in the TO mythology. Robin had seven different names for the coyote in mind, his favorite being “Bao Wao Wao”. “Bao” is reminiscent of baryon acoustic oscillations (BAO), the primary cosmological observable DESI is measuring to infer the expansion history of the universe, and “Wao” represents the coyote’s howl.

A new coyote is born

The DESI logo inspired Claire Lamman, PhD student at Harvard University and member of the DESI EPO committee, to transform Robin’s profile-view creation into a fully-fledged comic figure.  As you can see in her comic strips, at first the coyote seems nice and harmless, but the sheer power of the Dark Energy Spectroscopic Instrument occasionally evokes his dark side. All Claire’s comic strips can be found here.

Left: Claire’s first comic strip featuring the DESI coyote. Right: The second installment. Not only was the DESI logo inspiration for the coyote, but also for his shirt! (click to enlarge)

Amazed by his strong character, the EPO committee considered how to introduce Claire’s extraordinary art to the public. There was only one thing missing for Claire’s comic figure to become even more successful than Looney Tunes legend Wile E. Coyote: a proper name!

Setting up a poll

Several candidates emerged from our initial brainstorming, playing either on the location of the telescope (Coyote-Kitt, Maya), on the pursued science (Cosmo-Coyote, Bao), or simply on the survey name itself (Desiree). This was so much fun that we decided to poll the entire collaboration for suggestions. Other names received were Can-do Canis, Desita, and the name of the original coyote in Robin’s DESI logo: Bao Wao Wao. Around 60 collaboration members voted in just one day, and the majority decided to conduct a naming contest within the Tohono O’odham school district (see the compilation of Slack messages below).

Compilation of Slack messages showing the result of the DESI internal poll about asking the TO community for help with finding a name. (click to enlarge)
Back to the roots

We first consulted Jacelle Erin Ramon-Sauberan, PhD Candidate at the University of Arizona, faculty at Tohono O’odham Community College, and information specialist for AURA/NOIRLab, and worked closely with KPNO. Jacelle put us in contact with the TON Youth Council  (TONYC). The TONYC consists of four representatives from each of the 11 districts, and their mission is to enhance the cultural awareness and self-esteem of TON youth within modern times by organizing social events. The Council holds monthly meetings, which are open to the public. Francine Senechal, the TONYC Manager, kindly invited us to present the coyote naming contest at a Council meeting.

At the same time we decided to reach out to the TON, two collaboration members independently raised the idea that the name include “Ban”, the word for “coyote” in the TO language. It was suggested that we connect “Ban” with the TO word “Ba:”, meaning “Where”, such that the combination “Ba:Ban” is extendable to “Where is coyote looking?” This would allude to the mysteries of dark energy DESI is trying to unravel, and sparked the obvious idea of “BaoBan”, combining “Ba:Ban” with the previous suggestions that include “Bao”.

The day of the TONYC meeting arrived, and fortunately it was held virtually so I could attend from Barcelona. After introducing DESI and the science we pursue with it, I talked about our plan to find a name for the DESI coyote. I provided a list of all the suggestions we had collected so far, as well as their variants, meanings, pronunciations, etc., and asked them to vote for the name they found most suitable. The TONYC members were interested and very keen to help. They agreed to bring the list of names into the local youth communities of the district each of them represents, engage their members to discuss the different options, and choose their favorite name.

The final decision

After thoroughly considering all names, discussing them within each district, and exchanging their ideas at a meeting, the TONYC voted, and Francine communicated the official result:

  1. BaoBan
  2. Cosmo Coyote

What a great choice! Within the EPO committee we immediately fell in love with the name BaoBan, as it nicely combined all the different ideas the collaboration had in mind throughout the process. “Ban” as the TO word for coyote, reminding us of the roots of where the DESI telescope is built, and “Bao” as both the sound the coyote makes, and a clear reference to DESI’s primary science goal: measuring BAO from galaxy maps. These ideas culminated in another new comic strip by Claire (below), which celebrates that together with the TONYC we found such a beautiful name for our DESI ambassador! And there is even more to the story…

Claire’s new comic strip explaining the meaning of BaoBan. (click to enlarge)
An alternative meaning

Not only did the TONYC vote for the name, they also put me in contact with TO language experts Leslie Luna and Ronald Geronimo from the TO Community College, with whom I discussed the prospect of connecting “BaoBan” to the meaning behind the similar suggestion “Ba: Ban”, where “Ba:” = “Where?” as mentioned before. As it turns out, the TO expression “Ba: ‘o …” actually means “Where is …”, but this does not imply that “Ba: ‘o Ban” would mean “Where is coyote”, because “‘o” is an auxiliary verb that must be accompanied by a full verb. However, we can extend the expression to “Ba: ‘o ñia g Ban” (audio below), which literally means “Where is coyote looking?” and argue that “BaoBan” (audio below) is just the short form of that longer name. In this way, the name BaoBan also serves as a symbol that we and the TON may work together to explore new discoveries in our beautiful sky.

Pronunciation of “Ba: ‘o ñia g Ban”
Pronunciation of “BaoBan”
Final remarks

Throughout this process it has been amazing to see how an enjoyable drawing and a simple idea (finding a name for that drawing) can lead to something big, both engaging the collaboration and establishing a new link between DESI scientists and the TO community.

BaoBan symbolizes how the enormous scientific effort by ~70 member institutions with over 700 active collaboration members from all over the world is deeply connected with the TO, who share part of their homeland to discover the mysteries of our universe. BaoBan reminds us that the night sky is the same for everyone, independent of national or cultural identity. Furthermore, BaoBan reminds us to always respect our roots and our environment, and to never forget that the deeper our maps of the cosmos become, the deeper the relationships we will foster among different cultures and people.

It is no coincidence that Robin Lafever began this processes at the very moment his pencil touched paper to create the DESI logo. Robin was known as a man with a wonderfully warm and engaging personality, who delighted everyone around him with his creativity. Almost two years after his passing he would surely be flattered that people enjoy his creation enough that they continue to develop it, from Bao Wao Wao to BaoBan.

Acknowledgements

I would like to express deep thanks to all the wonderful DESI collaborators involved in this journey, those who participated in the poll and brought in their naming suggestions, and especially Claire Lamman, Angela Berti, Biprateep Dey, Parker Fagrelius, and everyone from the DESI EPO committee. Special thanks also to Daniel Eisenstein, Dustin Lang, Eric Linder, David Sprayberry, Lori Allen, Arjun Dey, Nathalie Palanque-Delabroullie, Kyle Dawson, and Michael Levi. Finally, I am indebted to Jacelle Erin Ramon-Sauberan, Francine Senechal, Leslie Luna, and Ronald Geronimo for all their effort and kindness giving me insight into their fascinating culture.

Filed Under: blog, feature on homepage

Filed Under: uncategorized

What is your position or role in the DESI project?
I helped design the DESI peculiar velocity survey and also work on BAO measurements, of which the later are the main science driver of DESI.

Where were you born?
I was born in a small town in Austria, where people only ever come from, but never go to.

Where do you live now?
I currently live in Daejeon, which is a city close to the centre of South Korea, where I work as postdoc at the Korea Astronomy and Space Science Institute.

What do you do as part of DESI?
Besides working on the DESI peculiar velocity survey and the BAO measurements, which are both currently my main focus in DESI, I tend to spread my time between far too many projects within the collaboration. For example I am involved in the stellar mass measurements, looking for rare galaxies, doing observations, helping with the weak lensing project, just to name a few. My daily routine is mostly focused developing code to analyze data form simulations and since recently also actual DESI data from observations. But I also organize meetings, seminars and have to attend many telecons with my collaborators.

What is the most interesting or exciting thing about your job?
Being able to be among the first people to explore new data and thereby helping to improve our knowledge of the universe.

Any advice for an aspiring scientist?
It might be survivorship bias, but “don’t give up and be proactive.”

What do you do for fun?
Hiking, board games, traveling, board games, cooking, board games, archery, and have I mentioned board games yet?

If you weren’t a scientist, what would be your dream job?
A very difficult question as almost all my dream jobs were various types of scientist, but if I had to pick another line of work, it would probably be diplomat.

What excites/interests you most about DESI?
The enormous amount of data collected and the impressive efficiency of the survey. Just to give an example, I was part of the observing team on a very good night in which we collected in a single night as many spectra of galaxies as it took another survey several years to reach the same number only 15 years prior.

Filed Under: meet a DESI member

Claire Lamman, Harvard University
April 7, 2023
Audience at the Chabot premiere watch the movie’s opening scene. Photo credit: Marilyn Sargent, LBNL. © The Regents of the University of California, Lawrence Berkeley National Laboratory

DESI’s planetarium show, “5000 Eyes”, was recently released to the public. It will be shown in hundreds of planetariums around the world and translated into ten languages. The support and contributions of many DESI members grew this project far beyond the little film I initially imagined. Here is how “5000 Eyes” went from the daydream of a first-year graduate student to a global production.

A couple months after delivering my final show at Fiske Planetarium, I was sitting in a session at DESI’s 2019 summer collaboration meeting. I had committed to starting graduate school at Harvard in the fall but was undecided about a research path. I was new to cosmology and just starting to learn about DESI. When a talk started to go over my head, which was often, I imagined what a planetarium show about DESI might look like.

Kitt Peak was building an outreach center and I thought it would be nice to record myself giving a short planetarium talk about DESI that could be shown at the center. A leader from our Education and Public Outreach Committee, Parker Fagrelius, encouraged me to reach out to DESI’s director, Michael Levi, and seek funding from the DESI Institutional Board. With the enthusiastic support from Parker and Michael, I formulated a proposal to create a small planetarium film. My idea was to use as much existing media as possible—such as 3D models of the Mayall telescope, footage on Kitt Peak, and DESI data, to make the best use of any resources given to the project. It received unanimous support from the Institutional Board and I found myself, a graduate student still unsure about what my thesis would be on, in charge of a full-scale production.

Fortunately, I helped Fiske make a series of short films during my time as an undergrad at CU Boulder and generally knew what went into making a planetarium film. I developed a script based on the media available and what I knew of Fiske’s software. After many iterations on the script and feedback from DESI people, we began working with Fiske to produce the movie.

There is so much to say about DESI (just check out all the blog posts below this one!), so it was not easy to decide what to include in a 20 minute movie. One idea we wanted to make sure to communicate was that advances in modern cosmology don’t magically spring from the minds of a couple scientists. It takes many people, including many young people, with a variety of backgrounds. We came up with a selection of six DESI members from four continents. The international participants all found ways to get high-quality recordings themselves! For those of us in the U.S., we were able to coordinate an in-person shoot on Kitt Peak.

Our visit to Kitt Peak was my favorite part of making the film. We had two days with the videographer from Fiske to shoot interviews and capture footage of the telescope and mountain. During this time, the Kitt Peak Staff was especially helpful and accommodating. I was even able to carry out one of my support observing shifts in person. Up until this trip, I was hesitant about representing DESI as such a new member. But observing on the mountain made me feel like I was truly part of the collaboration for the first time.

Behind the scenes of our shoot on Kitt Peak. Pictures as they appear: focal plane expert Kevin Fanning, Fiske videographer Thor Metzinger, DESI lead observing scientist Satya Gontcho A Gontcho, film director Claire Lamman, and manager of the Mayall telescope David Sprayberry.

As main production ramped up, I directed the Fiske team and coordinated some additional contributions of DESI members. In particular, once I found out that David Kirkby could make a moving 3D model of the focal plane, I knew we absolutely had to include it. Who doesn’t want to fly through a forest of robots?? He put in an impressive amount of work to faithfully bring the focal plane to life and create a memorable scene.

Fiske’s team was also very excited about the film, especially once we had the go-ahead to use galaxy positions from DESI’s full year one data. This was somewhat of a technical challenge, since they were determined to render every single galaxy and, unlike DESI, did not have access to a supercomputer! The resulting fly-through is stunning. All the time I spent using DESI data in my research did not compare to soaring through the most detailed map ever made of our nearby universe in a planetarium. I am very impressed with the work of Fiske’s production team.

Because DESI is an international collaboration, it was important to make the film widely available and in multiple languages. Many DESI members have volunteered to help create translations. As of the writing of this blog, there are plans to translate the film into 10 different languages! Small planetariums all over the world are excited to have access to a free film in their local language. The film’s download site also includes an educational guide and outreach package filled with additional material that DESI people have put together. Our science will reach a large, diverse audience thanks to the work of our collaboration!

It has been exciting to see the ways that DESI members are using this film to engage with their local communities. At the premieres, it’s also been a joy to see our family members, especially kids, get a glimpse into what we work on. Looking back, it’s a bit staggering to see how much this project has grown and how many people contributed. This truly is a film about DESI, by DESI!

As of the writing of this blog, the film has been downloaded by 112 planetariums in 31 states and 24 countries.

More photos from the Chabot premiere. Photo credit:  Marilyn Sargent, LBNL. © The Regents of the University of California, Lawrence Berkeley National Laboratory

Filed Under: blog, feature on homepage

NOIRLab, 2 March 2023

Filed Under: in the news

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