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Tsinghua’s Zheng Cai Wins 2024 "Science Exploration Award"
On August 26, 2024, the winners of the 6th “Science Exploration Award” were announced. Among the 49 outstanding young scientists recognized was Associate Professor Zheng Cai from Tsinghua University’s Department of Astronomy, who also leads the MUST project. Cai joined Tsinghua in 2019. He earned his Ph.D. from the University of Arizona in 2015, received the NASA Hubble Fellowship in 2016, and was selected for a national talent program in 2018. His research focuses on high-redshift galaxies, intergalactic gas, and large-scale structures. He has built a major sample of giant gaseous nebulae and identified “recycling inflows” around high-redshift galaxies as a key driver of the formation and growth of massive galaxies. He also investigates the enrichment of heavy elements in the high-redshift intergalactic medium. Cai’s achievements have earned him multiple honors, including the Tsinghua University Young Faculty Award (2021) and the “Excellent Mentor Award” (2022). His work has appeared in leading journals such as Science and Nature Astronomy, and was selected as one of Tsinghua’s Top 10 Research Highlights of 2023. He is currently spearheading the Wide-Field Survey Telescope (MUST) project. Source: Tsinghua University Department of Astronomy Official WeChat
2024-08-26
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A collaboration to push the boundaries of cosmos mapping
EPFL officially joined the Multi Spectroscopic Telescope (MUST) project, led by China’s Tsinghua University, as a founding member. This flagship project will enable scientists to better understand the young universe, dark energy and dark matter. Approximatively 13.8 billion years ago the Universe began with what we call the Big Bang. It expanded explosively, faster than the speed of light. Even though gravity immediately slowed this process down, physicists discovered more than 100 years ago that the Universe continues to expand. More recently, they found out that a mysterious form of energy – called dark energy – began speeding up its expansion again about 6 billion years ago. It’s a phenomenon still going on today and that holds a lot of unanswered questions. The MUlti Spectroscopic Telescope (MUST) project, led by Tsinghua University’s Department of Astronomy, is set to become a landmark in cosmological research and give insights of the young universe with unprecedented detail. For the first time, scientists will be able to trace the filamentary structure of the Universe in its first 3-billion years, using a detailed map made of tens of millions of measurements. Today, Martin Vetterli, President of EPFL, and Li Luming, President of Tsinghua University, signed a research collaboration agreement in Beijing, officially establishing EPFL as a member of the project. “With a 10 to 20-fold increase in survey capacity over current spectroscopic surveys, MUST will map the universe more comprehensively and at greater distances than ever before, deepening our knowledge of dark energy and dark matter,” explained Professor Jean-Paul Kneib, head of the Laboratory of Astrophysics (LASTRO) and the EPFL lead in this project. “This is very important because dark energy and dark matter account respectively for 70% and 26% of the content of the Universe and are critical elements influencing its expansion and structure,” he continued. A touch of EPFL’s expertise in the MUST telescope EPFL will contribute significantly to the 6.5-meter telescope with state-of-the-art high precision technology. Scientists in the Astrobots group will design modular fibre positioner robotic system, involving novel mechanical assembly, electronics, control, calibration, and testing. With the initial research undertaken in the past years, supported by Innosuisse and in partnership with the companies MPS Micro Precisions Systems from Switzerland and Orbray from Japan, EPFL has developed a strong expertise in fiber positioned robots for massive spectroscopic surveys and their miniaturization. The robots that will be developed for MUST will allow the project to conduct the extremely high-density galaxy mapping of the Universe. Analysis and outlook Through MUST, EPFL will also have access to a next generation spectroscopic survey with the ability to uncover hundreds of millions of distant galaxies and is committed to developing theoretical models that will play a pivotal role in the analysis of the vast amount of data expected. The project’s open-source philosophy ensures broad access to both software and hardware innovations. “The EPFL-Tsinghua collaboration will develop global scientific partnerships, promising transformative discoveries in our understanding of the universe and fundamental science, also taking advantage of the numerous data-science expertise at EPFL” said Martin Vetterli. “Joining MUST further increases EPFL’s participation in large international astrophysics projects, including DESI, Euclid and the Square Kilometer Array Observatory (SKAO), positioning us at the forefront of many exciting discoveries to come,” said Carolyn Crichton, EPFL MUST project manager and program director of SKACH. Authors: Julie Haffner, Tanya Petersen Source: EPFL
2024-07-02
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The Center for Astronomy Technology Tsinghua University has officially been renamed the Deep Space Technology Center Tsinghua University
On June 6, 2024, the Laboratory Management Office organized a symposium on the renaming of the university-level scientific research condition platform—the Center for Astronomy Technology. The expert panel reviewed the presentation from the Center for Astronomy Technology regarding its application for a name change. After thorough discussion and deliberation, the attending experts unanimously agreed to rename the Center for Astronomy Technology Tsinghua University to the Deep Space Technology Center Tsinghua University.
2024-06-06
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Farewell to American Academician Steve Shectman
—— Adapted from the article on "Zhengcai's Essay" by Cai Zheng, Associate Professor of Astronomy at MUST and Project Manager of MUST Dear colleagues from the Technology Center, It has been a year and a half since the "2030" initiative was established for MUST. Under the banner of the university, with the efforts of the technical team led by Professor Huang and the meticulous work of the management team, we have made progress. Recently, I would like to share some thoughts about the visit of the distinguished visiting professor from Tsinghua University, American academicians of both the National Academy of Sciences and the National Academy of Engineering, Steve Shectman. Steve stayed with us for nearly a month. He is straightforward, direct; he is proactive and honest. He "always cares" and "shares everything he knows, and spares no effort in his communication." Often, when the discussion was supposed to be over, a casual question from us would lead him to the blackboard to spend another half hour explaining things. He embodied the concept of "completely transparent," a phrase he emphasized many times. Despite being a member of the National Academies, he did not have any pretentious airs. He showed no impatience with "Telescope 101" questions. Even though I am considered a poor student in the team, often late or having to leave early due to other tasks, I have deepened my understanding of scientific engineering and learned some "system optimization" from him. I also realized how to discuss and collaborate effectively. Steve rode bikes and exercised with our younger team members, constantly conveying enthusiasm. There were times when Steve disagreed with us, such as on the positioning and size of the mirrors, the arrangement of the focal plane, etc. However, he was always candid and direct, explaining not just his thoughts but the reasons behind them. When we made decisions that differed from his, as long as they were carefully considered and well-reasoned, he accepted them with a smile and would draw out a long "fine...". He also admitted when he didn’t understand something and would happily laugh like a child when we came to the same conclusion or solved a problem he had trouble with. Through Steve, we can catch a glimpse of the reasons behind the success of the Magellan Telescope. Perhaps the most important factor is not how advanced your technology is, how rich your funding is, how big your team is, or how intelligent your members are. It’s about people, about whether you can be sincere, and about whether the team can unite as one. This includes both internal unity and communication with external partners—being open, transparent, and discussing things fully and honestly. By dedicating ourselves to the cause with our whole heart, letting go of personal attachment, confronting ingrained habits, and each member becoming an integral part of a collective endeavor, we can make the project flourish. As the saying goes, "The situation changes as the heart changes." If the heart is right, everything else will fall into place. In Steve, I see the spirit of Norman Bethune, the Canadian thoracic surgeon. When I studied in Yan’an, I was deeply moved by the story of Bethune. Even when he was critically ill, with poor treatment conditions and great physical pain, he would say, "I have no pain. I am very happy." Perhaps this happiness came from his devotion to his cause, from his fulfillment in realizing his own value, and from the deep love and trust between people. As Steve told us, the joy in life is not just about mastering more technology; it’s about being fortunate enough to work with outstanding friends in a team over a long period of time. I believe Steve must have felt the same way about his month at Tsinghua—sweet and fulfilling. MUST is one of the most challenging scientific engineering projects in China, and it is expected to become an internationally leading spectral survey facility. However, the "fifth stage" and "internationally leading" labels are not self-assigned. They have been recognized and anticipated by the global high-energy physics and cosmology community (such as NOIRLab), which puts a lot of pressure on us. MUST is tasked with building a 6.5-meter primary mirror, the largest aspherical convex mirror in China (2.4 meters), the largest lens array in history (1.7 meters), and the smallest, most precise 20,000 optical fiber positioning systems for controlling 6.2 mm robots. This survey will complement China’s space station survey telescope (CSST) and take humanity to the edges of the known and unknown universe. Along this journey, we have also received assistance from many American academicians and experts. For example, in the field of primary mirrors, we received help from Professors Roger Angel and Jeff Kingsley of the University of Arizona. In optical design, we benefited from the careful review by David Schlegel of the Lawrence Berkeley National Laboratory (LBNL). The project has also received encouragement from Sandra Faber of the University of California and Robert Williams, who was received by President Xi. In software systems, we have been guided by candid advice from Robert Lupton of Princeton University... We have also collaborated with domestic professional teams such as the Nanjing Institute of Astronomical Optics and Technology, the National Astronomical Observatory, the Chengdu Institute of Optics and Electronics, and the Changchun Institute of Optics, Fine Mechanics and Physics. What we are working on is not just a scientific engineering project, but an extraordinary top-tier research collaboration between China and the United States, aiming for a new exploration of the universe and deep space. No matter how the external environment changes, we must be grateful to and learn from scholars like Steve. We must learn from his straightforwardness, transparency, seriousness, and high standards. As the saying goes, "Think carefully before taking a step, and never look back after making a decision." When everyone is united, the MUST project will definitely reach a new level. Finally, I have attached two photos for everyone and wish that direct flights between China and the U.S. will increase and our cooperation will continue to improve.
2023-11-03
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The MUST team wins the group championship at the Tsinghua DoA Fun Sports Meeting
On October 19th, 2023, the Department of Astronomy, Tsinghua University held a unique fun sports meeting. Approximately 90 faculty and students actively participated and were divided into 9 groups to compete in a series of exciting sports events. The atmosphere throughout the sports meeting was enthusiastic, and members of each group participated actively in the competitions. Everyone invested their efforts, demonstrating high-level athletic skills and a spirit of teamwork, which garnered warm applause from the audience. After entertaining and intense competitions, the MUST team ultimately emerged as the first-place winner due to its outstanding performance. Collective strength was fully demonstrated during the games, and the team’s members’ coordinated collaboration earned recognition from other groups. The members of the MUST team feel immensely proud and honored for winning the championship. Team captain Lao Junsen expressed sincere gratitude to all the members for their hard work and selfless dedication, stating that the success of the sports meet was a result of teamwork and cooperation. He hopes that this spirit of unity and cooperation will enhance the team’s cohesion in their work. The fun sports meeting not only improved participants’ physical fitness but also further ignited their enthusiasm for sports and raised their awareness of teamwork. The successful organization of the sports meet provided a platform for faculty and students to showcase their individual skills and teamwork abilities, and also offered an opportunity for mutual exchange and deepening friendships between participants.
2023-10-19
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Professor Stephen Alan Shectman, a Fellow of the National Academy of Sciences of the United States, Visits Tsinghua University to Guide the Work of the MUST Team
From October 7 to November 3, 2023, Professor Stephen Alan Shectman, an outstanding visiting professor at Tsinghua University and a Fellow of the National Academy of Sciences of the United States , visited Tsinghua. During the nearly one-month period, Steve had in-depth discussions and communications with members of each subsystem of the MUST team, sharing his experience from working on the Magellan Telescope project. He maintained a candid and proactive attitude in technical exchanges. Whether discussing theoretical issues or optimizing technical solutions, Steve always enthusiastically provided assistance and guidance to the team. Despite the differing opinions among team members on technical approaches, Steve always respected others’ opinions and candidly shared his own thoughts. He was willing to listen to different views and showed understanding and support for the team’s decisions, which were made after careful consideration. When interacting with young team members, Steve taught them how to wholeheartedly engage in scientific engineering and encouraged everyone to unite and cooperate with each other. Through the close interaction with Steve, the MUST team further realized that the success of scientific endeavors depends not only on advanced technology and abundant resources but also on sincere and unified collaboration between team members. The MUST team will learn from Steve and take every step thoughtfully, jointly leading the way to new heights in the MUST project.
2023-10-07
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The Precision Optoelectronic System R&D Center of MUltiplexed Survey Telescope (MUST), Tsinghua University Signs an Agreement to Settle in Xiake Bay Intelligent Park
On the morning of August 28, 2023, the signing ceremony for the entry projects of Xiake Bay Intelligent Park was held in Jiangyin. This event aims to build Xiake Bay Science City as a highland for technological innovation, promote high-quality development of the science and technology innovation industry, and inject vigorous energy into the modernization construction of “strong, prosperous, beautiful, and high-quality” new Jiangyin. Xu Feng, member of the Standing Committee of the Wuxi Municipal Party Committee and Secretary of the Jiangyin Municipal Party Committee, announced the opening of Xiake Bay Intelligent Park. Professor Gao Song, academician of the Chinese Academy of Sciences and President of Sun Yat-sen University, sent a video address. Mayor Bao Ming, Wang Qi, and other city leaders attended the event. Associate Professor Cai Zheng, Vice Director of the Department of Astronomy, Tsinghua University and MUST project manager, gave a speech, and Professor Huang Lei, Chief Engineer of MUST and long-term professor of the Department of Precision Instruments, Tsinghua University , was also present. The unveiling ceremony of Wuxi Applied Technology Research Institute Precision Optoelectronics R&D Center (MUST) of Tsinghua University will promote resource sharing and complementary advantages between Xiake Bay Science City and the MUST project, creating a new situation of win-win cooperation. Source:“Jiangyin Release” official WeChat account
2023-08-28
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Representatives of École Polytechnique Fédérale de Lausanne (EPFL) Visit Tsinghua University for In-depth Communication with the MUST Team
From August 27 to 31, 2023, international collaborator and renowned cosmologist Professor Jean-Paul Kneib from École Polytechnique Fédérale de Lausanne (EPFL) visited Tsinghua University for in-depth discussions with the MUST scientific team. They worked together to outline and develop a work plan for the writing of the MUST Astrophysics Science White Paper. They also reported their findings and had exchanges with Vice President Wang Hongwei. Astrophysics science is an important component of the MUST project. During this visit, Professor Jean-Paul Kneib had in-depth discussions and exchanges with the MUST team on the research direction, key areas, and research plans of astrophysics science in the MUST project. He provided valuable opinions and suggestions for the writing of the MUST Astrophysics Science White Paper. Professor Jean-Paul Kneib is an outstanding representative in the field of international astrophysics. He has published papers in numerous top international academic journals and served as the chief scientist for several important international astrophysics projects. His visit not only provided valuable support and guidance for the research on astrophysics science in the MUST project but also played a positive role in promoting international cooperation and academic improvement at Tsinghua University. The writing of the MUST Astrophysics Science White Paper will provide important strategic references for the development of astrophysics science in the MUST project at Tsinghua University. It will also promote the integration and coordinated development of disciplines. In the future, Tsinghua University will continue to advance the research and development of astrophysics science in the MUST project and make positive contributions to the global astrophysics research.
2023-08-27
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Signing Ceremony of MUST Precision Optoelectronic System R&D Base Held in Jiangyin
On May 7, 2023, the precision optoelectronic system research and development base of MUST, Tsinghua University, signed a contract in Jiangyin. Guo Yong, Vice Secretary of the Party Committee of Tsinghua University, Xu Feng, member of the Standing Committee of the Wuxi Municipal Committee and Secretary of the Jiangyin Municipal Committee, Zheng Yongping, Dean of the Wuxi Applied Technology Research Institute of Tsinghua University, Niu Ben, Director of Domestic Cooperation Office of Tsinghua University, Cai Zheng, MUST Project Manager and Associate Chair of the Department of Astronomy, Tsinghua University, Huang Lei, MUST Project Chief Engineer, and Assistant Dean of the Department of Precision Instruments, and Jiangyin municipal leaders Wu Liping, Chen Hanjie, Cao Xinghua, and Qi Jun attended the signing ceremony. Xu Feng expressed a warm welcome to Guo Yong and his delegation. He said that Tsinghua University is a world-renowned institution of higher education with a long history and profound background, and has made outstanding contributions to the country's construction and development, social civilization, and progress. Jiangyin is the flag of county-level economic development in the country, and is currently accelerating the construction of "Science and Technology Innovation Jiangyin". The project will be settled in the Xiake Bay Science City, which is a high-quality development, high-quality growth pole, vibrant innovation source, beautiful ecological area, and digital new height, which Jiangyin key builds. Xu Feng stated that the Jiangyin Municipal Party Committee and the government will fully support the project's landing, provide all convenience for the project construction, and sincerely invite Tsinghua University to establish more cooperation with Jiangyin, and create a new highland of school and land cooperation and a new model of political and research cooperation. Guo Yong stated that Jiangyin is blessed with both fine people and excellent geographical location, and the Jiangyin Municipal Party Committee and Government have left a deep impression on everyone by focusing on technological innovation to promote high-quality economic and social development. He pointed out that in 2021, Tsinghua University released the "Tsinghua University 2030 Innovation Action Plan", which focuses on optimizing disciplinary layout, strengthening disciplinary construction, intensifying basic research and tackling key core technologies, and prosperous development of humanities and social sciences. The Wide-Field Survey Telescope Project signed this time is an important part of it. Guo Yong hopes that both sides will continue to deepen and expand the breadth and depth of university-local cooperation, steadily promote the construction of large scientific facilities, and provide strategic support for serving the country's technological independence and self-improvement. Deep space exploration is the "blue ocean" for breakthrough discoveries in the field of basic science. In the next decade, the development of deep space exploration will show further accelerated trends. However, in the extremely important fields of optics and infrared, the new generation of wide-field survey telescopes has yet to be completed internationally. In view of this, Tsinghua University has taken the lead in launching the important layout of constructing MUST, planning to build a large aperture, wide field of view, and high-efficiency spectral telescope. This facility belongs to the internationally leading large scientific installation, and is expected to achieve major fundamental and original breakthroughs in frontier directions such as dark energy evolution, nature of dark matter, and extrasolar planets, and obtain first-class international results. The MUST team will rely on the Wuxi Applied Technology Research Institute of Tsinghua University to establish the "Precision Optoelectronic R&D Center." They will focus on topics such as base construction, technology research and development, and outcome transfer and transformation, closely related to the large-scale optoelectronic equipment construction of MUST. They will accelerate the gathering of talents in the aerospace technology and high-end optical equipment manufacturing fields, and create a world-class scientific frontier R&D platform and application base to foster a good environment for scientific and technological innovation. Source: Wuxi Applied Technology Research Institute of Tsinghua University
2023-05-07
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The MUST scientific team published a paper on Science as the first author. Direct Imaging of Gas Recycling around a Massive Galaxy 11 Billion Years Ago
Galaxies are the birthplace of most stars and black holes. However, scientists are still debating, how galaxies accrete the fuel to sustain their growth and how they in turn pollute their environment with elements heavier than helium. The scientific team led by MUST project manager Cai Zheng at Tsinghua University has now directly observed the neighborhood of a massive galaxy in the early Universe. They find that the gas all around the galaxy is enriched with heavy elements, which means it has been polluted by the galaxy itself and by embedded satellite galaxies. Furthermore, this gas is spiraling onto the massive galaxy, fueling further star formation. According to the first models of galaxy formation, gas fell isotropically onto dark matter halos, was shock-heated to very high temperatures (millions of degrees), and subsequently cooled to form stars in the emerging/growing central galaxy. However, it is now clear that this so-called ‘hot-mode’ accretion accounts for only a small fraction of the fuel powering the violent star formation in massive galaxies in the early universe. Instead, cosmological hydrodynamical simulations indicate that a ‘cold-mode’ accretion (thousands of degrees) onto galaxies occurs along filaments. This accretion process is more efficient in transporting gas down to the galaxy, providing a natural mechanism to sustain the observed large star-formation rates. In turn, stars pollute their surrounding environment with elements heavier than helium, globally referred to as “metals”. The most energetic phenomena (supernova explosions) are even able to generate galactic outflows, enriching the circumgalactic gas. Recent cosmological simulations indicate that this metal-enriched gas ejected by the galaxy could fall back, resulting in a further supply mechanism to sustain intense star-forming activity. Therefore, a massive galaxy will both recycle its metal-polluted gas and use pristine, inflowing gas, which should have a non-zero metal content. However, direct observational evidence for the presence of such recycled inflows had not been obtained so far. An international team of astronomers has therefore targeted a massive system in the early universe, to get a first glimpse on how such galaxies accrete their gas. The chosen system, MAMMOTH-1, can be observed at an epoch corresponding to 11 billion years ago. It is a galaxy group embedded in large-scale cold circumgalactic gas, which shines bright in Lyman-alpha emission from hydrogen. With data from the Keck Cosmic Web Imager (KCWI, Keck II telescope) and narrowband imaging from the Subaru telescope, the team detected circumgalactic line emission in hydrogen, helium, and carbon extending for 300 000 light years. An analysis of the line ratios allowed the team to obtain the gas properties throughout the halo. The results show that the circumgalactic gas has already been enriched to solar metallicity, which is quite surprising at this early cosmic epoch. Further, the KCWI data allowed the team to analyse the kinematics of the emitting gas in the observed region. A detailed comparison of the data with cosmological simulations and an analytical model can explain the observed velocity patterns, which are most likely due to recycled inflow gas. The kinematic model indicates that the gas accretion is occurring at a rate of about 700 solar masses per year, much more than the measured star-formation rate of the central galaxy (81 solar masses per year). The metal-enriched inflow could thus fully sustain the intense star formation in the massive galaxy. “Our observations give a first hint that recycled inflows might be an ubiquitous supply mechanism for massive star-forming galaxies in the early universe”, remarks Zheng Cai of Tsinghua University, the Principle Investigator of this study and corresponding author of this paper. In addition, the team also found that satellite galaxies in this galaxy group have the same motion as the circumgalactic gas, indicating that they are embedded in the inspiraling streams. Therefore, these satellite galaxies could interact with and pollute the circumgalactic gas. “This makes the galaxy-gas ecosystem even more complex, but also it makes more plausible that gas recycling is an important ingredient,” adds Shiwu Zhang of Tsinghua University and first-author of the study. In future, one could have a lot more sensitive observations of circumgalactic emission to give us more insights on the intricate ecosystem of galaxies. The upcoming exquisite datasets, such as from the MUSE/VLT, KCWI instruments, and JWST, allows astrophysicists to directly study the circumgalactic gas in detail and thus better understand the physical processes governing the gas cycle around galaxies. Source: Official website of Tsinghua University. official website of Department of Astronomy, Tsinghua University
2023-05-05
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