A normal process called cell competition, in which healthy tissues eliminate unhealthy cells, could be responsible for cancer relapses in patients months or years after they were declared cancer-free
Astronomers using the International Gemini Observatory, operated by NSF’s NOIRLab, have discovered the closest-known black hole to Earth. This is the first unambiguous detection of a dormant stellar-mass black hole in the Milky Way. Its close proximity to Earth, a mere 1600 light-years away, offers an intriguing target of study to advance our understanding of the evolution of binary systems.
The European Microwave Association (EuMA) has announced Marian Pospieszalski— a senior research engineer at the National Science Foundation’s National Radio Astronomy Observatory (NRAO)— as the recipient of its 2022 Pioneer Award. The EuMA Pioneer Award recognizes individuals responsible for noteworthy advances in the field of microwaves that have had a lasting and significant impact on the microwave community.
Rutgers researchers are seeking to develop the technology to modify or “edit” protein molecules in the body—an advance that could spur major breakthroughs in human health.
A multi-institution team of researchers led by Indiana University chemist Sara Skrabalak has been awarded $1.8 million from the NSF to establish a research center focused on transforming nanocrystal discovery and design.
Following a generous grant from the National Science Foundation’s Spectrum Innovation Initiative (SII), NSF’s National Radio Astronomy Observatory (NRAO) will expand efforts to establish and support the co-existence of research and commercial entities across the radio spectrum.
While observing a newly-dormant galaxy using the Atacama Large Millimeter/submillimeter Array (ALMA) and the Hubble Space Telescope (HST), scientists discovered that it had stopped forming stars not because it had used up all of its gas but because most of its star-forming fuel had been thrown out of the system as it merged with another galaxy. The result is a first for ALMA scientists. What’s more, if proven common, the results could change the way scientists think about galaxy mergers and deaths.
Irvine, Calif., Aug. 25, 2022 — From monitoring sandy beaches to gauge the effects of sea-level rise to holding clinical trials for potentially lifesaving cancer treatments, scholars, scientists and physicians at the University of California, Irvine are blazing new paths to help change the world. And their impact keeps growing.
Los datos observacionales sin precedentes de HL Tau obtenidos por el Atacama Large Millimeter/submillimeter Array (ALMA) en 2014 han sido citados en más de mil estudios científicos en los últimos 7 años y medio. Ello ha permitido que la comunidad astronómica logre importantes avances en el estudio de la formación de planetas.El hito se produce cuando los ingenieros del Observatorio Nacional de Radioastronomía (NRAO) de la Fundación Nacional de Ciencias de EE. UU. se embarcan en ambiciosas actualizaciones de los receptores responsables de la claridad de las observaciones iniciales.
Ground-breaking 2014 HL Tau observational data from the Atacama Large Millimeter/submillimeter Array (ALMA) has been cited in more than 1,000 scientific studies in the past 7.5 years, aiding in major breakthroughs in scientists’ understanding of planet formation. The milestone comes as engineers at the U.S. National Science Foundation’s National Radio Astronomy Observatory (NRAO) embark on ambitious upgrades to the receivers responsible for the clarity of initial observations.
Scientists using the Atacama Large Millimeter/submillimeter Array (ALMA)— in which the National Radio Astronomy Observatory (NRAO) is a partner— to study planet formation have made the first-ever detection of gas in a circumplanetary disk. What’s more, the detection also suggests the presence of a very young exoplanet.
Gracias al Atacama Large Millimeter/submillimeter Array (ALMA) por primera vez un equipo de investigación detectó luz en longitudes de onda milimétricas proveniente de una fuerte explosión causada por la fusión de una estrella de neutrones con otra estrella.
Scientists using the Atacama Large Millimeter/submillimeter Array (ALMA) have for the first time recorded millimeter-wavelength light from a fiery explosion caused by the merger of a neutron star with another star.
Using a $7.5 million grant from the National Science Foundation (NSF), University of Florida engineers are leading a new effort to understand how groups like the poor, children and the elderly, and the disabled are marginalized by current technologies like smartphones and video conferencing and how current and future technologies can be designed to be more inclusive.
The $8.2 million grant is the largest is the largest ever direct NSF award to Tulane.
Six NAC alums have accepted offers from outstanding graduate programs around the country. Each will receive a $5,000 AUI Board of Trustees NAC Bridge Scholarship Award, with AUI and NRAO’s congratulations and best wishes for a smooth start to an exciting new chapter of their lives.
Tras usar el Atacama Large Millimeter/submillimeter Array (ALMA) para observar regiones donde se forman estrellas en la Gran Nube de Magallanes, un equipo de investigación descubrió la existencia de un turbulento fenómeno de tira y afloja en la incubadora 30 Doradus. Las observaciones revelaron que, a pesar de una intensa retroalimentación estelar, la gravedad está incidiendo en la forma de la nube molecular y, contra todo pronóstico, fomentando la formación de estrellas jóvenes y masivas. Los resultados de las observaciones se presentaron hoy en una conferencia de prensa durante la asamblea n.o 240 de la Sociedad Astronómica Estadounidense (AAS, en su sigla en inglés), celebrada en Pasadena (California, EE. UU.), y se publicarán la revista The Astrophysical Journal (ApJ).
While using the Atacama Large Millimeter/submillimeter Array (ALMA) to observe large star-forming regions in the Large Magellanic Cloud (LMC), scientists discovered a turbulent push-and-pull dynamic in the star-forming region, 30 Doradus. Observations revealed that despite intense stellar feedback, gravity is shaping the molecular cloud, and against scientific odds, is driving the ongoing formation of young, massive stars. The observations were presented today in a press conference at the 240th meeting of the American Astronomical Society (AAS) in Pasadena, California, and are published in The Astrophysical Journal (ApJ).
Scientists using the Atacama Large Millimeter/submillimeter Array (ALMA)— an international observatory co-operated by the US National Science Foundation’s National Radio Astronomy Observatory (NRAO)—have observed a significant amount of cold, neutral gas in the outer regions of the young galaxy A1689-zD1, as well as outflows of hot gas coming from the galaxy’s center. These results may shed light on a critical stage of galactic evolution for early galaxies, where young galaxies begin the transformation to be increasingly like their later, more structured cousins. The observations were presented today in a press conference at the 240th meeting of the American Astronomical Society (AAS) in Pasadena, California, and will be published in an upcoming edition of The Astrophysical Journal (ApJ).
Using the Atacama Large Millimeter/submillimeter Array (ALMA), astronomers have imaged the debris disk of the nearby star HD 53143 at millimeter wavelengths for the first time, and it looks nothing like they expected. Based on early coronagraphic data, scientists expected ALMA to confirm the debris disk as a face-on ring peppered with clumps of dust. Instead, the observations took a surprise turn, revealing the most complicated and eccentric debris disk observed to date.
Gracias al Atacama Large Millimeter/submillimeter Array (ALMA), un equipo de astrónomos y astrónomas obtuvo la primera imagen de un disco de escombros de la estrella cercana HD 53143 en longitudes de onda milimétricas, y el resultado dista mucho del que se esperaba. Sobre la base de datos coronagráficos, la comunidad científica esperaba que ALMA confirmara que el disco tenía el aspecto de un anillo visto de frente y con aglomeraciones de polvo. En cambio, el estudio reveló el disco más complejo y excéntrico observado a la fecha.
Seven new scientific results from the Atacama Large Millimeter/submillimeter Array (ALMA), the Very Large Array (VLA), and the Very Large Array Sky Survey (VLASS) will be revealed at multiple press conferences during the 240th meeting of the American Astronomical Society (AAS) between June 13-15, 2022 in Pasadena, California.
FAU’s Reza Azarderakhsh, Ph.D., was among 34 investigators nationwide selected by the NSF for RINGS, which is short for Resilient and Intelligent Next-Generation Systems. His project is the only one working on taking post-quantum cryptography to next generation systems.
At simultaneous press conferences around the world, including at a National Science Foundation-sponsored press conference at the US National Press Club in Washington, D.C., astronomers have unveiled the first image of the supermassive black hole at the center of our own Milky Way galaxy. This result provides overwhelming evidence that the object is indeed a black hole and yields valuable clues about the workings of such giants, which are thought to reside at the center of most galaxies. The image was produced by a global research team called the Event Horizon Telescope (EHT) Collaboration, using observations from a worldwide network of radio telescopes.
The National Science Foundation (NSF) has awarded Cornell College W.H. Norton Professor of Geology Rhawn Denniston a $199,785 grant to study the use of stalagmites as records of prehistoric fire activity in the Australian tropics.
Irvine, Calif., May 2, 2022 — The National Science Foundation has awarded a Rapid Response Research grant of nearly $175,000 to University of California, Irvine researchers seeking to gauge the effect that the reporting of Russia’s invasion of Ukraine in traditional and social media outlets has on the mental health of U.S. citizens.
Se creía que las galaxias post brotes de formación estelar agotan a gran velocidad y en violentas erupciones de energía todo el polvo y gas necesario para fabricar estrellas. Los nuevos datos obtenidos por el Atacama Large Millimeter/submillimeter Array (ALMA) revelaron que, en realidad, estas galaxias no se despojan de todo su combustible, sino que entran en un letargo en el que conservan y comprimen grandes cantidades de gas ultraconcentrado y turbulento. No obstante, al contrario de lo que se esperaría, tampoco lo usan para dar nacimiento a nuevas estrellas.
Post-starburst galaxies were previously thought to scatter all of their gas and dust—the fuel required for creating new stars—in violent bursts of energy, and with extraordinary speed. Now, new data from the Atacama Large Millimeter/submillimeter Array (ALMA) reveals that these galaxies don’t scatter all of their star-forming fuel after all. Instead, after their supposed end, these dormant galaxies hold onto and compress large amounts of highly-concentrated, turbulent gas. But contrary to expectation, they’re not using it to form stars.
The University at Buffalo will lead a $10 million project to develop software that academia, industry and government agencies use to manage high-performance computing infrastructure, the U.S. National Science Foundation (NSF) announced on Friday.
The NSF has awarded $7.5 million over five years to the RAMPS project, a next-generation system for awarding computing time in the NSF’s network of supercomputers. RAMPS is led by the Pittsburgh Supercomputing Center and involves partner institutions in Colorado and Illinois.
Matt Ajemian, Ph.D., has received a $1,103,081 NSF CAREER grant for a project that will build fundamental knowledge on where and when large shell-crushing predators feed in order to ensure a sustainable future for shellfish species. Further, the work can provide guidance to shellfish restoration programs that are currently “flying blind” with respect to predation risk.
Thanks to a $14 million infrastructure grant from the National Science Foundation, the University of Kentucky is poised to tell multiple heritage science stories in new, groundbreaking ways.
Just like humans, autonomous robots need to communicate with one another to learn together and to accomplish a team mission such as search and rescue. Researchers are developing the nation’s first-of-its-kind testbed platform that connects robots using high-frequency radio waves (30 to 300 gigahertz). The robots will be able communicate at ultra-high speeds of gigabits per second by forming and directing ‘beams’ toward each other that also will enable them to see through objects as needed. They will see what the other robots are sensing in real-time, resulting in five times the eyes thanks to the nearly instantaneous exchange of high volumes of data.
The National Science Foundation has awarded almost $3 million over a five-year period to The Institute for Meaningful Engagement at the University of California, Irvine. This new education project will explore the environmental factors prompting underrepresented students to leave science, technology, engineering and math programs and investigate how faculty can foster better classroom cultures to retain them. A multidisciplinary leadership team will partner with the deans of UCI’s six STEM schools to accomplish this.
Michael Méndez of the University of California, Irvine has received a two-year, $400,000 grant from the National Center for Atmospheric Research’s Early Career Faculty Innovator Program. It will fund a joint project with researchers at NCAR – which is sponsored by the National Science Foundation – exploring the disparate treatment of undocumented Latino/Latina and Indigenous migrant farmworkers during extreme wildfire events in Sonoma County.
The University of Notre Dame-led SpectrumX project is bringing together experts from 29 organizations to transform the landscape of spectrum research, education, collaboration and management.
Advancing its mission and leadership role to improve climate risk management critical to societal well-being, Rutgers, The State University of New Jersey will lead a multi-university Megalopolitan Coastal Transformation Hub (MACH) made possible by a grant through the National Science Foundation’s Coastlines and People (CoPe) Program with expected total funding of $19.9+ million over the next five years.
Notre Dame researchers have developed a prototype of an electronic nose, using nanoengineered materials to tune the sensitivity and selectivity to mimic the performance and capabilities of a human nose.
As a key player in developing and transforming innovators into entrepreneurs that improve people’s lives, Rutgers, The State University of New Jersey will expand its entrepreneurship training programming and further equip faculty and student researchers with the skills and strategy needed to transition their discoveries into technologies and products, as a partner in the newly created NSF I-Corps™ Hub: Northeast Region.
Binghamton University faculty will lead a $587,853 National Science Foundation project examining how brain folds form.
Case Western Reserve University and the University of Pittsburgh will launch a joint center this fall that uses cutting edge data-science and materials research to help companies make more reliable and durable products.
The Center for Materials Data Science for Reliability and Degradation (MDS-Rely) is a $3 million center supported by a $1.5 million grant from the National Science Foundation (NSF) .
Irvine, Calif., Aug. 2, 2021 — From cutting-edge research for advancing precision medicine to an innovative new effort for improving public water infrastructure to increase conservation, University of California, Irvine scholars, scientists and physicians are blazing new paths to help change the world. And their impact keeps growing.
An expert in applying artificial intelligence (AI) to problems in animal ecology at Rensselaer Polytechnic Institute will join a team of researchers in a new $20 million National Science Foundation (NSF) Artificial Intelligence Research Institute announced on Thursday.
Join NRAO to learn why scientists are so interested in hydrogen in the galaxy and beyond.
AUI and NRAO have established the National Astronomy Consortium (NAC) Bridge Scholarship Award program to assist and recognize NAC alums on their achievements as they enter graduate school.
A team of astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) has completed the first census of molecular clouds in the nearby Universe. The study produced the first images of nearby galaxies with the same sharpness and quality as optical imaging and revealed that stellar nurseries do not all look and act the same. In fact, they’re as diverse as the people, homes, neighborhoods, and regions that make up our own world.
NRAO, Green Bank Telescope, and Raytheon Intelligence & Space (RI&S) are working in collaboration to improve planetary radar capabilities. With the addition of Qorvo’s Spatium power amplifier technology, the project now has the power to identify and characterize even small NEOs earlier with more precision.
Recently, NSF’s NSO successfully transitioned the processing of these important observations of the Sun’s magnetic field and lower atmosphere to the operational control of NOAA’s Space Weather Prediction Center (SWPC), a move that will ensure reliable delivery of the data to the NOAA’s space weather forecasters who are the nation’s official civilian source for space weather watches, warnings, alerts, and forecasts.
New research is transforming understanding of the Mountain State’s famous landscape – and identifying ways to preserve it.
A new online mathematics tutoring program at West Virginia University is helping students navigate virtual learning.