جست‌وجوی استاد و پژوهشگر

• Elementary Particle Physics
• High-Energy Physics
• Astroparticle Physics
• +۷ مورد دیگر

Diego Cauz is a tenured researcher in the Department of Mathematics, Computer Science and Physics at the University of Udine, where he also serves in the Faculty of Engineering. He has been actively involved in teaching General Physics, particularly Physics 1 and 2, for various engineering degree programs since the 2006–2007 academic year. His institutional roles include organizing and managing physics teaching laboratories for engineering and science students. His research focuses on experimental high-energy and astroparticle physics, with extensive participation in major international collaborations. He has contributed to the CDF experiment at Fermilab, the ATLAS experiment at CERN, the Muon g-2 experiment at Fermilab, and the Cherenkov Telescope Array (CTA) project in La Palma, Spain. His technical expertise lies in detector instrumentation, particularly in the development of calibration systems using lasers and silicon photomultipliers (SiPMs), as well as in managing complex data acquisition and monitoring setups. The most recent publications reflect his work on precision calibration systems for the Muon g-2 and CTA experiments, emphasizing his role in ensuring detector stability and measurement accuracy. These works highlight trends in high-precision particle physics and next-generation gamma-ray observatories. He has no listed scientific awards in the provided materials. His advisory and grant-related activities are not explicitly detailed, though he has coordinated significant technical components of large collaborations and led local teams in multi-institutional projects. He has also contributed to educational initiatives, including the design of modern physics laboratories and teacher training programs. Diego Cauz leads research activities in the Sensor Development Laboratory at the University of Udine, where work is conducted for the Muon g-2, CTA, and HERMES/PRID SenSiA experiments. The lab supports the construction and testing of calibration hardware, sensor characterization, and development of electronic systems for particle and astroparticle detection.

• Experimental Particle Astrophysics
• Ultra-high Energy Cosmic Rays
• Gamma-ray Astronomy
• +۱۱ مورد دیگر

Corbin Covault is Professor and Chair of the Department of Physics at Case Western Reserve University (CWRU), within the College of Arts and Sciences. He is a leading researcher in experimental particle astrophysics, focusing on ultra-high energy cosmic rays, gamma-ray astronomy, and advanced instrumentation for astroparticle detection. B.A., Massachusetts Institute of Technology (1985) Ph.D., Harvard University (1991) His research interests span Experimental Particle Astrophysics , Ultra-high Energy Cosmic Rays , Gamma-ray Astronomy , Dark Matter Detection , and Exoplanet Imaging . He leads the CWRU group in the Pierre Auger Cosmic Ray Observatory and contributes to the Cherenkov Telescope Array (CTA) , with expertise in photodetection, GPS timing, and wireless data systems. Additional projects include Optical SETI (SOFOS), spectral CT imaging, and macro dark matter searches. The selected publications reflect a strong focus on cosmic ray anisotropy, mass composition, neutrino searches, and instrumentation. Key themes include multi-messenger astrophysics , air shower detection , and precision calibration of large-scale observatories. His work is deeply collaborative, often involving major international teams such as the Pierre Auger, IceCube, and TOTEM collaborations. Scientific awards are not listed in the provided text. Dr. Covault leads active research groups involved in major funded projects, including an MRI grant for CTA camera development. His leadership in large collaborations implies advising roles for graduate students and postdoctoral researchers. He is involved in developing next-generation detectors and instrumentation for cosmic ray and gamma-ray observatories. His research group at CWRU is engaged in multiple experimental efforts, including instrumentation development for Auger and CTA, data analysis, and prototype testing at facilities like Mt. Hopkins Observatory. The team collaborates widely across institutions and international consortia.

David Bergeمشاهده پروفایل

استاد

• Gamma-ray astronomy
• Multi-messenger astronomy
• Astroparticle physics
• +۲ مورد دیگر

David Berge is a Professor at Humboldt University of Berlin and Lead Scientist at Deutsches Elektronen-Synchrotron (DESY) in Zeuthen, where he heads the Gamma-Ray Astronomy group. He coordinates DESY's contributions to the Cherenkov Telescope Array Observatory (CTAO) and serves as Principal Investigator for the ULTRASAT camera project. Dr. Berge's research focuses on cosmic particle accelerators and multi-messenger astronomy, studying cosmic objects and events through photons, neutrinos, and gravitational waves. His work combines methodologies from both particle physics and astroparticle physics, reflecting his diverse career path that includes significant time at CERN working on the ATLAS detector. His team works with gamma-ray telescopes including HESS and the future CTAO, utilizes multi-wavelength data from other telescopes, and collaborates with DESY's IceCube Neutrino Group. They also observe regions of the sky where LIGO, VIRGO, and KAGRA have detected gravitational wave events. Berge is actively involved in major international collaborations including HESS, CTAO, and ULTRASAT, and serves as Chair of the CTAO Council's Administration and Finance Committee. He is also the Spokesperson for the Helmholtz-Weizmann Graduate School Multi-Messenger Astronomy. German Physical Society German Astronomical Society European Astronomical Society International Astronomical Union As a reviewer for various peer-reviewed journals and European research proposals, Berge contributes significantly to the scientific community. His group is currently building a 90-million-pixel CMOS sensor camera for the ULTRASAT satellite mission, which will measure UV light in collaboration with the Weizmann Institute and NASA.

• Astroparticle Physics
• Theoretical Physics
• Cosmic Ray Physics
• +۵ مورد دیگر

Martin Pohl is a Lead Scientist at DESY (Deutsches Elektronen-Synchrotron) and Professor of Theoretical Physics at the University of Potsdam. He works in the field of astroparticle physics, investigating energetic particles in the universe, their origin, interactions with their environment, and decay products. His research focuses on understanding how cosmic sources accelerate particles to very high energies, how jets and energetic particles form around supermassive black holes, and the nature of dark matter. The universe contains systems capable of accelerating particles to energies many orders of magnitude higher than human-built accelerators can achieve. Professor Pohl leads a research group in Theoretical Astroparticle Physics at both DESY in Zeuthen and the University of Potsdam. His group is involved in projects related to: TeV gamma-ray astronomy with VERITAS Science with the Cherenkov Telescope Array (CTA) Kinetic modeling of space plasma with energetic particles Development of publicly available data resources including gamma-ray production matrices and 3D models of galactic gas distribution He is also affiliated with the International Helmholtz-Weizmann Research School on Multimessenger Astronomy, providing international training in this emerging field. At the University of Potsdam, Professor Pohl teaches courses in Astroparticle Physics and supervises graduate research.

• Astroparticle Physics
• Cosmic Rays
• Gamma-Ray Astronomy
• +۳ مورد دیگر

Martin Karl Wilhelm Pohl is a Leading Scientist at DESY (Deutsches Elektronen-Synchrotron) and Full Professor of Theoretical Physics at the University of Potsdam since 2009. His work spans both institutions, with his primary research base at DESY Zeuthen and his academic appointment at the University of Potsdam's Institute of Physics and Astronomy. Professor Pohl's academic journey began with a PhD from the University of Bonn in 1991. He held research positions at prestigious institutions including the Max Planck Institute for Radio Astronomy, Max Planck Institute for Extraterrestrial Physics, and the Danish Space Research Institute. After completing his habilitation in Theoretical Physics at Ruhr University of Bochum in 2002, he served as Assistant and Associate Professor at Iowa State University before returning to Germany in 2009. His research focuses on astroparticle physics, particularly the study of energetic particles in the universe. Key scientific questions driving his work include: How do cosmic sources accelerate particles to very high energies? How do supermassive black holes form jets and energetic particles therein? What is the nature of dark matter in the universe? His group conducts kinetic modeling of space plasma with energetic particles and participates in major observational projects including VERITAS and the Cherenkov Telescope Array (CTA). Pohl's research encompasses several critical areas in modern astrophysics: Cosmic ray acceleration mechanisms at shock fronts of supernova remnants Propagation of high-energy particles through the Galaxy Anomalies in cosmic particle spectra that may indicate dark matter signatures Very-high-energy gamma ray astronomy As an educator, Professor Pohl teaches astroparticle physics courses at the University of Potsdam and maintains active research collaborations. His group provides valuable public resources including gamma-ray production matrices, lepton production matrices, and 3D models of the molecular-gas distribution in the Galaxy. He is also involved with the International Helmholtz-Weizmann Research School on Multimessenger Astronomy, which connects DESY with the University of Potsdam and other international partners to advance research in this emerging field.

Gilles MAURINمشاهده پروفایل

استاد

• Astroparticle Physics
• Gamma-ray Astronomy
• High-energy Astrophysics
• +۲ مورد دیگر

Gilles Maurin is a University Professor at the University of Savoie Mont Blanc and serves as Assistant Director of the Annecy Laboratory of Particle Physics (LAPP) in Annecy, France. LAPP operates as a joint research unit between IN2P3 (National Institute of Nuclear and Particle Physics) and the university, positioning Professor Maurin at the intersection of academic leadership and experimental particle physics research. His institutional affiliations span university teaching, laboratory administration, and national research coordination through IN2P3. Professor Maurin's research focuses on astroparticle physics and gamma-ray astronomy, with significant contributions to major international observatories. His expertise in HESS (High Energy Stereoscopic System) and CTA (Cherenkov Telescope Array) projects drives investigations into cosmic particle acceleration mechanisms and high-energy astrophysical phenomena. This work bridges theoretical astrophysics and advanced detector technology development, emphasizing data analysis from ground-based gamma-ray telescopes. As Assistant Director of LAPP, Professor Maurin oversees laboratory operations within the broader IN2P3 framework, which coordinates particle physics research across France. The laboratory maintains active participation in global collaborations requiring substantial grant funding, though specific projects aren't detailed in the source material. LAPP's infrastructure supports experimental work in particle detection and cosmic ray analysis, contributing to France's role in international astroparticle physics initiatives.

Nicholas Tothillمشاهده پروفایل

دانشیار

• Astrophysics
• Radio Astronomy
• Millimetre-wave Astronomy
• +۵ مورد دیگر

Associate Professor Nicholas Tothill is a Senior Lecturer and Director of WSU Penrith Observatory at Western Sydney University's School of Science. With extensive international experience including positions at Harvard-Smithsonian Center for Astrophysics and Max Planck Institute for Astronomy, he specializes in astrophysics, radio astronomy, and astronomical instrumentation. Education BA in Natural Sciences (Physics and Theoretical Physics), Cambridge University, UK MSc in Radioastronomy, University of Manchester, UK PhD in Astrophysics, University of London, UK Research Interests Nicholas Tothill's research focuses on astronomical and space science applications of event-based cameras, radio astronomy, millimetre-wave astronomy, optical spectroscopy, and cosmic-ray astronomy. His work spans the astrophysics of distant galaxies, star formation processes, and galactic cosmic rays. He has conducted research at the South Pole running radio telescopes and has extensive experience with various astronomical instrumentation and data analysis techniques. Publication Trends Tothill's recent publications (2019-2023) show strong focus on binary star systems, radio astronomy surveys of Magellanic Clouds, and development of astronomical instrumentation, particularly neuromorphic event-based cameras for space imaging. His work bridges observational astronomy with instrument development, contributing to major projects like the Cherenkov Telescope Array. Scientific Awards Antarctica Service Medal, US NSF Member, Astronomical Society of Australia Advising and Grants Professor Tothill supervises research students in computational astrophysics and has been involved in significant research projects including the European Commission-funded "Advancing European submillimetre/terahertz astronomy in Antarctica" (2006-2008). His work combines theoretical astrophysics with practical observational techniques across multiple wavelengths. Laboratories and Teams As Director of WSU Penrith Observatory, Tothill leads observational astronomy efforts at Western Sydney University. He is associated with the International Centre for Neuromorphic Systems and has collaborated extensively with international teams on projects including the JCMT Gould Belt Survey, ASKAP surveys, and Cherenkov Telescope Array development.