جستجوی استاد راهنمای دانشگاهی

• Astronomy
• Data Intensive Computing
• Radio Astronomy
• +۳ مورد دیگر

Andreas Wicenec is a Professor and Senior Principal Research Fellow at the University of Western Australia (UWA), leading the Data Intensive Astronomy Program (DIA) at the International Centre for Radio Astronomy Research (ICRAR). He specializes in data-intensive astronomy, high-performance computing, and large-scale data management systems. His work supports the Square Kilometre Array (SKA) and other major observatories. Education: PhD in Astronomy from the University of Tübingen (1994), Physics Diploma (1989). Professional roles include Archive Scientist at the European Southern Observatory (ESO) and leadership in the International Virtual Observatory Alliance (IVOA). Research focuses on petascale data flows, reproducible science workflows, and next-generation archive systems like NGAS. Current projects include the DALiuGE engine, SKA data handling, and gravitational wave detection pipelines using deep learning. Key Projects: SKA Science Data Processing (7M AUD contract), Data Activated Flow Graph Engine (DALiuGE), and NGAS archive system Awards: ACM Gordon Bell Prize 2020 finalist Grants: Includes SKA Bridging Design (2019–2021), ICRAR IV (2025–2030) Labs/Teams: Active in ICRAR's Data Intensive Astronomy group, collaborating internationally on large-scale astronomy initiatives.

Kevin Vinsenمشاهده پروفایل

پژوهشگر ارشد

• Machine Learning
• High-performance Computing
• Peta-scale systems
• +۷ مورد دیگر

Kevin Vinsen is a Senior Research Fellow at the University of Western Australia, working in the Data Intensive Astronomy (DIA) Program of the International Centre for Radio Astronomy Research (ICRAR) since 2009. He is also affiliated with the UWA Defence and Security Institute and holds an ORCID ID of 0000-0001-5332-3784. His work focuses on translating ICRAR software capabilities into practical industry applications across diverse domains. His research interests include: Peta-scale systems High-performance Computing Machine Learning applications in multiple fields Wave and weather forecasting Digital Assistive Technologies Agricultural applications of ML Large language models Vinsen heads the Translation and Impact work of the DIA team and leads the development of Machine Learning systems. His current projects include ML for wave forecasting on the NW shelf, wind and temperature forecasting, honey traceability and provenance, and digital assistive technology for people with disabilities. His work contributes to UN Sustainable Development Goals related to industry, oceans, agriculture, food, disability, and defense. His research output demonstrates a strong trend toward applying machine learning techniques to solve real-world problems across astronomy, environmental science, agriculture, and disability support. This interdisciplinary approach showcases the versatility of his computational expertise across scientific and social domains. Vinsen has an h-index of 11 with 621 citations across 33 research outputs. As the ICRAR/UWA Summer Studentship Co-ordinator, he mentors emerging researchers and contributes to building research capacity. His collaborative network spans multiple institutions and research areas, reflecting his ability to bridge academic research with practical applications.

• Scientific Computing
• GPU Computing
• Signal Processing
• +۵ مورد دیگر

Professor Wes Armour is a Professor of Scientific Computing at the University of Oxford and serves as the Associate Head of Department for Research in the Department of Engineering Science. He previously directed the Oxford e-Research Centre, an interdisciplinary research center within the Engineering Science Department. With over £31 million secured as PI or Co-I, his work spans supercomputing, signal processing, machine learning, computational fluid dynamics, and protein crystallography. Professor Armour's research focuses on extracting science from data through fundamental challenges in modeling, simulation, and data processing. His work draws from numerical analysis, signal processing, and machine learning to develop technologies enabling future scientific discoveries, particularly for the Square Kilometre Array (SKA) telescope. Key interests include GPU computing, high performance computing, and machine learning applications across diverse domains from radio astronomy to finance. As Director and Principal Investigator of JADE and JADE2, a 700-GPU machine, he established the UK's first national High Performance Computer facility dedicated to advancing Artificial Intelligence and Machine Learning. His research group has pioneered GPU applications across multiple fields, including Square Kilometre Array data processing, protein crystallography, and graphene simulations. Current projects span energy-efficient machine learning, stock price prediction in finance, prime number prediction in cryptography, and multi-modal CCTV data analysis. Professor Armour has been instrumental in developing real-time signal processing techniques for astronomical observations, including the ARTEMIS system for millisecond radio transient detection. His publications demonstrate consistent innovation in GPU-accelerated computing dating back to early work in 2008 on accelerating conjugate gradient routines for electron transport in graphene.

• Astrophysics
• Radio Pulsars
• Neutron Stars
• +۴ مورد دیگر

Benjamin Stappers is a Professor of Astrophysics at the University of Manchester's Jodrell Bank Centre for Astrophysics within the School of Physics and Astronomy. His research focuses on radio pulsars, neutron stars, and rapid radio transients. He is part of the European Pulsar Timing Array (EPTA) and International Pulsar Timing Array (IPTA), which aim to detect nanohertz gravitational waves from early universe processes. He co-leads the transients project for LOFAR and heads the pulsar science group for the Square Kilometre Array (SKA). Research interests include using pulsars as probes of gravity and the interstellar medium, and expanding pulsar population studies via LOFAR surveys. His work involves hardware/software development for radio astronomy data analysis. Publications focus on pulsar timing, transients, and gravitational wave detection, with recent work exploring millisecond pulsars and radio transients. Awards include contributions to the Square Kilometre Array's development.

• Artificial Intelligence
• Machine Learning
• Deep Learning
• +۴ مورد دیگر

Prof. Frank-Peter Schilling is a Senior Lecturer at Zurich University of Applied Sciences (ZHAW) School of Engineering and Deputy Director of the Centre for Artificial Intelligence (CAI). He leads the Intelligent Vision Systems group and coordinates the PhD Programme in Data Science with the University of Zurich. As an Adjunct Professor at Victoria University of Wellington, he specializes in AI, Machine Learning, and applications in healthcare and physical sciences. His research focuses on deep learning-based computer vision, MLOps, and trustworthy AI certification frameworks. Education: PhD in Physics (University of Heidelberg, 2001) Dipl.-Phys. (MSc equivalent in Physics, University of Heidelberg, 1998) CAS University Didactics (PH Zurich, 2024) Research Interests: Developing AI systems for medical imaging (e.g., CBCT artifact reduction) Certification schemes for AI trustworthiness (e.g., certAInty project) Applications of deep learning in particle physics and industrial vision Achievements: Recipient of the EPS HEP Prize (2013) for contributions to the Higgs boson discovery at CERN Lead author of over 20 peer-reviewed articles on AI, MLOps, and medical imaging Principal investigator for projects like AI-BRIDGE (responsible AI development) and GenAI4SKA (Square Kilometre Array simulations) Teaching: Courses in MLOps, Machine Learning Operations, and Computer Vision at BSc and MSc levels. Developed the CAS Advanced Machine Learning program. Labs & Networks: Active in ELLIS (European Lab for Learning and Intelligent Systems), CLAIRE (AI research), and ZHAW’s Digital Health/Datalab initiatives.

• Astrophysics
• Radio Astronomy
• Pulsar Studies
• +۳ مورد دیگر

Dr. Ramesh Bhat is a Senior Research Fellow at Curtin University's School of Electrical Engineering, Computing and Mathematical Sciences (EECMS), affiliated with the Curtin Research Institute and Curtin Institute of Radio Astronomy (CIRA). His primary affiliation is with the Faculty of Science and Engineering. He is based at Curtin Perth Campus in Brodie Hall, Room 161. His research focuses on astrophysics and radio astronomy, particularly pulsar timing, gravitational wave detection using pulsar timing arrays, and the study of transient phenomena such as fast radio bursts (FRBs). He contributes to major projects like the High Time Resolution Universe (HTRU) survey, MeerTime, and the Murchison Widefield Array (MWA). Key research interests include pulsar population studies, interstellar medium interactions, signal processing for radio astronomy, and instrumentation development for next-generation telescopes like the Square Kilometre Array (SKA). His work spans theoretical models of pulsar emission mechanisms to observational studies of pulsar nulling, subpulse drifting, and gravitational wave backgrounds. Recent publications highlight advancements in pulsar survey techniques (e.g., GPU-accelerated analysis), discovery of new pulsars and FRBs, and constraints on cosmological models via pulsar timing arrays. His research often involves international collaborations, leveraging facilities like the Parkes radio telescope and the MWA. He actively contributes to radio interferometry, transient detection algorithms, and pulsar timing array data analysis. His work bridges observational astronomy with computational methods, aiming to advance understanding of compact objects and gravitational physics.

Mohammed Nabil EL KORSOمشاهده پروفایل

استاد

• Statistical Signal Processing
• Machine Learning
• Detection and Estimation Theory
• +۵ مورد دیگر

Mohammed Nabil EL KORSO is a Professor at CentraleSupélec, part of the University of Paris-Saclay. He is affiliated with the Laboratoire des Signaux et Systèmes (L2S). His research focuses on statistical signal processing, machine learning, detection/estimation theory, and robust signal processing, with applications in radioastronomy, radar systems, and source localization. He has contributed extensively to methodologies like Kalman filtering, covariance estimation, and array processing. His work emphasizes robust techniques for handling non-Gaussian noise and interference, particularly in radio interferometry and SAR imaging. Key contributions include algorithms for array calibration, RFI mitigation, and subspace estimation. His research also addresses challenges in distributed and adaptive signal processing, with applications to vital signs monitoring and robotic systems. He has published over 50 journal articles and conference papers, focusing on performance bounds (Cramér-Rao, Weiss-Weinstein), Bayesian methods, and practical implementations for large-scale systems. His recent work includes advancements in low-cost interferometric imaging and phase estimation for SAR time series. EL KORSO collaborates with international projects like the Square Kilometre Array (SKA), contributing to technological developments in radio astronomy. He supervises research in signal processing labs and actively participates in academic conferences such as EUSIPCO and ICASSP.

Peter Quinnمشاهده پروفایل

استاد

• Dark Matter
• Galaxy Formation and Evolution
• Computational Astrophysics
• +۳ مورد دیگر

Professor Peter Quinn is a distinguished astrophysicist at the University of Western Australia , serving as Chairman of the Board at the International Space Centre and affiliated with the International Centre for Radio Astronomy Research (ICRAR) and the Office of DVC Research . He received his BSc(Hons) in Mathematics and Physics from the University of Wollongong in 1978 with the University Medal in Physics, and his PhD in astronomy and astrophysics from the Australian National University (ANU) in 1982. His research centers on galaxy formation and evolution , dark matter dynamics , and the Epoch of Reionization . He has pioneered computational astrophysics, particularly through the discovery of the Quinn-Goodman effect and contributions to the MACHO Dark Matter Search Project . He has led major initiatives in the European Southern Observatory (ESO) , including the Very Large Telescope (VLT) data flow system and the Astrophysical Virtual Observatory (AVO) project. His scholarly work spans radio astronomy , supercomputer simulations , and data-intensive science , with a strong focus on the Square Kilometre Array (SKA) and gravitational wave detection . His work has earned him several prestigious accolades including a NASA High Performance Computing Award and a Computerworld 21st Century Achievement Award . He is a Fellow of the Australian Academy of Science (FASA) and a Fellow of the Australian Institute of Physics (FTSE) . His research also extends to large-scale international infrastructure projects and planning for the Square Kilometre Array and gravitational wave observations . He has served as Division Head at ESO and as a Chief Investigator for numerous grants, including the Australian SKA Regional Centre and ICRAR core funding .

Cathryn Trottمشاهده پروفایل

استاد

• Radio Astronomy
• Signal Processing
• Interferometry
• +۳ مورد دیگر

Professor Cathryn Trott is a leading academic in radio astronomy at Curtin University, holding roles in the Curtin Research Institute and Curtin Institute of Radio Astronomy (CIRA). She serves as the Deputy Director and Chief Investigator (Curtin Node Leader) for ARC CoE All-Sky Astrophysics in 3D (ASTRO 3D), and has a part-time secondment as ATNF Chief Scientist at CSIRO. Her education includes a PhD from the University of Melbourne (2005) and a BSc (Honours H1) from the same university (2001). Professor Trott has held significant leadership roles, including President of the Astronomical Society of Australia (2019–2021) and Board Member of the Murchison Widefield Array (MWA). She is actively involved in the design and data analysis of the Square Kilometre Array (SKA) and its precursors, focusing on Epoch of Reionization (EoR) and Cosmic Dawn experiments. Her research emphasizes signal processing, calibration of radio interferometers, and mitigating systematics in cosmological observations. She has secured substantial grants, including ARC DECRA ($325k) and ARC Future Fellowships ($855k). Professor Trott collaborates globally, contributing to the SKA EoR/CD Science Working Group and IEEE. She also teaches advanced astronomy modules and has affiliations across Curtin University's global campuses. Research interests include signal estimation, radio source modeling, and interferometry. Key projects involve leading the ICRAR EoR initiative, optimizing the MWA, and preparing for the SKA. She has pioneered calibration methods and foreground subtraction techniques critical for EoR studies. Awards include Fellowships from the Australian Institute of Physics (FAIP) and Astronomical Society of Australia (FASA), along with executive training from the Australian Institute of Company Directors (GAICD).

David Gozzardمشاهده پروفایل

پژوهشگر ارشد

• Quantum Metrology
• Laser Communication Systems
• Precision Measurements
• +۴ مورد دیگر

Dr David Gozzard is a Senior Research Fellow at the University of Western Australia (UWA) and the International Centre for Radio Astronomy Research (ICRAR). His research focuses on quantum imaging, high-precision measurement systems, and satellite laser communications. He holds a Forrest Fellowship, recognizing his contributions to advancing Australia’s space technology capabilities. Dr Gozzard earned his PhD in Physics from UWA in 2018, specializing in stabilized reference frequency transfer systems for the Square Kilometre Array telescope. His postdoctoral work at the Australian National University further developed optical phased arrays and laser systems for metrology and communication. Research Interests Quantum metrology and optical frequency stabilization High-bandwidth satellite laser communication systems Free-space optical links and atmospheric turbulence mitigation Optical ground station networks and tactical deployment His recent work demonstrates advancements in optical communication systems, including record-breaking 100 Gbps free-space links and drone-based geopotential measurements. He leads projects funded by the Australian Research Council (DECRA), the Department of Defence, and international partnerships. Awards Forrest Fellowship (2019) Advising & Grants Supervises Higher Degree by Research students in optical communication and quantum systems. Active in securing grants such as the $14M Quantum Australia initiative and the Australian Space Agency’s optical communications projects. Labs & Teams A core member of the Western Australian Optical Ground Station (WAOGS) team, developing next-generation laser communication infrastructure for space missions and Earth observation.

Caroline Fosterمشاهده پروفایل

مدرس ارشد

• Astrophysics
• Observational Astronomy
• Radio Astronomy
• +۳ مورد دیگر

Dr Caroline Foster is a Senior Lecturer at the School of Physics, UNSW Sydney, with a focus on mitigating satellite constellation impacts on Australian astronomy. Her research bridges astrophysics, radio/optical data analysis, and stakeholder advocacy. She supervises students in interdisciplinary projects, emphasizing independent learning and collaboration with institutions like the Square Kilometre Array (SKA) and the International Astronomical Union's Centre for the Protection of the Dark and Quiet Sky (CPS). Affiliation: UNSW Sydney (Senior Lecturer) Key collaborations: Square Kilometre Array (SKA), International Astronomical Union (IAU) Her research projects aim to quantify satellite interference in Australian astronomy, focusing on data loss mitigation and policy recommendations. She encourages student-led inquiry, fostering skills in programming, image analysis, and cross-sector communication.

Jonghwan Rheeمشاهده پروفایل

پژوهشگر ارشد

• Astrophysics
• Radio Astronomy
• Extragalactic Astronomy
• +۵ مورد دیگر

Jonghwan Rhee is an Adjunct Research Fellow at the International Centre for Radio Astronomy Research (ICRAR) within The University of Western Australia. He earned his PhD from the Australian National University in 2015 and has since focused on neutral hydrogen gas surveys using the Australian Square Kilometre Array Pathfinder (ASKAP), particularly the WALLABY and DINGO projects. Role : Adjunct Research Fellow, ICRAR (UWA) Education : PhD (2015) from Australian National University Expertise : Radio astronomy, extragalactic studies, HI gas surveys, and machine learning for galaxy classification His research examines galaxy evolution through neutral hydrogen gas distributions, tidal interactions, and star formation processes in low surface brightness galaxies. Recent work includes developing machine learning frameworks for source-finding in radio data and analyzing perturbed galaxies via H i morphometrics. Key collaborations include contributions to the WALLABY pilot survey datasets, with focus areas in stellar mass dynamics, galaxy clusters, and gas scaling relations. His outputs have been referenced in news outlets, academic networks, and software repositories.

David Kaplanمشاهده پروفایل

دانشیار

• Astrophysics
• Neutron Stars
• Radio Astronomy
• +۴ مورد دیگر

David Kaplan is an Associate Professor of Physics at the University of Wisconsin-Milwaukee (UWM) and holds a Visiting Professor position at the University of Wisconsin-Madison. His primary research focuses on multi-wavelength observations of neutron stars, including isolated thermally emitting neutron stars and magnetars, as well as radio transient detection using facilities like the Murchison Widefield Array (MWA) and the Australia Square Kilometre Array Pathfinder (ASKAP). He currently chairs the MWA Transient Science Team and serves as a peer reviewer for journals such as the Astrophysical Journal and Astronomy & Astrophysics . Education: PhD in Astrophysics from California Institute of Technology (2004) Pappalardo Fellow at MIT Kavli Institute (2004-2007) Hubble Postdoctoral Fellow at MIT Kavli Institute and KITP (2007-2010) His research interests span astrophysical transients, pulsar astronomy, and the development of radio instrumentation. He is particularly known for studies of neutron star systems and the application of widefield radio surveys to discover new astrophysical phenomena. His work with the MWA has expanded our understanding of low-frequency radio sources, including contributions to space debris detection and polarization surveys. Kaplan’s research bridges observational astronomy with theoretical astrophysics, leveraging large-scale observational facilities to explore extreme astrophysical environments. While no formal student advisement is listed, his involvement in major observational projects suggests an active role in training graduate students and postdocs through collaborative research teams. His grants and funding are tied to his roles in leading large-scale telescope initiatives like the MWA. Kaplan leads the Murchison Widefield Array Transient Science Team, fostering interdisciplinary collaboration in radio astronomy. His website ( http://www.gravity.phys.uwm.edu/~kaplan/ ) provides further details on his research activities and publications.

• Neutron Star Phenomena
• Radio Pulsar Timing
• Gravitational Wave Astronomy
• +۴ مورد دیگر

Benjamin Shaw is a Research Associate in the Astronomy and Astrophysics Theory Group at the University of Manchester’s School of Physics and Astronomy. His primary research focuses on neutron star phenomena, particularly radio pulsar timing, pulsar variability, and real-time data processing pipelines. He contributes to the Jodrell Bank pulsar timing program and the Square Kilometre Array (SKA) pulsar search initiative. Shaw holds a PhD from the University of Manchester (2018) under supervisors Willem Stappers and Pieter Weltevrede, focusing on 'Timing and emission variability in radio pulsars.' His work spans gravitational wave detection using pulsar timing arrays, pulsar glitch dynamics, and magnetar evolution. He has collaborated internationally, including with LIGO-Virgo-KAGRA consortia and major radio observatories. Shaw actively participates in academic activities, organizing conferences like 'Science Possibilities Investigating Neutron Stars in the UK' (2022) and delivering invited talks on pulsar astrophysics. His research has been featured in outlets like the Astrophysical Journal and Monthly Notices of the Royal Astronomical Society. Key areas of contribution include Bayesian modeling of pulsar spin behavior, radio/X-ray correlations in magnetars, and developing software for real-time pulsar data analysis. He has no listed awards but maintains an active media presence through BBC Radio 5 LIVE segments discussing astrophysical topics.

• Cosmic Ray Physics
• Neutrino Astronomy
• Astroparticle Physics
• +۳ مورد دیگر

Associate Professor Clancy James is a researcher at Curtin University, affiliated with the Curtin Research Institute and Curtin Institute of Radio Astronomy (CIRA) within the School of Electrical Engineering, Computer and Mathematical Sciences. His research focuses on astroparticle physics, cosmic rays, and neutrino astronomy, leveraging radio telescopes like the Murchison Widefield Array and the Square Kilometre Array. He collaborates with international projects such as CRAFT, KM3NeT, and ANTARES to study fast radio bursts (FRBs), neutrino detection, and cosmic ray showers. Clancy James holds a PhD from the University of Adelaide (2009) and has held postdoctoral roles at the University of Erlangen-Nuremberg and Radboud University. He teaches courses in electromagnetism and particle physics. His work bridges radio astronomy with particle physics, aiming to uncover the origins of cosmic rays and neutrinos. He has contributed to over 100 publications, including studies on FRB populations, neutrino telescope analyses, and high-energy cosmic particle studies. Research interests include cosmic ray air showers, neutrino detection via the Mediterranean-based KM3NeT, and radio transient surveys with ASKAP. His expertise spans instrumentation development for radio telescopes and multi-messenger astrophysics. He leads efforts to correlate FRBs with gravitational wave events and cosmic neutrino signals.