جستجوی استاد راهنمای دانشگاهی

Jay Strader is a Professor in the Department of Physics and Astronomy at Michigan State University, where he serves as Graduate Director for the astronomy PhD program and Associate Chair for astronomy. His research focuses on compact objects, particularly black holes and neutron stars in globular clusters, neutron star binaries in Fermi gamma-ray sources, and intermediate-mass black holes. He has received a Packard Fellowship for Science and Engineering and grants from NSF and NASA. His research group includes postdoc Ryan Urquhart, graduate students Thomas Do and Rebecca Kyer, and several undergraduates, with past students like Teresa Panurach (now director of NoVEL Consortium) and Samuel Swihart (NRC fellow at Naval Research Lab). Education: PhD in Astronomy, UC-Santa Cruz/Lick Observatory Awards: Packard Fellowship Collaborations: Member of Rubin Observatory's Stars, Milky Way, and Local Volume science collaboration since 2008 Previous Positions: Hubble Fellow and Menzel Fellow at Harvard-Smithsonian Center for Astrophysics (2007-2012) Program Initiatives: Co-founder of PAREDS program for early research opportunities at MSU His work has been supported by NSF and NASA grants, and he has contributed to studies on black holes in M22, hypervelocity globular clusters around M87, and transitional millisecond pulsars. His group collaborates with Laura Chomiuk and contributes to data catalogs like the M31 globular cluster velocity dispersion database.

• Compact Objects
• Black Holes
• Neutron Stars
• +۵ مورد دیگر

Matt Nowinski is a Collegiate Associate Professor in the Department of Mechanical Engineering at Virginia Tech's College of Engineering. His professional roles include advisory board memberships and leadership positions within the department. He holds multiple degrees including a Ph.D. in Mechanical Engineering from ETH Zurich (1999), an M.S. in Computer Science from Syracuse University (2022), and prior mechanical/aerospace engineering degrees from Virginia Tech. His research focuses on asteroid dynamics (particularly D-type and V-type asteroids), gas turbine engines, aeroelasticity, and education technology. Notable areas include lightcurve analysis, surface mineralogy modeling, and machine learning applications in astronomy. His work bridges aerospace engineering with astrophysics, leveraging both experimental and computational methods. Dr. Nowinski has over 24 years of industry experience as a Boeing subject matter expert in military communications systems, complemented by academic roles at George Mason University and University of Chicago. He is a recipient of the John Jones Faculty Fellowship and Society of Distinguished Alumni honor. His research contributions span asteroid characterization, turbine blade flutter mechanisms, and telescope instrumentation. Current work emphasizes observational astronomy through the Stone Edge Observatory and Slack-based collaborative platforms. He actively contributes to advancing STEM education through innovative curricula and research integration.

• Aerospace Engineering
• Asteroid Dynamics
• Machine Learning
• +۵ مورد دیگر

Manuel Linares Alegret is a Professor in the Department of Physics at the Norwegian University of Science and Technology (NTNU) in Trondheim, Norway, where he has been employed since September 2021. He also holds an Associate Professor position at the Polytechnic University of Catalonia (UPC) in Barcelona, Spain, since 2018. His research focuses on high-energy astrophysics with particular emphasis on neutron stars, black holes, white dwarfs, and compact objects in binary systems. Dr. Linares earned his Physics Degree from Universitat de Barcelona (1998-2004) followed by a PhD in Astronomy from Universiteit van Amsterdam (2004-2009). His subsequent career includes prestigious fellowships including Rubicon Fellow at MIT (2009-2012), IAC Fellow (2012-2017), and Marie Curie Fellow at UPC (2017-2018). His research interests primarily center on compact binary systems, particularly millisecond pulsars known as 'spiders' (including black widows and redbacks), neutron star physics, accretion flows, thermonuclear bursts, and the search for super-massive neutron stars. His work combines observational astronomy with theoretical modeling to understand extreme physics in these systems. He leads the LOVE-NEST project, which investigates compact binary millisecond pulsars to find the most massive neutron stars and understand the interaction between accretion flows, pulsar winds, and neutron star magnetospheres. An analysis of his recent publications reveals a strong focus on spider pulsar systems, with particular attention to mass measurements, orbital dynamics, irradiation effects, and the relationship between accretion and rotation-powered states. His work spans multiple observational wavelengths including optical, X-ray, and radio, often utilizing data from major telescopes and space observatories. ERC Consolidator Grant for LOVE-NEST project Marie Curie Fellow IAC Fellow Rubicon Fellow Dr. Linares has supervised numerous students at various levels, including PhD candidates, Master's students, and undergraduate research projects. He currently leads a substantial research team under the LOVE-NEST project, which has received 2M EUR in funding. His group includes multiple postdoctoral fellows and PhD candidates working on various aspects of compact object astrophysics. He teaches Observational Astrophysics (FY3215) at NTNU and has previously taught Quantum Physics and Physics I at UPC. He is the principal investigator of the LOVE-NEST (Looking for Super-Massive Neutron Stars) research group at NTNU, which focuses on compact binary millisecond pulsars. This team conducts research using multiple observational facilities worldwide and collaborates with international groups including those at the Instituto de Astrofísica de Canarias and the University of Manchester.

• High-energy astrophysics
• Compact objects in binary systems
• Neutron stars
• +۷ مورد دیگر

Jarle Brinchmann is an Associate Professor at Leiden University's Leiden Observatory, part of the Faculty of Science. He holds a PhD from the University of Cambridge and has held postdoctoral positions at Oxford University, the Max Planck Institute for Astrophysics, and the University of Porto. His research focuses on galaxy evolution, active galactic nuclei (AGN), and interstellar medium dynamics. Notable contributions include studies on gas outflows in galaxies and emission line diagnostics for AGN identification. Recent work includes analysis of Lyman-alpha emitters and binary star systems in globular clusters using the MUSE instrument. Education: BSc and MSc in Astronomy from the University of Oslo, PhD from the University of Cambridge (thesis: 'The physical evolution of galaxies'). Research emphasizes observational and theoretical astrophysics, with a focus on high-redshift galaxies, intergalactic medium interactions, and stellar populations. Collaborates widely on large-scale surveys and spectroscopic analyses.

• Galaxy Evolution
• Active Galactic Nuclei (AGN)
• Interstellar Medium (ISM)
• +۳ مورد دیگر

Prof. Dr. Michael Kramer is a Professor of Astrophysics at the University of Manchester and a Scientific Member (Managing Director) at the Max Planck Institute for Radio Astronomy. He leads the COMPACT Research Group and specializes in radio astronomical fundamental physics. University of Manchester: Professor for Astrophysics Max Planck Institute for Radio Astronomy: Managing Director, Radio Astronomical Fundamental Physics Research Interests: Dr. Kramer focuses on pulsars , neutron stars , and gravitational physics , using these as tools to test general relativity , detect gravitational waves , and study transients in the Milky Way. Recent Research Trends: His 15 most recent publications emphasize fast radio bursts (FRBs) , axion dark matter searches , black hole imaging , and pulsar timing arrays for gravitational wave detection. Studies include the M87 jet, Galactic Center magnetars, and MeerKAT telescope optimizations.

• Pulsars
• Neutron Stars
• Gravitational Physics
• +۶ 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.

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

Professor Christian Knigge serves as Professor of Astrophysics at the University of Southampton and is a core member of the Southampton Theory Astrophysics and Gravity (STAG) Research Centre within the Institute for Life Sciences. His research program investigates accretion phenomena across diverse cosmic scales, from stellar-mass compact objects to supermassive black holes. Knigge's primary research focuses on accretion phenomena and associated outflows, cataclysmic variables, close binaries, globular clusters, and active galactic nuclei. He examines the physical mechanisms driving accretion disk instabilities, outflow generation, and explosive events in binary systems, with particular emphasis on white dwarf and black hole accretors. His work integrates observational data with theoretical modeling to unravel the complex physics of these high-energy environments. Recent publications (2024-2025) reveal a strong emphasis on multi-wavelength observational campaigns, especially leveraging JWST capabilities, alongside theoretical code development. Key research threads include characterizing disk winds in active galactic nuclei, identifying quasi-periodic oscillations in white dwarf systems, classifying optical outbursts in cataclysmic variables, and developing computational tools like the SIROCCO radiative transfer code. These studies demonstrate his leadership in connecting observational signatures with fundamental accretion physics across different astrophysical regimes. Supervision: Currently guides six PhD students in Physics (Austen George William Wallis, Cordelia Brown, Brian Luff, Zackery Alexander Irving, Arianna Clarissa Albayati, Pornisara Nuchvanichakul) Grants: Leads STFC-funded projects including 'Line-Driven Disk Winds in Active Galactic Nuclei', 'C Knigge - Astrophysics at Southampton', and previously held a Leverhulme Trust Research Fellowship for 'The Universal Nature of Accreting Compact Objects' As an integral member of the STAG Research Centre, Knigge collaborates within a multidisciplinary team investigating gravity-dominated systems, contributing to Southampton's prominence in theoretical and observational astrophysics through both individual research initiatives and institutional consolidation grants.

• accretion phenomena
• associated outflows
• cataclysmic variables
• +۳ مورد دیگر

Martin Rey is a Lecturer in the Department of Physics at the University of Bath, specializing in theoretical astrophysics with a focus on galaxy formation and evolution. His research employs advanced computational methods to investigate fundamental questions about dark matter, star formation, and cosmic structure. His primary research interests include: Modeling the formation and co-evolution of stars, galaxies, and cosmic structures Using supercomputers for detailed fluid dynamics models of galaxies Investigating the nature of dark matter and its distribution Exploring the formation of the first stars and early universe processes Understanding how chemical elements permeate the Universe Dr. Rey's research portfolio reveals a strong concentration in Dark Matter Physics (100%), Dwarf Galaxy Physics (80%), Galactic Evolution Physics (74%), and Stellar Mass Physics (63%). His recent publications demonstrate expertise in radiation-hydrodynamics simulations, particularly through the EDGE project framework, which examines various aspects of dwarf galaxy physics and dark matter distribution. His notable scientific achievements include: Christopher Skinner Prize for outstanding PhD research (2020) Fellow of the Royal Astronomical Society (awarded December 7, 2024) Beecroft Fellowship (awarded September 1, 2021) Dr. Rey is actively engaged in research leadership as Co-Principal Investigator on the MEGATRON project (2023-2028) and Engineering Dwarf Galaxy project (2019-2027), and as Co-Investigator on the Vintergatan project (2020-2025). He serves as a peer reviewer for prestigious journals including Monthly Notices of the Royal Astronomical Society, Astronomy & Astrophysics, and The Open Journal of Astrophysics, and regularly presents at international conferences such as his Maynooth University seminar (November 2024) and First Galaxies conference (April 2025).

• Astrophysics
• Theoretical Astrophysics
• Galaxy Formation
• +۶ مورد دیگر

Dr. Rebecca Smith is a Senior Lecturer in Psychology at the School of Human Sciences, University of Greenwich. Her academic career spans over 15 years, with a focus on social psychology. She specializes in teaching and research related to ostracism, rape myth acceptance, and homeless stigmatization, while also contributing to gender equality studies. Her work bridges theoretical and applied research in human behavior. PhD (Psychology), University of Dundee MA (Psychology), University of Dundee Research Interests: Dr. Smith’s work explores the psychological impacts of social exclusion, the cultural and cognitive underpinnings of rape myth acceptance, and societal biases toward marginalized populations like the homeless. She integrates these themes with broader social psychology frameworks. Article Trends: Her recent publications span social psychology (e.g., ostracism, homeless stigma) and interdisciplinary topics like IVF outcomes, galaxy dynamics, and West Nile virus surveillance. This reflects a diverse collaboration network across medical, astrophysical, and public health domains. Advising: Dr. Smith supervises PhD and EdD students in social psychology and gender equality, fostering research in human behavior and societal structures. She previously served as Deputy Head of Department (2015-16) and TMC Link Tutor (2009-13).

• social psychology
• ostracism
• rape myth acceptance
• +۲ مورد دیگر

Kristen Dage is a Lecturer at Curtin Institute of Radio Astronomy (Curtin University) in Perth, Australia, specializing in multiwavelength astrophysics. She holds a PhD in Astrophysics from Michigan State University (2020) and previously held positions as a NASA Einstein Fellow at Wayne State University and Postdoctoral Fellow at McGill University. Her research investigates black holes and neutron stars within dense star clusters using radio to gamma-ray observations. Key interests include accretion physics, ultraluminous X-ray sources (ULXs), intermediate mass black holes, and gravitational wave progenitors. She co-chairs Rubin Observatory's Stars, Milky Way and Local Volume Collaboration and leads its Star Clusters Science Working Group. Awards & Grants: NASA Einstein Fellowship (2023) Legacy Survey of Space and Time Discovery Alliance grant (2023) Karl G. Jansky Very Large Array research time (2022) NICER Cycle 3 grant (2021) She founded the Dead Stars Society initiative, providing astrophysics research opportunities for undergraduates from under-resourced institutions, supported by LSST Discovery Alliance and Michigan Space Grant Consortium.

• Astrophysics
• Black Holes
• Neutron Stars
• +۷ مورد دیگر

David J. Helfand is a Professor in the Department of Astronomy at Columbia University, serving as Chair (1992–present) and Co-Director of the Columbia Astrophysics Laboratory (1994–present). He has held visiting roles at Cambridge University and the Danish Space Research Institute. His research focuses on radio surveys (e.g., FIRST and MAGPIS), neutron stars, supernova remnants, and the cosmic X-ray background. He has pioneered large-scale radio surveys to study galactic and extragalactic structures, weak gravitational lensing, and high-redshift quasars. Helfand holds a Ph.D. in Astronomy from the University of Massachusetts (1977) and an A.B. in Physics from Amherst College (1973). He co-founded Quest University Canada in 2005 and became its President in 2008. Education: Ph.D. Astronomy, University of Massachusetts, 1977 M.S. Physics, University of Massachusetts, 1977 A.B. Physics (Independent Scholar), Amherst College, 1973 Research Interests: Helfand's work emphasizes radio surveys like FIRST (mapping 9200 square degrees of the sky) and MAGPIS (Galactic Plane imaging). He studies neutron stars' evolution, supernova remnants (e.g., Vela and 3C58), and contributions of starburst galaxies/AGN to the cosmic X-ray background. He employs Chandra/XMM-Newton observations to probe obscured quasars and high-redshift clusters. Grants & Collaborations: Leadership roles include founding Quest University Canada and directing Columbia's astronomy department. His surveys have identified thousands of radio sources, enabled optical identifications, and explored cosmological structures via radio source correlations and lensing. Labs/Teams: Helfand collaborates with the Columbia Astrophysics Laboratory and international teams using facilities like the VLA, Chandra, and XMM-Newton. Projects include the MSX mid-IR survey and searches for obscured quasars and gravitational lenses.

• Astrophysics
• Radio Astronomy
• X-ray Astronomy
• +۵ مورد دیگر

Sotiria Fotopoulou is a Lecturer in the School of Physics at the University of Bristol. Her research focuses on astrophysics, particularly in active galactic nuclei (AGN), quasars, galaxy clusters, and cosmic web structure. She contributes to the Euclid mission's scientific objectives through studies of photometric redshifts, galaxy evolution, and environmental effects. Current Project: Principal Investigator for 'Co-evolution or co-existence? Growth of supermassive black holes in next generation surveys' (2023-2024) Research Themes: Quasar census, slitless infrared spectroscopy for high-redshift objects, cosmic web reconstruction, intracluster light analysis, and gravitational lensing detection. Her work integrates Euclid data with machine learning techniques for galaxy morphology and photometric studies. Award: Recipient of Undergraduate Bursary Grant (2020)

• Astrophysics
• Active Galactic Nuclei
• Galaxy Clusters
• +۴ مورد دیگر

Kerstin Bunte is a Professor of Machine Learning for interdisciplinary data analysis at the University of Groningen, affiliated with the Faculty of Science and Engineering and the Bernoulli Institute's Intelligent Systems Group. She holds an Honorary Fellowship at the University of Birmingham and leads the Intelligent Systems Group. Her research focuses on interpretable machine learning, interdisciplinary applications (e.g., astrophysics and biomedical data), and visualization techniques. Research Interests: - Machine Learning - Artificial Intelligence - Explainable AI (XAI) - Interpretable Models - Dimensionality Reduction - Data Visualization - Astrophysical Data Analysis - Medical Imaging Awards & Grants: - DSSC XS funding (2023) - NWO VIDI grant (2020) - Rosalind Franklin Fellowship (2016–present) Advising & Students: Supervised PhD students include Elisa Oostwal, Janis Norden, Matteo Marcantoni, and Petra Awad. Research spans topics like tumor segmentation in medical imaging, astrophysical structure detection, and autonomous navigation systems. Labs & Collaborations: Leads the Intelligent Systems Group, collaborating with institutions like the University of Birmingham and the University of Warwick. Work involves interdisciplinary projects combining machine learning with astronomy, biomedical sciences, and robotics.

• Machine Learning
• Artificial Intelligence
• XAI (Explainable Artificial Intelligence)
• +۷ مورد دیگر

Professor Duncan Forbes is an astronomer at Swinburne University of Technology's Centre for Astrophysics and Supercomputing, affiliated with the School of Science, Computing and Emerging Technologies. His research focuses on galaxy formation, dark matter distribution, and globular cluster systems. He has held roles such as Deputy Director of his Centre (2005–2008) and ARC DORA Fellow (2013–2015). His work includes studies using the Faulkes Telescope and collaborations on international projects like the LEWIS survey. Research interests span ultra-diffuse galaxies, dark matter-free dwarf galaxies, and the interplay between galaxy morphology and environmental effects. Recent grants include investigations into dark galaxies (ARC 2025–2027), AI-driven galaxy physics (ARC 2020–2024), and all-sky astrophysics in 3D (ARC Centre of Excellence). He has received the VC's Research Excellence Award (2004) and supervised 23 PhD/Master's projects on topics like UDG origins and stellar kinematics. Current research emphasizes combining observational data from instruments like MUSE with supercomputer simulations to model galaxy evolution.

• Galaxy Formation
• Dark Matter Studies
• Globular Cluster Systems
• +۳ مورد دیگر

Dan Wik is an Associate Professor in the Department of Physics & Astronomy at the University of Utah . His research focuses on observational X-ray astronomy, particularly galaxy clusters, inverse Compton scattering, X-ray binaries, and the X-ray background. He has extensive experience in data calibration, analysis tool development, and mission collaborations such as NuSTAR, Chandra, and XRISM. Wik holds a PhD in Astronomy from the University of Virginia (2010) and a BS in Astrophysics from Ohio University . His research interests span galaxy cluster mergers, nonthermal emission processes, high-energy astrophysics, and cross-calibration studies between X-ray observatories. Recent articles highlight his work on NuSTAR observations of galaxy clusters, X-ray binary populations in M31 and M33, inverse Compton emission constraints, and stray light background analysis techniques. His studies often integrate multiwavelength data and address cosmological implications of X-ray observations. Wik has received multiple grants from NASA for projects like Time Domain X-ray Studies of AGN and Hard Bandpass Extension of XRISM Cluster Observations . He supervises undergraduate and graduate researchers and teaches courses from general education to advanced graduate levels, including Foundations of Astronomy and High Energy Astrophysics .

• X-ray astronomy
• Galaxy clusters
• Inverse Compton scattering
• +۱۰ مورد دیگر