Find Academic Supervisors

• Artificial Intelligence for Science
• Explainable AI
• Trustworthy AI
• +7 more

Wei (Celia) Xu serves as Research Professor in the Computer Science Department at Stony Brook University and Computational Scientist/Trustworthy AI (TAI) Group Lead at Brookhaven National Laboratory's Computational Science Initiative, driving innovation in AI for scientific discovery across multiple domains. Her educational foundation includes a Ph.D. in Computer Science from Stony Brook University and dual M.S. degrees in Computer Science from Zhejiang University, establishing expertise in computational methods and visualization. Dr. Xu's research centers on developing explainable and trustworthy AI frameworks for scientific applications, with notable contributions in digital twins for simulation workflows, performance evaluation of quantum/classical computing systems, and visual analytics for X-ray imaging and climate science. Her work integrates GPU acceleration and virtual reality to enhance scientific data interpretation, emphasizing model interpretability and reliability in high-stakes domains. Analysis of her 15 most recent publications (2019-2025) reveals a strategic evolution toward trustworthy AI systems, with increasing focus on counterfactual explanations for medical diagnostics, digital twin implementations for ensemble simulations, and quantum state visualization—demonstrating cross-disciplinary impact in materials science, climate modeling, and high-energy physics. Her exceptional contributions have been recognized with prestigious awards: Best Paper Award, PacificVis (2025) Best Paper Award, IEEE SC/ISAV (2020) Honorable Mention Award, IEEE VIS (2018) Women@Energy Recognition (2014) Best Paper Award, Fully3D/HPIR (2009) Dr. Xu actively mentors through her TAI research group while securing sustained funding from DOE's Biological and Environmental Research (BER) program and SciDAC initiatives, complemented by Brookhaven National Laboratory internal projects (LDRD and NSLSII DSSI). She serves on program committees for SC, VIS, and AAAI conferences and has organized workshops including NYSDS and Fully3D, demonstrating leadership in advancing trustworthy AI methodologies for scientific communities.

• Astrophysics
• Cosmology
• Radio Astronomy
• +2 more

Nceba Mhlahlo is a Lecturer in the School of Physics at the University of the Witwatersrand, where he conducts research in astrophysics and cosmology. He holds a BSc, BScHons, MSc, and PhD from the University of Cape Town. His contact information includes phone: 0117176831 and email: Nceba.Mhlahlo@wits.ac.za . His ORCID profile is accessible via 0000-0001-7435-2269 . Dr. Mhlahlo's research focuses on several interconnected domains: Galaxy clusters : Investigating shock acceleration, non-thermal pressure, and merger dynamics using multiwavelength data. Radio galaxies : Discovering and characterizing giant radio sources with instruments like MeerKAT and KAT-7. Cosmological fluid dynamics : Modeling interactions of dust fluids in expanding universes. Telescope surveys : Leading observational programs including the MeerKAT Galaxy Cluster Legacy Survey. His 15 publications (1999–2024) reveal thematic shifts: early nuclear physics (1999) and cataclysmic variables (2004–2007), transitioning to radio astronomy and galaxy clusters (2013–present). Recent works emphasize radio telescope discoveries, while earlier studies centered on stellar binaries. No awards, grants, or student mentoring activities are documented.

• High Energy Astrophysics
• Dark Matter Detection
• Gamma-ray Astronomy
• +4 more

Dr. Anthony Brown is an Assistant Professor in the Department of Physics at Durham University, affiliated with the Institute of Hazard, Risk and Resilience. His research focuses on high-energy astrophysics and dark matter detection through gamma-ray observations. Key research areas: Dark Matter Detection, Gamma-ray Astronomy, Cherenkov Telescopes, Cosmic Ray Interactions Instrumentation expertise: Atmospheric Cherenkov Detectors, Balloon-borne Platforms, UAV Calibration Systems Supervision: Mentored three postgraduate research students (Amrit Nayak, Ed Dewit, Ieva Jankute) Recent publications highlight his work on Cherenkov Telescope Array calibration techniques (2022), millisecond pulsar gamma-ray modeling (2024), and dark matter signatures in globular clusters (2018). His research spans ultra-high energy neutrino detection (2021), extragalactic cosmic ray propagation (2017), and multi-messenger astronomy approaches combining gamma-ray and neutrino observations (2015). Scientific contributions include: Development of airborne calibration systems for ground-based observatories Analysis of gamma-ray emission from active galactic nuclei (2017-2024) Investigations into dark matter annihilation signatures in galaxy clusters Innovations in stratospheric imaging telescope performance (2020) Current projects involve the Cherenkov Telescope Array's line search capabilities for dark matter (2024) and studying pulsar geometry effects on emission spectra (2024). His work bridges experimental astrophysics with particle physics, particularly in high-energy cosmic phenomena and neutrino detection.

• Astrophysics
• Globular Clusters
• Star Formation
• +3 more

Nate Bastian is a Honorary Visiting Professor at the Astrophysics Research Institute , Liverpool John Moores University. His research focuses on the formation and evolution of star clusters, globular clusters, and their connections to galaxy assembly and dark matter halos. Key areas: Globular Clusters , Multiple Populations , Binary Stars , Black Hole Detection , Dark Matter Tracing Email: N.J.Bastian@ljmu.ac.uk Recent publications highlight his work with the E-MOSAICS simulations to study globular cluster populations, their kinematics, and their role in reconstructing galaxy merger histories. He has also contributed to understanding the physics of globular cluster mass functions and nitrogen variations in star clusters. Scientific awards include a Royal Society grant for his work on globular cluster formation and evolution in cosmological contexts.

• Stellar Astrophysics
• Supernovae
• Massive Stars
• +4 more

Dr. Emma Beasor is a Royal Society Dorothy Hodgkin Fellow at the Astrophysics Research Institute, Liverpool John Moores University, with future appointment as Senior Lecturer starting 2025. She previously held prestigious fellowships at NSF's NOIRLab (NASA Hubble Fellow 2019-2022) and University of Arizona (Bart J. Bok Fellow 2022-2024). PhD in Astrophysics (2015-2019), MPhys (2011-2015) from University of Liverpool Her research focuses on massive star evolution, particularly red supergiants, combining observational data from JWST/Hubble with theoretical models like MESA. Key questions address mass-loss effects, supernova progenitors, and compact remnant formation. Her work includes 15 recent publications (2020-2025) analyzing red supergiant mass loss, supernova progenitor identification, and stellar death mechanisms. Articles often employ multi-wavelength observations and computational modeling. Royal Society Dorothy Hodgkin Fellowship NASA Hubble Fellowship Bart J. Bok Fellowship Grants and awards support her studies on massive star evolution, supernovae, and galactic abundance mapping. She collaborates with institutions like NOIRLab, University of Arizona, and international observatories.

• Astrophysics
• Stellar Physics
• Massive Stars
• +5 more

Ignacio Negueruela Díez is a Full Professor in the Applied Physics Department at the Faculty of Sciences, University of Alicante. He holds an office in the Faculty of Sciences II building (P2 - 0007P2060) and can be reached at ignacio.negueruela@ua.es or +34 965903400 x 2754. He is affiliated with the Institute of Computer Research and leads the Stellar Astrophysics research group. His academic credentials include a Doctorate in Sciences from the University of Zaragoza (2000), a PhD from the University of Southampton (1997), and a Licentiate in Physical Sciences from the University of Zaragoza (1993). Negueruela Díez specializes in astrophysics with particular focus on massive stars, stellar evolution, and binary star systems. His research encompasses red supergiants, high mass X-ray binaries, stellar clusters, and massive star populations across the galaxy. He has made significant contributions to understanding the properties of massive stars, their evolution, and their role as progenitors of supernovae and gravitational wave sources. His work combines observational data with theoretical models to advance our understanding of stellar physics. His publication record shows a consistent focus on massive stars and their environments, with recent work centered on creating large-scale spectroscopic databases of massive stars, studying stellar evolution in clusters, and investigating binary interactions. His research spans from stellar formation to end states, including supernova progenitors and gravitational wave sources. Negueruela Díez has directed 8 doctoral theses, with several receiving 'Excellent Cum Laude' distinctions. His research is supported by numerous competitive grants from Spanish and Valencian government agencies, including projects running through 2025 on massive star research and AI applications for stellar analysis. He is actively involved in research management, having coordinated multiple research projects including 'Herramientas de Inteligencia Artificial para estrellas masivas' (2022-2025), 'Exploración exhaustiva de la infancia y vejez de las estrellas masivas' (2022-2025), and previous projects on massive star evolution and databases.

Barbara CatinellaView profile

Professor

• Galaxy evolution
• Interstellar medium and star formation
• Atomic and molecular gas surveys
• +3 more

Professor Barbara Catinella is an observational astronomer at the International Centre for Radio Astronomy Research (ICRAR), The University of Western Australia. She leads the Local Universe research group and serves as Chief Investigator for ASTRO 3D. Her international roles include co-chairing the SKA HI Galaxy Science Working Group and membership on the IAU Division J steering committee. PhD in Astronomy (2005), Cornell University M.S. in Astronomy (2002), Cornell University Her research focuses on cold gas dynamics in galaxies, particularly atomic/molecular gas surveys and their connections to star formation processes. Key projects include the WALLABY and MAUVE galaxy surveys using ASKAP and ESO's VLT. Recent publications analyze: HI emission mapping in edge-on galaxies Gas scaling relations in stellar discs Machine learning applications for HI detection Scientific recognition: Recipient of The Anne Green Prize (2018) Active in Australian Research Council funded projects, including Discovery Projects and Future Fellowships. Collaborates with institutions in Korea, Germany, and USA. Currently involves datasets from: ASKAP Pilot Survey for WALLABY IllustrisTNG galaxy simulations

Jean-Paul KneibView profile

Professor

• Cosmology
• Gravitational Lensing
• Redshift Surveys
• +5 more

Jean-Paul Kneib is a Full Professor at the Laboratory of Astrophysics (LASTRO) within the School of Basic Sciences (SB) at École Polytechnique Fédérale de Lausanne (EPFL), Switzerland. He is also involved in the Space Sustainability initiative at EPFL and has held visiting positions at Caltech and CNRS institutions. His research focuses on cosmology, gravitational lensing, and next-generation spectroscopic surveys like DESI and Euclid. Education : PhD in Astrophysics (1993), Master in Astrophysics, Geophysics & Space Technics (1990), Engineer degree in Aerodynamics & Space Technics (1990), all from Toulouse University and École Nationale Supérieure de l'Aéronautique et de l'Espace. Research Interests : Kneib specializes in cosmology, using galaxy surveys and gravitational lensing to study dark matter and dark energy. His work includes strong lensing in galaxy clusters, redshift surveys for cosmic expansion analysis, and robotic fiber-positioner systems for spectroscopic instruments. He also contributes to space sustainability initiatives addressing orbital debris. Recent Publications emphasize deep learning for radio interferometry, Euclid mission early data, DESI BAO analysis, and novel methods for asteroid detection. Collaborative projects involve JWST observations of high-redshift galaxies and digital twins for CubeSats. Scientific Awards : ERC Advanced Laureate (for project "Light on the Dark") Marie Curie Fellowship Leadership Roles : Co-Lead of ESA Euclid "Strong Lensing" Working Group Co-Principal Investigator for CFHT-Stripe 82 project Developer of Fiber-Robot Positioner System for DESI collaboration

• Science Education
• Classroom Technology
• Space Mission Research
• +3 more

Melodi Rodrigue is an Associate Teaching Professor in the Department of Physics at University of Nevada, Reno. With expertise in astrophysics and science education, she bridges research in galaxy interactions with innovative STEM pedagogy. Education: Ph.D. in Physics (1998), M.S. Physics (1994), B.S. Physics (1987) from University of Nevada, Reno. Professional experience includes lecturer positions at UNR and Truckee Meadows Community College since 1994. Research encompasses science education technology, space mission research facilities, interacting galaxies, and exoplanet detection. Current projects focus on K-12 science education enhancement through telescope facilities and curriculum development. Publications demonstrate interdisciplinary focus spanning astronomy education, galaxy spectroscopy, and biosensing technology. Recent pedagogical work develops laboratory assessment methods while astronomical research examines galaxy interactions using multi-wavelength data. Honors include Distinguished Teaching Assistant (1993) and NASA Research Fellowship (1992-1996). Advised 10 PhD students in astrophysics and education research.

• Dual/binary active galactic nuclei
• Star-formation in galaxy mergers
• Kilo-parsec structure in low-luminosity AGN
• +5 more

Rubinur Khatun is a Research Fellow at the Institute of Theoretical Astrophysics , University of Oslo. Her research focuses on dual/binary active galactic nuclei (AGN) , star-formation in galaxy mergers , and kilo-parsec structures in low-luminosity AGN . She holds a Ph.D. in Physics from the Indian Institute of Astrophysics (2019) and an M.Sc. in Physics from St. Xavier's College, Kolkata (2013), where she received a Gold Medal for academic excellence. Research Interests : Khatun’s work explores feedback mechanisms in galaxies, peculiar radio galaxies, and observational studies of galaxy mergers. She uses advanced techniques like adaptive-optics spectroscopy and multi-telescope observations (e.g., VLT/ERIS, uGMRT) to detect binary AGN systems and study their dynamics. Her recent work includes analyzing Fe K lines in binary AGN and UV emission signatures of AGN feedback. Key Contributions : Detection of binary AGN via Fe K lines, confirmation of lensed systems via near-IR spectroscopy, and studies of molecular gas in low-mass galaxies. Awards : Gold Medal for M.Sc., St. Xavier’s College (2013). Research Groups : Cosmology and Extragalactic Astronomy, Nordic Radio and Millimeter Astronomy Network (NoRMA).

Ian HewittView profile

Lecturer

• Extra-galactic astronomy
• galaxy morphology
• machine learning and data analysis in astronomy
• +7 more

Ian Hewitt serves as a Teaching Associate in the Department of Computing Sciences within the College of Science at Coastal Carolina University. His career transitioned from technical roles at Motorola in hardware, software, and global communications systems to astronomy research, where he now integrates computational expertise with astronomical studies. Education: M.S. in Astronomy, Swinburne Institute of Technology M.S. in Electrical Engineering, University of South Carolina B.S. in Computer Engineering, University of South Florida His research spans extra-galactic astronomy and galaxy morphology with specialized focus on machine learning applications for astronomical image analysis and observational data processing. Complementing this, he maintains active interests in computer architecture, machine language, and performance analysis, which directly inform his pedagogical approach to teaching scientific reasoning and programming fundamentals. Professional Recognition: Fellow of the Royal Astronomical Society Ian Hewitt leads the Spiral Graph project on the Zooniverse citizen science platform as its principal programmer, facilitating public participation in galaxy morphology classification. His industry background in high-availability systems informs his research methodology, though specific student advising relationships or grant funding details are not documented in the available materials.

Claudia MarastonView profile

Professor

• Astrophysics
• Cosmology
• Stellar Population Modelling
• +3 more

Claudia Maraston is a Professor of Astrophysics at the University of Portsmouth, affiliated with the Faculty of Technology and the Institute of Cosmology and Gravitation. She holds a PhD from the University of Bologna, followed by postdoctoral positions at the Ludwig-Maximilian University of Munich and the Max-Planck Institute for Extraterrestrial Physics. In 2005, she received a Marie-Curie Fellowship at the University of Oxford, later joining Portsmouth in 2007 as a Senior Lecturer and advancing to her current role. Her research focuses on stellar population modeling, galaxy evolution, and high-redshift phenomena. Maraston's work includes groundbreaking studies using the MaNGA survey and contributions to the Euclid mission. She has authored over 240 publications, with recent articles addressing neutron star/black hole graveyards, quiescent galaxy spectral features, and the Euclid mission's observational framework. She has supervised 13 PhD students and holds grants like the Marie-Curie Excellence Team Grant (2007). Her lab, the Institute of Cosmology and Gravitation, is a leading center for cosmological research.

• Astronomical Sciences
• Cosmology
• Astrophysics
• +5 more

Prof. Jeff Cooke is a Professor at Swinburne University of Technology's School of Science, Computing and Emerging Technologies. He leads research in high-redshift galaxies, supernovae, fast transients, and gravitational waves. As a Chief Investigator at OzGrav and Associate Investigator at ASTRO-3D, he explores cosmic reionization, galaxy evolution, and transient phenomena. His work includes detecting Lyman continuum galaxies and pioneering techniques for super-luminous supernova studies. He chairs the Deeper, Wider, Faster (DWF) program to detect fast transients like FRBs and gravitational wave counterparts using global telescope networks. Professional activities include committee roles in SATCON, Keck Observatory, and international conferences. Awards include ARC Future Fellowship (2013) and multiple Vice-Chancellor's Research Excellence Awards. He supervises PhD students on topics like host galaxy studies and AI-driven transient detection. Key grants include ARC funding for DWF and Keck Wide-Field Imager development. His lab collaborations span over 30 institutions globally. Research focuses on multiwavelength surveys, real-time data analysis, and cosmic baryon distribution studies via FLIMFLAM. His expertise bridges observational astronomy, instrumentation, and computational methods to address fundamental questions in astrophysics and cosmology.

Adi FoordView profile

Assistant Professor

• Supermassive Black Holes
• Galaxy Mergers
• X-ray Astronomy
• +3 more

Adi Foord is Assistant Professor of Physics at UMBC, specializing in supermassive black hole evolution. She holds a Ph.D. from University of Michigan and was previously Porat Fellow at Stanford's Kavli Institute. Leads research group studying dual AGN in merging galaxies. Research Focus: Combines X-ray (Chandra, XMM-Newton), optical (HST), and infrared (WISE) data to probe black hole-galaxy co-evolution during cosmic mergers. Develops detection methods for binary AGN systems. Key Projects: AXIS probe mission science team member; develops 'Dual AGN Finder' for Rubin Observatory LSST data; investigates hyperluminous X-ray sources. Honors: RCSA Scialog Fellowship for LSST early science. Secured NSF funding for multi-wavelength AGN studies. Team: Mentors 3 graduate and 2 undergraduate researchers in high-energy astrophysics.

Maria BergemannView profile

Researcher

• Stellar Spectroscopy
• Galactic Structure
• Chemical Evolution
• +7 more

Maria Bergemann is a Lise Meitner Group Leader and Independent Research Group Lead at the Max Planck Institute for Astronomy in Heidelberg, heading the Stellar Spectroscopy and Populations research group within the Galaxies and Cosmology department. Her research spans theoretical and observational astrophysics with a focus on stellar physics, galactic evolution, and cosmic nucleosynthesis. Her work encompasses non-equilibrium (Non-LTE) radiative transfer modeling and 3D radiation-hydrodynamics simulations of stellar atmospheres, lifting canonical approximations to provide new insights into stellar structure. She is actively involved in major astronomical programs including the Gaia-ESO survey, 4MOST, PLATO, WEAVE, and MSE projects, analyzing multi-million datasets to address fundamental questions about the origins of chemical elements, galactic structure, and star-planet connections. Her group has made significant contributions to understanding galactic chemo-dynamics, including studies of stellar clusters, abundance gradients, and the structure of the Milky Way disk and bulge. Dr. Bergemann's research has received support from the Max Planck Society, European Research Council, and the German Research Foundation. Her team develops sophisticated mathematical and statistical algorithms for robust model-data comparison and pattern recognition in multi-dimensional parameter spaces, including adaptation of the Payne code for Gaia-ESO and 4MOST data analysis and introduction of Bayesian spectroscopy methods. Max Planck Society funding recipient European Research Council funding recipient German Research Foundation funding recipient She has supervised numerous PhD students, postdocs, and master's students who have gone on to faculty positions at institutions worldwide including Purdue University, Frankfurt University, Yunnan University, and the University of Sheffield. Her current research group includes several members working on diverse projects related to stellar atmospheres, galactic structure, and nucleosynthesis. The group maintains the public database http://nlte.mpia.de for 3D Non-LTE models, which are essential for deriving accurate fundamental parameters of stars and their detailed chemical compositions.