Find Academic Supervisors

• Quantum Physics
• Condensed Matter Physics
• Nanotechnology
• +4 more

Ester Jódar Ferrández is a Professor at the Universidad Politécnica de Cartagena, specifically affiliated with the School of Telecommunications Engineering. Her academic career spans over two decades with continuous research output from 1998 to the present, demonstrating sustained scholarly activity without indication of retirement or emeritus status. Her research interests focus on: Quantum Physics and Condensed Matter Physics Nanotechnology and Graphene Research Quantum Entanglement and Quantum Information Magneto-optic Effects including Faraday and Kerr effects PT-symmetric systems and quantum tunneling phenomena Her work demonstrates a strong interdisciplinary approach bridging theoretical physics with practical applications in materials science and nanotechnology. She has published extensively in high-impact physics journals including Physical Review series, Europhysics Letters, and Nanoscale Research Letters. Dr. Jódar Ferrández has also contributed to astronomical research through her involvement with the Euclid space mission, which focuses on dark matter and dark energy studies. Her 2017 book 'Problemas resueltos de matemática aplicada para ingeniería' demonstrates her commitment to engineering education and applied mathematics. Her recent research (2022-2024) shows a continued focus on quantum phenomena in PT-symmetric systems, with multiple publications examining tunneling time and magneto-optic effects. This work represents cutting-edge research at the intersection of quantum mechanics and optical physics, building upon her earlier foundational work in graphene systems and nanotube physics.

• Astrophysics
• Black Hole Physics
• Relativistic Jets
• +4 more

Dr. Alexandra Tetarenko is an Assistant Professor in the Department of Physics and Astronomy at the University of Lethbridge. She holds a BSc in Astrophysics from the University of Calgary and earned her MSc (2014) and PhD (2018) from the University of Alberta. Prior to her current role, she worked at the James Clerk Maxwell Telescope in Hawaii and held a NASA Einstein Fellowship at Texas Tech University. Her research focuses on black hole astrophysics and relativistic jet phenomena , using stellar-mass black holes as laboratories to study accretion-jet coupling. She develops novel observational techniques and computational tools for multi-wavelength data analysis, with specialization in radio/submillimeter astronomy. Key research areas include: Jet formation mechanisms in X-ray binaries Accretion dynamics during transient outbursts Submillimeter polarimetry of relativistic outflows Time-domain spectroscopy of compact objects Computational modeling of jet thermodynamics Her recent publications demonstrate strong emphasis on multi-wavelength monitoring of transient jets (particularly in Swift J1727.8–1613 and GRS 1915+105), ALMA/JWST instrumentation development, and black hole accretion physics across spectral states. Research frequently utilizes cutting-edge facilities including ALMA, JWST, and the Event Horizon Telescope. Honors: NASA Einstein Fellowship (postdoctoral award)

John BochanskiView profile

Associate Professor

• Astronomy
• Physics
• Galactic Structure
• +4 more

John Bochanski is an Associate Professor of Computer Science & Physics at Rider University, specializing in using large astronomical surveys to study the formation and evolution of the Milky Way galaxy. He is actively involved in major astronomical projects including the Sloan Digital Sky Survey (SDSS) and the Large Synoptic Survey Telescope (LSST) Science Collaborations. His educational background includes a Ph.D. in Astronomy from the University of Washington (2008), an M.S. in Astronomy from the same institution, and a B.S. in Astronomy & Astrophysics from Villanova University, where he graduated magna cum laude. Bochanski's research focuses on galactic structure and kinematics using cool, red stars as tracers. He employs large surveys like SDSS and Gaia to study two key regimes in the Milky Way: using cool red dwarfs to examine galactic structure near the Sun, and utilizing brighter red giants to investigate the distant Milky Way halo. His work is particularly relevant to upcoming surveys with the Nancy Grace Roman Space Telescope and the Vera Rubin Observatory. Supported by the LSST Discovery Alliance in cooperation with Princeton University's Department of Astrophysical Sciences, his research spans stellar kinematics, low-mass stars, and advanced data analysis techniques. His publication record shows a consistent focus on galactic structure, brown dwarfs, and large astronomical surveys, with recent work centered on SDSS-V and Gaia data analysis. The trend in his publications demonstrates increasing involvement in large-scale collaborative projects and data-intensive astronomy. Corporation for Science Advancement - Scialog Fellow (2018) Namesake of Main–belt asteroid 141414 Bochanski (2002 AK205) (2012) MIT Spot Award (2009, 2010) Elected to Phi Beta Kappa (2002) Jason Cardelli Memorial Undergraduate Research Award (2002) National Barry M. Goldwater Scholar (2001) Elected to Phi Kappa Phi (2001) Elected to Sigma Pi Sigma Physics (2000) Bochanski has held positions at multiple prestigious institutions including Rider University, Haverford College, Pennsylvania State University, and MIT. His current research is supported by the LSST Discovery Alliance, indicating significant grant funding for his work. He has mentored numerous students through his position as Program Founder & Director of Computer Science at Rider University since 2016. His technical expertise includes working with the FIRE (Magellan FIRE) spectrograph and developing data analysis pipelines for large astronomical surveys. His work with the Sloan Digital Sky Survey and Gaia mission data places him at the forefront of modern galactic astronomy research.

• Nanomaterials
• Electrocatalysis
• Inorganic Chemistry
• +3 more

Baiyu Wang serves as a Guest Researcher in the Department of Chemistry at the University of Copenhagen, located at Universitetsparken 5, 2100 København Ø. With an active research profile evidenced by publications spanning 2022-2025, Wang maintains laboratory contact through phone numbers +4535330268 and +4591922592, and email wang@chem.ku.dk. The research portfolio indicates strong integration within the university's chemistry research community, particularly collaborating with prominent researchers including Professor K. M. Ø. Jensen and Professor M. Arenz. Wang's research interests center on advanced nanomaterials for energy applications, with particular expertise in electrocatalysis and nanoparticle synthesis . The work demonstrates sophisticated understanding of structure-property relationships in catalytic materials, especially for water splitting and oxygen evolution reactions. Wang employs cutting-edge characterization techniques including in situ X-ray total scattering , operando diffraction studies , and pair distribution function analysis to investigate material transformations during electrochemical processes. This research bridges fundamental chemistry with practical energy applications, focusing on improving catalyst efficiency and durability through precise structural control. Analysis of Wang's publication record from 2022-2025 reveals a consistent trajectory in nanomaterials for electrocatalysis, with increasing sophistication in characterization methodologies. The research spans fundamental nanoparticle synthesis challenges to applied electrocatalytic systems, demonstrating both breadth and depth in materials chemistry. Wang's work shows particular strength in correlating atomic-scale structural features with macroscopic catalytic performance, especially regarding bimetallic systems and layered double hydroxides. The inclusion of a 2025 paper (likely in press) indicates ongoing active research contributions to the field.

Amy ReinesView profile

Associate Professor

• Massive black holes
• Dwarf galaxies
• Supermassive black holes
• +3 more

Amy Reines is an Associate Professor in the Department of Physics at Montana State University's College of Letters & Science, specializing in massive black holes in dwarf galaxies and star formation. Her groundbreaking work has identified over 100 dwarf galaxies hosting supermassive black holes, including the smallest known (~50,000 solar masses). Education: Ph.D. in Astronomy, University of Virginia (2011) M.S. in Astronomy, University of Virginia (2007) M.S. in Physics, San Francisco State University (2002) B.S. in Astronomy, University of Maryland (1998) Research Interests: Professor Reines pioneers the study of black holes in dwarf galaxies to unravel the origins of supermassive black holes. Her research demonstrates that black hole growth is intrinsically linked to galaxy evolution, even in the smallest systems. She investigates off-nuclear "wandering" black holes and their role in triggering star formation, utilizing multi-wavelength observations from Hubble, Chandra, and ground-based telescopes. Article Trends: Her publications reveal a consistent focus on observational detection of black holes in low-mass galaxies, spanning optical, radio, and X-ray techniques. Key themes include black hole demographics in dwarf systems, AGN identification methods, and the connection between black hole activity and star formation. Her work has established dwarf galaxies as critical laboratories for understanding primordial black hole seeds. Scientific Awards: Hubble Fellowship (2014) Einstein Fellowship (2011) Advising and Grants: Dr. Reines leads multiple NASA-funded projects including "The Origin of Supermassive Black Holes" and "Testing Mid-Infrared AGN Selection in Dwarf Galaxies with Chandra and HST." Her STScI and Smithsonian grants support studies of radio-selected black holes and dwarf irregular galaxies. She mentors graduate students in observational astrophysics and teaches courses like Astrophysics of Galaxies. Labs and Teams: She directs an active research group at Montana State University analyzing data from major observatories. Her team collaborates internationally on projects requiring Hubble Space Telescope, Chandra X-ray Observatory, and Very Large Array observations to study black hole-galaxy coevolution in low-mass systems.

• Star Formation
• Planet Formation
• Protostellar Disks
• +5 more

Rajeeb Sharma serves as a Guest Researcher at the Astrophysics and Planetary Science section of the Niels Bohr Institute, Faculty of Science, University of Copenhagen. His research focuses on the earliest stages of star and planet formation through high-resolution observational studies of embedded protostellar systems. Sharma's research interests center on observational astrophysics of star-forming regions, with specific expertise in: High-resolution ALMA observations of Class 0/I protostars Dust and gas dynamics in embedded disks Early planet formation mechanisms Snowline chemistry and dust evolution Protostellar multiplicity and disk alignment His work primarily analyzes submillimeter continuum and molecular line data to understand disk formation, structure, and evolution during the earliest phases of stellar birth. Analysis of his publication record reveals a strong focus on the eDisk (Early Planet Formation in Embedded Disks) survey, with contributions spanning disk kinematics, dust settling processes, snow surface chemistry, and magnetic field effects. His research demonstrates consistent use of cutting-edge interferometric techniques to probe protostellar environments at unprecedented resolution. Sharma actively collaborates with major international teams including the eDisk collaboration led by prominent researchers like Jes K. Jørgensen. His work has generated significant scientific impact, with multiple publications receiving notable citations and media coverage across astronomy news outlets. As a researcher at the Niels Bohr Institute, Sharma contributes to one of Europe's leading centers for astrophysics research, working within the Faculty of Science's Astrophysics and Planetary Science department. His position involves independent research, data analysis, and collaborative projects investigating the physical and chemical conditions in nascent planetary systems.

• Astrophysics
• Theoretical Astrophysics
• High-Energy Astrophysics
• +3 more

Clément Alexandre Bonnerot serves as a Guest researcher at the Niels Bohr Institute's Niels Bohr International Academy, University of Copenhagen, specializing in theoretical and observational astrophysics with emphasis on extreme gravitational phenomena. His research centers on tidal disruption events (TDEs), where stellar bodies are torn apart by supermassive black holes. Key investigations include relativistic hydrodynamics of debris streams, accretion disc formation mechanisms, and multi-wavelength emission signatures. Bonnerot employs advanced numerical simulations to model general relativistic effects, black hole spin dynamics, and collision-induced outflows, bridging theoretical frameworks with observational data from X-ray and radio telescopes. Analysis of his 8 recent publications (2022-2024) reveals dominant focus on TDE physics, with growing integration of AGN disc modeling techniques. The Nature-published study on quasi-periodic X-ray eruptions demonstrates impactful observational contributions, while his pAGN computational framework advances theoretical modeling capabilities. Collaborative patterns show extensive international partnerships across 44+ co-authors per major study. As part of the Niels Bohr International Academy's theoretical physics ecosystem, Bonnerot contributes to Copenhagen's leadership in gravitational astrophysics research through active participation in interdisciplinary seminars and computational working groups.

Axel SchwopeView profile

Associate Professor

• Compact Binaries
• White Dwarfs
• Neutron Stars
• +6 more

PD Dr. Axel Schwope serves as head of the X-ray astronomy group at the Leibniz Institute for Astrophysics Potsdam (AIP) and holds the position of Privatdozent (Associate Professor) at the University of Potsdam. He actively supervises Bachelor's, Master's, and doctoral students in astrophysics research, welcoming new students to his research group. Dr. Schwope's research focuses on compact binaries (particularly those with white dwarfs), neutron stars, and large-scale surveys at X-ray and optical wavelengths. He serves as co-investigator of eROSITA and the XMM-Newton Survey Science Centre, and leads activities to identify Compact Binaries in SDSS-V. His work spans multiple areas of high-energy astrophysics, including active galactic nuclei (AGN), clusters of galaxies, light pollution (sky protection), and Doppler tomography. His recent publications demonstrate a strong emphasis on X-ray astronomy, particularly using data from the eROSITA mission, SDSS surveys, and other major astronomical facilities. His research frequently employs multi-wavelength approaches, combining X-ray, optical, and other observations to study compact objects and their environments. A significant portion of his recent work focuses on white dwarfs, cataclysmic variables, and binary star systems. Main-belt asteroid 278513 named in his honor Dr. Schwope maintains extensive collaborations with both professional and amateur astronomers. He is deeply involved in major international projects including eROSITA, XMM-Newton, and SDSS-V, as evidenced by his numerous co-authorships across multiple institutions. His group at AIP appears to be well-integrated with the broader astronomical community, contributing significantly to large-scale survey science. His research group at AIP focuses on X-ray astronomy with particular emphasis on compact objects and large-scale surveys. The group utilizes data from multiple space-based and ground-based observatories, including eROSITA, XMM-Newton, and SDSS, to advance our understanding of high-energy astrophysical phenomena.

Sydney BarnesView profile

Researcher

• Stellar Astrophysics
• Stellar Rotation
• Exoplanets
• +3 more

Dr. Sydney Barnes serves as Group Head of the Stellar Activity research group within the Stellar Physics and Exoplanets section at the Leibniz Institute for Astrophysics Potsdam (AIP). Barnes leads cutting-edge research on stellar rotation dynamics, magnetic activity cycles, and their applications in exoplanet characterization and stellar age determination through gyrochronology. Barnes' research program centers on observational studies of stellar rotation evolution across diverse stellar populations. By analyzing open clusters of varying ages (including NGC 2281, NGC 6709, M 67, and NGC 3532), Barnes investigates angular momentum loss mechanisms and establishes precise rotation-age relationships. Significant contributions include the discovery of Hale-like magnetic cycles in solar twins such as 18 Scorpii, providing critical insights into stellar dynamo processes. Current work integrates TESS photometry with ground-based spectroscopy to study grazing exoplanet systems and characterize stellar activity signatures that impact exoplanet detection. Analysis of Barnes' publication record reveals a strategic focus on leveraging major observational facilities and upcoming missions. The research trajectory shows increasing involvement in flagship projects like PLATO (2025) and ELT-ANDES (2024), indicating a shift toward space-based instrumentation and high-resolution spectroscopic capabilities for studying stellar populations. Collaborative patterns demonstrate strong integration with AIP's technical divisions including High-resolution Spectroscopy and Polarimetry, Telescope Control and Robotics, and the Technical Section's optics group. Through leadership of the Stellar Activity group, Barnes maintains close collaboration with the University of Potsdam Astrophysics Network while directing research that bridges stellar astrophysics and exoplanetary science. The group's work on rotational evolution provides fundamental constraints for stellar evolution models and enhances the precision of exoplanet host star characterization.

• Galactic Astronomy
• Stellar Populations
• Chemical Abundances
• +3 more

Puragra Guhathakurta is a Professor of Astronomy and Astrophysics at the University of California Santa Cruz, where he has held a continuous faculty position since November 1994. His research focuses on galactic structure and evolution through detailed studies of stellar populations in the Milky Way, Andromeda (M31), and Triangulum (M33) galaxies using multi-wavelength surveys. His educational background includes: PhD and MS in Astrophysical Sciences, Princeton University (1985-1989) Physics, University of Calcutta, Science College, Rajabazar (1984-1985) BSc in Physics, Saint Xavier's College, Kolkata (1980-1983) La Martiniere for Boys, Kolkata (1970-1980) GuhaThakurta's primary research interests encompass: Galactic and Extragalactic Astronomy Stellar Populations and Chemical Abundances Galactic Structure and Kinematics Chemical Evolution of Galaxies Stellar Halos and Tidal Streams Dwarf Galaxy Dynamics Analysis of his 15 most recent publications (2023-2025) reveals a consistent focus on chemical abundances and kinematics in nearby galaxies. His work integrates Hubble Space Telescope imaging, ground-based spectroscopy, and Gaia astrometry to investigate weak CN absorption features in evolved stars, stellar halo structures, and the evolutionary histories of dwarf galaxies. A significant theme involves using resolved stellar populations to constrain galaxy formation models in the local universe. His major professional recognitions include: Hubble Fellowship (Princeton University, 1992-1994) Three-year Membership at the Institute for Advanced Study (1989-1992) While specific details of his advising and grant history are not documented in the source material, his extensive publication record demonstrates sustained research leadership. He is a principal investigator or key collaborator in major observational programs including SPLASH, PHATTER, HALO7D, and TREX, which have produced foundational datasets for studies of M31 and M33.

Vadim BurwitzView profile

Researcher

• high-energy astrophysics
• X-ray astronomy
• stellar variability

Dr. Vadim Burwitz serves as a Senior Scientist at the Max Planck Institute for Extraterrestrial Physics (MPE) in Garching, Germany, where he leads the PANTER X-ray test facility and is a key member of MPE's High Energy Astrophysics Group. His professional work centers on high-energy astrophysical phenomena and X-ray observational techniques. Dr. Burwitz's primary research interests focus on high-energy astrophysics, X-ray astronomy, and stellar variability phenomena. His work involves detailed investigation of celestial objects emitting X-rays, with particular attention to binary star systems and supersoft X-ray sources. His research contributes significantly to our understanding of accretion processes and evolutionary pathways of compact stellar objects. His publication record demonstrates consistent expertise in analyzing variable phenomena in high-energy astrophysical systems, with emphasis on temporal behavior of X-ray sources. His work bridges observational data with theoretical models to advance our understanding of extreme physical processes in the universe. As Head of the PANTER X-ray test facility, Dr. Burwitz oversees critical instrumentation development, calibration procedures, and testing protocols for X-ray astronomy missions. The facility plays an essential role in verifying performance characteristics of X-ray telescopes and detectors prior to space deployment, ensuring mission success for international X-ray observatories.

Yuan ZhangView profile

Professor

• program analysis
• software testing
• system security
• +9 more

Yuan Zhang is a Professor in the School of Computer Science at Fudan University, where he co-directs the System Software and Security Laboratory. He is also the co-founder and coach of Fudan University's CTF team, Whitzard, which has participated in numerous international competitions. His academic journey includes earning a Ph.D. from Fudan University (2009-2014) and a B.Eng. from Nanjing University (2005-2009), progressing from Assistant Professor to Associate Professor and finally to Professor at Fudan University. Dr. Zhang's research focuses on system security for widely-deployed critical targets, with current emphasis on open-source software, kernels, Android/Web platforms, firmware, LLM-based agents, and autonomous driving systems. His work spans vulnerability discovery/exploitation/mitigation, malware/attack detection, and privacy protection, utilizing interdisciplinary techniques such as Program Analysis, LLMs, and Machine/Deep Learning. His research demonstrates a consistent trajectory from traditional software security toward emerging AI-driven security challenges. His recent publications (2024-2025) reveal a strong focus on novel security challenges in emerging technologies, particularly LLM-based systems and autonomous driving security, while maintaining expertise in traditional software security domains like Android, web applications, and firmware. His work combines practical vulnerability discovery with innovative detection methodologies, often achieving recognition through distinguished paper awards. Honorable Mention Award at USENIX Security 2025 Distinguished Paper Award at IEEE S&P 2025 ACM SIGSOFT Distinguished Paper Award Dr. Zhang actively contributes to the academic community through teaching courses including Principles of Reverse Engineering, System Security: Attacks & Defenses, and Emerging Attack & Defense Techniques. He serves on editorial boards for ACM Transactions on Security and Privacy and Cybersecurity, and participates in numerous top security conference program committees including USENIX Security, IEEE S&P, and ACM CCS. His laboratory, the System Software and Security Laboratory at Fudan University, focuses on practical security research with real-world impact, particularly in the rapidly evolving landscape of AI security.

Lucas LabadieView profile

Professor

• Astronomy
• Astrophysics
• Experimental Physics
• +8 more

Lucas Labadie is a Professor of Experimental Physics at the I. Physics Institute of the University of Cologne, where he has been employed since 2011. He leads an active research group focused on observational astronomy and astrophysics, with particular emphasis on star and planet formation processes. His educational background includes: 1997-2000: École de Physique de Marseille (now Ecole Centrale Marseille) 2000: DEA in Physics (Master's degree), Université Paul Cézanne, Marseille 2006: PhD in Physics & Astronomy, Université Grenoble Alpes Professor Labadie's research spans multiple areas in astrophysics, with primary focus on protoplanetary disks, young stellar objects across the mass spectrum, and the development of high-angular resolution instrumentation. His work combines observational approaches with innovative instrumentation development, particularly in interferometry and astrophotonics. The research group employs techniques from optical to mid-infrared wavelengths to probe the physics of star and planet formation. His publication record shows consistent contributions to the Astronomy & Astrophysics journal, with significant involvement in the GRAVITY Young Stellar Object Survey. Recent work focuses on disk structures around young stars, interferometric techniques, and astrophotonics applications. The publications demonstrate an evolution from studying individual objects to systematic surveys of young stellar populations. Professor Labadie actively mentors students at all levels, supervising PhD candidates, master's students, and bachelor's students. His research is supported by grants from German funding agencies including DFG and BMBF, with involvement in major international projects like the Extremely Large Telescope instrumentation. His group maintains active collaborations with major observatories and participates in the development of next-generation astronomical instruments, particularly METIS for the ELT and interferometric beam combiners. The team combines theoretical modeling with observational data and instrument development to address fundamental questions in star and planet formation.

• Geophysics
• Planetary Science
• Computational Modeling
• +3 more

Ulrich Christensen is a Professor at the Faculty of Physics (including GAUSS) at Georg-August-Universität Göttingen, specializing in geophysics and planetary science. His research employs computational modeling to study planetary dynamics, including zonal winds on gas giants, dynamo processes in planetary cores, and thermal evolution of terrestrial planets. Key research areas include: Numerical simulations of planetary interiors and atmospheres Dynamo theory and magnetic field generation Mantle convection and plate tectonics modeling Thermal evolution of Mars and Mercury As a doctoral advisor, Professor Christensen has supervised 8 PhD students between 2000-2023, with dissertations covering topics ranging from seismic tomography to binary eutectic systems in planetary cores.

Saskia HekkerView profile

Researcher

• Stellar Ages
• Galactic Evolution
• Asteroseismology
• +5 more

Saskia Hekker leads the Max Planck Research Group in Stellar Ages and Galactic Evolution (SAGE) at the Max Planck Institute for Solar System Research. Her research focuses on asteroseismology to determine fundamental stellar properties including ages, masses, and radii, with particular emphasis on red giants and subgiant stars across various evolutionary stages. Dr. Hekker's work centers on using stellar oscillations to probe internal stellar structure and evolution. Her research spans asteroseismic analysis of red giants, subgiants, and dwarf stars, with applications to galactic archaeology and evolution. She leverages data from major space missions (Kepler, TESS) and ground-based spectroscopic surveys (APOGEE, GALAH, RAVE) to extract precise stellar parameters and understand galactic chemical evolution. Her work has significantly advanced our understanding of stellar rotation, internal structure, and the connection between stellar properties and galactic history. Her publication record demonstrates extensive collaboration across the international astrophysics community. Dr. Hekker has made key contributions to major projects including the K2 Asteroseismic KEYSTONE sample and multiple Sloan Digital Sky Survey data releases. Her research has helped establish asteroseismology as a critical tool for determining precise stellar ages, which is essential for reconstructing the Milky Way's formation history. Quentin Charles Yvon Hugues Coppée: Characterising the suppression of non-radial modes in red giants Lynn Buchele: Asteroseismic structure inversions of solar-like oscillators Nathalie Themeßl: Asteroseismic inferences from red-giant stars Earl Patrick Bellinger: Inverse Problems in Asteroseismology As leader of the SAGE research group, Dr. Hekker directs investigations into how asteroseismic techniques can precisely determine stellar ages and illuminate galactic evolution pathways. The group's work combines theoretical modeling with analysis of large observational datasets to extract detailed information about stellar structure, evolution, and the history of our galaxy.