جست‌وجوی استاد و پژوهشگر

Susan E. Clarkمشاهده پروفایل

استادیار

• Cosmic Magnetic Fields
• Interstellar Medium
• Astrophysical Magnetic Fields
• +۶ مورد دیگر

Susan E. Clark is an Assistant Professor of Physics at Stanford University, where she investigates cosmic magnetic fields, magnetohydrodynamic processes, and the interstellar medium (ISM) through observation, simulation, and analytic theory. Prior to Stanford, she was a NASA Hubble Fellow and postdoctoral member at the Institute for Advanced Study in Princeton, New Jersey, after earning her Ph.D. in Astrophysics from Columbia University (2017) and B.S. in Physics from the University of North Carolina at Chapel Hill (2012), supported by a Morehead-Cain scholarship. Education: Ph.D., Astrophysics, Columbia University (2017) — NSF Graduate Fellow B.S., Physics, University of North Carolina at Chapel Hill (2012) — Morehead-Cain scholarship Her research focuses on Galactic and extragalactic magnetism, interstellar turbulence, star formation, and polarized cosmological foregrounds. She leads an interdisciplinary group tackling these problems via observational data, numerical simulations, and machine learning techniques. Current projects include characterizing magnetic field alignment, modeling 3D ISM structure, and analyzing data from experiments like the Atacama Cosmology Telescope, Simons Observatory, CMB-S4, CCAT-Prime, LiteBIRD, and the Galactic Australian SKA Pathfinder (GASKAP). Recent publications highlight her work on dust filament misalignment, HI morphology for gas phase separation, equipartition magnetic field estimation, and tomographic MHD simulations of galactic magnetic fields. These studies integrate astrophysics, computational methods, and observational astronomy to decode the universe's magnetic structure and dynamics. Scientific Awards: Alfred P. Sloan Research Fellowship NSF Graduate Fellowship NASA Hubble Fellowship Clark co-founded the Pan-Experiment Galactic Science Group and co-directs Stanford's Center for Decoding the Universe, fostering interdisciplinary collaborations. Her lab includes postdocs, graduate students, and undergraduates, with alumni transitioning to roles in academia and industry. Funding comes from NSF, NASA, and the Sloan Foundation.

Elena D'Onghiaمشاهده پروفایل

دانشیار

• Galactic Dynamics
• Stellar Structure Formation
• Numerical Simulations
• +۳ مورد دیگر

Elena D'Onghia is an Associate Professor in the Department of Astronomy at the University of Wisconsin-Madison. Her research focuses on unraveling the dynamical processes that shape the stellar structure of the Milky Way and nearby galaxies using analytical models and high-resolution numerical simulations. She leverages data from the GAIA satellite to study galactic evolution, emphasizing the importance of understanding our cosmic environment beyond the Solar System. University: University of Wisconsin-Madison Department: Astronomy Contact: edonghia@astro.wisc.edu | 4504 Sterling Hall Research Interests D'Onghia's work spans galactic dynamics, stellar structure formation, and interstellar medium processes. She investigates how gravitational interactions, stellar bars, and supernova-driven outflows influence galactic morphology. Her studies often integrate multi-wavelength observations with cosmological simulations to trace the evolution of galaxies like the Milky Way and Magellanic Cloud analogs. Recent Publications Her recent articles highlight galactic disk corrugations, starburst outflows in the LMC, and the role of classical bulges in shaping stellar bars. Collaborative projects include the Sloan Digital Sky Survey and ALMA-based studies of high-redshift galaxies. Scientific Awards 2018-2020 Vilas Associate Professor Research Fellow 2013-2017 Alfred P. Sloan Research Fellow 2013 Kavli Fellow Frontiers of Science 2009-2012 Keck Fellowship (Harvard) 2005-2006 Max-Planck Research Fellowship

David A. Neufeldمشاهده پروفایل

استاد

• Theoretical Astrophysics
• Interstellar Medium
• Molecular Astrophysics
• +۳ مورد دیگر

David A. Neufeld is a Professor in the William H. Miller III Department of Physics & Astronomy at Johns Hopkins University (JHU), part of the Krieger School of Arts & Sciences. He holds a PhD from Harvard University and specializes in theoretical astrophysics, molecular astrophysics, and interstellar medium (ISM) studies. His research utilizes advanced observatories like the Herschel Space Observatory and SOFIA (Stratospheric Observatory for Infrared Astronomy), focusing on molecular line emission, cosmic ray ionization rates, and hydride molecules in diffuse clouds. Key projects include leading the HyGAL SOFIA Legacy Program to study hydrides in the Galactic ISM and participating in Herschel’s HEXOS, PRISMAS, and WISH Guaranteed Time programs. Neufeld has developed experimental methods to constrain sexaquark dark matter and contributed to the discovery of the helium hydride ion (HeH+) in planetary nebulae. He is also involved in GUSTO, a terahertz spectroscopic mission mapping [CII] and [NII] emissions. His research integrates observational astronomy with theoretical models, exploring topics like protostellar outflows, water ice chemistry, and shock dynamics. He has published extensively on infrared/submillimeter spectroscopy, molecular ion abundances, and the role of cosmic rays in interstellar chemistry. Neufeld’s work bridges laboratory experiments (e.g., dissociative recombination studies) with astrophysical observations, advancing understanding of the ISM and star formation processes.

• Applied Electromagnetics
• Computational Electromagnetics
• Metamaterials
• +۹ مورد دیگر

Francisco Javier Falcone Lanas is a Professor in the Department of Electrical, Electronic and Communication Engineering at the Public University of Navarre. He is affiliated with the Institute of Smart Cities and leads research in the Communication, Signals and Microwaves research group. He also participates in the Doctoral Program in Communications Technologies, Bioengineering, and Renewable Energy. His research focuses on applied and computational electromagnetics, with specializations in: Analysis and design of complex electromagnetic media and metamaterials Design of communication devices (filters, diplexers, couplers, antennas) Implementation of devices on flexible/paper substrates Wireless power transfer systems Computational electromagnetic code development (FDTD, 3D Ray Launching, Radar RCS) Implementation of devices for PLMN, WSN, LPWAN and Radar systems Radioelectric analysis at physical layer and system level His recent publications demonstrate a strong focus on millimeter-wave technology, MIMO antenna systems, 5G/6G communications, and wireless sensor networks. His work often addresses optimization challenges related to energy consumption, interference handling, and capacity/coverage in communication systems. He has made significant contributions to the fields of metamaterials and their application in antenna design and performance enhancement. With an H-index of 58 in Scopus, Professor Falcone Lanas has established himself as a leading researcher in his field. His research has practical applications in various domains including: 5G/6G mobile communication systems Wireless body area networks Vehicle-to-everything (V2X) communications Wireless sensor networks for industrial applications Digital twin modeling for UAV communications Earthquake disaster management systems

Susan Clarkمشاهده پروفایل

استادیار

• Astrophysical Magnetism
• Interstellar Medium Physics
• Cosmic Magnetic Fields
• +۶ مورد دیگر

Susan Clark is an Assistant Professor of Physics at Stanford University and a Senior Member of KIPAC (Kavli Institute for Particle Astrophysics and Cosmology). She leads the Cosmic Magnetism & Interstellar Physics research group and serves as co-director of the Center for Decoding the Universe at Stanford. Her research focuses on understanding astrophysical magnetism and the physics of the interstellar medium across multiple scales, from diffuse gas to dense star-forming regions. Clark received her Ph.D. in 2017 from Columbia University as an NSF Graduate Fellow, following undergraduate studies at the University of North Carolina at Chapel Hill on a Morehead-Cain scholarship. Prior to joining Stanford in September 2021, she was a NASA Hubble Fellow at the Institute for Advanced Study in Princeton. Her research tackles fundamental questions about the structure of the Milky Way's magnetic field, the nature of interstellar turbulence, and the role of magnetism in star formation. Clark and her group decipher the magnetic interstellar medium using multiwavelength observations and innovative data analysis techniques, employing tracers including gas line emission and absorption, polarized dust and synchrotron emission, starlight polarization, Zeeman splitting, and Faraday rotation. Her work has significant implications for cosmic microwave background research, particularly in understanding and removing galactic foregrounds. Clark collaborates on numerous major telescope projects including the Atacama Cosmology Telescope (ACT), Simons Observatory (SO), CMB-S4, CCAT-Prime, LiteBIRD, and the Galactic Australian SKA Pathfinder (GASKAP). She co-founded the Pan-Experiment Galactic Science Group to facilitate Milky Way science with CMB experiment data. 2025 AAS Warner Prize 2024 Sloan Research Fellowship Unsung Hero Award (2019) for prison teaching work Clark mentors a large research group comprising postdoctoral fellows, graduate students, and undergraduate researchers. Her group's work is funded by grants from the NSF and NASA. Beyond research, Clark is committed to teaching and outreach, having previously taught through the Princeton Prison Teaching Initiative and expressing enthusiasm for making STEM more inclusive. She particularly enjoys teaching courses related to radiative processes, fluid dynamics, and the interstellar medium. The Cosmic Magnetism & Interstellar Physics group maintains active collaborations across multiple institutions and telescope facilities worldwide, with particular emphasis on developing new data analysis techniques for studying magnetic fields in both galactic and extragalactic contexts.

• Mechanical Engineering
• Robotics
• Materials Science
• +۳ مورد دیگر

Cristina Alén Cordero is an Associate Professor at the University of Alcalá, Department of Signal and Communication Theory. She is affiliated with the TM Tecnologías Mecánicas, Eléctricas y Térmicas research group. Her academic career includes a PhD from Universidad Politécnica de Madrid (2010) with a thesis on market inspection reliability modeling. Her research spans mechanical engineering, robotics, safety engineering, and nuclear materials science. Key areas include advanced mechanical design, ITER-related technologies (optical coatings, diagnostics), and safety assessment in machinery. She has also contributed to educational methodologies in engineering and assistive robotics for mobility. Her recent publications highlight work on stair-climbing wheelchair control systems, radiation-resistant optical materials for ITER, and vibration damping technologies for space applications. She has collaborated on international projects such as ITER diagnostics and safety standards for machinery compliance. Her work integrates experimental and theoretical approaches, addressing challenges in mechanical systems, fusion engineering, and human-centric robotics. Despite no listed awards, her contributions reflect impactful research in applied engineering domains.

• Astronomy
• Astrophysics
• Interstellar Dust
• +۵ مورد دیگر

Karl Gordon is a Visiting Professor at the Department of Physics and Astronomy, Ghent University (Faculty of Sciences). His research focuses on interstellar dust, radiative transfer, and galaxy evolution, with extensive work on dust extinction curves, stochastic heating of dust grains, and computational modeling. Primary Fields: Interstellar Medium, Dust Grain Physics, Infrared Astronomy, Radiative Transfer Recent Article Trends include studies on JWST observations of photodissociation regions, dust-gas interactions in Magellanic Clouds, UVJ diagrams at cosmic noon, and 3D radiative transfer simulations. His collaborations span international teams working on James Webb Space Telescope and Herschel key projects. Notable Contributions Dust extinction curve analysis across multiple wavelengths Gas-dust ratio variations in interstellar medium phases Stochastic heating of dust grains validation Monte Carlo radiative transfer heuristics PAH mass fraction mapping in Magellanic Clouds Technical Affiliations include the James Webb Space Telescope Mid-Infrared Instrument (MIRI) team and Herschel Key Project on Magellanic Clouds. No formal advising roles or grants are explicitly detailed in the provided texts.

Jörg Enderleinمشاهده پروفایل

استاد

• Biophysics
• Single-Molecule Spectroscopy
• Super-Resolution Microscopy
• +۵ مورد دیگر

Prof. Dr. Jörg Enderlein is a Professor of Biophysics at the III. Physics Institute (Biophysics) of the Faculty of Physics at Georg-August-University Göttingen. He holds an Advanced Grant from the European Research Council (ERC) and serves as founding Editor-in-Chief of Biophysical Reports . His research focuses on single-molecule spectroscopy, super-resolution microscopy, and nanooptics/plasmonics. He has held positions at institutions including the University of Regensburg, Forschungszentrum Jülich, and Eberhard Karls University Tübingen. Education: 1981–1986: Physics studies at Ilya Mechnikov University, Odessa 1991: PhD in Physical Chemistry (Humboldt University Berlin) 1996–1997: PostDoc at Los Alamos National Laboratory (USA) 2000: Habilitation in Physical Chemistry (University of Regensburg) Research Interests: Advanced optical microscopy techniques, metal-induced energy transfer (MIET), graphene-based imaging, single-molecule localization microscopy, and applications in biophysical systems. His group develops methods for ultra-high resolution imaging of biological structures at sub-nanometer scales. Key Achievements: ERC Advanced Grant (2021–2026) Heisenberg Fellowship (2001–2006) Georg Märkl Prize (2000) Pioneered Image Scanning Microscopy (ISM) and MIET-based nanoscopy Advising & Grants: Supervised over 15 PhD students and postdocs. Active in funding via DFG, ERC, and international collaborations. His lab hosts visiting scholars from institutions like Harvard and the University of Texas. Labs/Teams: Leads the Biophysics/Complex Systems research group at Göttingen, affiliated with the GGNB (Göttingen Graduate School for Neurosciences, Biophysics, and Molecular Biosciences). Collaborates with microscopy facilities like EMBL Heidelberg and Max Planck Institutes.

Sorokhaibam KHABAمشاهده پروفایل

استادیار

• Lean Production
• Sustainable Supply Chain Management
• Sustainable Operations Management
• +۳ مورد دیگر

Sorokhaibam KHABA is an Assistant Professor of Supply Chain Management and Logistics at EM Normandie since 2024. He holds a PhD in Operations and Supply Chain Management from IIT Dhanbad (2018). His research focuses on Lean Production, Sustainable Supply Chains, Industry 4.0, and operational efficiency in mining industries. He has served in accreditation committees (AACSB, IACBE) and engaged in UN SDG-aligned community programs. Education: PhD (2018) from IIT Dhanbad. Previous roles include Assistant Professorships at Institute of Management Technology Dubai (2019-2024) and Lovely Professional University (2018-2019), plus Visiting Professorships in Mexico and India. He actively participates in academic conferences, presenting on topics like quantum computing in logistics, IoT barriers in SMEs, and 3D printing pricing strategies. Research interests span lean methodologies in mining, sustainable practices, and emerging technologies in supply chains. His articles analyze barriers to lean adoption, IoT implementation challenges, and food waste behavior. He co-authored works on RFID in supply chains, SWOT analysis of coal mining, and ethical green procurement in automobiles. Professional contributions include organizing conferences and publishing in journals like TQM Journal and Benchmarking: An International Journal. He emphasizes bridging theory with practical applications in emerging markets, particularly through community outreach and UN SDG initiatives.

Nicolas Lehnerمشاهده پروفایل

استاد پژوهشی

• Galaxy Formation and Evolution
• Circumgalactic Medium
• Astrophysics
• +۳ مورد دیگر

Nicolas Lehner is a Research Professor in the Department of Physics & Astronomy at the University of Notre Dame. His research focuses on understanding galaxy formation and evolution through multi-wavelength spectroscopy and imaging. He investigates large-scale baryon flows and the circumgalactic medium (CGM) to validate galaxy growth models. Key projects include studies of the Andromeda galaxy’s circumgalactic gas (Project AMIGA), the Large Magellanic Cloud’s (LMC) winds, and the interstellar medium in the Milky Way using the ULLYSES survey. Education: B.Sc., Université Louis Pasteur, France (1994) M.Sc., Université Louis Pasteur, France (1995) Ph.D., Queen’s University Belfast, Northern Ireland (2000) Research Interests: Lehner specializes in the dynamics of circumgalactic gas, galactic winds driven by supernovae, and the interplay between galaxies and their environments. His work bridges observational studies (e.g., HST/COS surveys like KODIAQ and CASBaH) and simulations (e.g., FOGGIE project) to map gas phases, metallicity distributions, and cosmic baryon cycles. Publications Trends: Recent work emphasizes high-redshift CGM metallicity, Milky Way halo interfaces, and Magellanic system dynamics. Collaborations with Howk, Prochaska, and O’Meara dominate, focusing on HI absorption, O VI tracing, and multi-phase gas structure. Awards/Grants: No awards explicitly listed, but active in NSF-funded projects (e.g., KODIAQ Survey). Labs/Teams: Leads the AMIGA project and collaborates on the FOGGIE simulations. Involved in ULLYSES and CASBaH surveys.

• Astronomical Sciences
• Space Sciences
• Particle and High Energy Physics
• +۲ مورد دیگر

Dr. Themiya Nanayakkara is a Research Fellow at the Swinburne University of Technology , associated with the School of Science, Computing and Emerging Technologies. Her research focuses on high-redshift galaxy formation, cosmology, and astrophysical applications of JWST data. Active in galaxy spectral modeling and chemical evolution studies Key participant in the UNCOVER and GLASS-JWST programs Recipient of grants like the Space Data Analysis Workshop for African Researchers (2024) Her recent work analyzes stellar mass gradients , ionizing photon production , and dust distribution in quiescent galaxies using NIRSpec , NIRCam , and ALMA data. Publications demonstrate expertise in galaxy morphology , metallicity calibration , and reionization-era AGN detection . As a Laureate Postdoctoral Research Associate , she develops 3D spectroscopy pipelines for slit-stepping techniques and explores non-parametric star formation histories that challenge traditional models. Her work bridges observational data with cosmological simulations (IllustrisTNG, SHARK) to understand early galaxy quenching mechanisms.

Adam Ginsburgمشاهده پروفایل

دانشیار

• High-mass Star Formation
• Radio and millimeter astronomy
• Molecular Interstellar Medium
• +۳ مورد دیگر

Adam Ginsburg is an Associate Professor and Graduate Coordinator in the Department of Astronomy at the University of Florida, College of Liberal Arts and Sciences. His research focuses on high-mass star formation, radio and millimeter astronomy, and the interstellar medium. He holds a Ph.D. in Astrophysics from the University of Colorado (2013), preceded by an M.S. (2009) and B.S. (2007) from the same university. Prior to UF, he held postdoctoral positions at the European Southern Observatory (2013–2016) and the National Radio Astronomy Observatory (2016–2019). His research interests include turbulence in the interstellar medium, astrochemistry, and the development of astronomical software tools. Recent work emphasizes the Central Molecular Zone (CMZ) and massive protoclusters, utilizing ALMA and JWST data to study star formation dynamics, magnetic fields, and molecular cloud structures. He leads the ALMA-IMF survey and contributes to projects like CASCADE and ACES, advancing understanding of galactic center physics and star formation mechanisms. Ginsburg is also actively involved in software development for observational astronomy, including tools like ndcube and photutils . Notable research trends include 3D structural analysis of the CMZ, magnetic field studies in star-forming regions, and the interplay between turbulence and star formation efficiency. His work bridges observational data with theoretical models, leveraging multi-wavelength observations to address fundamental questions about galactic evolution and stellar birth processes. Grants and collaborations include leadership roles in large-scale surveys and software development initiatives. He advises students through the UF astronomy graduate program and maintains active involvement in departmental governance as Graduate Coordinator.

Luciana Bianchiمشاهده پروفایل

استاد پژوهشی

• Observational Astrophysics
• Hot Stars
• Stellar Populations
• +۳ مورد دیگر

Luciana Bianchi is a Research Professor in the Department of Physics and Astronomy at Johns Hopkins University. She earned her PhD in Astronomy (summa cum laude) from the University of Padua. Her research focuses on massive stars, stellar populations, and galaxy evolution using ultraviolet (UV) space telescopes like GALEX and HST. She co-led the GALEX mission and pioneered the 'UV sky' project, which mapped the UV universe and revealed new insights into hot white dwarfs and stellar formation. Active in international collaborations, she contributed to missions like IUE, FUSE, and UVIT. She is a member of major astronomical societies and has advised numerous young researchers. Her work bridges observational astronomy with technological innovation, emphasizing global scientific cooperation. Education: PhD in Astronomy, University of Padua (1978–1982). Research Interests: Observational astrophysics, hot stars, UV instrumentation, galaxy evolution, and stellar populations. Key Projects: GALEX mission, UV sky project, HST treasury programs, and FUSE collaboration. Awards: 2019 ICCM Montalcini Prize for Science, recognition in Elsevier's Women in Physical Sciences, and featured in the Encyclopedia of Italian Women Scientists. Grants & Advising: Extensive funding from NASA, European Research Council, and national agencies. Mentored a global team ('Dolomiti group') of young researchers. Labs/Teams: Leads the UV sky project team and collaborates internationally on space instrumentation and observational campaigns.

• RFID Technology
• Antenna Design
• Electromagnetics
• +۳ مورد دیگر

Delphine Bechevet is an Associate Professor at the Geneva School of Landscape, Engineering and Architecture, part of HES-SO (University of Applied Sciences and Arts Western Switzerland). She specializes in RFID technology, antenna design, electromagnetics, and printed electronics. Her work focuses on miniaturization of wireless systems for outdoor sports equipment and medical applications, particularly neonatal monitoring. BSc in Computer Science and Communication Systems (HES-SO) MSc in Applied Electromagnetics (HES-SO Master) Her research explores low-cost antenna fabrication using conductive inks on plastics, material characterization for wireless applications, and RFID systems in harsh environments. Recent projects include 3D GPS antennas for sports watches and battery-less temperature sensors via RFID-polymer integration. Scholarly trends show expertise in RFID tag innovation (UHF/microwave frequencies), ultra-wideband antennas, and radiation effects on silicon detectors. She leads projects like UHF RFID tags for livestock tracking while collaborating on medical IoT systems and conference organization (IoT Week 2017). Current projects involve the Conception de tag RFID UHF miniaturisé (2017-2021) as main applicant and the Montre connectée (2020) as co-applicant. Completed initiatives include GPS antenna design for sports watches (2017-2019), the BB-Sensors medical monitoring system (2015-2017), and IoT Week 2017 organization.

• X-ray astronomy
• Supernova remnants
• Neutron stars
• +۴ مورد دیگر

Dr. Sangwook Park is a Professor of Physics at the University of Texas at Arlington, where he has served since 2010, progressing from Assistant Professor to Associate Professor and finally to Professor in 2021. His research focuses on high-energy astrophysics, particularly X-ray observations of supernova remnants, neutron stars, and the interstellar medium. Dr. Park received his PhD in Physics with emphasis in Astrophysics from Purdue University in 1998, followed by postdoctoral work at NASA Goddard Space Flight Center and Pennsylvania State University. His undergraduate degree is in Computer Science from Illinois Institute of Technology (1992), with a minor in Physics. Dr. Park's research centers on observational astronomy using X-ray telescopes to study the aftermath of stellar explosions. His work primarily investigates supernova remnants including SN 1987A, Kepler's SNR, Tycho's SNR, and others in our galaxy and the Magellanic Clouds. Through high-resolution spectroscopy with Chandra and other X-ray observatories, he has made significant contributions to understanding ejecta dynamics, nucleosynthesis, and shock physics in these cosmic laboratories. His research has revealed detailed kinematic structures of supernova ejecta, metal distributions in remnants, and the interaction between supernova shocks and surrounding interstellar material. His work often bridges theoretical models with observational data to refine our understanding of stellar evolution and explosive phenomena. Analysis of Dr. Park's recent publications shows a consistent focus on supernova remnants, particularly SN 1987A, with increasing multi-wavelength approaches combining X-ray, infrared, and radio observations. His work has evolved from basic imaging to sophisticated kinematic and spectral analyses, increasingly incorporating data from newer observatories like JWST alongside traditional X-ray facilities. A notable trend is the detailed study of dust formation and destruction in supernova environments, connecting high-energy processes with the evolution of interstellar material. His research demonstrates a progression from single-observatory studies to complex multi-messenger investigations that provide comprehensive views of supernova remnants. Dr. Park has received numerous prestigious awards and grants throughout his career: Multiple NASA Chandra Guest Observer grants (2004-2024) PI NASA Chandra Multi-Cycle Guest Observer (2021-2023) PI NASA NuSTAR Guest Observer (2017) Faculty Development Leave awards (2017-2018, 2024-2025) Multiple NASA Suzaku and XMM-Newton observation grants Dr. Park has been an active mentor to numerous graduate students, serving as Dissertation Committee Chair for at least eight PhD students and as committee member for many others. His research has been consistently supported by substantial NASA and NSF funding, with recent grants totaling over $500,000 for projects studying supernova remnants like Kepler's SNR and SN 1987A. He has established himself as a leading expert in X-ray studies of supernova remnants, frequently collaborating with international teams and serving on review panels for major observatories. His service includes committee work within his department and university, as well as extensive peer review activities for journals and funding agencies.