جستجوی استاد راهنمای دانشگاهی

Dan McCammonمشاهده پروفایل

استاد

• X-ray Astronomy
• Astrophysics
• Diffuse X-ray Background
• +۵ مورد دیگر

Dan McCammon is a Professor in the Department of Physics at the University of Wisconsin-Madison, affiliated with the College of Letters & Science. His research focuses on X-ray astronomy, including studies of the diffuse X-ray background, interstellar and intergalactic media, and the development of advanced X-ray instrumentation. He is a key contributor to the XRISM (X-ray Imaging and Spectroscopy Mission) satellite, leading efforts in high-resolution X-ray spectroscopy and mission operations. McCammon's work emphasizes understanding cosmic plasma dynamics, galaxy cluster physics, and supernova remnant evolution through cutting-edge observational techniques and detector technology. His research interests span multiple subfields, including the thermodynamic properties of galactic clusters, charge-exchange processes in astrophysical plasmas, and the design of cryogenic microcalorimeters for space-based observatories. He has pioneered advancements in transition-edge sensors (TES) and superconducting detectors, enhancing the precision of X-ray spectral measurements. McCammon has contributed to numerous sounding rocket missions, such as Micro-X, and has been instrumental in the development of the Line Emission Mapper (LEM) probe concept, aimed at mapping the soft X-ray sky with unprecedented resolution. His work on the Hitomi (ASTRO-H) satellite demonstrated breakthroughs in resolving the thermal and dynamic properties of cosmic plasmas, such as the Perseus galaxy cluster and the Crab Nebula. His publications highlight a focus on high-resolution X-ray spectroscopy of cosmic sources, including galaxy clusters, active galactic nuclei, and supernova remnants. He has explored topics like non-thermal pressure contributions in cluster cores, ionized plasma diagnostics, and the role of charge-exchange emissions in interpreting diffuse X-ray backgrounds. McCammon's instrumentation innovations have enabled breakthroughs in measuring spectral features with sub-eV resolution, advancing our understanding of astrophysical processes. Despite the absence of explicitly listed awards or grants in the provided text, his leadership in major space missions and pioneering detector technologies underscores his contributions to the field. His research team collaborates on international projects, such as XRISM and LEM, reflecting a commitment to advancing observational astrophysics through interdisciplinary collaboration.

James Unwinمشاهده پروفایل

دانشیار

• Theoretical Particle Physics
• Astrophysics
• Cosmology
• +۵ مورد دیگر

James Unwin is an Associate Professor in the Department of Physics at the University of Illinois Chicago (UIC), affiliated with the College of Liberal Arts and Sciences. He holds a DPhil in Physics from the University of Oxford (2013) and has held postdoctoral positions at the University of Notre Dame. His research focuses on theoretical particle physics, astrophysics, and cosmology, particularly exploring physics beyond the Standard Model, dark matter models, and interdisciplinary applied mathematics. Current interests include dark matter interactions, primordial black holes, and novel experimental approaches like Coulomb explosion imaging. Research Interests: Dark Matter Models: Including freeze-in mechanisms, annihilation signatures, and cosmological constraints Particle Astrophysics: Supersymmetry, LHC searches, and Grand Unified Theories Interdisciplinary Work: Applications of mathematics to epidemiology (e.g., COVID-19 forecasts via stock market indicators) and social dynamics Recent publications emphasize ultrafast molecular dynamics, XUV spectroscopy, and cosmological impacts of primordial black holes. He has advised PhD students Prolay Chanda and Qingyun Wang, both advanced to candidacy in 2021. Professional activities include visiting roles at UC Berkeley (2022–2023) and a Distinguished Academic Visitor appointment at Queen’s College, Oxford (2023). Affiliations: UIC Department of Physics Adjunct roles at UC Berkeley and University of Oxford Collaborations with institutions like Fermilab and CERN

Alec M. Wodtkeمشاهده پروفایل

استاد

• Surface Chemistry
• Molecular Dynamics
• Energy Conversion at Interfaces
• +۳ مورد دیگر

Alec M. Wodtke serves as Director at the Max Planck Institute for Biophysical Chemistry and holds a Professorship at the University of Göttingen. He leads the Dynamics at Surfaces research group, which employs cutting-edge laser, molecular beam, and ultrahigh vacuum technologies to study molecular interactions at interfaces. His research focuses on understanding the fundamental rules governing energy conversion at molecular interfaces. Wodtke's work bridges macroscopic energy conversion phenomena with molecular-scale processes, investigating how energy transfers occur one molecule and one collision at a time. His group specializes in designing well-defined experiments that capture molecules in the act of reacting, providing benchmark measurements for theoretical advances in surface chemistry. Recent research trends show a strong focus on ultrafast molecular dynamics, with significant contributions to understanding hydrogen-graphene interactions, energy dissipation mechanisms at surfaces, and atomic-scale reaction kinetics. His work has important implications for developing heterogeneous catalysts, photovoltaics, and fuel cell technologies. Alexander von Humboldt Professorship (2011) ERC Synergy Grant worth 12 million euros (2024) Ertl Lecture Prize (2022) Somorjai Visiting Miller Research Professorship Moore Distinguished Scholar at Caltech Wodtke directs multiple project groups including Atom-surface scattering dynamics, Chemical dynamics using ultra-short atom pulses, First-principles simulations of molecule-surface dynamics, and Time-resolved spectroscopy of surface adsorbates. His research team has secured significant funding including Advanced ERC Grants and operates specialized facilities for surface science research.

David A. Hammerمشاهده پروفایل

استاد

• Plasma Physics
• High Energy Density Plasma Physics
• Nuclear Energy Engineering
• +۱۲ مورد دیگر

David A. Hammer is the J. Carlton Ward, Jr., Professor of Nuclear Energy Engineering and Professor of Electrical and Computer Engineering at Cornell University's College of Engineering. He has been a faculty member since 1977 and has held visiting positions at Imperial College London, Applied Materials, Inc., and the Paris Observatory. His work bridges nuclear engineering, plasma physics, and electromagnetics. His research focuses on high energy density plasmas generated by pulsed power systems, particularly through wire explosions, X-pinches, and gas-puff Z-pinches. Key areas include inertial confinement fusion, magneto-Rayleigh-Taylor instabilities, and plasma diagnostics using visible and X-ray spectroscopy, laser-based methods, and electro-optical instruments. He also explores the application of X-pinch radiation for biomedical radiography. His recent publications reveal a strong emphasis on Z-pinch and hybrid X-pinch dynamics, plasma turbulence, magnetic field diagnostics using Faraday rotation and Zeeman splitting, and the development of advanced imaging and spectroscopic techniques. His work frequently involves the COBRA pulsed-power generator and addresses fundamental questions in plasma stability, implosion dynamics, and radiative collapse. Distinguished Career Award, Fusion Power Associates Board of Directors (2018) Cornell College of Engineering Teaching Award (2006, 1998) Cornell IEEE Professor of the Year Award (2006) McCormack Advising Award (2005) IEEE Plasma Science and Applications Committee Award (2004) Hammer has advised numerous graduate students and led experimental campaigns involving plasma diagnostics, liner implosions, and laboratory astrophysics. His work is supported by grants from agencies interested in fusion energy, plasma science, and advanced diagnostics. He has developed innovative platforms, including 3D-printed plasma loads, to study turbulent plasma jets and magnetization. His lab at Cornell is a key facility for high-energy-density plasma research. He leads a research group focused on plasma diagnostics and pulsed power experiments, operating the COBRA generator and developing novel measurement techniques. His team investigates plasma instabilities, magnetic field generation, and the transition from radial implosions to collimated jets, with implications for both fusion and astrophysics.

• Cosmochemistry
• Presolar Grains
• Nucleosynthesis
• +۴ مورد دیگر

Sachiko Amari serves as a Research Professor of Physics in the Department of Physics at Washington University in St. Louis, where she conducts pioneering research in cosmochemistry through the McDonnell Center for the Space Sciences. Her work bridges laboratory astrophysics and planetary science, focusing on extraterrestrial materials to unravel solar system formation and stellar processes. Amari's educational foundation includes a PhD from Kobe University and both Master of Engineering and Bachelor of Engineering degrees from Waseda University in Japan. This engineering background informs her precise analytical approach to meteoritic materials. Her research centers on presolar grains—stardust formed in stellar outflows that were incorporated into primitive meteorites. Using secondary ion mass spectrometry, she analyzes isotopic ratios to investigate nucleosynthesis in stars, mixing processes in stellar ejecta, and Galactic chemical evolution. A secondary focus examines noble gas trapping mechanisms in meteorites to understand volatile origins and early solar system processes. Her work reveals how microscopic grains preserve macroscopic cosmic histories. Analysis of her recent publications shows consistent emphasis on silicon carbide and graphite presolar grains, with increasing technical sophistication in NanoSIMS analysis. Research trends include correlating multi-element isotopic systems, identifying rare stellar sources like novae, and resolving phase Q—the elusive noble gas carrier in meteorites. Her work demonstrates how laboratory studies of individual grains constrain astrophysical models. Amari leads an active research group within the McDonnell Center for the Space Sciences and collaborates on major initiatives including the Mars Sample Return Science Definition Team. She mentors graduate students in meteoritics research while developing analytical protocols for extraterrestrial material characterization. Her laboratory serves as a hub for stardust analysis, utilizing advanced mass spectrometry techniques to decode isotopic fingerprints of stellar processes.

• AGN
• Galaxy surveys
• Radio interferometry
• +۴ مورد دیگر

Professor Leah Morabito is a Professor (Research) - UKRI Future Leaders Fellow at Durham University, affiliated with the Department of Physics and the Institute for Computational Cosmology. She specializes in high-resolution imaging at low frequencies using the LOFAR telescope to study how supermassive black holes co-evolve with their host galaxies. As leader of the LOFAR Imaging of Resolved AGN (LIRA) group, she has made significant contributions to our understanding of active galactic nuclei and galaxy evolution through numerous high-impact publications. Professor Morabito's research primarily focuses on AGN physics, galaxy surveys, and radio interferometry. She has pioneered techniques for sub-arcsecond imaging at low radio frequencies, which has opened new windows for studying radio jets, galaxy evolution, and the interstellar medium. Her work reveals critical insights about AGN feedback mechanisms and the connection between supermassive black holes and their host galaxies across cosmic time. The analysis of her recent publications shows a strong emphasis on utilizing LOFAR's unique capabilities to study radio sources with unprecedented resolution at low frequencies. Scientific Recognition: UKRI Future Leaders Fellowship Professor Morabito actively mentors the next generation of astronomers, currently supervising PhD students Benite Tantely, Ciera Sargent, and Emmy Escott. Her research is supported by significant funding through her UKRI Future Leaders Fellowship and her role as co-Principal Investigator of the new LOFAR2.0 Large Programme, which extends her work on high-resolution low-frequency radio surveys. She has secured substantial research funding that enables cutting-edge observations and supports her research team. As leader of the LOFAR Imaging of Resolved AGN (LIRA) group, Professor Morabito oversees a collaborative research effort focused on advancing our understanding of how AGN help shape galaxy evolution. Her team utilizes unique high-resolution, low-frequency observations to study radio jets, AGN feedback mechanisms, and the connection between supermassive black holes and their host galaxies, contributing significantly to one of the most fundamental questions in modern astrophysics.

Martin Reyمشاهده پروفایل

مدرس

• Astrophysics
• Theoretical Astrophysics
• Galaxy Formation
• +۶ 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).

Daniel M. Scolnicمشاهده پروفایل

دانشیار

• Cosmology
• Supernovae
• Dark Energy
• +۳ مورد دیگر

Daniel M. Scolnic is an Associate Professor of Physics at Duke University's Trinity College of Arts & Sciences and holds a joint appointment in the Department of Electrical and Computer Engineering at the Pratt School of Engineering. His research focuses on cosmology, particularly using Type Ia supernovae and near-infrared observations to probe dark energy and resolve the Hubble tension. Ph.D. (2013), Johns Hopkins University B.S. (2007), Massachusetts Institute of Technology As a leading figure in supernova cosmology, Scolnic works on refining the cosmic distance ladder, studying time-evolving dark energy, and analyzing systematic uncertainties in cosmological measurements. His work leverages data from the Dark Energy Survey (DES), Pantheon+ collaboration, and James Webb Space Telescope (JWST) to address discrepancies in the Hubble constant (H₀) derived from early- and late-universe observations. His recent publications highlight advancements in inverse distance ladder techniques, host galaxy dust modeling, and the role of photometric redshifts in cosmological analyses. Notably, his team's JAGB 2.0 study improves Hubble constant constraints using JWST. Defense Science Study Group (DSSG) Clarivate Most Highly Cited Scientists Fred Kavli Plenary Lectureship Sloan Research Fellowship in Physics Department of Energy Early Career Award Packard Fellowship Scolnic leads major grants from NASA, the Packard Foundation, and the Department of Energy, including a NASA Roman Project Infrastructure Team grant (2023-2028) and a Packard Fellowship (2019-2027) to investigate cosmological tensions. He actively collaborates with the Duke Cosmology Group and contributes to the Nancy Grace Roman Space Telescope's High-Latitude Time-Domain Survey.

Daniel Apaiمشاهده پروفایل

استاد

• Exoplanet science
• Brown dwarf atmospheres
• Space telescopes
• +۳ مورد دیگر

Daniel Apai is Professor of Optical Sciences and Professor of Astronomy & Planetary Sciences at the University of Arizona, where he also serves as Associate Dean for Research in the College of Science. His core appointments span the Department of Optical Sciences and the Department of Astronomy & Planetary Sciences, reflecting a dual expertise in instrumentation and astrophysical research. He earned a MSc from the University of Szeged, Hungary (2000) and a PhD from the University of Heidelberg, Germany (2004). Research Interests Space telescopes and next-generation instrumentation Infrared spectroscopy of exoplanets and brown dwarfs Habitability assessment of terrestrial and sub-stellar worlds Atmospheric dynamics and weather patterns in ultracool atmospheres Advanced optical systems including multi-order diffractive Fresnel lenses Across his 2022–2025 publication record, Apai’s work reveals a consistent focus on leveraging JWST, HST, and forthcoming missions such as NASA’s Pandora SmallSat to characterize exoplanet atmospheres, map brown-dwarf weather, and refine habitability metrics. Studies span from detecting the faintest brown dwarfs in globular clusters to building quantitative frameworks for biosignature assessment, illustrating a trajectory that couples cutting-edge observations with theoretical modeling. Awards & Honors No specific awards are listed in the provided text; the narrative is limited to appointments and scholarly output. Students & Grants The supplied text does not enumerate graduate students or funding details. Laboratories & Teams While no formal lab names are given, Apai’s leadership in space-telescope instrumentation and participation in large JWST and HST programs suggest active involvement in multi-institutional collaborations centered on exoplanet characterization and infrared instrumentation development.

• Astronomical Sciences
• Space Sciences
• Particle and High Energy Physics
• +۳ مورد دیگر

Assoc Prof Ivo Labbe is an Associate Professor and ARC Future Fellow at Swinburne University of Technology's School of Science, Computing and Emerging Technologies. His research focuses on galaxy formation and evolution, particularly at high redshifts, leveraging JWST observations to study quiescent galaxies, active galactic nuclei (AGN), and cosmic reionization. He leads the UNCOVER Treasury Survey, analyzing over 700 galaxies using JWST/NIRSpec and NIRCam data. His work includes uncovering reddening in cosmic noon galaxies, AGN contributions to reionization, and the discovery of ultra-massive spiral galaxies at z ~5.2. Labbe has secured ARC grants totaling $A millions to study first stars/galaxies and dark matter via microlensing. He supervises PhD students on topics like primordial black holes and early galaxy evolution. His team's findings challenge traditional models of galaxy growth and shed light on early Universe processes. Education: Not explicitly stated in text. Grants: ARC Future Fellowship funding (2023–2027). "Unveiling the Dead and Dusty Universe with JWST" (2023–2026). "Uncovering the First Stars and Galaxies with JWST" (2023–2027). Awards: ARC Future Fellow. Key Projects: UNCOVER Survey: Explores high-redshift galaxies via JWST spectroscopy. PANORAMIC Survey: Unveils galaxy structures in early Universe. FRESCO Survey: Maps Hα emission in z>5 galaxies. Research Themes: Cosmic Dawn, Galaxy Quenching, AGN Feedback, Dust Extinction, Gravitational Lensing. Labbe's work bridges observational astrophysics with theoretical modeling, emphasizing spatially resolved studies of galaxy components. His teams collaborate globally, using cutting-edge facilities like JWST and ALMA to probe galaxy evolution across cosmic time.

Kevin Linمشاهده پروفایل

دانشیار

• Astronomy
• Astrophysics
• Cosmology
• +۳ مورد دیگر

Kevin Lin serves as an Associate Professor in the Department of Mathematics at the University of Arizona, where he bridges mathematical rigor with cutting-edge astrophysical research. His work centers on observational cosmology using James Webb Space Telescope (JWST) data, particularly through the JADES (JWST Advanced Deep Extragalactic Survey) collaboration, focusing on galaxy formation during the universe's first billion years. Dr. Lin's research spans redshifts z>3 to beyond z=14, probing the epoch of reionization and the properties of primordial galaxies. His primary research interests encompass high-redshift galaxy evolution, chemical enrichment processes in the early universe, and the physical mechanisms driving star formation and black hole growth. Lin specializes in analyzing multi-wavelength JWST data (NIRCam, NIRSpec, MIRI) to study stellar populations, nebular emission, and gas dynamics in galaxies at cosmic dawn. Key areas include the star-forming main sequence at z>3, metallicity evolution in infant galaxies, and the nature of obscured active galactic nuclei during reionization. His methodology integrates advanced statistical techniques with deep field spectroscopy to constrain galaxy assembly histories. Analysis of Lin's 15 most recent publications reveals a concentrated research trajectory centered on JADES survey results, with 100% of 2024-2025 output examining z>5 galaxies. Dominant themes include the discovery and characterization of 'Little Red Dots' (LRDs), metal enrichment signatures at z>10, and Lyman-alpha emitter properties during reionization. His work consistently leverages JWST's unprecedented resolution to dissect galaxy morphologies, stellar masses, and ionized gas kinematics in the high-redshift universe, with particular emphasis on JWST instrument capabilities and survey methodologies. As an active JADES collaboration member, Lin contributes to major international efforts mapping cosmic structure formation. His work interfaces with complementary surveys including BlackTHUNDER and SAPPHIRES, focusing on transient phenomena and emission-line galaxies. Current research directions involve resolving the stellar components of z>10 galaxies and investigating the connection between AGN activity and host galaxy evolution during cosmic noon.

• Galaxy Formation and Evolution
• Black Holes
• Active Galactic Nuclei (AGN)
• +۶ مورد دیگر

Erin Hicks, Ph.D., is Chair and Professor in the Department of Physics & Astronomy at the University of Alaska. She holds a Ph.D. in Astronomy & Astrophysics from the University of California, Los Angeles (2006), an M.S. in Astronomy & Astrophysics (2001), and a B.S. in Physics with minors in Astronomy and Mathematics from Washington State University (1999). Education: Ph.D., Astronomy & Astrophysics, UCLA, 2006 M.S., Astronomy & Astrophysics, UCLA, 2001 B.S., Physics, Washington State University, 1999 Her research focuses on galaxy formation and evolution, particularly the roles of black holes and active galactic nuclei (AGN) in shaping galaxy dynamics. Key interests include AGN feedback mechanisms, high-redshift galaxy properties, and observational techniques like adaptive optics and integral field spectroscopy. Her work integrates n-body simulations to model galaxy evolution. Publications highlight studies on molecular inflows/outflows in AGN, kinematics of high-redshift galaxies, and the interplay between star formation and AGN activity. Recent work emphasizes spatially resolved observations of gas dynamics in distant galaxies. No scientific awards were explicitly mentioned. She advises no listed students and has no noted lab affiliations. Career highlights include postdoctoral fellowships at the University of Washington and the Max Planck Institute for Extraterrestrial Physics.

Christopher S. Mooreمشاهده پروفایل

استاد

• Solar Physics
• Stellar Astrophysics
• Space Instrumentation
• +۵ مورد دیگر

Christopher S. Moore is a Professor of Astrophysical and Planetary Sciences at the University of Colorado Boulder, affiliated with the Center for Astrophysics and Space Astronomy (CASA) and the Laboratory for Atmospheric and Space Physics (LASP). His research focuses on solar atmospheres, magnetic cycles, and the development of advanced space instrumentation, including CubeSat missions like MinXSS. He leads investigations into coronal heating mechanisms, solar flare dynamics, and the energy budget of eruptive events. Moore has pioneered innovations in UV coatings for space telescopes and contributed to the design of multi-wavelength observatories such as SSAXI-Rocket and ECCCO. Awarded the IAU PhD Prize (2017) and AAS Rodger Doxsey Travel Prize (2018) Principal Investigator for MinXSS CubeSat missions and co-author of over 50 peer-reviewed articles Co-developed the Marshall Grazing Incidence X-ray Spectrometer and Wolter-I X-ray optics His work integrates observational data from satellites (e.g., RHESSI, Hinode) with numerical simulations to address fundamental questions in solar physics. Moore has advised multiple undergraduate researchers and mentored teams in NASA-funded projects, emphasizing STEM diversity through initiatives like the Black Student Alliance and NASA Student Ambassador programs.

Casey Papovichمشاهده پروفایل

استاد

• Observational Cosmology
• Galaxy Evolution
• Large-Scale Structure of Galaxies
• +۳ مورد دیگر

Casey Papovich is a Professor of Physics and Astronomy at Texas A&M University, holding the Marsha L. '69 and Ralph F. Schilling '68 Chair in Physics and Astronomy. He is a Fellow of the American Physical Society and affiliated with the Mitchell Institute for Fundamental Physics & Astronomy. Education: PhD in Physics from Johns Hopkins University (2002), BS in Physics from College of William and Mary (1995). His research focuses on observational cosmology, galaxy evolution, and large-scale structures. He uses data from NASA's Great Observatories (Hubble, Spitzer, Chandra) and telescopes like Gemini, Magellan, Keck, and ALMA. Key projects include GMACS, ZFOURGE, CANDELS, and CEERS. Recent work emphasizes early galaxy formation, reionization constraints, and dark matter studies via satellite galaxies. He is involved in JWST programs like CEERS and NGDEEP, exploring high-redshift galaxies and their properties. Major awards include the APS Fellowship and the Schilling Chair. His grants and collaborations span international projects, including HETDEX and Dark Energy Survey. Labs/Teams: Mitchell Institute for Fundamental Physics & Astronomy, Giant Magellan Telescope (GMT) project (GMACS role), and multiple international collaborations (e.g., ZFOURGE, CANDELS). Publications span over 200 articles in leading journals, with recent emphasis on JWST-era studies, metallicity gradients, AGN feedback, and early-universe galaxy properties.

Matthew Hayesمشاهده پروفایل

دانشیار

• Galaxy Formation and Evolution
• Cosmic Reionization
• Interstellar Medium (ISM)
• +۴ مورد دیگر

Matthew Hayes is an Associate Professor in Astrophysics at Stockholm University 's Department of Astronomy and a Wallenberg Academy Fellow. His research focuses on the formation and evolution of galaxies, particularly during the reionization epoch, using multi-wavelength observations (JWST, Hubble, ESO) and computational modeling. Research Pillars: Cosmic reionization, Lyman-alpha emission physics, stellar feedback mechanisms, circumgalactic medium properties, and diagnostics of ionizing radiation Key Instruments: James Webb Space Telescope, Hubble Space Telescope, VLT/MUSE, Nordic Optical Telescope His recent work uses UV spectral diagnostics to trace the ionization state of the intergalactic medium and constrain the escape fraction of Lyman continuum photons. Current teaching includes graduate-level courses on the Physics of the Interstellar Medium (AS7001) and Observational Techniques in Astrophysics II (AS7004) featuring hands-on radio/optical observations. Scientific Contributions: Developed novel methods for measuring ionized bubble sizes around high-redshift galaxies Advanced understanding of Lyman-alpha as a probe for galactic winds and outflows Calibrated UV diagnostic tools for metallicity and ionization parameters in the JWST era Funding Sources: Swedish Research Council, Knut and Alice Wallenberg Foundation, Swedish National Space Board