Dr. Brandon Marshall serves as an Assistant Professor in the Department of Physics and Astronomy at the University of Nebraska at Kearney (UNK), a position he assumed in 2019. His academic focus lies in observational infrared astronomy, particularly the formation and evolution of high-mass stars and their interactions with the interstellar medium. His educational qualifications include: Ph.D. in Astronomy (2018) from Iowa State University B.Sc. in Physics (2012) from Western Michigan University Dr. Marshall's research centers on high-mass star formation, with specific interest in accretion disks and their role in the development of young stellar objects. He employs infrared observational techniques to study the impact of massive stars on surrounding molecular clouds and star-forming regions, contributing to our understanding of the lifecycle of stars in dense environments. His recent scholarly output examines molecular clouds associated with HII regions, the spectral characteristics of Herbig Oe stars, and Lyman excess in HII regions. These works demonstrate a consistent emphasis on observational astrophysics, particularly in the context of massive star formation and interstellar processes. No scientific awards are listed in the provided information. Details regarding graduate student mentorship and external research funding are not specified in the available text. Information about specific laboratories or research teams directed by Dr. Marshall is not included in the current profile.
Marina Kounkel is an Assistant Professor in the Physics and Astronomy Department at the University of North Florida. Her research focuses on observing dynamics of young stars and investigating the clumpy process of star formation across various scales, from individual stellar systems to the distribution of star-forming regions across the Milky Way Galaxy. Dr. Kounkel's research interests include stellar kinematics, star formation processes, Galactic astronomy, and the analysis of large astronomical surveys. She utilizes data from the Gaia space telescope (measuring positions of over 1.6 billion stars) and spectroscopic surveys like SDSS-V APOGEE to identify kinematically coherent groups of stars that likely formed together from the same molecular cloud. Her work aims to reconstruct the initial conditions that influenced star formation, including events like supernovae, cloud-cloud collisions, and gravitational feedback. Her research program examines how star-forming structures have formed, how they will evolve over time, and what fundamental properties can be inferred from stellar kinematics. She emphasizes the importance of better understanding stellar properties (masses, radii, temperature, rotation rate, magnetic activity) as these parameters allow for more precise age determinations, which in turn enable reconstructions of Galactic history. Featured as cover of 'Sound of Interstellar Space' music album by TRIFID Dr. Kounkel has developed interactive visualization tools for exploring stellar structures, including 2D projections, HR diagrams, and 3D maps of moving groups. She continues to advance our understanding of Galactic archaeology through careful analysis of stellar ages and motions.
Bryan M Gaensler is the Dean of the Science Division at the University of California, Santa Cruz (UCSC), and holds a professorship in the Department of Astronomy and Astrophysics. His career includes roles as Harvard University’s associate professor, Canada Research Chair at the University of Toronto, and director of the Dunlap Institute for Astronomy and Astrophysics. He specializes in cosmic magnetism, time-domain astrophysics, and interstellar gas dynamics. Education: Undergraduate/graduate degrees from The University of Sydney and CSIRO’s Australia Telescope National Facility. Postdoctoral work at MIT and Smithsonian Astrophysical Observatory. Research focuses on the Polarisation Sky Survey of the Universe's Magnetism (POSSUM), using ASKAP to study magnetic fields via Faraday rotation. He also studies Fast Radio Bursts (FRBs) as part of the CHIME/FRB team. His work bridges instrumentation (e.g., SKA prototypes) and theoretical astrophysics. Key awards include Australian Laureate Fellow, ARC Federation Fellow, and Scopus Young Researcher Award. He has authored over 80 publications and co-edited works on cosmic magnetism and astrophysics strategy. Labs/Teams: Leads the B-Force team, POSSUM collaboration, and CHIME/FRB group. Advocates for equity in science and public outreach through books like Extreme Cosmos and media engagements.
Edwin A. Bergin is Professor of Astrophysics and Chair of the Department of Astronomy at the University of Michigan, within the College of Literature, Science, and the Arts. He is a leading researcher in the fields of star and planet formation, interstellar chemistry, and astrobiology. His educational background includes a BS from Villanova University and a PhD from the University of Massachusetts. He previously worked as an astronomer at the Harvard-Smithsonian Center for Astrophysics before joining the University of Michigan. Bergin’s research focuses on the molecular origins of life, particularly the chemistry of water and organic molecules in space. He uses observational and theoretical methods to study how these molecules form and evolve from interstellar clouds to planetary systems. His work has significantly advanced our understanding of how Earth acquired its water and carbon, with implications for the potential habitability of exoplanets. His recent publications reflect a strong emphasis on protoplanetary disk chemistry, molecular detection using facilities like ALMA and Herschel, and the interplay between stellar radiation and disk chemistry. Themes include water vapor in habitable zones, carbon processing, and the chemical evolution of planet-forming regions. U-M Henry Russel Award for exceptional scholarship and teaching Bergin has advised several graduate students, including Jeffrey Fogel and Nathan Crockett. He has led major research initiatives such as HEXOS and utilizes advanced observational tools like ALMA and SOFIA. He teaches a range of courses from introductory astronomy to graduate-level astrophysics of the interstellar medium. He is affiliated with the Michigan Institute for Research in Astrophysics and conducts research through observational campaigns, theoretical modeling, and interdisciplinary collaboration with geochemists to understand planetary composition and evolution.
Stephen Chi Yung Ng is an Associate Professor in the Department of Physics at The University of Hong Kong's Faculty of Science. His office is located in Room 517 of the Chong Yuet Ming Physics Building. He has been actively teaching undergraduate and graduate courses in astrophysics, including Stellar Physics, Advanced Astrophysics, and Astronomy Laboratory courses from 2018-2022. B.Sc. (1st class honors) in Maths/Physics, The University of Hong Kong (1996-1999) M.Phil. in Physics, The University of Hong Kong (1999-2001) Ph.D. in Physics, Stanford University (2001-2006) Professor Ng is a high energy astrophysicist specializing in radio and X-ray observations of neutron stars, pulsar wind nebulae, and supernova remnants. His research focuses on understanding these extreme objects as laboratories for physics under conditions unattainable on Earth. He studies the remarkable properties of neutron stars, which are ultra-dense objects with masses greater than the Sun but smaller than a city, rotating rapidly with the strongest magnetic fields in the Universe. His recent publications reveal a strong focus on X-ray polarimetry using missions like IXPE to study magnetic field structures in pulsar wind nebulae and supernova remnants. His work also examines particle acceleration mechanisms and the physics of neutron stars in various environments, including galactic centers and binary systems. Early Career Award: University Grants Committee (2013) Professor Ng has supervised numerous research students, including 7 PhD candidates and 3 MPhil students. He has secured significant research funding as Principal Investigator for 11 projects since 2013, with recent grants including 'Unveiling the Nature of PeVatron' (2023) and 'Exploratory Study of the Impact of Artificial Light at Night on Birds at Mai Po Nature Reserve' (2022). He also serves as Co-Investigator on projects studying high-energy emission from pulsars. He is an active member of several professional societies including the American Astronomical Society and multiple satellite mission science working groups, demonstrating his leadership in the international high-energy astrophysics community.
Jorma Harju serves as a Docent (Adjunct Professor) in the Department of Physics at the University of Helsinki, specializing in observational astronomy and space science. His research centers on interstellar molecular clouds and the initial conditions of star formation, utilizing advanced radio telescopes including ALMA and ESO facilities. Harju's primary research focuses on physical and chemical processes in pre-stellar cores, with particular expertise in nuclear spin ratios of deuterated molecules, cosmic-ray ionization rates, and molecular depletion patterns. His work bridges molecular astrophysics and star formation theory through high-precision radio observations of regions like L1544 and Ophiuchus, revealing critical insights into deuterium fractionation and core evolution. Analysis of his recent publications (2023-2025) shows consistent emphasis on observational studies of prestellar environments using molecular tracers like ammonia and deuterated species. His research increasingly incorporates international collaborations and interdisciplinary approaches, as evidenced by his work on Near-Earth Object radar systems alongside traditional astrophysics. Harju actively mentors the next generation of scientists, having supervised 6 doctoral theses and 3 Master's/Licentiate theses. His research is supported by significant projects including the ERC Advanced Grant SAEMPL (2013-2018), NEO-RADAR (2020-2021), and two long-term investigations into star formation stages (2007-2009 and 2010-2013). He maintains extensive international engagement through 17 academic visits to institutions like the Max Planck Institute for Extraterrestrial Physics (2015-2017), membership in the Space Research Advisory Committee (2016-2019), and participation in ALMA review committees. His 56 recorded activities include conference organization, peer review, and committee service across European astronomy networks.
Marianne Vestergaard is a Professor at the Niels Bohr Institute, University of Copenhagen, specifically affiliated with the Dark Cosmology Centre (DARK). She has been a faculty member since returning to the University of Copenhagen in 2009 as a Freja Fellow. Her research focuses on distant, young galaxies called quasars, particularly studying the physics of supermassive black holes at their centers. Dr. Vestergaard earned her PhD in Astrophysics from the Niels Bohr Institute in 1999 with a dissertation titled "Are Radio-loud Quasars Rebellious or Are Radio-quiets Just Plain Untalented? A Study of the Ultraviolet Broad Emission Line Profiles in High-Redshift Radio-loud and Radio-quiet Quasars." Prior to her PhD, she completed her Master of Science at the University of Copenhagen in 1992. She conducted research at the Harvard-Smithsonian Center for Astrophysics during her PhD studies and subsequently worked at Ohio State University, University of Arizona, and Tufts University before returning to Copenhagen. Marianne Vestergaard's primary research interest is in the physics of distant, young galaxies called quasars. These objects emit powerful radiation due to material falling onto supermassive black holes at the centers of galaxies. She specializes in determining the mass of these black holes and investigating how the powerful energy emission from the central active nucleus affects their surroundings. Her work employs a wide array of telescopes both in space and on Earth, sensitive to X-ray, ultraviolet, visible, infrared, sub-millimeter and radio radiation. Recently, she has utilized data from the Very Large Telescope at the European Southern Observatory in Chile, Atacama Pathfinder Experiment (APEX), Atacama Large Millimeter Array (ALMA), Hubble Space Telescope, and Swift X-ray and UV-optical telescope. Analysis of Dr. Vestergaard's recent publications (2024-2025) reveals a strong focus on active galactic nuclei (AGN) physics, particularly through the AGN STORM 2 project. Her work examines accretion disk dynamics, black hole mass measurements, reverberation mapping techniques, and the relationship between central black holes and their host galaxies. She frequently collaborates on multi-wavelength observational campaigns, combining data from X-ray through radio wavelengths to build comprehensive models of AGN structure and behavior. A significant portion of her recent work involves studying specific AGN like Mrk 817 and NGC 7469 to understand accretion physics in detail. Året Harald (2016) KIF (Women in Physics) Honorary Award (2024) Jens Martin Prisen (2015) Dr. Vestergaard has been actively involved in numerous international collaborations and research projects throughout her career. Her work has generated significant interest in the scientific community, with her publications being referenced by multiple news outlets, blogged about, and shared across social media platforms. She has participated in public outreach activities, giving lectures at institutions like Folkeuniversitetet in Aarhus and Copenhagen on topics including "Giant black holes, quasars and baby galaxies." Her research has been featured in media outlets such as Videnskabernes Verden ("World of the Sciences"). As a member of the Dark Cosmology Centre at the Niels Bohr Institute, Dr. Vestergaard is part of a research environment dedicated to understanding the dark components of the universe - dark matter and dark energy. The center combines observational, theoretical, and computational approaches to cosmological research, with particular strengths in high-redshift astronomy, galaxy formation and evolution, and the physics of active galactic nuclei.
Antonella Palmese is an Assistant Professor in the Department of Physics at Carnegie Mellon University's Mellon College of Science. She specializes in observational cosmology, gravitational wave astronomy, and galaxy evolution, with affiliations to the Dark Energy Survey (DES), Dark Energy Spectroscopic Instrument (DESI), Laser Interferometer Space Antenna (LISA), Rubin Observatory Legacy Survey of Space and Time (LSST), and the Cosmic Explorer Consortium. Her research leverages galaxy surveys and gravitational wave data to study cosmic dynamics, dark energy, and the formation of compact object binaries. Ph.D., University College London (2018) M.Sc. and B.Sc., La Sapienza University of Rome (2013, 2011) Previous roles: NASA Einstein Fellow at UC Berkeley (2021–2022), Postdoctoral Research Associate at Fermilab (2018–2021), Associate Fellow at the University of Chicago (2019–2021) Her research lies at the intersection of gravitational wave experiments , large galaxy surveys , and time domain astronomy . Key projects include standard siren cosmology, GW follow-up with DECam, and galaxy cluster studies. She leads or co-leads initiatives like the DESI Transients and Low-redshift Cosmology Working Group, the GW-MMADS survey, and the DESIRT project. Recent publications focus on gravitational wave cosmology (e.g., Hubble constant measurements), binary black hole mass distributions , AGN flare correlations , and dust attenuation in galaxies . Her work integrates data from LIGO/Virgo runs, DES, DESI, and LSST to address fundamental cosmological questions. 2022 : Leonardo Da Vinci Award for Physics, Math, and Engineering 2021 : NASA Einstein Fellowship 2020 : Fermilab Exceptional Performance Recognition Award 2019 : Royal Astronomical Society Michael Penston Prize runner-up 2014 : Enrico Persico award Antonella uses facilities like the Dark Energy Camera (DECam) and contributes to multi-messenger astronomy by linking gravitational waves to electromagnetic transients. Her extracurricular interests include beach volleyball, crossfit, and visual arts.
Bethany Rigby is a Lecturer in Design at Goldsmiths, University of London, with a focus on speculative practices that interrogate relationships between technology, environment, and extraterrestrial landscapes. Position: Lecturer in Design Department: Design, Goldsmiths, University of London Her research interests include: Speculative design projects exploring space mining and terraforming Art-science collaborations examining planetary environments Science fiction narratives as design methodology Critical engagement with extractive industries in space exploration Recent projects include: Martian Golf Ball (2022): Speculative object critiquing interplanetary elitism Mining The Skies (2023): Sculptural display of extraterrestrial mining samples At Sea (2023): Film capturing St Kilda residency's embodied maritime experience Deep Sea Range 1 and 2 (2023): Military radar infrastructure in Hebrides landscapes Navigation Plaque (2023): Sea chart-inspired interstellar wayfinding artwork She collaborates on initiatives like the Design Department Buffets (DDB) seminar series (2024) with colleagues Soomi Park, Katherine May, and Agatha Haines.
Renaud Toussaint is a Professor at the University of Oslo , affiliated with the Department of Physics within the Faculty of Mathematics and Natural Sciences . He leads research in the Porous Media Laboratory SFF , focusing on granular flows, geophysical phenomena, and fluid dynamics in disordered systems. His research interests include: Granular flow dynamics and seismic signal generation Porous media drainage and multiphase flow instabilities Earthquake mechanics and soil liquefaction Interstellar object modeling (e.g., 'Oumuamua) Fracture mechanics and thermal dissipation in materials Recent work emphasizes experimental and computational studies of granular media, with key contributions on drainage dynamics, seismic proxies for flow behavior, and interfacial fracture mechanics. Collaborations with institutions like the University of Oslo and international researchers highlight his interdisciplinary approach. Publications span Physical Review Letters , Nature Communications , and Journal of Geophysical Research , reflecting his impact in physics and geophysics. No awards or advisory roles are explicitly listed in the provided text.
Dr. Sandra De Jesus Raimundo is a Lecturer in Astronomy at the University of Southampton's Department of Physics and Astronomy, where she conducts cutting-edge research on supermassive black holes and active galactic nuclei. She is a member of the Southampton Theory Astrophysics and Gravity (STAG) Research Centre and actively supervises multiple PhD students while teaching undergraduate physics courses including PHYS1005 and PHYS1201. Her research focuses on understanding the complex relationship between supermassive black holes and their host galaxies, with particular expertise in changing-look AGNs and tidal disruption events. Dr. Raimundo employs multi-wavelength observations and theoretical modeling to investigate how black holes accrete material and influence galactic evolution across cosmic time. Her work bridges observational astronomy with theoretical astrophysics to unravel the mysteries of galaxy-black hole co-evolution. Analysis of her recent publication record (2023-2025) reveals a strong emphasis on active galactic nuclei variability, black hole fueling mechanisms, and transient phenomena in galactic nuclei. Her research spans observational studies of specific objects like Mrk 590 and NGC 5806, as well as broader investigations into AGN populations in dwarf galaxies and the effects of fresh gas on nuclear activity. She frequently collaborates on major observational campaigns and contributes to the development of new astronomical methodologies. Dr. Raimundo is an active member of the astronomical community, contributing to significant projects like the AtLAST science initiative. Her work appears regularly in top-tier journals including The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society. As an educator, she holds Fellowship of the Higher Education Academy and is currently accepting new PhD students interested in black hole astrophysics and galaxy evolution. Her research group investigates the dynamic processes at the centers of galaxies, utilizing data from major observational facilities to advance our understanding of cosmic structure formation.
Gregory Dobler is an Associate Professor in the Department of Physics & Astronomy at the University of Delaware, part of the College of Arts & Sciences. He joined UD in 2019. His research bridges astrophysics and urban science, leveraging machine learning and data science to explore topics such as interstellar medium physics, particle dark matter, strong gravitational lensing, and urban energy dynamics. Dobler holds a B.S. from Haverford College and a Ph.D. from the University of Pennsylvania. His work spans innovative applications of AI in astronomy, including automated detection of light echoes and transient phenomena, while also advancing urban studies through hyperspectral imaging of vegetation health, air quality monitoring, and magnetic field analysis of cities. Notable contributions include the development of the Urban Observatory platform for multiscale urban systems analysis and the Multi-city Urban Observatory Network. Recent research trends emphasize interdisciplinary approaches, integrating deep learning with environmental sensing to address urban challenges like energy consumption and public health. His publications highlight collaborations across fields such as remote sensing, climate science, and smart city technologies. Dobler’s lab focuses on creating novel imaging systems and algorithmic frameworks to study complex systems, from galactic structures to urban infrastructure dynamics.
Henrik Beuther is an Associate Professor at the University of Heidelberg and research scientist at the Max Planck Institute for Astronomy, focusing on Planet and Star Formation. He holds a PhD from Max Planck Institute for Radioastronomy and was an Emmy-Noether Fellow at Harvard-Smithsonian CfA. Research Focus: His group studies high-mass star formation using millimeter interferometry (ALMA/NOEMA) and JWST. Projects include CORE (fragmentation/disk formation), THOR (Galactic HI/OH survey), and RIMORPHIS (river morphology informatics). Publication Trends: Recent work explores magnetic fields in star formation, JWST-based protostellar chemistry, Galactic structure mapping, and accretion dynamics. His articles frequently combine multi-wavelength data to address star-formation physics across scales. Awards: ERC Consolidator Grant (2015) He mentors 12+ PhD students on projects ranging from molecular cloud formation to JWST protostellar analysis. Leads collaborative networks including CASCADE and the Puzzles of Star Formation conferences.
Professor Alan Fitzsimmons is a leading astrophysicist at Queen's University Belfast's School of Mathematics and Physics, affiliated with the Astrophysics Research Centre. His research focuses on icy comets and near-Earth asteroids, using large telescopes worldwide to study their physical characteristics and origins. He has led studies on historic events like the Comet Shoemaker-Levy 9 impact on Jupiter and the first observed interstellar object 'Oumuamua. Member of European Space Agency (ESA) and European Research Council (ERC) teams evaluating asteroid threats Recipient of prestigious awards including the Royal Astronomical Society George Darwin Lecturer (2022) Active in public engagement through media appearances and asteroid-related outreach His research interests span asteroid/comet physical properties, planetary defense, and emerging space mining technologies. Recent work includes studies on interstellar objects and the DART asteroid deflection mission.
Professor Poshak Gandhi is a Professor of Astrophysics at the University of Southampton, affiliated with the Department of Physics and Astronomy. His research focuses on time-domain astrophysics, black holes, lunar astronomy, and data-intensive astronomy. He leads projects like the Leverhulme Emeritus Fellowship and the Formation of Compact-objects Under Scrutiny (FoCUS) initiative. His work leverages advanced observatories such as the James Webb Space Telescope (JWST) to study active galactic nuclei (AGN) and their dynamics. Notable accolades include the NASA Group Achievement Award (2016) and the STFC Ernest Rutherford Fellowship (2014). He currently supervises five PhD students in Physics, focusing on topics like galactic nuclei and astrophysical phenomena. Professor Gandhi collaborates with global teams through the Southampton Theory Astrophysics and Gravity (STAG) Research Centre and the Multiwavelength Accretion and Astronomical Transients group. Research Projects: Leverhulme Fellowship, FoCUS, JWST spectral timing studies. Awards: Nature Astronomy Cover (2017), Higher Education Academy Fellowship (2020). Advising: 5 current PhD students in Physics. Teams: STAG Research Centre, GATOS Survey collaboration.
