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Aghakhanloo, Mojgan

Postdoctoral Research Associate
Ph.D., 2020, Florida Sate University
Areas of Interest: Massive stars and binary evolution, Stellar cluster, and Statistical techniques.

Mojgan will be joining Steward Observatory in the fall 2020 semester to work with Prof. Nathan Smith. Mojgan’s research focuses on constraining the late-stage evolution of massive stars. In particular, she is unraveling the evolutionary history of luminous blue variables (LBVs), the mysterious massive stars which for unknown reasons expel much of their mass in small, modest, and giant eruptions. She is passionate and curious about exploring large datasets like Gaia to discover new information in stellar evolution and beyond. Her projects have included developing analytical and statistical modeling to constrain fundamental parameters of massive stars.

Andrews, Jennifer

Senior Research Associate
Ph.D., 2011, Louisiana State University
Areas of Interest: Core-Collapse SNe, Evolved Massive Stars, Stellar Clusters, Initial Mass Function

Jennifer is involved in mapping the late-time evolution of massive stars using multi-wavelength observations of their interaction with their surrounding environment. This includes optical and IR light echoes and spectral changes due to circumstellar interaction. She is also interested in how, when, and where dust is formed in CCSNe, particularly with regards to mass loss from the progenitor star.

Anugu, Narsireddy

Steward Observatory Prize Fellow in Astronomical Instrumentation and Technology
Ph.D., 2017, University of Porto, Portugal Areas of Interest: Protoplanetary Disks, Extrasolar planets, Interferometry, Adaptive optics, high contrast imaging

Narsireddy Anugu joined Steward Observatory in August 2019. Currently, he is a postdoctoral fellow at the University of Michigan and University of Exeter, UK. His main research focuses on optical/near-infrared high-angular resolution instrumentation. He worked on the development of ESO GRAVITY and CHARA MIRC-X interferometric instruments. Currently, he is working on CHARA adaptive optics and MYSTIC instrument developments. He has been involved and interested in imaging disks around protoplanetary and post-AGB binary objects.

Byun, Joyce

Postdoctoral Research Associate
Ph.D, 2015, Cornell University
Areas of Interest: Areas of Interest: cosmology, Large-Scale Structure, galaxy surveys, higher-order statistics, Dark Energy, modified gravity, primordial non-Gaussianity

Joyce will be joining Steward Observatory in the fall of 2020 to work in the Arizona Cosmology Lab. She is interested in using cosmological galaxy surveys to test inflationary scenarios, dark energy models, and modified gravity theories. Her work focuses on developing methods for extracting maximal information from galaxy clustering observables, including higher-order statistics, through a combination of improved theoretical modeling, simulations, and statistical methods. She received her PhD from Cornell University in 2015 and was previously a postdoctoral fellow at the University of Sussex in the United Kingdom and the University of Geneva in Switzerland.

Christian, Pierre

SO Prize Fellow in Theoretical and Computational Astrophysics
Ph.D., 2018, Harvard University
Areas of Interest: Black hole astrophysics and gravitational waves

Pierre is interested in studying the interaction of black holes with its environments, and how such interactions could be used to probe the physics of extreme spacetimes. He is also interested in studying the population and formation of gravitational wave sources, e.g. his latest paper studied how gravitational wave observations can be leveraged to constrain the modification of the black hole mass function due to merging black holes in star clusters. Pierre joined Steward Observatory in the fall 2018 semester.

Chung, Haeun

Postdoctoral Research Associate
Ph.D., 2019, Seoul National University Areas of Interest: Astronomical instrumentation and observational astronomy including Integral Field Spectograph, System Engineering, Galaxy Kinematics and Dynamics, Environmental Effects on Galaxy Properties, Optical Design, Software Development, Galaxy Formation and Evolution, Galaxy Interactions and Mergers

Haeun Chung joined Steward Observatory in the 2019 fall semester to work with Prof. Erika Hamden. Haeun’s research focus is on astronomical instrumentation and observational astronomy in the areas of optical spectrograph and kinematics/dynamics of galaxies. During his Ph.D., he worked on building an optical multi-IFU spectrograph (DOTIFS) from overall conceptual design to the spectrograph optical design and the software development. He is also studying environmental effects on galaxy kinematics using SDSS MaNGA data and developing an IFU data post-processing technique (deconvolution).

Esplin, Taran

Peter A. Strittmatter Fellow in Astronomy & Astrophysics
Ph.D., 2017, Pennsylvania State University
Areas of Interest: Nearby Star-forming Regions, Brown Dwarfs, Circumstellar disks, Initial Mass Function, Brown Dwarf Atmospheres

Taran's research has included: searching for the classifying circumstellar disks in nearby star-forming regions, characterizing the photometric variability of the coldest known brown dwarf, measuring a new distortion correction for the Infrared Array Camera on the Spitzer Space Telescope, and determining precise parallaxes for ultra-cool brown dwarfs. He completed his Ph.D. in 2017 advised by Kevin Luhman at Pennsylvania State University. Currently Taran is searching for the least-massive members in nearby star-forming regions as the inaugural Strittmatter Fellow.

Fang, Xiao

Postdoctoral Research Associate
Ph.D., 2018, Ohio State University
Areas of Interest: Survey Cosmology, Large-Scale Structure, Compact Objects, Hierarchical Systems, stellar dynamics, Type Ia Supernovae

Xiao joined Steward Observatory on September 1, 2018 to work with Prof. Tim Eifler. As a Ph.D. student at Ohio State University, he worked on a broad range of topics, from observational cosmology to compact objects and stellar dynamics. He was also involved in analysis for the upcoming WFIRST mission.

Gralla, Megan

Senior Research Associate
Ph.D., 2011, University of Chicago
Areas of Interest: Galaxy Clusters, Active Galactic Nuclei, Dusty star-forming galaxies

Megan studies galaxy clusters and groups, active galactic nuclei, and the relationship between galaxies and their environments. She works with surveys and data sets spanning the radio, millimeter-wavelength, optical and X-ray regimes. Before joining Steward Observatory, Megan worked at Johns Hopkins University and the Smithsonian Astrophysical Observatory.

Haffert, Sebastiaan

NHFP Sagan Fellow
Ph.D., 2019, Leiden University
Areas of Interest: Circum-stellar disks, Planet Formation, Exoplanet Detection and Characterization, Exoplanet Atmospheres, High-Contrast Imaging, high-spatial and spectral instrumentation, remote sensing

Sebastiaan joined Steward Observatory in October 2019 as an NHFP Sagan Fellow to work together with Dr. Jared Males and the MagAO-X team. Sebastiaan’s research focuses on the development of high spatial and spectral resolution instrumentation for the detection of exoplanets and characterization their atmospheres. During his PhD he developed the Leiden Exoplanet Instrument (LEXI), which was a pathfinder instrument for optical/NIR high-resolution integral-field spectroscopy. One of his interests is the use of optical integral-field spectroscopy for the characterization of proto-planets and their formation. He is also interested in the applying the instruments and techniques developed for astronomy in other fields.

Huang, Hung-Jin

Postdoctoral Research Associate
Ph.D., 2019, Carnegie Mellon University Areas of Interest: Weak gravitational lensing, Cosmic structure formation

Hung-Jin joined Steward Observatory in September 2019 to work with Profs. Tim Eifler, Elisabeth Krause, and Eduardo Rozo. She investigates the growth of structure in our Universe to understand both cosmology and galaxy formation physics. During her Ph.D. at Carnegie Mellon University, she studied astrophysical systematics on weak lensing, with focuses on intrinsic alignment of galaxies and modeling uncertainties of baryonic physics.

Jencson, Jacob

Postdoctoral Research Associate
Ph.D., Astrophysics, 2019, Caltech
Areas of Interest: Observational astrophysics, with an emphasis ontime-domain surveys, obscured supernovae, and infrared transients.

Jacob joined Steward Observatory in the fall of 2019 to work with Prof. David Sand. For the last four years, he has helped lead the Spitzer InfraRed Intensive Transients Survey, or SPIRITS, a search for transients with Spitzer/IRAC in nearby galaxies within about 20 Mpc from Earth. His primary research interests are uncovering hidden, heavily obscured supernovae and other kinds of dusty eruptions and explosions of massive stars.

Jones, Michael

Postdoctoral Research Associate
Ph.D., 2016, Cornell University
Areas of Interest: Galaxy Formation and Evolution, galaxy environment, Dwarf Galaxies, Radio Astronomy

Michael will be joining Steward Observatory in the fall 2020 semester to work with Prof. David Sand. Michael’s research interests focus on the properties of galaxies in the nearby Universe, in particular dwarf galaxies. He studies the gas and stellar content of galaxies across a range of environments from clusters and groups to isolated galaxies, to try to untangle the competing roles of "nature" and "nurture" in galaxy evolution. He completed his PhD working on the ALFALFA survey at Cornell University and was previously a post-doctoral fellow at the Instituto de Astrofíscia de Andalucía in Granada, Spain.

Kong, Shuo

Postdoctoral Research Associate
Ph.D., 2016, University of Florida
Areas of Interest: Galactic Star Formation, Molecular Clouds, Jets and Outflows, Radio Interferometry, Astrochemistry

Shuo is interested in understanding all aspects of the star formation process, including the initial conditions, the protostellar accretion, and feedback. His research focuses on the physical and chemical properties of giant molecular clouds (including infrared dark clouds), the interplay between filaments, magnetic fields, and protostellar accretion, and the radiative and mechanical feedback effects from young massive stars. Shuo mainly uses mm radio single-dish and interferometric telescopes (e.g., SMT, ALMA) for his research. He is leading the data reduction and reporting of two CARMA large programs that produce degree-size maps of the Orion A Cloud and the North American Nebula. Recently, he is interested in how Galactic-scale structures regulate star formation.

Krapp, Leonardo

Postdoctoral Research Associate
Ph.D., Astrophysics, 2019, University of Copenhagen Denmark
Areas of Interest: Plasma physics in the framework of non-ideal Magnetohydrodynamics and multi-species dynamics

Leonardo is currently a PhD student working in the Theoretical Astrophysics Group, at the Niels Bohr International Academy, Niels Bohr Institute, University of Copenhagen, Denmark. He joined Steward Observatory in fall 2019 as a Postdoctoral Research Associate to work with Professors Kaitlin Kratter and Andrew Youdin. Leonardo obtained his degree in Astronomy in 2015 at Universidad Nacional de Córdoba, Córdoba, Argentina. His research is focused on numerical Astrophysics applied to planet formation and protoplanetary disk dynamics. His interests include plasma physics in the framework of non-ideal Magnetohydrodynamics and multi-species dynamics accounting for the momentum transfer between multiple species, in particular, the aerodynamics coupling between gaseous fluids and dust grains.

Krijt, Sebastiaan

NASA Hubble Fellow
Ph.D., 2015, Leiden University, The Netherlands
Areas of Interest: Protoplanetary Disks, dust coagulation, Planet Formation

Sebastiaan joined Steward Observatory on September 1, 2018 to work with Prof. Daniel Apai. Sebastiaan uses numerical simulations to study the behavior of dust particles in protoplanetary disks. He is interested in understanding how, where, and when microscopic dust grains coagulate to form km-size planetesimals (the building blocks of planets), and how the dynamical behavior of dust grains influences the chemical composition of the growing solids and the protoplanetary nebula as a whole.

Lesser, David

Postdoctoral Research Associate
Ph.D., 2019, University of Arizona

David received his my bachelor's degree in physics from Oberlin college and his PhD in Astronomy and Astrophysics from the University of Arizona. His research focuses on studying the lifecycle of the interstellar medium, and building terahertz instrumentation to do so. He also works on improving undergraduate and K-12 STEM education through exposing students to practical design experiences.

Lundquist, Michael

Postdoctoral Research Associate
Ph.D., Physics, 2015, University of Wyoming
Areas of Interest: Star Formation, Stellar Clusters, Massive Stars, time domain astronomy, Instrumentation

Michael Lundquist joined Steward Observatory on August 1, 2018. Michael is an observational astronomer with broad research interests. His research background includes studies of classical novae, massive stellar binaries, and intermediate-mass star-forming regions. Michael works with Prof. David Sand as part of the DLT40 supernova survey.

Lyu, Jianwei

Postdoctoral Research Associate
Ph.D., Astronomy & Astrophysics, 2020, University of Arizona Areas of Interest: Extragalactic IR astronomy, black hole/galaxy connection

Jianwei is working with Prof. George H. Rieke on the IR properties of AGNs and their host galaxies from z=0 to z=6. Specifically, he carries out comparative SED analysis of low-z objects and high-z ones to obtain insights on the AGN dusty environment, uses multi-wavelength and multi-epoch observations to probe the interplay between supermassive black holes and their host galaxies, and develops new tools for galaxy SED decomposition and AGN selection for the upcoming JWST and future IR missions.

Martin, Garreth

KASI-Arizona Joint Postdoctoral Fellow for Advanced Study in Astronomy & Astrophysics
Ph.D., Astrophysics, 2019, University of Hertfordshire
Areas of Interest: cosmological simulations, data-mining / unsupervised machine-learning techniques, low-surface-brightness galaxies, Galaxy Formation and Evolution, galaxy-black-hole co-evolution, galaxy mergers and galaxy morphology

Garreth joined Steward Observatory in the fall of 2019. His research lies at the interface between observational and theoretical astronomy, combining state-of-the-art hydrodynamical simulations, survey data and machine-learning techniques. He is interested in how the diversity of present-day galaxy populations arises during their assembly and how underlying processes like mergers, feedback and environmental processes drive these changes. His current work focusses on the formation mechanisms, evolution and morphology of low-surface-brightness galaxy populations that have gone almost unnoticed in previous wide-area surveys and represent an important additional axis for constraining our understanding of galaxy evolution.

Miranda, Vivian

Postdoctoral Research Associate
Ph.D., 2015, University of Chicago
Areas of Interest: Dark Energy, Inflation, Cosmic Microwave Background, Weak Lensing, Cluster Cosmology

Vivian Miranda joined Steward Observatory on September 1, 2018, to work with Prof. Elisabeth Krause. Vivian's research is focused on probing inflation, the epoch of reionization and dark energy with the Cosmic Microwave Background. She has done her Ph.D. at the University of Chicago under the guidance of Prof. Wayne Hu. Vivian is also keen on understanding how extensions of the LCDM model can be constrained via the combination of the CMB with low redshift probes. As a postdoc at the University of Pennsylvania, she has developed research on how to test fundamental assumptions about the standard model using model-independent techniques. At the University of Arizona, Vivian intends to dedicate her time to the Dark Energy Survey (DES), in particular, to cluster cosmology and weak lensing. Vivian's work stands on the bridge between theory and data, and she is open to radically new ideas, as long as it can be falsified by either the CMB or the DES/LSST/WFIRST surveys. In 2019, Vivian was awarded the Leona Woods Distinguished Postdoctoral Lectureship Award.

Moe, Maxwell

Postdoctoral Research Associate
Ph.D., 2015, Harvard University
Areas of Interest: Binary Star Formation and Evolution, Eclipsing Binaries, Type Ia Supernovae

Max utilizes large datasets of eclipsing binaries (EBs) to understand the formation, environments, and evolution of massive stars and binaries. In particular, Max measures the statistical distributions of binary star properties to test binary formation models and to provide initial conditions for binary population synthesis studies. He also incorporates EB populations to investigate tidal evolution, binary mass transfer and accretion processes, pre-main-sequence evolution, triple stars, feedback and dust content in young stellar nurseries, and the progenitors of Type Ia supernovae and X-ray binaries.

Mutlu-Pakdil, Burçin

Postdoctoral Research Associate
Ph.D. , 2017, University of Minnesota, Twin Cities Areas of Interest: Structure, Morphology, and Dynamics of Galaxies; Galaxy Evolution; Black Hole-Galaxy Co-evolution

Burcin's research interests encompass both theoretical and observational aspects of extragalactic astronomy. She studies the structure and dynamics of galaxies, and examines what these can tell us about the galaxy formation process. Her recent research in galaxy structure has led to a discovery of an extremely rare galaxy. This work has provided a first description of a double ringed elliptical galaxy. Currently, she works on the general topics of nearby galaxies, resolved stellar populations and near-field cosmology.

Olsen, Karen

Postdoctoral Research Associate
Ph.D., Astronomy, 2015, Copenhagen University
Areas of Interest: Galaxy Formation and Evolution, ISM Emission Modeling, cosmological simulations, ISM Properties of Galaxies, Far-infrared Line Emission, Intensity Mapping in the Far-infrared

Dr. Karen Olsen works to better understand galaxy evolution by studying the properties of the interstellar matter (ISM). Her overarching goal is to bridge the gap between spectroscopic observations of the ISM and numerical models of galaxy formation. In that quest, Karen has built a unique and world-leading tool called SIGAME to model line emission from the ISM in the far-infrared (FIR) utilizing state-of-the-art cosmological galaxy simulations. By comparing the output of this modeling to observations with large interferometers such as ALMA, VLA and NOEMA, SIGAME helps to unveil the physics of the ISM - the driving component in galaxy evolution. Before coming to Steward Observatory, Karen received her PhD from the Dark Cosmology Centre at the Niels Bohr Institute in Denmark, and enjoyed a three-year postdoctoral fellowship at Arizona State University.

Petrovich, Cristobal

Bart J. Bok Fellow for Advanced Study in Astronomy and Astrophysics
Ph.D., 2015, Princeton University Areas of Interest: Orbital dynamics, Exoplanets, Compact Objects, Gravitational wave source and Disk-planet interactions

Cristobal joined Steward Observatory in August 2019. His research focuses on understanding the formation and evolution of planetary and stellar systems using the information encoded in their orbits and astrophysical environments. He did his PhD at Princeton where he studied the role of orbital migration at shaping the architecture of observed exoplanet systems. Currently, as a postdoc at CITA, he has also worked on the dynamics of multi-stellar systems and their role at producing gravitational wave sources.

Plat, Adèle

Postdoctoral Research Associate
Ph.D., Astrophysics, 2019, Sorbonne Université
Areas of Interest: Galaxy formation and evolution.

Adele’s research mainly concerns the formation and evolution of galaxies, in particular, she is interested in studying the spectral properties of galaxies, with a focus on the emission from their stellar populations and surrounding interstellar medium.

Sarma Bohurah, Supranta

Postdoctoral Research Associate
Ph.D., 2020, University of Waterloo Areas of Interest: peculiar velocities, reconstruction of the large-scale structure, Weak Lensing, statistical methods and machine learning

Supranta will be joining Steward Observatory in the Fall of 2020 to work in the Arizona Cosmology Lab. He is interested in the data analysis of upcoming cosmological surveys using state-of-art statistical and computational methods. During his PhD, his research involved the study of peculiar velocities of galaxies and forward-modelled reconstruction of the large-scale structure.

Shivaei, Irene

NASA Hubble Fellow
Ph.D., 2017, UC Riverside

Irene Shivaei earned her Ph.D. at UC Riverside, advised by Professor Naveen Reddy. Her work is part of the MOSDEF project to use the multi-object near-infrared spectrograph MOSFIRE on the Keck I Telescope to study the high redshift (z~2) Universe. She has focused on determining accurate star formation rates, comparing estimates from H alpha and H beta with those from infrared measurements, and on the behavior of the mid-infrared aromatic bands with metallicity. She will expand this work with JWST, using MIRI GTO data in the Hubble Ultra-Deep Field region. Irene is also involved in outreach, for example as a co-founder of the StarYab astrophysical literature website with weekly discussions of recent astronomy research results in Persian.

Stone, Jordan

NASA Hubble Fellow
Ph.D., 2015, University of Arizona Areas of Interest: Star and Planet Formation, Brown Dwarf and Exoplanetary Atmospheres, High-Contrast Imaging, Interferometry

I've been working to understand the physical nature of protoplanetary disks around young stars to better understand how the late evolution of proto-star--disk--proto-planet systems produce the variety of planetary systems observed.

Tang, Mengtao

Postdoctoral Research Associate
Ph.D., Astronomy & Astrophysics, 2020, University of Arizona
Areas of Interest: Areas of Interest: galaxy formation and evolution, cosmic reionization, high-redshift galaxies

Mengtao works with Prof. Daniel Stark on understanding the physical properties of metal-poor star-forming galaxies at high-redshift (z > 1) and their role in cosmic reionization. Using the spectroscopy obtained from HST, MMT, Magellan, LBT, and Keck, his research focuses on investigating the radiation fields, stellar populations, and nebular gas properties of high-redshift star forming galaxies, and constraining their contribution to the reionization of intergalactic hydrogen. He will also be involved in defining applications for future surveys with WFIRST, JWST, and GMT.

Vargas, Carlos J.

Postdoctoral Research Associate
Ph.D., 2018, New Mexico State University
Areas of Interest: Galaxy Evolution, Star Formation, ISM/CGM, Disk-halo interface, Radio/sub-mm Astronomy

Carlos studies the relationship between star formation and the diffuse inner halos of spiral galaxies. He is particularly interested in the mechanisms behind the prevalence and support of matter residing outside of star-forming galaxy disks. He has led studies analyzing the cycling of gas and cosmic rays between galaxy disks and halos, as well as a study of high redshift Lyman-alpha emission. Carlos joined Steward Observatory in September of 2018 to work with Dr. Erika Hamden.

Wagner, Kevin

B.S., 2015, University of Cincinnati Areas of Interest: Exoplanets, Circumstellar disks, and Planet formation

Kevin is using ground-based adaptive optics systems (such as VLT/SPHERE and MagAO) to search for young and forming planetary systems, and to study these archetypes of mature planetary systems through high-contrast imaging and spectroscopy.

Wang, Feige

NHFP Hubble Fellow
Ph.D., 2017, Peking University
Areas of Interest: High Redshift Quasars, cosmic reionization, Black Hole Growth, Galaxy Formation and Evolution

Feige Wang joined Steward Observatory as an NHFP Hubble Fellow in the fall of 2019, and will be working with Prof. Xiaohui Fan. His research focuses on finding the most distant super-massive black holes (SMBHs) and using the most distant quasars to investigate when did reionization occur, what was the SMBH accretion history and how was the growth of the SMBHs linked to the assembly of early massive galaxies. He obtained his Ph.D. from the Peking University in 2017. Afterwards, he moved to the University of California, Santa Barbara as a post-doc for two years.

Wen, Sixiang

Postdoctoral Research Associate
Ph.D., 2018, Sun Yat-sen University
Areas of Interest: Tidal Disruption Events, Dark Energy

Sixiang Wen joined Steward Observatory in January 2019 working with Prof. Ann Zabludoff. His research focuses on modeling the accretion of Tidal Disruption Events from first principles. Sixiang is currently working on fitting the X-ray spectrum and light curve of TDEs to constrain the mass and spin of the central supermassive black hole. His other interests include dark energy and black hole astrophysics.

Westernacher-Schneider, Ryan

Postdoctoral Research Associate
Ph.D., Physics, 2018, University of Guelph
Areas of Interest: Turbulence, core-collapse supernovae, Relativistic Astrophysics, Gravitational Waves, Numerical Relativity, Fluid-Gravity Duality

Ryan Westernacher-Schneider joined Steward Observatory on September 1, 2018 to work with Prof. Vasilis Paschalidis. Ryan grew up in Toronto, Canada. He was an undergraduate at the University of Toronto, and did his graduate studies at the University of Guelph and the Perimeter Institute for Theoretical Physics with Luis Lehner. He has worked on the statistical theory of relativistic turbulence using analytic techniques and numerical simulations, and applied it to turbulent black holes via the fluid-gravity duality. He has ongoing work on tidal disruption events, as well as gravitational wave asteroseismology of core-collapse supernovae and associated multimessenger detection strategies.

Yang, Jinyi

Postdoctoral Research Associate
Ph.D., 2017, Peking University
Areas of Interest: High-z Universe & Reionzation, High-z Quasar/AGN evolution, Super massive black hole growth, Quasar surveys at multi-redshift ranges, and Absorption Systems in quasar spectra

Dr. Yang joined Steward Observatory in November 2017. Jinyi's research focuses on quasar evolution and quasar surveys at high redshift. During her thesis, she measured the quasar luminosity function at z ~ 5 and studied the quasar evolution model at high redshift. She carried out a survey of quasars at the redshift gap (z~5.5) of quasar color selection using a new selection pipeline. She is working on the study of multi-wavelength properties of quasars and the co-evolution between SMBHs and quasar host galaxies at z>~5, and is also involved in searching and follow-up works of quasars at z>~6. Additionally, she is interested in absorption systems towards quasar spectra, which can trace the redshift evolution of neutral hydrogen and metals in the intergalactic and galactic scales. At Steward Observatory, she will continue the research on high redshift quasars and the cosmic reionization.

Zhang, Huanian

Postdoctoral Research Associate
Ph.D., 2016, University of Arizona
Areas of Interest: Galaxy structure and gas halos, low surface brightness galaxies.

Huanian received his Ph.D in theoretical particle physics, specifically in new physics beyond Standard Model. Huanian's research mainly focuses on ionized gas halos of low redshift galaxies. Using a sample of nearly half a million foreground galaxies, probed by over 7.4 million low-background spectra from the Sloan Digital Sky Survey Data Release 12, Huanian traces Halpha emission to about 100 kpc galactocentric radius. Huanian has also presented the first evidence for a widely distributed, neutral, excited hydrogen component of the Milky Way Galaxy that is observed only as slight absorption in the combined spectra of millions of galaxy spectra. Huanian's research interests also include mapping the CGM of individual galaxies, searching for globular clusters within the local volume, and building the all-sky catalog of Ultra Diffuse Galaxies.