Undergrad USRA Projects 2025
To find out how to apply for USRAs, visit the department's Undergraduate Summer Research Awards page.
2025 Summer project descriptions will be updated as projects are submitted. Please see previous years' projects for more information about PHAS Faculty projects.
*Students: This will be a continuously growing list. Faculty members who are not listed here might be interested in supervising USRA students; please contact them directly (listed here or not) if they are engaged in research that interests you.
1.CHIME telescope: options for Pulsar and/or FRB projects
Contact: Ingrid Stairs | Email: stairs@astro.ubc.ca
This summer project will entail Pulsar and/or FRB work with the CHIME telescope: in particular, looking at slow pulsars to measure diffractive scintillation properties as a function of frequency; CHIME's wide fractional bandwidth could allow new probes of the predicted scaling of this phenomenon. Also, this project can include an investigation of wideband profile changes in these pulsars and comparison to narrowband literature measurements and conclusions. FRB projects could involve, for example, interference-excision improvements and testing.
For more information about the CHIME telescope, see here.
2. Scanning Tunnelling Microscopy in the Laboratory for Atomic Imaging Research
Contact: Sarah Burke | Email: saburke@phas.ubc.ca
Scanning Tunnelling Microscopy, and related Scanning Probe Microscopy techniques allow for the visualization of surface structure and probing of electronic properties on the atomic scale. These powerful techniques provide a “bottom-up” view of materials properties and their relationship to local structure. The LAIR has ongoing projects spanning single-molecule optoelectronics to superconductivity and 2D materials. Undergraduate students have opportunities to pursue projects related to specific materials under study, instrumentation and technique development, and development of analysis tools. Please contact saburke@phas.ubc.ca for more details.
3. Quantum Coherent Control
Contact: V. Milner | Email: vmilner@phas.ubc.ca | Web: http://coherentcontrol.sites.olt.ubc.ca/
Our research group on Quantum Coherent Control uses ultrafast lasers to control and study the behaviour of molecular "super-rotors" and their interaction with quantum media, such as helium nanodroplets or ultracold plasmas. Super-rotors are extremely fast rotating molecules produced in our laboratory (and not available anywhere else!) using a unique laser system known as an "optical centrifuge". Many fascinating properties of molecular super-rotors have been theoretically predicted. A few of them have been already shown by our group in the last five years, but many more await discovery.
In the summer of 2025, the USRA student will help a senior PhD student with an ongoing experiment on the laser centrifugation of molecules captured by the beam of helium nanodroplets. For specific tasks and projects, please contact Dr. Milner at vmilner@phas.ubc.ca.
4. Charting the Growth of Galaxies
Contact: Allison Man | Email: aman@phas.ubc.ca | Web: https://phas.ubc.ca/users/allison-man
Galaxies evolve on astronomical timescales of millions or even billions of years. The study of galaxy evolution is therefore based on inferring connections between various galaxy populations across cosmic time. This requires knowledge of galaxy properties, such as distances, sizes, masses, ages, and star formation rates. The student will learn now to extract such information from galaxy images and spectra. Driven by the student's interest, the project will tackle these important scientific questions: What triggers or shuts down star formation in galaxies? How do active supermassive black holes influence star formation of their host galaxies? What happens to galaxies when they collide with each other?
The student will apply their Python computing skills to handle large datasets and images, to visualize and to present findings. These skills are relevant for a variety of projects in astronomy, other research disciplines and beyond academia.
Experience with Python programming is required. Knowledge of physics, astronomy, statistics, data analysis, LaTeX and Git will be considered a plus. The ideal candidate will have taken at least one ASTR course at the 200-level and above.
5. Ultrafast optical spectroscopy
Contact: David Jones | Email: djjones@phas.ubc.ca | Web: www.phas.ubc.ca/~djjones
We have openings on two projects employing Ultrafast Optical Spectroscopy. In the first, we are developing laser-ablation dual comb spectroscopy to be employed as a mining ore sensor for real-time evaluation of mineralogy. Skills developed on this project can include: optical alignment, data analysis, machine learning, plasma physics, nonlinear optics, Python programming, atomic and molecular spectroscopy, and numerical simulations. In the second project we need help finishing the construction and commissioning of a field-resolved THz spectrometer for studies of quantum materials. Skills developed on this project can include: optical alignment, nonlinear optics, Python programming, cryogenics, vacuum technology, and numerical simulations. Please contact me for further details.
6. Emergent space-time structures and Dynamic horizons in Quantum Many-body Dynamics
Contact: Fei Zhou | Email: feizhou@phas.ubc.ca
Conformal symmetry plays a paramount role in quantum many-body dynamics where interactions are scale symmetric. It has been shown that conformal symmetry can lead to distinct structures in N-body density matrices (including the Wigner function) and many-body auto-correlation functions. It can further result in entirely reversible far-away-from equilibrium dynamics.
In this project, the student will explore a close connection between such quantum dynamics and the expansion of our universe. Especially, the student will learn how to simulate the Friedmann-Einstein dynamics for the FLRW universe using an emergent space-time structure in conformal dynamics. The main objectives are to understand 1) the nature of curvature and dark matter effects in the context of quantum many-body dynamics and 2) possibilities of observing cosmological redshifts, and cosmic horizons etc in N-body quantum dynamic states that can be initialized in laboratories.
7. Statistics of CMB Polarization
Contact: Dr. Douglas Scott | Email: dscott@phas.ubc.ca | Web: https://www.astro.ubc.ca/people/scott/basic.html
The cosmic microwave background allows us to probe the Universe on the largest length scales possible. There are several hints or "anomalies" that may suggest modifications to physics on large scales or at very early times in the history of the Cosmos. In order to assess if such anomalies are real or just mild statistical excursions in the data, it is necessary to find new ways to probe the large-scale Universe. One such new probe is provided by sensitive measurements of CMB polarization, which comes from new modes in the early Universe. The latest maps of large-angle polarization have been provided by the Planck satellite. In this project we will study aspects of sky polarization, and investigate statistical techniques that can be used to distinguish the cosmological signals and to test for deviations from statistical anisotropy. Additionally, it will be useful to assess the power of future (more sensitive) polarization measurement using simulations.
8. Deep Learning in Astronomy
Contact: Dr. Douglas Scott | Email: dscott@phas.ubc.ca | Web: https://www.astro.ubc.ca/people/scott/basic.html
There are many data analysis problems in astronomy that are best approached using simple likelihood function methods. However, there are other questions (involving non-linear selection tasks, or pattern-matching in huge databases) that are more efficiently performed with "machine-learning" (ML) methods, such as neural networks. One downside to the use of ML approaches is that it is often difficult to determine robust uncertainties on derived parameters. Another unresolved issue is how to combine traditional and ML methods in tasks that use both approaches for different parts. We will investigate these topics by looking at the use of ML in astronomy, combining data at multiple wavelengths to identify and categorize distant galaxies and assess their statistical properties.
9. Looking for New Physics with ATLAS Precision Measurements
Contact: Alison Lister and Colin Gay| Emails: alister@phas.ubc.ca and cgay@phas.ubc.ca | Web: https://atlas.cern/
Q: How do we learn something about new physics beyond the Standard Model (BSM) without measuring it directly? A: We look for its impact on things we can measure! The UBC ATLAS group is working to constrain new physics using precision measurements of Standard Model particles. Different hypothetical BSM particles can cause subtle changes to what we see in the detector. By putting together these measurements we can look for any anomalies that could hint at new physics.
The student will work on translating individual measurements into a combined framework, and optimizing variables to maximize sensitivity. See more information about ATLAS and new physics here.
10. Constructing Silicon Inner Tracker (ITk) for ATLAS Detector Upgrade
Contact: Alison Lister and Colin Gay| Emails: alister@phas.ubc.ca and cgay@phas.ubc.ca | Web: https://atlas.cern/
The UBC ATLAS group is among several institutions around the world participating in the construction of the new, all silicon, Inner Tracker (ITk) for the upgrade of the ATLAS detector for the High Luminosity Large Hadron Collider (HL-LHC) at CERN. Each module of the silicon strip tracker must undergo a series of thermal and electrical quality control measurements before they are installed in the ATLAS detector. Here at UBC, we are performing these critical tests in our newly commissioned cleanroom.
The student will work on building and improving the test setup, optimizing and automating the testing procedure, and analyzing and presenting the results from electrical tests to the wider ATLAS community. See more information about the ATLAS silicon Inner Tracker here.
11. Deep Learning with ATLAS
Contact: Alison Lister and Colin Gay| Emails: alister@phas.ubc.ca and cgay@phas.ubc.ca | Web: https://atlas.cern/
The ATLAS UBC Group is developing new deep learning techniques for both signal vs. background classification problems as well as inference problems (given what we see in our detector, what are the most likely properties of the particles that produce that signature). The students will work on further improvements of the method as well as develop techniques for mitigation of the impact of the systematic uncertainties on the deep learning model.
Experience and familiarity with Python is required.
Contacts: Jess McIver & Raymond Ng | Email: mciver@phas.ubc.ca and rng@cs.ubc.ca | Web: https://gravitational-waves/phas.ubc.ca
Gravitational-wave detector data, including the LIGO detectors, contains a high rate of instrumental artifacts that mask or mimic true astrophysical gravitational wave (GW) signals. This project will characterize noise sources in the Advanced LIGO detectors with the goal of reducing the number of 'false alarm' GW candidates and improving the reach of GW searches for the current observing run. Students will work with a team of physicists and data scientists, and gain transferable skills in data visualization, machine learning, Python programming, gravitational-wave astrophysics, and large-scale physics experimental instrumentation. Familiarity with Python is preferred.
13. Planetary Astronomy topics
Contact : Brett Gladman | Email : gladman@astro.ubc.ca
Project A: Lunar Meteorite Arrival times. Asteroids or comets can impact the lunar surface and launch intact fragments into space which later fall on Earth as lunar meteorites. We have dozens of examples of such meteorites; measurements of the radionuclide activites inside them indicate when they were launched, how long they spent in space, and how long ago they landed on Earth. There is a recent claim of a particularly large lunar impact about 9 million years ago. This project is to compute the rate of deposition on Earth for lunar impact ejecta to see if such a large impact can be reconciled with the lunar meteorite record. The student would perform large-scale numerical simulations of objects leaving the Moon and determining their impact rate onto the Earth.
Project B: Stability maps of transneptunian resonances. Transneptunian objects, in the Kuiper Belt beyond 30 au, can inhabit mean-motion resonances with Neptune. This project would use a GPU-accelerated integrator (GLISSE) to map the stability boundaries of a set of such resonances to serve as a phase space map of where one would find such objects at the present day. Comparison to the locations of real Kuiper Belt objects in and near the resonance will be examined to shed light on the process of resonant capture.
Project C: Multicolour photometry of moons of Jupiter and Saturn. A data set of imaging from the Palomar 200-inch telescope (with supporting data from other telescopes) has been acquired. This project would be to analyze this data to analyze this data (taken in several different astronomical filters) to determine if some moons in different orbital groupings also share similar colours.
Contact: Prof. Michael Hasinoff | Email: hasinoff@physics.ubc.ca | Web: https://phas.ubc.ca/users/michael-hasinoff
Dr. Katherine Pachal | Email: kpachal@triumf.ca | Web: http://darklightariel.mit.edu
We are preparing a new experiment at the TRIUMF/ARIEL e-linac accelerator to search for a possible new particle that could be the mediator between the Dark Matter and Standard Model particles. The student will participate in installation and commissioning measurements of the tracking detectors ( fast trigger ( 200 psec ) segmented scintillator counters read out my solid state photomultipliers, and high resolution ( 100 um ) gas electron multiplier tracking detectors . She/He will learn to use the sophisticated CERN data analysis program ROOT as well as hone their skills in both C++ and Python based analysis. All the work will take place at TRIUMF and the student will be able to participate in all the activities planned for the other ~30 Co-op/USRA students working at TRIUMF. Knowledge of C++ and Python will be considered an asset.
15. Gravitational Wave Astronomy with LISA
Contact: Jess McIver & Scott Oser | Emails: mciver@phas.ubc.ca and oser@phas.ubc.ca
LISA is a proposed spaced-based gravitational wave detector that will consist of three spacecraft flying 2.5 million kilometers apart in an equilateral triangular configuration. Each spacecraft shines a laser at the other two, and all three measure the interference between incoming and outgoing beams of light. These interferometric measurements will allow LISA to measure the minuscule modulation of the separation distances between spacecraft caused by gravitational waves produced by distant sources such as massive black holes, binary star systems, or even the aftermath of the Big Bang itself. We will examine analysis techniques for how we can identify and model short-duration gravitational wave burst signals, especially from black holes orbiting in close proximity to supermassive black holes. Familiarity with Python is strongly preferred. The awardee will learn signal processing, time series analysis, Fourier methods, and gain experience with interferometry methods and astrophysical LISA sources.
16. Crystal Clear: Developing outreach material related to the crystal growth of quantum materials
Contact: Alannah Hallas | Email: alannah.hallas@ubc.ca
- Developing a crystal growth outreach activity using everyday household equipment while prioritizing cost and safety considerations so that the activity can be widely implemented in classrooms across British Columbia.
- Developing pedagogical tools explaining the process of crystal growth. This may include posters or interactive computer-based experiences. These pedagogical tools should be written in accessible terms and should feature engaging visuals.
- Designing a crystal library. The student will grow several reference materials and select the most pristine specimens for a display feature that can be used in outreach.
18. One-upping mother nature with synthetic quantum minerals
Contact: Alannah Hallas and Austin Ferrenti | Emails: alannah.hallas@ubc.ca and austin.ferrenti@ubc.ca
In the development of new magnetic materials, we’re usually limited by the types of crystal structures stabilized in the lab by conventional synthesis methods. However, natural geologic processes often produce minerals with more exotic arrangements of magnetic cations. Exploring synthesis methods that mimic these processes offers the potential to grow our own, entirely new magnetic versions of natural minerals. The student working on this project will join the Hallas group and work in our state-of-the-art crystal growth laboratories at Blusson QMI. Their research project will involve learning hydrothermal and hydroflux crystal growth techniques, toward the stabilization of new magnetic materials based on the natural minerals zemannite and corkite.
No prior knowledge or experience is required, but an interest and prior coursework in chemistry, physics, and/or geology is an asset.
19. Earth-Space Sustainability
Contact: Aaron Boley | Email: acboley@phas.ubc.ca
Humanity’s rapid and accelerating expansion into space benefits society, opens pathways to scientific discoveries, and advances economic opportunities. Satellites already play vital roles in weather forecasting, food production, forest fire detection, climate science, communications, navigation, search and rescue, disaster relief, military operations, and arms control verification. There are also negative consequences, from the loss of dark and radio-quiet skies, to space debris and collision risks on orbit, casualty risks from reentering rocket bodies and satellites, and changes to the atmosphere from both launches and reentries.
These negative consequences arise because space is generally not regarded as an environment in need of protecting, nor is it seen as being closely connected to Earth’s environment. In reality, the two are so closely related that we need to speak of the Earth-Space system. Adding to the challenges, the expansion into space is driven by a handful of powerful states and large private companies who see themselves competing for national, economic, and military advantage in an “area beyond national jurisdiction” that is largely devoid of clear, widely agreed, enforceable rules. Yet the negative consequences of their actions are borne by everyone on Earth, including succeeding generations.
Positions are available under this theme that would explore one or more of the following:
* Calculations of orbital carrying capacities
* Observations of satellites and debris
* Upper atmosphere impacts arising from spacecraft launch and reentries
* Disarmament and space weapons
Contact: Sabrina Leslie | Email: sabrina.leslie@msl.ubc.ca | Web: https://leslielab.msl.ubc.ca/
Nanoparticles are increasingly used in pharmaceutical applications. This research project will use single-particle confinement microscopy to investigate the biophysical properties, stoichiometry and kinetics of nanoparticle assemblies and their interactions. This technique entraps particles in femto-liter reaction wells and allows prolonged monitoring of reactions. It also enables direct visualization of interactions between chemical species and nanoparticles.
For this project, the student will perform single-particle experiments to investigate and quantify probe nanoparticle interactions as well as being part of developing image analysis tools to extract detailed particle information from the microscopy videos. For example, particle tracking algorithms can be used to extract valuable information such as diffusion coefficients and fusion kinetics. Moreover, by using deep learning image analysis it is possible to improve the characterization of nanoparticles with weak signal. This project is best suited for engineering physics students with an interest in computer science and biology since we will be applying physical tools to understand out data.
The student will receive training in quantitative image analysis as well as hands-on microscopy and will work closely with a research fellow and graduate student. Weekly meetings with the supervisor and collaborators, and daily interactions with members of our interdisciplinary research group including the nanomedicine network, will support and guide the project. In addition to gaining hands-on research experience, anticipated outcomes of this summer research project include virtual presentations with lab members, providing key training in writing and oral communication.
21. Single-molecule imaging of DNA-DNA interactions within live Escherichia coli cells.
Contact: Sabrina Leslie | Email: leslielab@msl.ubc.ca | Web: https://leslielab.msl.ubc.ca/
DNA, as a long, double-stranded polymer, can form a variety of secondary structures at sequence specific locations. Such structures have important impacts on cellular function. For example, single-stranded regions within DNA can serve as binding sites for proteins and play a role in regulating gene transcription. Previous work in the Leslie Lab has investigated sites susceptible to forming single-stranded regions when the DNA is supercoiled (over- or under-twisted). These studies investigated how environmental factors, such as temperature, salt and macromolecular crowders, affected the denaturation of these regions, to better understand the biophysics underpinning these transitions. However, the environment within a cell is complicated, and to fully understand how environment impacts secondary structure formation, these in vitro results should be complemented with in vivo measurements.
In this project, the student will build upon our in vitro assays to study structural transitions within DNA plasmids in live E. coli cells. They will test methods to introduce a fluorescent oligonucleotide probe into the cells without killing the cells. They will then use state-of-the-art confocal imaging to follow the probes within the cells and image them binding to target structures within DNA plasmids. Finally, they will compare the probe binding in vivo to our results obtained in vitro.
The student will receive hands-on training and guidance from the Leslie Biophysics Research Group, including day-to-day guidance from graduate students and postdoctoral fellows in the lab, regular meetings with the research team and principal investigator, and interactions with the surrounding interdisciplinary environment at the Michael Smith Labs. Through the course of the summer, the student will hone their oral communication skills through opportunities to present at group meetings and interact at local events such as the Michael Smith Labs Summer Poster Fair.
22. Implementation of deep learning algorithms to improve detection of probe-plasmid interactions within single-molecule Convex Lens-induced Confinement microscopy videos
Contact: Sabrina Leslie | Email: leslielab@msl.ubc.ca | Web: https://leslielab.msl.ubc.ca/
DNA is a long polymer molecule and when it is supercoiled (over- or under-twisted), secondary structures can form in the DNA at predictable, sequence specific locations. To study the formation of these structures, the Leslie Lab has developed an assay where small fluorescently-labelled probes are mixed with plasmids containing the sequence of interest, such that the probe will bind to the plasmid only if the structure is present. The probe-plasmid solution is then imaged with Convex Lens-induced Confinement (CLiC) microscopy, where small volumes of the solution are trapped in microwells and the number of probes bound to plasmids is identified. However, background fluorescence within the microwells, the low signal produced by diffusing single-fluorophores, and the fast photobleaching of these fluorophores provide difficulties in developing an algorithm to automatically detect the number of probes bound to plasmids in a given video. Recent advances in machine learning provide a wide array of tools that can help address these issues and improve the robustness of image analysis of single-molecule videos, increasing the throughput of analysis.
In this project, the student will test and implement deep learning models to automate the detection of probes bound to plasmids in CLiC microscopy videos. They will first identify, train and test a variety of existing models on simulated videos. Once they identify and train a suitable model, they will test it on a range of real data, where the signal, noise, and background signal varies. Finally, once a model is developed that attains a suitable accuracy, they will incorporate the model into the existing analysis pipeline.
The student will receive hands-on training and guidance from the Leslie Biophysics Research Group, including day-to-day guidance from graduate students and postdoctoral fellows in the lab, regular meetings with the research team and principal investigator, and interactions with the surrounding interdisciplinary environment at the Michael Smith Labs. Through the course of the summer, the student will hone their oral communication skills through opportunities to present at group meetings and interact at local events such as the Michael Smith Labs Summer Poster Fair.
23. Exoplanet and Solar System Science
Contact: Michelle Kunimoto | Email: mkuni@phas.ubc.ca
Summary: There are multiple possible summer projects within exoplanet and/or Solar System science. Below are some examples, but these are not exhaustive. Some experience with Python is required for all projects.
Project A: Transiting Exoplanet Photometric Follow-Up. Most exoplanets have been discovered using the "transit method", which involves looking for repeating dips in the observed brightness of a star due to a planet passing in front of the star and blocking a portion of the star's light. This project will involve observing exoplanet transits with the UBC Thunderbird South telescope for two primary purposes: (a) observing that the planet transits the star we expect, which is a crucial step towards planet confirmation, and (b) refreshing the planet's orbital ephemerides (period and transit times), which is crucial for planning time-sensitive follow-up observations such as atmospheric characterization with the James Webb Space Telescope.
Project B: Multi-Survey Asteroid Light Curve Modelling. Wide-field surveys (e.g. the upcoming LSST, ZTF, WISE) are the largest sources of photometric data for asteroids. However, light curves from wide-field surveys are usually sparse in time and scarce in data volume per asteroid. Such light curves are often insufficient to infer even basic properties such as spin periods. This project aims to combine data from multiple wide-field surveys to build a large catalog of asteroid photometry – which could be leveraged to derive thousands of new asteroid rotation periods and possibly other more complex physical properties.
24. Summer USRA Project in Computational Materials Physics
Contact: Prof. Joerg Rottler | Email: jrottler@physics.ubc.ca
My group at QMI is looking for a summer USRA with interest in atomistic modeling and simulations of materials. Topics of interest might include block copolymer vitrimers, functionalized associative poiymers, and disordered multicomponent oxides. Good computational skills and an interest in condensed matter physics are required.
25. AI-Driven Advancements in Nuclear Medicine: Optimizing Language Models for Clinical Reporting for PET scan
Contact: Arman Rahmim | Email: arman.rahmim@ubc.ca | Web: http://qurit.ca/
At the Quantitative Radiomolecular Imaging & Therapy (Qurit) Lab (Qurit.ca), our interdisciplinary team is dedicated to enhancing image analysis for Positron Emission Tomography (PET) scans with the ultimate goal of improving cancer diagnosis, staging, and therapy response assessment. We achieve this through close collaboration with nuclear medicine physicians, ensuring that our advancements are both clinically relevant and impactful.
Artificial Intelligence (AI) and large language models (LLMs), similar to ChatGPT, are rapidly transforming the field of radiology by excelling in tasks such as label extraction, summarization, and report generation from medical images. While LLMs have shown remarkable success across various domains, their optimization for nuclear medicine applications remains relatively unexplored. Preliminary efforts indicate that additional training on domain-specific texts, such as clinical reports in radiology, can significantly enhance their performance. However, adapting these models to the specialized vocabulary of nuclear medicine reports poses challenges in achieving accurate interpretation. Moreover, nuclear medicine physicians meticulously review prior reports to compose comprehensive evaluations, a process that advanced LLMs have the potential to streamline by summarizing existing data and generating concise clinical histories, thereby increasing both efficiency and accuracy.
Our long-term research plan at Qurit Lab focuses on evaluating and optimizing LLMs for nuclear medicine applications through several key initiatives. Firstly, we aim to assess the performance of language models in interpreting PET text reports for lymphoma cases, specifically targeting the generation of therapy assessments using the Deauville score. Secondly, we seek to fine-tune LLMs to produce accurate and personalized impressions for multi-institutional whole-body PET reports, ensuring consistency and reliability across different clinical settings. Lastly, we are developing models to generate comprehensive text reports based on PET scans, further automating and enhancing the reporting process.
The Student's Role:
We invite motivated co-op students to join our team and contribute to these cutting-edge research projects. As a co-op student at Qurit Lab, you will acquire proficiency in AI-based techniques and deep learning approaches through self-study and access to our extensive lab resources. You will engage directly with patient imaging data (PET/CT) and their corresponding reports, collaborating with our researchers to explore and refine language models tailored to the unique demands of nuclear medicine. Depending on your interests and expertise, you will participate in one or more of our key research initiatives, assisting in the fine-tuning of language models for interpreting imaging reports and generating treatment assessments using methods such as retrieval-augmented generation (RAG). Additionally, you will contribute to the generation of text reports based on PET scans, gaining hands-on experience in both AI and medical imaging.
The student's contributions will extend to various clusters within our lab, focusing on cancers such as lymphoma, cervical, prostate, and lung. You will be an active participant in our dynamic research environment, with opportunities to engage in AI competitions and contribute to conference and journal publications alongside our team members. Throughout the program, the co-op student will benefit from daily and weekly mentorship, immersive collaboration with clinical and technical experts, and a deep understanding of the latest developments in imaging and AI. Our lab fosters an environment that emphasizes effective communication and collaborative problem-solving, aligning with our commitment to mentorship driven by your eagerness to learn and excel.
Join us at Qurit Lab and embark on a transformative journey where your contributions will help shape the future of nuclear medicine imaging through innovative AI solutions. Apply now to become a part of our dynamic team and make a meaningful impact in the fields of cancer diagnosis and treatment. For more information about us, visit Qurit.ca.