Cristina Lagunas Gualda
- Astrophysics and Cosmic Phenomena
- Neutrino Physics Research
- Dark Matter and Cosmic Phenomena
- Radio Astronomy Observations and Technology
- Particle physics theoretical and experimental studies
- Gamma-ray bursts and supernovae
- Pulsars and Gravitational Waves Research
- Radio Wave Propagation Studies
- Particle Detector Development and Performance
- Particle accelerators and beam dynamics
- Gyrotron and Vacuum Electronics Research
- Computational Physics and Python Applications
- Precipitation Measurement and Analysis
- Atmospheric Ozone and Climate
- Radiation Detection and Scintillator Technologies
- Radio, Podcasts, and Digital Media
- Ionosphere and magnetosphere dynamics
- Cryospheric studies and observations
- Solar and Space Plasma Dynamics
- Advanced Optical Sensing Technologies
- Particle Accelerators and Free-Electron Lasers
- Genetics, Bioinformatics, and Biomedical Research
- Optical Wireless Communication Technologies
- Planetary Science and Exploration
- GNSS positioning and interference
Deutsches Elektronen-Synchrotron DESY
2021-2025
Lawrence Berkeley National Laboratory
2023-2024
Southern University and Agricultural and Mechanical College
2021-2024
Clark Atlanta University
2021-2024
Providence College
2021-2024
University of Alaska Anchorage
2021-2024
The University of Texas at Arlington
2021-2024
UCLouvain
2023
TU Dortmund University
2023
University of Wisconsin–Madison
2021-2023
Sources of astrophysical neutrinos can potentially be discovered through the detection in coincidence with electromagnetic counterparts. Real-time alerts generated by IceCube play an important role this search, acting as triggers for follow-up observations instruments sensitive to signals various wavelengths. In previous studies, we investigated treatment systematic uncertainties on reconstruction method currently used IceCube's real-time program, concluding that a new approach, more robust...
Sources of astrophysical neutrinos can potentially be discovered through the detection in coincidence with electromagnetic or gravitational waves. Real-time alerts generated by IceCube play an important role this search, acting as triggers for follow-up observations instruments sensitive to other wavelengths. Once a high-energy event is detected real-time program, complex and time consuming direction reconstruction method run order calculate accurate localisation. To investigate effect...
Abstract Searches for dark matter (DM) have not provided any solid evidence the existence of weakly interacting massive particles in GeV-TeV mass range. Coincidentally, scale new physics is being pushed by collider searches well beyond TeV domain. This situation strongly motivates exploration DM masses much larger than a TeV. Secluded scenarios contain natural way around unitarity bound on mass, via early domination induced mediator its interactions with Standard Model. High-energy neutrinos...
Sources of astrophysical neutrinos can potentially be discovered through the detection in coincidence with electromagnetic or gravitational waves. Real-time alerts generated by IceCube play an important role this search, acting as triggers for follow-up observations instruments sensitive to other wavelengths. Once a high-energy event is detected real-time program, complex and time consuming direction reconstruction method run order calculate accurate localisation. To investigate effect...