Cristina Lagunas Gualda

ORCID: 0000-0002-9040-7191
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About
Contact & Profiles
Research Areas
  • 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...

10.22323/1.444.1186 article EN cc-by-nc-nd Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) 2023-07-27

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...

10.22323/1.395.1045 article EN cc-by-nc-nd Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) 2021-07-05

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...

10.1088/1475-7516/2022/06/028 article EN Journal of Cosmology and Astroparticle Physics 2022-06-01

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...

10.48550/arxiv.2107.08670 preprint EN other-oa arXiv (Cornell University) 2021-01-01
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