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Collaboration

Cherenkov Telescope Array

Cherenkov Telescope Array

Building on the technology of current generation ground-based gamma-ray detectors (H.E.S.S., MAGIC and VERITAS), CTA will be ten times more sensitive and have unprecedented accuracy in its detection of high-energy gamma rays. Current gamma-ray telescope arrays host up to five individual telescopes, but CTA is designed to detect gamma rays over a larger area and a wider range of views with more than 100 telescopes located in the northern and southern hemispheres.
[Text from https://www.cta-observatory.org/ ; Image credit: Gabriel Pérez Diaz, IAC]

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Name Role Affiliations Email Phone Office Centers Research topics
Abe Falcone Abe Falcone Faculty Astronomy adf15@psu.edu +1 814 863 5364 516 Davey Laboratory CMA Cosmic Rays, Multimessenger Astrophysics, Quasars, Dynamic Universe
Kohta Murase Kohta Murase Faculty Astronomy, Physics kum26@psu.edu +1 814 863 9594 321B Osmond Laboratory CMA Cosmic Rays, Dark Matter, Gravitational Waves, Multimessenger Astrophysics, Neutrinos
About our wordmark
Monica Rincon Ramirez

The IGC wordmark was created by Monica Rincon Ramirez while she was a graduate student at the Institute. Monica enjoys drawing new connections between fundamental theory and observations. Her graduate work included general relativity, loop quantum gravity, and quantum fields in cosmological backgrounds; her thesis focused on effective quantum corrections to gravitational phenomena from spinfoams and applications to cosmology. She received her PhD in 2024.

The wordmark symbolizes the scope of research at the IGC. The base represents quantum gravity, evoking the quantum geometrical picture from spinfoams and loop quantum gravity — approaches studied at the Center for Fundamental Theory. The middle shows galaxies embedded in a smooth surface characteristic of spacetime in general relativity and the larger physical scales studied at the Center for Theoretical and Observational Cosmology. The top curves to an extreme representing a supermassive black hole accompanied by an energetic jet, with a binary black hole pair nearby — the high-energy phenomena studied at the Center for Multimessenger Astrophysics.