activity
20052025
most citedDesign Concepts for the Cherenkov Telescope Array

902 citations · 10.1k across the 78 of their papers we have counts for

collaborators

78 papers

q-fin.ST2025

To Trade or Not to Trade: An Agentic Approach to Estimating Market Risk Improves Trading Decisions

Dimitrios Emmanoulopoulos, Ollie Olby, Justin Lyon +1

Large language models (LLMs) are increasingly deployed in agentic frameworks, in which prompts trigger complex tool-based analysis in pursuit of a goal. While these frameworks have…

quant-ph2022★ 32 cited

Quantum Machine Learning in Finance: Time Series Forecasting

Dimitrios Emmanoulopoulos, Sofija Dimoska

We explore the efficacy of the novel use of parametrised quantum circuits (PQCs) as quantum neural networks (QNNs) for forecasting time series signals with simulated quantum forwar…

astro-ph.HE2018★ 17 cited

The absence of a thin disc in M81

A. J. Young, I. McHardy, D. Emmanoulopoulos +1

We present the results of simultaneous Suzaku and NuSTAR observations of the nearest Low-Luminosity Active Galactic Nucleus (LLAGN), M81*. The spectrum is well described by a cut-o…

astro-ph.HE2017★ 131 cited

X-ray/UV/optical variability of NGC 4593 with Swift: Reprocessing of X-rays by an extended reprocessor

I M McHardy, S D Connolly, K Horne E M Cackett +25

We report the results of intensive X-ray, UV and optical monitoring of the Seyfert 1 galaxy NGC 4593 with Swift. There is no intrinsic flux-related spectral change in the the varia…

astro-ph.HE2017★ 3 cited

Cherenkov Telescope Array Contributions to the 35th International Cosmic Ray Conference (ICRC2017)

F. Acero, B. S. Acharya, V. Acín Portella +1137

List of contributions from the Cherenkov Telescope Array Consortium presented at the 35th International Cosmic Ray Conference, July 12-20 2017, Busan, Korea.

astro-ph.HE2017★ 150 cited

Swift monitoring of NGC 4151: Evidence for a Second X-ray/UV Reprocessing

R. Edelson, J. Gelbord, E. Cackett +41

Swift monitoring of NGC 4151 with ~6 hr sampling over a total of 69 days in early 2016 is used to construct light curves covering five bands in the X-rays (0.3-50 keV) and six in t…