no code implementations • 23 Jul 2022 • Jingkai Yan, Robert Colgan, John Wright, Zsuzsa Márka, Imre Bartos, Szabolcs Márka
Various approaches have been proposed for improving the efficiency of the detection scheme, with hierarchical matched filtering being an important strategy.
no code implementations • 9 Mar 2022 • Robert E. Colgan, Zsuzsa Márka, Jingkai Yan, Imre Bartos, John N. Wright, Szabolcs Márka
As engineered systems grow in complexity, there is an increasing need for automatic methods that can detect, diagnose, and even correct transient anomalies that inevitably arise and can be difficult or impossible to diagnose and fix manually.
no code implementations • 27 Feb 2022 • Robert E. Colgan, Jingkai Yan, Zsuzsa Márka, Imre Bartos, Szabolcs Márka, John N. Wright
As our ability to sense increases, we are experiencing a transition from data-poor problems, in which the central issue is a lack of relevant data, to data-rich problems, in which the central issue is to identify a few relevant features in a sea of observations.
no code implementations • 8 Apr 2021 • Jingkai Yan, Mariam Avagyan, Robert E. Colgan, Doğa Veske, Imre Bartos, John Wright, Zsuzsa Márka, Szabolcs Márka
Moreover, we show that the proposed neural network architecture can outperform matched filtering, both with or without knowledge of a prior on the parameter distribution.
no code implementations • 3 Mar 2021 • Shigeo S. Kimura, Kohta Murase, Imre Bartos
We propose a novel scenario for possible electromagnetic (EM) emission by compact binary mergers in the accretion disks of active galactic nuclei (AGNs).
High Energy Astrophysical Phenomena
no code implementations • 8 Oct 2020 • Doğa Veske, Zsuzsa Márka, Imre Bartos, Szabolcs Márka
Quantification of the significance of a candidate multi-messenger detection of cosmic events is an emerging need in the astrophysics and astronomy communities.
High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics
1 code implementation • 10 Mar 2020 • Nihar Gupte, Imre Bartos
The identification of electromagnetic emission from gravitational-wave sources typically requires multiple follow-up observations due to the limited fields-of-view of follow-up observatories compared to the poorly localized direction of gravitational waves.
Instrumentation and Methods for Astrophysics High Energy Astrophysical Phenomena