Gamma-ray Transient Network Science Analysis Group Report
- Creators
- Burns, Eric
- Coughlin, Michael
- Ackley, Kendall
- Andreoni, Igor
- Bizouard, Marie-Anne
- Broekgaarden, Floor
- Christensen, Nelson L
- d'Ammando, Filippo
- Delaunay, James
- Fleischhack, Henrike
- Frey, Raymond
- Fryer, Chris L
- Goldstein, Adam
- Grossan, Bruce
- Hamburg, Rachel
- Hartmann, Dieter H
- Ho, Anna Y.Q
- Howell, Eric J
- Hui, C. Michelle
- Jenks, Leah
- Joens, Alyson
- Lesage, Stephen
- Levan, Andrew J
- Lien, Amy
- Meli, Athina
- Negro, Michela
- Parsotan, Tyler
- Roberts, Oliver J
- Santander, Marcos
- Smith, Jacob R
- Tohuvavohu, Aaron
- Tomsick, John A
- Wadiasingh, Zorawar
- Veres, Peter
- Villar, Ashley V
- Zhang, Haocheng
- Zhu, Sylvia J
- Others:
- Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS) ; Université Nice Sophia Antipolis (1965 - 2019) (UNS) ; COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur ; COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)
- Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab) ; Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)
Description
The Interplanetary Network (IPN) is a detection, localization and alert system that utilizes the arrival time of transient signals in gamma-ray detectors on spacecraft separated by planetary baselines to geometrically locate the origin of these transients. Due to the changing astrophysical landscape and the new emphasis on time domain and multi-messenger astrophysics (TDAMM) from the Pathways to Discovery in Astronomy and Astrophysics for the 2020s, this Gamma-ray Transient Network Science Analysis Group was tasked to understand the role of the IPN and high-energy monitors in this new era. The charge includes describing the science made possible with these facilities, tracing the corresponding requirements and capabilities, and highlighting where improved operations of existing instruments and the IPN would enhance TDAMM science. While this study considers the full multiwavelength and multimessenger context, the findings are specific to space-based high-energy monitors. These facilities are important both for full characterization of these transients as well as facilitating follow-up observations through discovery and localization. The full document reports a brief history of this field, followed by our detailed analyses and findings in some 68 pages, providing a holistic overview of the role of the IPN and high-energy monitors in the coming decades.
Abstract
International audience
Additional details
- URL
- https://hal.science/hal-04186974
- URN
- urn:oai:HAL:hal-04186974v1
- Origin repository
- UNICA