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High Energy Network Archive



High Energy Network News

New items:

Doroshenko, V. et al “Observations of GRO J1744−28 in quiescence with
XMM-Newton” September 2020,

Bochenek, C, et al, “Localized FRBs are Consistent with Magnetar Progenitors
Formed in Core-Collapse Supernovae” September 2020,


High Energy Space-based and Ground-based Observatories

NASA 's Swift Spacecraft launched in November 2004
Computer rendering of the Swift satellite.
(Credit: NASA E/PO, Sonoma State University, Aurore Simonnet)



Classes of High Energy Objects

Active Galactic Nuclei (AGN)

AGN is a catch-all term for most types of galaxies that have extremely bright and concentrated emission from their central regions. This light is believed to come from matter in the form of gas, dust, and even whole stars being sucked into the central black hole. As all of this material spirals in, it gets very hot and very bright, much brighter than the stars and other luminous material in the center of the galaxy.


Optical observations of GRB 130427A

We're pleased to note that GCN Circular #14490 has been published, detailing time-series photometry of the bright GRB 130427A by Patrick Wiggins.  His observations provide a comprehensive record of the three hours of the early evolution of this incredibly bright afterglow.

Congratulations to Patrick on his observations!

AAVSO High Energy Network: GRB 030329


Thanks to the Curry Foundation and NASA for support of the AAVSO International High Energy Network. Thanks to all the observers across the world for their hard work.

AAVSO International High Energy Network: Our Successes!


Detections, near detections, and upper limits of GRB afterglow fields by AAVSO High Energy Network Members

GRB130427A photometry by P. Wiggins

GRB110918A photometry by A. Oksanen, C. Harlingten, B. Schaefer, and M. Templeton


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