Broadband multi-wavelength campaign on PKS 2005-489
S. Kaufmann, M. Hauser, K. Kosack, M. Raue, O. Tibolla, F. Volpe, S., Wagner (for the HESS collaboration), and P. Fortin, W. McConville, D.J., Thompson (for the Fermi/LAT collaboration)

TL;DR
This paper reports on a comprehensive multi-wavelength observational campaign of PKS 2005-489 during a high emission state, covering UV to TeV energies to analyze its broadband spectral energy distribution and emission mechanisms.
Contribution
First simultaneous multi-wavelength campaign covering UV to TeV for PKS 2005-489, providing detailed insights into its high state emission processes.
Findings
PKS 2005-489 was in a high emission state across all observed wavebands.
The campaign captured the SED peaks in UV-X-ray and GeV-TeV regimes.
Data enables detailed modeling of emission mechanisms during high activity.
Abstract
The spectral energy distribution (SED) of high-frequency peaked BL Lac objects (HBL) is characterized by two peaks: one in the UV-X-ray and one in the GeV-TeV regime. An interesting object for analyzing these broadband characteristics is PKS 2005-489, which in 2004 showed the softest TeV spectrum ever measured. In 2009, a multi-wavelength campaign has been conducted with, for the first time, simultaneous observations by H.E.S.S. (TeV), Fermi/LAT (GeV), RXTE (keV), Swift (keV, UV, optical) and ATOM (optical) to cover the two peaks of the SED. During this campaign PKS 2005-489 underwent a high state in all wavebands which gives the opportunity to study in detail the emission processes of a high state of this interesting HBL.
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Astrophysics and Cosmic Phenomena · Particle Accelerators and Free-Electron Lasers
