Auxiliary Information on the collaboration publication: Observation of the gamma-ray binary HESS J0632+057 with the H.E.S.S., MAGIC, and VERITAS telescopes

Link to ArXiv
Link to the data on Zenodo
Corresponding authors: Gernot Maier, Daniela Hadasch, Alicia Lopez-Oramas, Denys Malyshev, Gerd Puelhofer.

Main paper

Figure 2 and Figure 3

Data points - H.E.S.S. light curve
Data points - MAGIC light curve
Data points - VERITAS light curve
Data points - X-rays light curve
fig2.jpg fig3.jpg

Figure 4

Data points - optical light curve

Figure 5

Data points - TeV vs keV fluxes
Data points - correlation coefficient

Figure 6

Data points - TeV vs Halpha
Data points - keV vs Halpha

Figure 7 and Figure 8

Data points - HESS (orbital phases 0.2-0.4)
Data points - MAGIC (orbital phases 0.2-0.4)
Data points - VERITAS (orbital phases 0.2-0.4)
Data points - Swift/XRT (orbital phases 0.2-0.4)
Data points - HESS (orbital phases 0.4-0.6)
Data points - MAGIC (orbital phases 0.4-0.6)
Data points - VERITAS (orbital phases 0.4-0.6)
Data points - Swift/XRT (orbital phases 0.4-0.6)
Data points - HESS (orbital phases 0.6-0.8)
Data points - VERITAS (orbital phases 0.6-0.8)
Data points - Swift/XRT (orbital phases 0.6-0.8)
Data points - HESS (orbital phases 0.8-0.2)
Data points - MAGIC (orbital phases 0.8-0.2)
Data points - VERITAS (orbital phases 0.8-0.2)
Data points - Swift/XRT (orbital phases 0.8-0.2)
fig7.jpg fig8.jpg

Figure 9

Data points - H.E.S.S. light curve
Data points - MAGIC light curve
Data points - VERITAS light curve
Data points - X-rays light curve

Figure 10

Data points in tgz archive

Collaboration Acknowledgement

The support of the Namibian authorities and of the University of Namibia in facilitating the construction and operation of H.E.S.S. is gratefully acknowledged, as is the support by the German Ministry for Education and Research (BMBF), the Max Planck Society, the German Research Foundation (DFG), the Helmholtz Association, the Alexander von Humboldt Foundation, the French Ministry of Higher Education, Research and Innovation, the Centre National de la Recherche Scientifique (CNRS/IN2P3 and CNRS/INSU), the Commissariat A l'AŠnergie atomique et aux AŠnergies alternatives (CEA), the U.K. Science and Technology Facilities Council (STFC), the Knut and Alice Wallenberg Foundation, the National Science Centre, Poland grant no. 2016/22/M/ST9/00382, the South African Department of Science and Technology and National Research Foundation, the University of Namibia, the National Commission on Research, Science & Technology of Namibia (NCRST), the Austrian Federal Ministry of Education, Science and Research and the Austrian Science Fund (FWF), the Australian Research Council (ARC), the Japan Society for the Promotion of Science and by the University of Amsterdam. We appreciate the excellent work of the technical support staff in Berlin, Zeuthen, Heidelberg, Palaiseau, Paris, Saclay, TA?bingen and in Namibia in the construction and operation of the equipment. This work benefited from services provided by the H.E.S.S. Virtual Organisation, supported by the national resource providers of the EGI Federation.