Auxiliary information for "Very-high-energy γ-Ray Emission from Young Massive Star Clusters in the Large Magellanic Cloud" (Astrophysical Journal Letters, 970:L21, 2024)

Link to the paper: https://doi.org/10.3847/2041-8213/ad5e67

Figure 1

Flux maps

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Panel (a): [FITS]
Panel (b): [FITS]

Figure 2

Optical image of 30 Dor C with MWL data overlaid.
Background image credit: ESO, https://www.eso.org/public/images/eso1816a

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Figure 3

Infrared image of R136 with MWL data overlaid.
Background image credit: NASA/JPL-Caltech, https://www.spitzer.caltech.edu/image/ssc2020-06b-tarantula-nebula-spitzer-3-color-image

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Figure 4

Luminosities of 30 Dor C and R136.
(Errors contain statistical uncertainties only. Upper limits are at 95% confidence level.)

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For flux points in machine-readable format, see Figure 7 below.

Figure 5

Significance maps.

Panel (a): [PDF]
Panel (b): [PDF]

Figure 6

Residual significance maps.

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Figure 7

Flux points for N 157B, 30 Dor C, and R136.

Figure 8

X-ray image of N 157B with extent of H.E.S.S. model overlaid.
Background image credit: Chen et al., ApJ 651, 237 (2006).

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Figure 9

Count profiles.

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Figure 10

Evaluation of PSF systematics using PKS 2155–304.

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H.E.S.S. 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 à l’énergie atomique et aux énergies alternatives (CEA), the U.K. Science and Technology Facilities Council (STFC), the Irish Research Council (IRC) and the Science Foundation Ireland (SFI), the Knut and Alice Wallenberg Foundation, the Polish Ministry of Education and Science, agreement no. 2021/WK/06, 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, the University of Amsterdam and the Science Committee of Armenia grant 21AG-1C085. We appreciate the excellent work of the technical support staff in Berlin, Zeuthen, Heidelberg, Palaiseau, Paris, Saclay, Tübingen 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.