Auxiliary Information for the paper "H.E.S.S. follow-up observations of Binary Black Hole Coalescence events during the second and third Gravitational Waves observing runs of Advanced LIGO and Advanced Virgo”
(H.E.S.S. Collaboration, ApJ 2021)

Link to the paper: To be added after publication



Content     GW170814     GW190512_180714     GW190728_064510     S200224ca    
Integral upper limits assuming an E^-2 spectrum

1TeV < E < 10TeV

Fig. 2 and Fig.6

GW170814_1-10_IntULMap_published_version.fits

S190512at_1-10_IntULMap_published_version.fits

S190728q_1-10_IntULMap_published_version.fits

S200224ca_1-10_IntULMap_published_version.fits
Integral energy flux limits assuming an E^-2 spectrum

1TeV < E < 10TeV


GW170814_1-10_ULIntEFlux_published_version.fits

S190512at_1-10_ULIntEFlux_published_version.fits

S190728q_1-10_ULIntEFlux_published_version.fits

S200224ca_1-10_ULIntEFlux_published_version.fits
Luminosity limits

1/(1+z)TeV < E < 10/(1+z)TeV

Fig. 3 and Fig.8

GW170814_1-10_Lum_published_version.fits

S190512at_1-10_Lum_published_version.fits

S190728q_1-10_Lum_published_version.fits

S200224ca_1-10_Lum_published_version.fits
Integral upper limits assuming an E^-2 spectrum and EBL absorption

individual energy ranges (cf. Tab. 2)

Fig. 7

GW170814_IntULMap_E0.42-34.8_published_version.fits

S190512at_IntULMap_E3.58_0.31-38.31_published_version.fits

S190728q_IntULMap_E0.35-26.10_published_version.fits

S200224ca_IntULMap_E0.24-38.31_published_version.fits
Integral energy flux limits assuming an E^-2 spectrum and EBL absorption

individual energy ranges (cf. Tab. 2)


GW170814_specificErange_ULIntEFlux_published_version.fits

S190512at_specificErange_ULIntEFlux_published_version.fits

S190728q_specificErange_ULIntEFlux_published_version.fits

S200224ca_specificErange_ULIntfFlux_published_version.fits




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 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, 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.