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ZENODO
Dataset . 2023
License: CC BY
Data sources: ZENODO
ZENODO
Dataset . 2023
License: CC BY
Data sources: Datacite
ZENODO
Dataset . 2023
License: CC BY
Data sources: Datacite
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Data products of A&A 680 A2 (2023) - Final Version

Authors: Scheel-Platz, Lukas Imanuel; Knollmüller, Jakob; Arras, Philipp; Frank, Philipp; Reinecke, Martin; Jüstel, Dominik; Enßlin, Torsten A.;

Data products of A&A 680 A2 (2023) - Final Version

Abstract

Data product release for the manuscript published at Scheel-Platz et al., A&A 680 A2 (2023) https://arxiv.org/abs/2204.09360v2 General DescriptionThis data collection contains the numerical results of the Gamma-ray sky reconstructions discussed in the above-mentioned paper. The results of the reconstructions based on models M1 and M2 are stored in separate ZIP archives. For each reconstruction (M1, M2) and sky component I^c (see Fig. A.1 for the model graph), we provide the following data products: the reconstructed posterior samples of I^c_ij posterior sample means and sample standard deviations of I^c_ij All maps are given in units of 1/(s m² sr) and are contained in HDF5 files named after the components, following the naming conventions in the paper. Each HDF5 file contains the data groups 'samples' and 'stats', with the former containing the posterior samples and the latter containing the posterior sample mean and standard deviation. Pixelation in the spatial domainThe sky sphere is pixelated following the HEALPix 'RING' scheme with a NSIDE of 128. This pixelation is used throughout all energy bins. Pixelation in the spectral (energy) domainThe energy dimension is pixelated as a regular grid on a logarithmic energy scale. The energy bin boundaries are the same for both reconstructions and are stored in the file 'energy_bins.hdf5'. A note on summary statisticsThe posterior mean and standard deviations contained in the HDF5 files are calculated directly from the posterior samples as given. However, for many analyses, it is more appropriate to use the mean and standard deviation on a logarithmic scale, which need to be computed from the given samples. Updates with respect to v2.1.1- adjusted description to be in sync with the peer-reviewed publication of the manuscript- added missing energy_bins.hdf5 file Updates with respect to v2.1.0- removed v1.0 README file

Keywords

gamma rays, ISM, diffuse

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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