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The tar file contains two separate data files. The file SNR_flux.txt contains the list of supernova remnants and their gamma-ray line fluxes from the decay of nucleus 126Sn at 666.3 keV (100% intensity). Fluxes are calculated by assuming a ejecta mass of 0.01 solar mass, containing number fraction of 126Sn of 1.7*10^-4. Note that this list only contains those SNRs with both the age and distance information available from http://www.physics.umanitoba.ca/snr/SNRcat/. The file magnetar_flux.txt contains instead the gamma-ray line fluxes from known magnetars with both the characteristic age and distance information available from http://www.physics.mcgill.ca/~pulsar/magnetar/main.html.
| 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). | 1 | |
| 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. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
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