PULSARS AND COMPACT X-RAY SOURCES : COSMIC LABORATORIES FOR THE STUDY OF NEUTRON STARS AND HADRON MATTER

compare our best-fit values to this and do not use it to limit the likelihood analysis. Both the OG and TPC model match the observed gamma-ray light curve well, but neither

As an alternative to the deterministic framework, we propose to handle the problem in the Bayesian framework which will provide a tight minimal bound over all the range of

The spectra provide a measure of the sLllke partial density of states (PDOS) localized at the A1 atoms and show prominant qualitative features that may be identified

The spectrum obtained with an excitation energy of 570 eV is very similar to the spectrum obtained by electron bombardment ( Fig. Figure 4b shows the h3 x-ray emission

L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des

For this research, we constructed a high intensity field emission x-ray source used at a lower photon energy region of less than lOOkeV and using a new spectrum function

The performance of the first machine is outlined, based on almost two years' routine operation, ideiltifying key factors such as output flux, beam lifetime and reliability..

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