Free Access

Fig. 7


Flux time history of 2FGL J1045.0−5941 as determined by likelihood analysis for ranges of the orbital phase of η Car (left) and the physical separation of the stellar components (right) for energies 0.2 to 10 GeV. Each data point represents 2.5 months of data. Because periastron is traversed very quickly, the data points around orbital phase 0 are very broad. The region between the two dashes at the left of the horizontal error bar of the leftmost data point on the right graph is traversed twice.

This figure is made of several images, please see below:

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.