Be an INTEGRAL astronomer: Task 2
Using the IBIS/ISGRI 18-40 keV data from 2005 to 2009, identify one (or more) period(s) when the sources were all “off” – i.e. when they were not detected.
Indicate how the X-ray emission of these sources compares to that from the Crab. (Hint: compare the average and extreme count rates for the sources – see note at end of Task 1.)
Source name | Source type | Data |
1A 1742-294 | Neutron star X-ray binary | |
1E 1740.7-2942 | Black-hole binary, micro-quasar | |
KS 1741-293 | Neutron star X-ray binary transient | |
SLX 1744-299 | Neutron star X-ray binary |
Last Update: 1 September 2019