Landi et al. 2012ATel 4233
:
- Swift observation => refined X-ray position
- XRT spectrum is well fitted with a power law having NH_Gal= 1.25 E21cm-2 and
Gamma ~1.5
- X-ray position is compatible with that of the bright ROSAT source
1RXS J171535.6-545015 and that of the Einstein Slew source 1ES 1711-54.7
- Association between the star HD 155573 and hard X-ray source ruled out
- X-ray source appears = blend of two distinct objects, both
detected above 3 keV
- Tentative positions and counterparts for these 2 sources
- Both X-ray sources have comparable fluxes => both contribute to the
high energy emission
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