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| Miscellaneous :
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Landi et al. 2007 ATel 1288:
- Association with SUMMS and 2MASS sources
- probable AGN
- Unabsorbed power law Γ=2.1
- 2-10 keV flux= 1.1x10-12 erg/s/cm2
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Masetti et al. 2008:
- Optical spectroscopy is presented and detailed
- Fluxes of Hβ and [OIII] are given
- Sey 1.2 at z=0.052
- MBH=62 x 107 Msun
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Zhang et al. 2009 (A&A):
- Detect the source in 1.4 Ms of INTEGRAL data with σ20-60 keV=9.4 sigma
- Source is therefore a real source
- Confirm the proposed associations with a Swift
X-ray source and a Sey 1.2 AGN.
- Rather steady in flux at hard X-rays, while it shows up to 39 % flux variations at soft X-rays
- Joint XRT-ISGRI spectrum well fitted by an absorbed power law:
NH=8.73 x1020 cm-2; Γ=2.11.
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