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| Miscellaneous :
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Landi et al. 2011 ATel
3185:
- Swift reveals two possible X-ray counterparts => 1st (compatible
with 1RXS J065230.8+533130) is favoured
- QORG J065231.2+533130 has B=18.3 and R=17.7, and is also
detected in 2MASS with J ~17, H ~16 and K ~15
- X-ray spectrum is well fitted by a power law with Gamma=1.8
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Halpern et al. ATel
3186:
- Optical observation of the suggested optical counterpart
in USNO B1.0 at R.A. = 06h 52m 31.407s, Decl. = +53d 31' 31.55" and
having B2 = 18.80, R2 = 18.12, I2 = 17.57
- Detection of [O III] 5007,4959 and broad Balmer emission lines
at z = 0.301
- => broad-line QSO a possible identification of the IGR
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Masetti et al. 2012 ATel
3186:
- Optical spectroscopy
- Source is a broad line AGN, Sey 1.2 at z=0.301
- MBH=3.6 x 107 Msun
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