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| Miscellaneous :
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Rodriguez et al. 2008:
- Refined X-ray position => Optical and IR counterpart
- Blend of sources at optical not excluded
- J=9.617, H=9.245, K=9.130, V=11.0, B=11.3, U<11.9, mUVM2=12.5, mUV>2=20.2
- Absorbed power law fits 0.5-9 keV spectra well, Γ= 3
NH<0.3 x1022cm-2; F2-10 keV=8.2 x 10-14 erg/s/cm2
- Black body also fits the spectrum well, kT=0.26 keV
- Distance not greater than 1kpc, then NS XRB or CV.
- If much closer than 1kpc, CV favoured
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Ratti et al. 2010:
- Chandra and Optical observations
- Source is probably not a CV given the very soft Swift spectrum
- confirm the association of IGR/Chandra source with TYC and 2MASS sources
- Source is a LMXB or IMXB
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Ratti et al. 2013 (MRAS):
- Phase resolved spectro and photmetry of optical counterpart
- Optical spectra dominated by absorption features+ 10-20 % contribution from disc
- Orbital period 14.662 hr
- Mass ratio M2/M1=1.78 => large for stable Roche lobe overflow
- Inclination 50°
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