All Figures

	Figure 1: Section (about 10 ) of the ISGRI mosaic of the two outbursts in the energy range 17-40 keV, with a net exposure time of 42.7 ks. Equatorial coordinates (J2000) are displayed.
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In the text

Figure 2: J-band image of the IGR J11215-5952 field (data taken from UK Schmidt telescope, and provided by the online Digitized Sky Survey, available at http://heasarc.gsfc.nasa.gov/). North to the top, East to the left. The large solid circle marks the ISGRI error circle (3' radius) from the 2005 outburst (Lubinski et al. 2005, ATel 496); the two thin smaller circles indicate the error regions from the analysis of the outbursts occurred in 2003 and 2004. The smaller thick solid circle indicates the error region derived in the mosaic of the two outburst in 2003 and 2004. The arrow indicates HD 306414, the likely optical counterpart (Negueruela et al. 2005).

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In the text

	Figure 3: Left: IGR J11215-5952 photon spectrum from the 2003 outburst (JEM-X and ISGRI, 5-100 keV) fit with a cutoff power law. Right: IGR J11215-5952 photon spectrum (only ISGRI data, 20-100 keV) from the 2004 outburst, fit with a single power law (see the text for the best fit parameters).
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In the text

	Figure 4: 68%, 90% and 99% confidence level contours for the photon index and the cutoff energy from the spectral analysis of the emission during the 2003 outburst.
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In the text