Masetti et al. 2013

Bibinfo (this paper at ADS): Masetti, N., Parisi, P, Palazzi, E., Jimenez-Bailon, E., Chavushyan, V., McBride, V., Rojas, A.F., Steward, L., Bassani, L., Bazzano, A., Bird, A.J., Charles, P.A., Galaz, G., Landi, R., Malizia, A., Mason, E., Minniti, D., Morelli, L., Schiavone, F., Stephen, J.B., Ubertini, P., 2013, A&A, 556, A120 (21 pp.).
Type: Observational: Optical identification.
Object(s): Swift J0958.0-4208, IGR J14257-6117, IGR J17014-4306, IGR J18051-1052, and AX J1832.3-0840, among 33 Integral sources.
Results: Five CVs identified as counterparts of Integral sources. Of these, the spectrum of Swift J0958.0-4208 is strongly suggestive of a polar; AX J1832.3-0840 has a proposed spin period; the other three could turn out to be IPs.

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