TITLE: GCN CIRCULAR NUMBER: 14974 SUBJECT: IPN localization of GRB 130702A (= Fermi 394416326) DATE: 13/07/03 19:03:54 GMT FROM: Kevin Hurley at UCBerkeley/SSL K. Hurley and J. Goldsten, on behalf of the MESSENGER NS GRB team, V. Connaughton, M. S. Briggs, C. Meegan, and V. Pelassa, on behalf of the Fermi GBM team, S. Golenetskii, R. Aptekar, E. Mazets, V. Pal'shin, D. Frederiks, D. Svinkin, and T. Cline, on behalf of the Konus-Wind team, and A. von Kienlin, X. Zhang, A. Rau, V. Savchenko, E. Bozzo, and C. Ferrigno, on behalf of the INTEGRAL SPI-ACS GRB team, report: MESSENGER (GRNS), INTEGRAL (SPI-ACS), Fermi-GBM, and Konus-Wind have detected GRB 130702A (= Fermi 394416326) so far. We have triangulated this burst to an annulus centered at RA, Dec (2000) = 293.0106 degrees, -18.3126 degrees, whose radius is 82.0991 +/- 0.4594 degrees (3 sigma). The distance between the annulus center line and the iPTF optical transient reported by Singer et al. (GCN 14967) is 0.16 degrees, strengthening the association of the transient with the GRB. A map has been posted at ssl.berkeley.edu/ipn3/130702 showing the annulus, the Fermi LAT position (GCN 14971), and the optical transient. This localization may be improved.