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Circular No. 6574 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Mailstop 18, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. IAUSUBS@CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions) BMARSDEN@CFA.HARVARD.EDU or DGREEN@CFA.HARVARD.EDU (science) URL http://cfa-www.harvard.edu/cfa/ps/cbat.html Phone 617-495-7244/7440/7444 (for emergency use only) GRB 970111 P. J. Groot and T. Galama, University of Amsterdam (UoA); J. Telting and R. G. M. Rutten, ING Telescopes, La Palma; and J. van Paradijs, UoA and University of Alabama in Huntsville, report: "We have obtained BVI images of the refined error-box of GRB 970111 (IAUC 6569) on Feb. 28.2 UT with integration times of 930, 405, and 695 s, respectively, and R images (405 s) on Mar. 1.1, using the 4.2-m William Herschel Telescope (prime focus) at La Palma. Comparison with the Digital Sky Survey shows no brightening of sources to V = 19. The three radio sources reported by Galama et al. (IAUC 6571) show no optical counterpart down to V = 24.0. The GRB error box contains two galaxies, at R.A. = 15h28m15s.2, Decl. = +19o35'55" (equinox 2000.0), with V = 20.2, B-V = +1.3, V-R = +0.7, V-I = +1.4; and at R.A. = 15h28m10s.8, Decl. = +19o35'35", with V = 20.5, B-V = +0.5, V-R = +0.4, V-I = +0.9. These galaxies are not detected in the radio observations reported by Galama et al." GRB 970228 Galama; R. Strom, Netherlands Foundation for Research in Astronomy, Dwingeloo, and UoA; van Paradijs; L. Hanlon and K. Bennett, European Space Agency/ESTEC; C. Kouveliotou, Universities Space Research Association; G. Fishman and C. Meegan, NASA Marshall Space Flight Center; J. Heise and J. in 't Zand, SRON, Utrecht; E. Costa, M. Feroci, and L. Piro, Istituto di Astrofisica Spaziale, CNR, Frascati; F. Frontera and G. Zavattini, Universita di Ferrara; L. Nicastro and E. Palazzi, Istituto Tecnologia e Studio Radiazioni Extraterrestri, CNR, Bologna; and K. Hurley, Space Sciences Laboratory, Berkeley, report: "We made radio observations (5 GHz, 3".8 x 17" beamwidth) with the Westerbork array of the SAX/WFC error box of GRB 970228 (IAUC 6572) on Feb. 28 (19.9 hr after the onset of GRB 970228) for 1.2 hr, and on Mar. 1 and 2 for 12 hr each. The error box contains no radio sources above 0.7 mJy (4 sigma)." Groot et al. (above), in 't Zand, Heise, Costa, Feroci, Frontera, and Palazzi further report: "We have obtained V and I images of the error box of GRB 970228 (IAUC 6572) on Mar. 1.0 UT (21 hr after the BeppoSAX trigger) with integration times of 300 s each using the same telescope. Comparison with the Digital Sky Survey shows no brightening of sources to V = 19. A spiral galaxy with V = 20.5 and V-I = +1.3 is located just outside the error box at R.A. = 5h01m46s.0, Decl. = +11o48'19" (equinox 2000.0)." (C) Copyright 1997 CBAT 1997 March 4 (6574) Daniel W. E. Green
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