SIMBAD references

R. J. Ivison, Royal Observatory, Edinburgh; and T. B. Lowe, James Clerk Maxwell Telescope, report flux densities for V4743 Sgr at various wavelengths with SCUBA, RxA3, and RxB3 detectors (0.45-1.4 mm) and with the Very Large Array (3.6 cm; uncertainties </= 25 percent in flux): Oct. 11.9 UT, VLA, < 0.12 mJy; 12.2, 0.45 mm, 369 ± 63; 12.2, 0.85 mm, 100 ± 10; 27.0, VLA, 0.20; 27.3, 0.85 mm, 177 ± 22; Nov. 6.2, 1.3 mm, 115 ± 23; 15.0, VLA, 1.21; 15.1, 0.9 mm, 276 ± 79; 15.1, 1.4 mm, 199 ± 57. The VLA source is located at R.A. = 19h01m09s.32, Decl. = -22o00'06".1 (equinox 2000.0; uncertainties </= 0".5).