SIMBAD references

G. C. Anupama, Indian Institute of Astrophysics, Bangalore; and N. G. Kantharia, National Center for Radio Astrophysics, Pune, report the low-frequency radio detection of the current outburst of the recurrent nova RS Oph (cf. IAUC 8671) using the Giant Metrewave Radio Telescope (GMRT), at the following flux densities: Feb. 24.12 UT, 49.5 ± 0.5 mJy at 23.3 cm; Mar. 2.04, 55.4 ± 2.8 mJy at 28.3 cm, 50.0 ± 0.8 mJy at 23.3 cm, and 56.8 ± 0.3 mJy at 21.6 cm; Mar. 5.09, 48.4 ± 2.0 mJy at 49.2 cm. This is the first detection of the nova at wavelengths longer than 21 cm. Further GMRT observations at low frequencies are underway.