Electronic Telegram No. 5625 Central Bureau for Astronomical Telegrams Mailing address: Hoffman Lab 209; Harvard University; 20 Oxford St.; Cambridge, MA 02138; U.S.A. e-mail: cbatiau@eps.harvard.edu (alternate cbat@iau.org) URL http://www.cbat.eps.harvard.edu/index.html Prepared using the Tamkin Foundation Computer Network COMET 3I/ATLAS J. Crovisier, N. Biver, and D. Bockelee-Morvan, LIRA, Observatoire de Paris, PSL University, report observations of the 18-cm line of OH in comet 3I/ATLAS with the Nancay radio telescope. From co-added observations obtained during Oct. 13-19, the 1667-MHz OH line intensity was 74 +/- 7 mJy*km/s, corresponding to a production rate Q[OH] = 5.7 +/- 0.6 10**28 molecules/s, assuming a standard Haser model with an inversion of 0.50 for the OH doublet ground state. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2025 CBAT 2025 October 21 (CBET 5625) Daniel W. E. Green