Electronic Telegram No. 5260 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 V6597 SAGITTARII = NOVA SAGITTARII 2023 No. 2 = TCP J17583414-2652300 Koichi Itagaki, Yamagata, Japan, reported his discovery of a variable star (unfiltered mag 12.0) on digital images obtained on May 16.698 UT with a 106-mm refractor (+ CMOS camera), with the position given as R.A. = 17h58m34s.14, Decl. = -26d52'30".0 (equinox J2000.0). When Itagaki posted the discovery to the Central Bureau's TOCP webpage, the provisional designation TCP J17583414-2652300 was automatically given. Additional CCD magnitudes for TCP J17583414-2652300 received by the Central Bureau: May 15.920, 13.1 (K. Sokolovsky, S. Korotkiy, N. Potapov, O. Smolyankina, A. Prokudina, and S. Ostapenko, 135-mm f/2.0 telephoto lens + unfiltered SBIG ST-8300M camera; pre-discovery); May 16.745, V = 13.91, R_c= 12.41, I_c = 11.03 (S. Kiyota, Kamagaya, Japan, 0.28-m reflector; annotated image posted at website URL https://meineko.com/ccd/TCP_J17583414-2652300.jpg); May 17.636, V = 14.77, B = 17.09 (A. Pearce, Nedlands, W. Australia, using a 0.35-m R-COP reflector at Perth Observatory; position end figures 34s.19, 29".5 using Gaia DR2 stars); May 18.07, 14.4 (Sokolovsky et al., 80-mm refractor + Canon EOS 600D camera); May 18.656, V = 14.90, I = 10.99, R = 12.76, B = 17.30 (Pearce). Sokolovsky et al. have posted their images at the following website URL: http://scan.sai.msu.ru/~kirx/img/TCPJ17583414-2652300/. K. Taguchi and K. Isogai, University of Kyoto, report on spectroscopy obtained by Taguchi on May 16.78 UT with a fiber-fed integral field spectrograph (KOOLS-IFU) on the 3.8-m telescope Seimei at the Okayama observatory of Kyoto University. The spectrum (resolution about 500) shows absorption velocities with P-Cyg profiles of -570 km/s for H-alpha and -450 km/s for O I 777.3-nm, with Taguchi judging this to be a slow-rising classical nova that is highly reddened. E. Kazarovets writes that the permanent GCVS designation V6597 Sgr has been assigned to this nova. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2023 CBAT 2023 May 19 (CBET 5260) Daniel W. E. Green