.dvi
or
.ps
format.
Circular No. 7384 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/iau/cbat.html ISSN 0081-0304 Phone 617-495-7244/7440/7444 (for emergency use only) SUPERNOVAE 2000R, 2000S, 2000T, 2000U, 2000V, 2000W, 2000X A. Amadon and G. Blanc, Service de Physique des Particules (SPP), Centre d'Etude de Saclay (CES); J. Haissinski, Laboratoire de l'Accelerateur Lineaire, Orsay; and J. Rich, SPP/CES, on behalf of the EROS collaboration, report the discovery of seven supernovae discovered in the course of the automated supernovae search with the European Southern Observatory (ESO) 1-m Marly telescope at La Silla (limiting mag about 21.5). Each supernova was found by subtraction of CCD images from reference images taken one year ago. SN 2000 UT R.A. (2000.0) Decl. V Offset 2000R Feb. 27 10 01 21.27 - 6 33 57.4 19.4 1".6 W, 1".7 S 2000S Feb. 28 10 34 55.89 - 6 28 26.0 20.9 3".9 E, 10".9 S 2000T Mar. 3 12 36 20.35 -12 28 23.3 21.0 2".7 W, 0".9 S 2000U Mar. 4 12 45 27.90 -12 10 34.3 20.2 3".9 W, 1".5 N 2000V Mar. 6 12 03 28.64 - 5 47 15.7 20.6 3".8 W, 0".6 S 2000W Mar. 9 11 10 59.53 - 4 43 46.8 20.4 6".4 E, 3".5 S 2000X Mar. 10 11 30 45.41 - 5 12 16.8 20.2 8".0 E, 5".7 S SN 2000R was confirmed via a CCD spectrum taken at the ESO 3.6-m telescope by C. Coutures (CES, ESO) on Mar. 6 that suggests it is a type-IIL supernova in its nebular phase with z = 0.01. SN 2000S in MCG -01-27-020 was also confirmed by Coutures with a CCD spectrum taken on Mar. 9, the data being consistent with a type-Ic event in its nebular phase, with z = 0.02. Spectra by Coutures on Mar. 6 and 9 of SNe 2000T and 2000V, respectively, are consistent with type-Ia supernovae near maxima and z = 0.18 and 0.10. SNe 2000U, 2000W, and 2000X were each confirmed by CCD images taken at the Marly telescope about 2 days after discovery, and these three appear to have been found premaximum. SN 2000U increased in brightness by about 0.5 mag between Mar. 4 and 12; SN 2000W increased by about 0.6 mag between Mar. 8 and 15; SN 2000X increased by about 0.5 mag between Mar. 10 and 15. V382 VELORUM Visual magnitude estimates by A. Pearce, Nedlands, W. Australia: Feb. 13.780 UT, 9.7; 16.823, 9.7; Mar. 5.769, 9.8; 6.790, 9.8; 7.781, 9.9; 13.771, 9.9; 15.781, 9.9; 17.794, 10.1. (C) Copyright 2000 CBAT 2000 March 20 (7384) Daniel W. E. Green
.dvi
or
.ps
format.
Our Web policy. Index to the CBAT/MPC/ICQ pages.