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Circular No. 8117
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)
CBAT@CFA.HARVARD.EDU (science)
URL http://cfa-www.harvard.edu/iau/cbat.html ISSN 0081-0304
Phone 617-495-7440/7244/7444 (for emergency use only)
SUPERNOVAE 2003dm, 2003dn, 2003do, 2003dp, 2003dq, 2003dr
Several additional supernovae found on unfiltered CCD images
have been reported -- SN 2003dr in NGC 5714 independently by T.
Puckett and D. Toth (cf. IAUC 8045) and by M. Schwartz and P. R.
Holvorcem (LOTOSS/Tenagra II; cf. IAUC 8111), and the rest by W. M.
Wood-Vasey, G. Aldering, P. Nugent, and A. Kulkarni (NEAT; cf. IAUC
8115). The tabulated data for SN 2003dr below are from Puckett.
SN 2003 UT R.A. (2000.0) Decl. Mag. Offset
2003dm Mar. 22.20 11 31 38.15 +25 34 14.3 19.2 2" W, 1" N
2003dn Apr. 7.30 11 20 08.03 +25 36 48.7 20.0 6" S
2003do Apr. 8.29 13 03 29.37 +27 19 11.1 19.9 1".4 E, 1".3 S
2003dp Apr. 8.36 13 13 24.23 +27 56 09.3 20.0 3".1 W
2003dq Apr. 10.15 11 04 45.44 +15 26 49.4 18.9 0".3 E, 1".9 S
2003dr Apr. 13.18 14 38 11.13 +46 38 03.4 18.0 3".7 W, 13".9 S
Additional approximate magnitudes from the respective observers:
2003dm, 2002 Mar. 31.38, [20.9; 2003 Jan. 19.54, [20.5; Apr. 7.33,
19.7. 2003dn, 2002 Mar. 31.37, [21.0; 2003 Feb. 21.50, [20.7; Apr.
10.15, 20.0. 2003do, 2002 Apr. 9.21, [21.6; 20.25, [20.9; 2003 Mar.
22.40, 20.2; Apr. 11.32, 19.9. 2003dp, 2002 May 3.21, [21.4; 2003
Mar. 22.40, [21.1; Apr. 11.32, 20.0. 2003dq, 2002 Apr. 2.27, [21.8;
2003 Mar. 24.16, [21.5; 25.24, [21.3; Apr. 9.42, 19.0. SN 2003dr,
1997 July 1, [21.0 (Palomar Sky Survey, via Puckett); 2003 Mar. 24,
[20.5 (Puckett); Apr. 8.3, [18.5 (Holvorcem); 12.4, 17.9
(Holvorcem); 14.16, 18.0 (Puckett); 14.4, 17.9 (Holvorcem).
SUPERNOVAE 2003cx AND 2003dc
M. Hamuy, Carnegie Observatories, reports that a spectrum
(range 370-900 nm) of SN 2003cx (cf. IAUC 8105), obtained on Apr.
10.39 UT with the Las Campanas Observatory Clay 6.5-m telescope (+
LDSS-2), shows it to be a normal type-II supernova with Balmer
lines exhibiting P-Cyg profiles. The expansion velocity of -10000
km/s, derived from the minimum of H_alpha (based on a redshift of
0.037, derived for the host galaxy from superimposed narrow
emission Balmer lines), and the relatively blue continuum suggest
that SN 2003cx is about 2-3 weeks old. A spectrum of SN 2003dc
(cf. IAUC 8111), taken on Apr. 10.37, shows it to be a type-Ia
supernova near maximum light. The minimum of the Si II 635.5-nm
line yields an expansion velocity of -10060 km/s (based on a
redshift of 0.067, derived for the host galaxy from superimposed
narrow H_alpha emission).
(C) Copyright 2003 CBAT
2003 April 14 (8117) Daniel W. E. Green
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