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IAUC 8117: 2003dm, 2003dn, 2003do, 2003dp, 2003dq, 2003dr; 2003cx, 2003dc

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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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