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Table 1

Summary of SALT observations.

Object Outburst Date Spectra Hα + [N ii] Imaging Known

name Year Time sincea exposure exposure nebular
(yr) (s) (s) remnant

T Pyx 2011b 1 27.02.2012 3 × 60 Yes1,2
21.03.2012 2 × 300 + 40
U Sco 2010b 2 29.04.2012 250 4 × 60
V445 Pup 2000 12 13.04.2012 2 × 35 3 × 40 Yes3
V382 Vel 1999 13 30.11.2011 2 × 130 1 × 60 Yes4
CP Cru 1996 16 27.02.2012 3 × 60 Yes5,6
01.03.2012 900
BY Cir 1995 17 25.02.2012 180 3 × 60
V888 Cen 1995 17 13.02.2012 130 6 × 60
V868 Cen 1991 21 26.01.2012 2015 2 × 60
V842 Cen 1986 26 13.02.2012 100 2 × 60 Yes7
GQ Mus 1983 29 01.04.2012 2 × 300 3 × 60
Nova Car 1972 1972 40 17.12.2011 180 3 × 60
HS Pup 1963 49 11.03.2012 380 3 × 60 Yes7
HZ Pup 1963 49 11.03.2012 130 3 × 60
V365 Car 1948 64 12.02.2012 300 1 × 60
CP Pup 1942 70 02.01.2012 3 × 60 Yes8
01.04.2012 40 2 × 60
BT Mon 1939 73 15.12.2011 130 3 × 60 Yes9
RR Pic 1925 87 07.11.2011 6 3 × 10 Yes8
GI Mon 1918 94 16.12.2011 3 × 60
01.01.2012 2 × 130
OY Ara 1910 102 22.09.2011 150 10 × 60
CN Vel 1905 107 16.01.2012 300 2 × 60
X Ser 1903 109 02.03.2012 2 × 60
12.03.2012 300
DY Pup 1902 110 13.03.2012 950 1 × 60 Yes7

Notes.

(a)

In all tables, figures, and Sect. 4 the objects are ordered by the time since the outburst.

(b)

Recurrent nova: only the most recent outburst is shown in the table.

Reference. (1) Williams (1982); (2) Schaefer et al. (2010); (3) Woudt et al. (2009a); (4) this paper; (5) Ringwald et al. (1998); (6) Downes & Duerbeck (2000); (7) Gill & O’Brien (1998); (8) Duerbeck (1987a); (9) Marsh et al. (1983).

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