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Table 2.

Observed objects.

Slit RA Dec r/R25 Class, Notice
3 23:57:50.2 −32:34:46 0.25 SC
4 23:57:47.1 −32:35:19 0.14 SCa
8 23:57:45.3 −32:33:41 0.71 EL nebula
9 23:57:43.9 −32:35:43 0.27 SCc
10 23:57:44.5 −32:34:13 0.55 SC
11 23:57:45.7 −32:36:30 0.39 SC
12 23:57:44.8 −32:34:08 0.57 SC
13 23:57:48.8 −32:34:54 0.22 EL nebula
14 23:57:40.3 −32:36:20 0.50 SC
15 23:57:39.9 −32:35:15 0.48 SCd
16 23:57:41.0 −32:34:52 0.49 EL nebulae
17 23:57:42.3 −32:36:36 0.49 SCf
18 23:57:43.1 −32:34:23 0.54 SC
19 23:57:41.4 −32:36:36 0.52 SC
20 23:57:38.9 −32:35:00 0.56 SC
21 23:57:42.7 −32:35:57 0.35 SCg
22 23:57:39.3 −32:37:25 0.78 WN10h
23 23:57:37.3 −32:34:50 0.66 SC
24 23:57:37.6 −32:35:39 0.56 SCi
25 23:57:38.3 −32:36:20 0.57 EL nebula
26 23:57:35.5 −32:34:50 0.74 EL nebula
28 23:57:34.0 −32:36:00 0.73 SC
29 23:57:36.6 −32:35:13 0.63 SC
30 23:57:35.8 −32:35:41 0.64 SCj
32 23:57:33.0 −32:34:31 0.90 SC

Notes. Columns list: (1) slit number; (2) and (3) right ascension and declination (J2000); (4) deprojected distance from the centre of the galaxy; and (5) object classification based on our spectroscopic and photometric data analysis.

(a)

Whitmore et al. (2014)-002; within 5″ of SNR (Blair & Long 1997).

(b)

Within ∼12″ of SNR-4 (Blair & Long 1997).

(d)

Mora et al. (2009) 1-28.

(e)

Within ∼12″ of SNR-1 (Blair & Long 1997).

(f)

Mora et al. (2009) 1-18.

(g)

Within ∼4″ of SNR-4 (Blair & Long 1997).

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