Table 2: PN candidates in NGC 147. Observed [O III]500.7 and H $\alpha$ fluxes are given in 10^-16 erg cm^-2 s^-1. $F_{\rm [OIII]}$ are corrected for the contribution of the companion oxygen line at 495.9 nm.
Id. RA (2000.0) Dec $F_{\rm [OIII]}$ $F_{\rm H\alpha}$ m $_{\rm [O~III]}$

1 0:32:59.97 48:32:26.0 2.63 1.71 25.21

2 0:33:03.78 48:31:25.2 11.7 4.14 23.59

3 0:32:58.79 48:27:40.5 13.8 8.99 23.41

4 0:33:12.66 48:28:18.1 31.8 37.3 22.50

5 0:33:12.29 48:30:09.3 3.05 - 25.05

6 0:33:13.63 48:30:49.4 0.83 5.77 26.46

7 0:33:11.76 48:32:17.8 31.1 12.1 22.53

8 0:34:03.25 48:32:18.3 10.4 0.41 23.72

9 0:34:02.87 48:36:28.0 7.29 3.55 24.10

**Table 2:** PN candidates in NGC 147. Observed [O III]500.7 and H $\alpha$ fluxes are given in 10^-16 erg cm^-2 s^-1. $F_{\rm [OIII]}$ are corrected for the contribution of the companion oxygen line at 495.9 nm.
Id.	RA (2000.0) Dec	$F_{\rm [OIII]}$	$F_{\rm H\alpha}$	m $_{\rm [O~III]}$
1	0:32:59.97	48:32:26.0	2.63	1.71	25.21
2	0:33:03.78	48:31:25.2	11.7	4.14	23.59
3	0:32:58.79	48:27:40.5	13.8	8.99	23.41
4	0:33:12.66	48:28:18.1	31.8	37.3	22.50
5	0:33:12.29	48:30:09.3	3.05	-	25.05
6	0:33:13.63	48:30:49.4	0.83	5.77	26.46
7	0:33:11.76	48:32:17.8	31.1	12.1	22.53
8	0:34:03.25	48:32:18.3	10.4	0.41	23.72
9	0:34:02.87	48:36:28.0	7.29	3.55	24.10

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations
	3 Data reduction and analysis
	4 Results
	5 Summary
	References