Table 1: List of brightest compact sources and their Flux Densities ( FD) inside OA184 and VRO42.05.01.
Source num. GLONG GLAT FD at 408 MHz FD at 1420 MHz Sp. index

deg deg mJy mJy $\alpha$

For OA184

1 165.887 2.055 664 $\pm$ 20 229 $\pm$ 9 0.86 (0.81 to 0.90)

2 165.735 2.450 309 $\pm$ 33 273 $\pm$ 22 0.10 (-0.05 to 0.25)

3 166.198 3.120 196 $\pm$ 8 93 $\pm$ 4 0.60 (0.56 to 0.65)

4 166.006 2.425 182 $\pm$ 6 88 $\pm$ 3 0.58 (0.54 to 0.62)

5 166.605 2.803 150 $\pm$ 10 60 $\pm$ 3 0.74 (0.67 to 0.81)

6 166.615 3.175 121 $\pm$ 7 53 $\pm$ 3 0.66 (0.60 to 0.73)

7 166.604 3.077 96 $\pm$ 7 24 $\pm$ 3 1.10 (0.99 to 1.23)

8 166.211 2.359 90 $\pm$ 6 36 $\pm$ 2 1.74 (1.68 to 0.81)

9 166.195 2.768 59 $\pm$ 4 31 $\pm$ 1 0.67 (0.61 to 0.75)

10 166.440 2.850 50 $\pm$ 4 28 $\pm$ 1 0.46 (0.40 to 0.52)

11 165.990 3.036 47 $\pm$ 14 14 $\pm$ 5 1.00 (0.68 to 1.53)

12 166.391 3.169 45 $\pm$ 5 17 $\pm$ 2 0.78 (0.66 to 0.92)

13 166.535 2.102 45 $\pm$ 3 31 $\pm$ 1 0.30 (0.25 to 0.36)

14 166.821 2.345 40 $\pm$ 5 26 $\pm$ 1 0.35 (0.25 to 0.47)

15 166.878 2.826 39 $\pm$ 10 20 $\pm$ 4 0.54 (0.32 to 0.85)

16 165.895 2.316 26 $\pm$ 7 14 $\pm$ 4 0.49 (0.24 to 0.84)

17 165.926 1.839 20 $\pm$ 2 10 $\pm$ 1 0.60 (0.50 to 0.71)

For VRO42.05.01

1 166.327 4.024 151 $\pm$ 17 70 $\pm$ 10 0.62 (0.41 to 0.83)

2 166.327 4.040 73 $\pm$ 16 35 $\pm$ 10 0.59 (0.34 to 0.96)

3 166.696 4.351 53 $\pm$ 4 26 $\pm$ 1 0.57 (0.50 to 0.65)

**Table 1:** List of brightest compact sources and their Flux Densities ( FD) inside OA184 and VRO42.05.01.
Source num.	GLONG	GLAT	FD at 408 MHz	FD at 1420 MHz	Sp. index
	deg	deg	mJy	mJy	$\alpha$
For OA184
1	165.887	2.055	664 $\pm$ 20	229 $\pm$ 9	0.86 (0.81 to 0.90)
2	165.735	2.450	309 $\pm$ 33	273 $\pm$ 22	0.10 (-0.05 to 0.25)
3	166.198	3.120	196 $\pm$ 8	93 $\pm$ 4	0.60 (0.56 to 0.65)
4	166.006	2.425	182 $\pm$ 6	88 $\pm$ 3	0.58 (0.54 to 0.62)
5	166.605	2.803	150 $\pm$ 10	60 $\pm$ 3	0.74 (0.67 to 0.81)
6	166.615	3.175	121 $\pm$ 7	53 $\pm$ 3	0.66 (0.60 to 0.73)
7	166.604	3.077	96 $\pm$ 7	24 $\pm$ 3	1.10 (0.99 to 1.23)
8	166.211	2.359	90 $\pm$ 6	36 $\pm$ 2	1.74 (1.68 to 0.81)
9	166.195	2.768	59 $\pm$ 4	31 $\pm$ 1	0.67 (0.61 to 0.75)
10	166.440	2.850	50 $\pm$ 4	28 $\pm$ 1	0.46 (0.40 to 0.52)
11	165.990	3.036	47 $\pm$ 14	14 $\pm$ 5	1.00 (0.68 to 1.53)
12	166.391	3.169	45 $\pm$ 5	17 $\pm$ 2	0.78 (0.66 to 0.92)
13	166.535	2.102	45 $\pm$ 3	31 $\pm$ 1	0.30 (0.25 to 0.36)
14	166.821	2.345	40 $\pm$ 5	26 $\pm$ 1	0.35 (0.25 to 0.47)
15	166.878	2.826	39 $\pm$ 10	20 $\pm$ 4	0.54 (0.32 to 0.85)
16	165.895	2.316	26 $\pm$ 7	14 $\pm$ 4	0.49 (0.24 to 0.84)
17	165.926	1.839	20 $\pm$ 2	10 $\pm$ 1	0.60 (0.50 to 0.71)
For VRO42.05.01
1	166.327	4.024	151 $\pm$ 17	70 $\pm$ 10	0.62 (0.41 to 0.83)
2	166.327	4.040	73 $\pm$ 16	35 $\pm$ 10	0.59 (0.34 to 0.96)
3	166.696	4.351	53 $\pm$ 4	26 $\pm$ 1	0.57 (0.50 to 0.65)

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and image analysis
	3 Results
	4 Discussion
	5 Conclusion
	References