Assessing the impact of two independent direction-dependent calibration algorithms on the LOFAR 21 cm signal power spectrum - And applications to an observation of a field flanking the north celestial pole

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Volume 669 (January 2023)

A&A, 669 (2023) A20

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Table B.2

Summary of the CLEAN component model and its clustering.

Cluster	Position (J2000.0) RA [hour], Dec [deg]	Number of sources	Maximum flux [Jy]	Total flux density [Jy]	Maximum separation [deg]
1	13^h 46^m06.446^s +85°30′02.564″	212	5.185	71.87	2.134
2	15^h 38^m57.775^s +86°46′08.711″	205	6.400	61.51	1.343
3	16^h 44^m56.439^s +82°00′46.566″	157	4.060	52.54	1.394
4	17^h 46^m29.922^s +85°25′39.948″	218	5.876	49.19	1.268
5	19^h 15^m00.497^s +84°26′46.767″	153	4.471	48.08	1.267
6	21^h 04^m07.835^s +84°12′30.181″	152	8.257	47.69	1.570
7	22^h 54^m00.975^s +88°23′08.218″	238	5.684	45.48	2.149
8	20^h 01^m40.512^s +85°59′54.030″	184	6.044	43.34	1.397
9	15^h 58^m32.933^s +84°33′04.712″	196	22.737	41.71	1.364
10	18^h 26^m15.815^s +87°37′23.340″	220	3.209	38.07	1.502
11	12^h 22^m01.146^s +88°28′52.985″	246	2.873	37.40	1.850
12	15^h 55^m46.173^s +81°59′38.825″	147	5.261	35.62	1.776
13	20^h 05^m39.918^s +83°06′40.170″	119	2.061	33.69	1.286
14	22^h 23^m24.174^s +86°16′28.896″	186	5.828	29.83	2.521
15	19^h 21^m26.177^s +82°13′33.547″	95	2.762	25.27	1.489
16	17^h 39^m37.842^s +82°09′27.905″	106	2.050	22.13	1.053
17	18^h 20^m56.808^s +83° 20v57.184″	150	1.014	21.49	1.097
18	17^h 04^m01.348^s +83°46′54.388″	155	2.962	21.04	1.173
19	15^h 08^m22.540^s +83°36′40.085″	166	2.361	20.83	1.440
20	18^h 31^m11.244^s +81°33′30.857″	84	2.125	19.51	1.250

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