Comparing extragalactic megahertz-peaked spectrum and gigahertz-peaked spectrum sources

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Table B.2.

144 MHz normalized differential radio source counts for the MPS sample of Slob et al. (2022)

⟨S_144 MHz⟩ [Jy]	N_S	$S^{5 / 2} d N / {ds}_{- σ}^{+ σ} [{Jy}^{1.5} / sr]$ $S^{5/2}\rm{d}N/\rm{ds}^{+\sigma}_{-\sigma}[\rm{Jy^{1.5}/sr}]$
0.06	101	$10 . 06_{- 1.00}^{+ 1.10}$ $10.06 ^{+ 1.10 }_{- 1.00 }$
0.12	81	$22 . 83_{- 2.53}^{+ 2.83}$ $22.83 ^{+ 2.83 }_{- 2.53 }$
0.24	63	$46 . 68_{- 5.86}^{+ 6.65}$ $46.68 ^{+ 6.65 }_{- 5.86 }$
0.45	29	$53 . 40_{- 9.85}^{+ 11.86}$ $53.40 ^{+ 11.86 }_{- 9.85 }$
0.86	22	$91 . 34_{- 19.31}^{+ 23.90}$ $91.34 ^{+ 23.90 }_{- 19.31}$
2.65	18	$207 . 4_{- 48.4}^{+ 61.3}$ $207.4 ^{+ 61.3 }_{- 48.4 }$

Notes. ⟨S⟩ is the central flux density of every flux bin in Jy, N_s is the number of sources in each bin, and $N_{- σ}^{+ σ}$ $N^{+\sigma}_{-\sigma}$ are the normalized differential source counts in [Jy^1./sr].

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