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1 z > 4 Radio-loud 2 Z. -Q. Shen VLBI

2

3

4 J ; z = pc Frey et al Figure 1. VLBI images at 1.6 GHz of three very high-redshift q left), J (z = 6.12, middle), and J (z = 6.2 are given in Frey et al. (2015), Frey et al. (2008), and Frey et a A prevalence of gigahertz peaked-spectrum (GPS) and co sources, which are believed to be young (i.e., being at earlie frustrated (i.e., confined by the dense interstellar medium) been predicted by Savage & Peterson (1983) and analysed by addressed samples of quasars at considerably lower redshifts the spectra and morphologies identified in the object J ) and suspected in J at z =6.21 (Frey et a what would be expected in a young GPS/CSS source.

5 J ; z = pc Frey et al Stanghelini et al., 2006 νc Figure 1. VLBI images at 1.6 GHz of < 500 three MHz, veryd = high-redshift 1-20 kpc q left), J (z = 6.12, middle), and J (z = 6.2 νc are given in Frey et al. (2015), Frey et = al. 1 -(2008), 5 GHz, and d < 1 Frey kpc et a νc > 5 GHz, d < 1 kpc A prevalence of gigahertz peaked-spectrum (GPS) and co sources, which are believed to be young (i.e., being at earlie frustrated (i.e., confined by the dense interstellar medium) been predicted by Savage & Peterson (1983) and analysed by addressed samples of quasars at considerably lower redshifts the spectra and morphologies identified in the object J ) and suspected in J at z =6.21 (Frey et a what would be expected in a young GPS/CSS source. ν < νc α = 5/2 ν > νc

6 βapp = 10c J ; z = pc Frey et al, 2013

7 βapp = 10c J ; z = pc Frey et al, 2013 FSRQ Blazar BL Lac z > 4.5

8 βapp = 10c J ; z = pc Frey et al, 2013 FSRQ Blazar BL Lac z > 4.5 Blazar Radio Galaxy Blazar CSO z = 4-6; e.g. Romani et al. 2006

9 z > 4

10

11 z z [20 m] [20 m] [20 m] [20 m] [32 m] [32 m] [34 m] [32 m] 2300 km EPOCH 1 [32 MHz] EPOCH 2 [32 MHz] EPOCH 3 [512 MHz] 8.4 GHz θ ~ 3.1 mas

12

13 Epoch Name Detection Peak flux r.m.s. Beam size SED (mjy/beam) (mas mas) (mjy) 1 J ± J ± J ± J ± J ± J < J ± J ± J ±

14 dcore = dbeam dcore < dmin dcore = dmin δ β: weight S/N: Signal to Noise Ratio (Fomalont 1999) TB,eq = K; Readhead 1994 Epoch Name Core size Total flux T b δ L (mas) (mjy) (K) (10 26 WHz 1 ) 1 J < ( ) 54.2 ± 1.2 > > J < ( ) 44.6 ± 1.9 > > (8.7 ± 0.4) J < ( ) 34.9 ± 1.4 > (8.3 ± 0.3) 10 5 > (5.3 ± 0.2) J ± 15.8 (25 ± 3) ± J < ± 62.1 > (15 ± 2) > 1.0 ± J < ± 2.5 > (4.3 ± 0.4) 10 9 > (2.7 ± 0.2) J < ± 1.9 > 6.5 ± > (4.1 ± 0.4) J < ± 1.6 > 4.7 ± > (2.9 ± 0.4)

15 Peak flux density [mjy] (1996) (1998) (2001) (2003) *x**(-0.21) *x**(-0.55) *x**(-0.43) 83.13*x**(0.28) Peak flux density [mjy] (1998) (1994) (2004/4/30) (2004/5/8) (2004/5/27) *x**(-0.025) *x**(0.017) *x**(0.46) *x**(0.43) *x**(0.44) 1 10 Frequency [GHz] Frequency [GHz] 1 10 δ > 1 α > - 0.5

16 δ > 10-6 δ > 10-6 δ > 10-2 δ > 10-2 δ > 10-2

17 L8.4GHz α 1 "Coppejans_alpha.txt" using 1:2:3 "Shen_sources.txt" using 1:2:3 "Shen_sources2.txt" using 1:2:3 20 "shen_alpha_hist.txt" using 1:($2+$3) "shen_alpha_hist.txt" using 1: α Number redshift α

18 L8.4GHz α 1 "Coppejans_alpha.txt" using 1:2:3 "Shen_sources.txt" using 1:2:3 "Shen_sources2.txt" using 1:2:3 20 "shen_alpha_hist.txt" using 1:($2+$3) "shen_alpha_hist.txt" using 1: α Number redshift α z = 4-5 α ~ 0 z > 5 α ~ -1 z ~ 4 z ~ 6

19 L8.4GHz α 1 "Coppejans_alpha.txt" using 1:2:3 "Shen_sources.txt" using 1:2:3 "Shen_sources2.txt" using 1:2:3 20 "shen_alpha_hist.txt" using 1:($2+$3) "shen_alpha_hist.txt" using 1: α Number redshift α z = 4-5 α ~ 0 z > 5 α ~ -1 z ~ 4 z ~ 6

20

atomic line spectrum emission line absorption line atom proton neutron nuclei electron Z atomic number A mass number neutral atom ion energy

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