Table 5.

Spectroscopic and photometric redshifts for the 16 galaxies labelled in Fig. 1. Dashes indicate any values that are unavailable.

GalaxySpectroscopic zaPhotometric zb
10.0869|$0.114 \pm 0.0241$|
20.0893|$0.107 \pm 0.0254$|
30.0887|$0.138 \pm 0.0138$|
40.0882|$0.102 \pm 0.0136$|
50.0877|$0.108 \pm 0.0137$|
60.0880|$0.120 \pm 0.0269$|
7|$0.118 \pm 0.0128$|
80.0893|$0.087 \pm 0.0090$|
90.0856|$0.101 \pm 0.0117$|
100.0894|$0.109 \pm 0.0196$|
110.0849
120.0901|$0.091 \pm 0.0124$|
130.0926|$0.068 \pm 0.0220$|
140.0831|$0.091 \pm 0.0084$|
150.0838|$0.114 \pm 0.0195$|
16|$0.132 \pm 0.0512$|
GalaxySpectroscopic zaPhotometric zb
10.0869|$0.114 \pm 0.0241$|
20.0893|$0.107 \pm 0.0254$|
30.0887|$0.138 \pm 0.0138$|
40.0882|$0.102 \pm 0.0136$|
50.0877|$0.108 \pm 0.0137$|
60.0880|$0.120 \pm 0.0269$|
7|$0.118 \pm 0.0128$|
80.0893|$0.087 \pm 0.0090$|
90.0856|$0.101 \pm 0.0117$|
100.0894|$0.109 \pm 0.0196$|
110.0849
120.0901|$0.091 \pm 0.0124$|
130.0926|$0.068 \pm 0.0220$|
140.0831|$0.091 \pm 0.0084$|
150.0838|$0.114 \pm 0.0195$|
16|$0.132 \pm 0.0512$|
a

Cited from Sargent (1972).

b

Cited from Ahumada et al. (2020).

Table 5.

Spectroscopic and photometric redshifts for the 16 galaxies labelled in Fig. 1. Dashes indicate any values that are unavailable.

GalaxySpectroscopic zaPhotometric zb
10.0869|$0.114 \pm 0.0241$|
20.0893|$0.107 \pm 0.0254$|
30.0887|$0.138 \pm 0.0138$|
40.0882|$0.102 \pm 0.0136$|
50.0877|$0.108 \pm 0.0137$|
60.0880|$0.120 \pm 0.0269$|
7|$0.118 \pm 0.0128$|
80.0893|$0.087 \pm 0.0090$|
90.0856|$0.101 \pm 0.0117$|
100.0894|$0.109 \pm 0.0196$|
110.0849
120.0901|$0.091 \pm 0.0124$|
130.0926|$0.068 \pm 0.0220$|
140.0831|$0.091 \pm 0.0084$|
150.0838|$0.114 \pm 0.0195$|
16|$0.132 \pm 0.0512$|
GalaxySpectroscopic zaPhotometric zb
10.0869|$0.114 \pm 0.0241$|
20.0893|$0.107 \pm 0.0254$|
30.0887|$0.138 \pm 0.0138$|
40.0882|$0.102 \pm 0.0136$|
50.0877|$0.108 \pm 0.0137$|
60.0880|$0.120 \pm 0.0269$|
7|$0.118 \pm 0.0128$|
80.0893|$0.087 \pm 0.0090$|
90.0856|$0.101 \pm 0.0117$|
100.0894|$0.109 \pm 0.0196$|
110.0849
120.0901|$0.091 \pm 0.0124$|
130.0926|$0.068 \pm 0.0220$|
140.0831|$0.091 \pm 0.0084$|
150.0838|$0.114 \pm 0.0195$|
16|$0.132 \pm 0.0512$|
a

Cited from Sargent (1972).

b

Cited from Ahumada et al. (2020).

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