MIGHTEE H I observations of low surface brightness and ultra-diffuse galaxies in the XMM-LSS field

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Table 4.

Comparison of photometric measurements.

Names	Property^a	This work	G18/L23
J021642.0-044221/	g − i	0.42 ± 0.04	0.43 ± 0.24
G267	m_i	18.85 ± 0.03	18.89 ± 0.24
	r_eff (″)^b	6.44 ± 0.42	6.27 ± 0.79
	${\bar{μ}}_{eff, g}$ $Mathematical equation: $ \overline{\mu}_{\mathrm{eff,g}} $$ ^c	25.18 ± 0.25	25.30 ± 0.24

J021759.3-041634/	g − i	0.59 ± 0.09	0.66 ± 0.05
L25657	m_i	17.07 ± 0.04	17.02 ± 0.07
	r_eff (″)^b	10.21 ± 0.76	8.52 ± 0.35
	${\bar{μ}}_{eff, g}$ $Mathematical equation: $ \overline{\mu}_{\mathrm{eff,g}} $$ ^c	24.66 ± 0.18	24.33 ± 0.05

J022138.1-052631/	g − i	0.54 ± 0.01	0.43 ± 0.05
L86749	m_i	16.73 ± 0.01	18.99 ± 0.08
	r_eff (″)^b	11.17 ± 0.48	5.37 ± 0.31
	${\bar{μ}}_{eff, g}$ $Mathematical equation: $ \overline{\mu}_{\mathrm{eff,g}} $$ ^c	24.24 ± 0.15	25.06 ± 0.06

Notes.

^(a)

Not corrected for extinction.

^(b)

Measured in the i band.

^(c)

${\bar{μ}}_{eff, g} = m_{g} + 2.5 {log}_{10} (2 π r_{eff}^{2})$ $Mathematical equation: $ \overline{\mu}_{\mathrm{eff,g}} = m_g + 2.5\log_{10}{(2\pi r_{\mathrm{eff}}^2)} $$ .

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