MUSE Analysis of Gas around Galaxies (MAGG) - VII. Emission line galaxies near strong blended Lyα absorption systems at z ≳ 3

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Table 1.

Statistics of LAEs and wavelength bins with F < 0.25 and Δv_spec = 138 km s⁻¹ associated with each other within |Δv| ≤ 300 km s⁻¹ and R ≤ 300 kpc.

	−0.05 < F < 0.05	0.05 < F < 0.15	0.15 < F < 0.25
$N_{SBLAs}^{(a)}$ $Mathematical equation: $ N_\mathrm{{SBLAs}}^{(a)} $$	164	275	442
$f_{SBLAs}^{(b)}$ $Mathematical equation: $ f_\mathrm{{SBLAs}}^{(b)} $$	0.45	0.27	0.19

Notes. ^(a)Total number of wavelength bins per interval of transmission. ^(b)Fraction of wavelength bins identified in each interval of transmission that is also associated with at least one LAE.

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