The MUSE Ultra Deep Field (MUDF) - VII. Probing high-redshift gas structures in the surroundings of ALMA-identified massive dusty galaxies

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Volume 696 (April 2025)

A&A, 696 (2025) A33

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Table B.1.

Properties of the additional emission lines of the ALMA-identified sources.

ID_1.2mm⁽¹⁾	C2 (QSO-SE)	C6
Line	CO(4–3)	[CI]_609 μm
z_line⁽²⁾	$3 . 2267_{- 0.0005}^{+ 0.0007}$ $3.2267^{+0.0007}_{-0.0005}$	$1 . 0544_{- 0.0003}^{+ 0.0004}$ $1.0544^{+0.0004}_{-0.0003}$
SΔv⁽³⁾(Jy beam⁻¹ km s⁻¹)	$0 . 70_{- 0.17}^{+ 0.18}$ $0.70^{+0.18}_{-0.17}$	$0 . 36_{- 0.09}^{+ 0.10}$ $0.36^{+0.10}_{-0.09}$
FWHM⁽⁴⁾(km s⁻¹)	$288_{- 80}^{+ 130}$ $288^{+130}_{-80}$	$448_{- 110}^{+ 150}$ $448^{+150}_{-110}$
L_line⁽⁵⁾(10⁷ L_⊙)	$6 . 4_{- 1.5}^{+ 1.7}$ $6.4^{+1.7}_{-1.5}$	$0 . 50_{- 0.10}^{+ 0.10}$ $0.50^{+0.10}_{-0.10}$
$L_{line}^{'}$ $L^{\prime }_{\rm line}$ ⁽⁶⁾ (10¹⁰ K km s⁻¹ pc²)	$2 . 1_{- 0.5}^{+ 0.5}$ $2.1^{+0.5}_{-0.5}$	$0 . 12_{- 0.03}^{+ 0.04}$ $0.12^{+0.04}_{-0.03}$

Notes.

⁽¹⁾

Identifier of ALMA 1.2-mm continuum-selected galaxies.

⁽²⁾

Redshift estimate for the emission lines. All reported uncertainties correspond to 1σ confidence interval as derived from the 16th and 84th percentile of the posterior probability distribution.

⁽³⁾

Velocity-integrated line flux.

⁽⁴⁾

Full Width at Half Maximum of the line.

^(5,6)

Line luminosities as derived from Eq. (2) and (3).

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