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 2.

ALMA CO(3–2) line emitters.

ID_1.2 mm ⁽¹⁾	C1	C3	C4
z_CO ⁽²⁾	$2 . 2529_{- 0.0003}^{+ 0.0003}$ $2.2529^{+0.0003}_{-0.0003}$	$2 . 2954_{- 0.0005}^{+ 0.0005}$ $2.2954^{+0.0005}_{-0.0005}$	$2 . 3676_{- 0.0003}^{+ 0.0003}$ $2.3676^{+0.0003}_{-0.0003}$
SΔv ⁽³⁾ (Jy beam⁻¹ km s⁻¹)	$0 . 63_{- 0.06}^{+ 0.06}$ $0.63^{+0.06}_{-0.06}$	$0 . 24_{- 0.06}^{+ 0.06}$ $0.24^{+0.06}_{-0.06}$	$0 . 23_{- 0.04}^{+ 0.04}$ $0.23^{+0.04}_{-0.04}$
FWHM ⁽⁴⁾ (km s⁻¹)	$510_{- 50}^{+ 50}$ $510^{+50}_{-50}$	$330_{- 80}^{+ 120}$ $330^{+120}_{-80}$	$320_{- 40}^{+ 50}$ $320^{+50}_{-40}$
L_CO ⁽⁵⁾ (10⁷ L_⊙)	$2 . 3_{- 0.2}^{+ 0.2}$ $2.3^{+0.2}_{-0.2}$	$0 . 9_{- 0.2}^{+ 0.2}$ $0.9^{+0.2}_{-0.2}$	$0 . 95_{- 0.14}^{+ 0.14}$ $0.95^{+0.14}_{-0.14}$
$L_{CO}^{'}^{(6)} (10^{10} K km s^{- 1} {pc}^{2})$ $L^{\prime }_{\rm CO}\,^{(6)}\,({\rm 10^{10}\,K\,km\,s^{-1}\,pc^2})$	$1 . 77_{- 0.17}^{+ 0.17}$ $1.77^{+0.17}_{-0.17}$	$0 . 70_{- 0.18}^{+ 0.18}$ $0.70^{+0.18}_{-0.18}$	$0 . 72_{- 0.10}^{+ 0.11}$ $0.72^{+0.11}_{-0.10}$

Notes. Derived properties from the CO(3–2) line. ⁽¹⁾Identifier of ALMA 1.2-mm continuum-selected galaxies. ⁽²⁾Redshift estimate for the CO(3–2) line. 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 Eqs. (2) and (3).

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