The ALMA-CRISTAL survey: Resolved kinematic studies of main sequence star-forming galaxies at 4 < z < 6

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Volume 701 (September 2025)

A&A, 701 (2025) A260

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Table 1.

Properties of the 32 galaxies in kinematics sample of ALMA-CRISTAL.

CRISTAL ID	Full name	z_[C II]	RA	Dec	$log (\frac{M_{⋆}}{M_{⊙}})$ $\log{\Big(\frac{M_\star}{\mathrm{M_\odot}}\Big)}$	$log [\frac{SFR}{(M_{⊙} {yr}^{- 1})}]$ $\log{\Big[\frac{\mathrm{SFR}}{(\mathrm{M_\odot}\,\mathrm{yr}^{-1})}\Big]}$ a	Beam size	Cube Noiseb
			(°)	(°)	(dex)	(dex)		(mJy beam⁻¹)
01a	DC_842313	4.554	150.2271	2.5762	10.65	2.31	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 42 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 47	0.13
01b	...	4.530	150.2282	2.5745	9.81	1.71	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 42 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 47	0.13
02	DC_848185, HZ6, LBG-1	5.294	150.0896	2.5864	10.30	2.25	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 45 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 55	0.13
03	DC_536534, HZ1	5.689	149.9719	2.1182	10.40	1.79	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 68 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 82	0.15
04a	vc_5100822662	4.520	149.7413	2.0809	10.15	1.89	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 57 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 75	0.18
04b	vc_5100822662	4.520	149.7414	2.0813	8.91	0.63	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 57 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 75	0.16
05	DC_683613, HZ3	5.541	150.0393	2.3372	10.16	1.83	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 31 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 38	0.16
06a	vc_5100541407	4.562	150.2538	1.8094	10.09	1.62	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 45 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 54	0.13
06b	...	4.562	150.2542	1.8097	9.19	1.07	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 45 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 54	0.13
07a	DC_873321, HZ8	5.154	150.0169	2.6266	10.00	1.89	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 49 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 74	0.18
07b	...	5.154	150.0166	2.6268	...	...	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 49 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 74	0.18
07c	...	5.155	150.0134	2.6271	10.21	1.92	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 49 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 74	0.18
08	vuds_efdcs_530029038	4.430	53.0793	–27.8771	9.85	1.88	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 54 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 80	0.17
09a	DC_519281	5.575	149.7537	2.0910	9.84	1.51	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 33 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 36	0.16
10a	DC_417567, HZ2	5.671	150.5172	1.9290	9.99	1.86	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 44 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 48	0.09
10a-E	...	5.671	150.5186	1.9304	...	...	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 44 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 48	0.09
11	DC_630594	4.439	150.1358	2.2579	9.68	1.57	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 38 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 47	0.22
12	CG_21	5.572	53.0498	–27.6993	9.30	0.98	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 42 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 58	0.12
13	vc_5100994794	4.579	150.1715	2.2873	9.65	1.51	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 44 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 52	0.18
14	DC_709575	4.411	149.9461	2.3758	9.53	1.45	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 11 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 12	0.15
15	vc_5101244930	4.580	150.1986	2.3006	9.69	1.44	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 36 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 42	0.17
16a	CG_38	5.571	53.0662	–27.6901	9.60	1.30	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 42 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 58	0.14
19	DC_494763	5.233	150.0213	2.0534	9.51	1.45	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 31 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 40c	0.15
20d	DC_494057, HZ4	5.545	149.6188	2.0518	10.11	1.82	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 41 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 45	0.06
21d	HZ7	5.255	149.8769	2.1341	10.11	1.80	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 32 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 35	0.22
22ad	HZ10	5.653	150.2471	1.5554	10.35	2.13	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 27 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 34	0.22
22bd	HZ10	5.653	150.2469	1.5554	...		0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 27 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 34	0.22
23ae	DC_818760	4.560	150.4786	2.5421	10.55	2.50	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 25 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 30	0.35
23be	DC_818760	4.562	150.4790	2.5421	10.46	1.72	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 25 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 30	0.35
23ce	...	4.565	150.4778	2.5421	...	...	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 25 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 30	0.35
24e	DC_873756	4.546	150.0113	2.6278	10.53	2.06	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 26 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 31	0.46
25e	vc_5101218326	4.573	150.3021	2.3146	10.90	2.75	0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 25 × 0 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 30	0.38

Notes. DC, vc, and CG stand for the following: DEIMOS_COSMOS, vuds_cosmos and CANDELS_GOODSS, respectively. CRISTAL-01c, 07d, 09b, 10b, 16b, 17, 18 are not included in this study because they are either too faint for kinematics analysis or not detected. SMG J1000+0234 and CRLE are excluded because they are starburst galaxies. A full table with all CRISTAL source is available in Table 1 of Herrera-Camus et al. (2025). aAdopted from Mitsuhashi et al. (2024) and Li et al. (2024). They are in broad agreement with the values inferred from existing L_[C II]-SFR relations as demonstrated by Li et al. (2024) and references therein. bCube noise are measured in cubes with 20 km s⁻¹ channel width. cBriggs-weighted data is used. dCRISTAL pilot targets. eFrom ALMA archive.

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