ALMA Lensing Cluster Survey: A spectral stacking analysis of [C II] in lensed z ∼ 6 galaxies

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Volume 652 (August 2021)

A&A, 652 (2021) A128

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Table B.1.

Sample source description.

RA ^(a)	Dec. ^(b)	Redshift ^(c)	Redshift Flag ^(d)	Catalogue ^(e)	Weight ^(f)	Multiple ^(g)	Sub-sample ^(h)
(deg)	(deg)		/precision
Abell_2744
3.5938	−30.4154	6.588	2	R	0.445	–	3
3.5801	−30.4079	6.556	1	R	0.102	–	0
3.5831	−30.4119	6.519	1	R	0.092	–	0
3.5769	−30.3863	6.457	0.01715	AD	0.482	–	0
3.5983	−30.4178	6.400	0.01555	AD	0.049	–	2
3.5728	−30.4145	6.477	0.0185	AD	0.08	–	2

MACS_J0416.1−2403
64.0508	−24.0664	6.148	3	R	0.097	96.3, 97.3	1
64.0482	−24.0624	6.147	3	R	0.122	96.2	3
64.0429	−24.0572	6.145	3	R	0.098	–	1
64.0435	−24.0590	6.147	3	R	0.106	96.1, 97.1	1
64.0478	−24.0621	6.147	3	R	0.121	97.2	3
64.0260	−24.0891	6.15	3	R	0.126	–	1
64.0318	−24.0889	6.405	0.01555	AD	0.76	–	0
64.0325	−24.0557	5.996	0.0195	AD	0.43	–	2
64.0459	−24.0742	6.457	0.01	AD	0.867	–	0
64.0537	−24.0711	6.385	0.01	AD	0.833	–	0
64.0330	−24.0662	6.455	0.0065	AD	1.0	–	2
64.0439	−24.0563	6.161	0.011	AD	0.079	–	0
64.0493	−24.0710	6.147	2	R	0.044	71.3	1
64.0398	−24.0669	5.998	2	R	0.569	77.2	1
64.0364	−24.0622	6.066	2	R	0.169	78.2	1
64.0484	−24.0736	6.066	2	R	0.057	78.3	1
64.0458	−24.0741	5.998	2	R	0.496	77.1	1
64.0517	−24.0695	6.561	2	R	0.047	–	1
64.0556	−24.0638	6.074	2	R	0.06	–	1
64.0520	−24.0705	6.067	2	R	0.043	–	1
64.0460	−24.0582	6.498	1	R	0.161	–	0
64.0410	−24.0641	6.066	3	R	0.196	78.1	1
64.0433	−24.0629	6.147	2	R	0.12	71.2	1
64.0389	−24.0606	6.147	1	R	0.106	71.1	0

Abell_S1063
342.1841	−44.5353	6.107	1LIN	NED	0.463	14.4	1
342.1924	−44.5157	6.50	SPEC	NED	0.417	–	3
342.1909	−44.5375	6.107	SPEC	HFFDS	0.202	14.1	3
342.1811	−44.5346	6.107	SPEC	HFFDS	0.458	14.2	1
342.1841	−44.5317	6.107	SPEC	HFFDS	0.451	14.5	3
342.1890	−44.5300	6.107	SPEC	HFFDS	0.455	14.3	3

MACS_J1149.5+2223
177.3793	22.4033	6.478	0.0185	AD	0.081	–	2

MACS1206.2−0847
181.5511	−8.8037	6.014	3	R	0.591	–	1
181.5533	−8.7988	6.063	2	R	0.347	27.1	1
181.5517	−8.7992	6.06	2	R	0.37	27.2	1

RXJ_1347−1145
206.8921	−11.7483	5.980	1	R	0.324	–	2
206.8762	−11.7386	6.457	3	R	0.344	–	3
206.8832	−11.7563	6.566	3	R	0.341	–	1

MACS0329.7−0211
52.4258	−2.1898	6.011	2	R	0.216	–	1
52.4312	−2.1914	6.026	2	R	0.103	9.1	1
52.4202	−2.1945	6.026	2	R	0.248	9.2	1
52.4169	−2.1977	6.1	2	C	0.259	–	0
52.4281	−2.1964	6.011	2	R	0.246	–	1
52.4310	−2.2044	6.075	1	R	0.06	–	0

MACS1115.9+0129
168.9553	1.4993	6.057	9	C	0.054	–	3

Abell 383
42.0136	−3.5263	6.027	Abell383	R11+KK	0.263	5.1	3
42.0192	−3.5329	6.027	Abell383	R11	0.218	5.2	3

Notes.

^(a)

Right Ascension coordinate of the source (degrees);

^(b)

Declination coordinate of the source (degrees);

^(c)

Redshift of the source;

^(d)

Redshift confidence flag, sources from Richard: 3= highly certain, no doubts, 2= very good, usually one very bright emission line or multiple faint features but matching in redshift, 1= uncertain redshift. Caminha: (2) likely; (3) secure measurement; (9) single line measurement. NED: (SPEC) secure spectroscopic redshift [∼100% reliability], (1LIN) single-line [> 90% reliability]. ASTRODEEP: Photometric redshift precision (Δz < 0.02);

^(e)

Source catalogue provider. R stands for Richard et al. (2021), AD for ASTRODEEP, HFFDS for Hubble Frontier Field DeepSpace, C for Caminha et al. (2019), R11 for Richard et al. (2011) and K for Knudsen et al. (2016);

^(f)

Source weight (normalised, 1/σ²);

^(g)

Image multiplicity, multiple images of the same source are indicated as x.y where x is the source number and y is the image number (from Karman et al. (2017), Richard et al. (2021));

^(h)

Sub-sample: 0 if the source does not belong to any sub-sample, 1 if it belongs to the good-z sub-sample, 2 if it belongs to the high-SFR sub-sample, 3 if it belongs to both the good-z and high-SFR sub-sample.

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