Table 1. Open in new tab ZFOURGE sources...

ID	RA_ZFOURGE^†	Dec_ZFOURGE^†	ID	S _ALMA	S/N_peak	RA_ALMA	Dec_ALMA	\|Δ_offset\|	p-value	\|$z$\| _photo	\|$z$\| _spec	Chandra
18658	53.18341	−27.77646	1	0.985 ± 0.036	25.995	53.18348	−27.77666	0.735	0.0578	2.83\|$^{+0.07}_{-0.08}$\|	—	Y
17856	53.11880	−27.78289	2	1.973 ± 0.075	25.625	53.11881	−27.78288	0.048	0.0003	2.38\|$^{+0.17}_{-0.10}$\|	—	Y
13086	53.14885	−27.82119	3	1.748 ± 0.070	24.008	53.14885	−27.82119	0.021	0.0	2.58\|$^{+0.04}_{-0.04}$\|	2.582	Y
18645	53.18137	−27.77756	4	0.906 ± 0.041	21.045	53.18137	−27.77757	0.044	0.0002	2.92\|$^{+0.06}_{-0.06}$\|	—
18701	53.16061	−27.77622	5	0.735 ± 0.039	18.101	53.16063	−27.77628	0.228	0.0057	2.61\|$^{+0.07}_{-0.05}$\|	2.543^‡	Y
22177	53.19835	−27.74788	6	0.922 ± 0.074	12.421	53.19830	−27.74790	0.153	0.0026	1.93\|$^{+0.04}_{-0.03}$\|	—	Y
20298	53.13735	−27.76163	7	0.778 ± 0.086	8.785	53.13710	−27.76141	1.124	0.13	0.52\|$^{+0.02}_{-0.01}$\|	0.523
19033	53.13112	−27.77319	8	0.610 ± 0.072	8.654	53.13115	−27.77320	0.084	0.0008	2.22\|$^{+0.03}_{-0.03}$\|	2.225	Y
21234	53.19656	−27.75704	9	0.457 ± 0.055	8.575	53.19656	−27.75708	0.123	0.0017	2.46\|$^{+0.05}_{-0.05}$\|	—
18912	53.17092	−27.77547	10	0.261 ± 0.031	8.550	53.17091	−27.77544	0.099	0.0011	2.36\|$^{+0.10}_{-0.11}$\|	—
21730	53.12185	−27.75278	11	0.635 ± 0.078	8.506	53.12186	−27.75277	0.071	0.0006	2.01\|$^{+0.06}_{-0.04}$\|	—	Y
16952	53.15405	−27.79093	12	0.376 ± 0.049	7.378	53.15401	−27.79087	0.251	0.0069	1.88\|$^{+0.04}_{-0.03}$\|	1.317^‡
17733	53.14349	−27.78328	13	0.400 ± 0.053	7.227	53.14351	−27.78329	0.05	0.0003	1.62\|$^{+0.04}_{-0.05}$\|	1.415^‡
18336	53.18053	−27.77972	14	0.238 ± 0.035	7.178	53.18053	−27.77971	0.038	0.0002	2.67\|$^{+0.11}_{-0.15}$\|	—	Y
15702	53.16692	−27.79882	15	0.416 ± 0.064	6.637	53.16694	−27.79881	0.082	0.0007	1.93\|$^{+0.03}_{-0.03}$\|	1.998	Y
19487	53.16558	−27.76987	16	0.488 ± 0.065	6.491	53.16562	−27.76991	0.194	0.0041	1.61\|$^{+0.08}_{-0.06}$\|	1.551^‡	Y
12438	53.20235	−27.82627	18	0.975 ± 0.172	5.803	53.20236	−27.82629	0.063	0.0004	1.07\|$^{+0.03}_{-0.03}$\|	—	Y
14580	53.18585	−27.81004	19	0.387 ± 0.073	5.659	53.18585	−27.81004	0.024	0.0001	2.81\|$^{+0.10}_{-0.10}$\|	2.593	Y
18270	53.14617	−27.77995	23	0.182 ± 0.037	5.360	53.14620	−27.77995	0.096	0.001	2.61\|$^{+0.05}_{-0.06}$\|	—	Y
14146	53.18201	−27.81420	26	0.222 ± 0.052	4.923	53.18198	−27.81420	0.107	0.0013	2.41\|$^{+0.18}_{-0.14}$\|^§	—	Y
14419	53.16144	−27.81116	29	0.197 ± 0.046	4.835	53.16141	−27.81114	0.115	0.0015	2.77\|$^{+0.11}_{-0.10}$\|	—	Y
13714	53.14167	−27.81665	31	0.733 ± 0.158	4.714	53.14175	−27.81670	0.328	0.0118	2.53\|$^{+0.09}_{-0.10}$\|	—	Y
14122	53.11914	−27.81402	33	0.318 ± 0.079	4.701	53.11911	−27.81405	0.136	0.002	3.32\|$^{+0.44}_{-0.45}$\|	—
14700	53.12011	−27.80834	44	1.768 ± 0.447	4.546	53.12018	−27.80825	0.401	0.0175	1.83\|$^{+0.05}_{-0.05}$\|	—

RA_ZFOURGE^†

Dec_ZFOURGE^†

S _ALMA

S/N_peak

RA_ALMA

Dec_ALMA

|Δ_offset|

p-value

|$z$| _photo

|$z$| _spec

Chandra

(ZFOURGE)

(°)

(ASAGAO)

(mJy)

(°)

(^″)

counterpart?

(1)

(2)

(3)

(4)

(5)

(6)

(7)

(8)

(9)

(10)

(11)

(12)

(13)

18658

53.18341

−27.77646

0.985 ± 0.036

25.995

53.18348

−27.77666

0.735

0.0578

2.83|$^{+0.07}_{-0.08}$|

—

17856

53.11880

−27.78289

1.973 ± 0.075

25.625

53.11881

−27.78288

0.048

0.0003

2.38|$^{+0.17}_{-0.10}$|

—

13086

53.14885

−27.82119

1.748 ± 0.070

24.008

53.14885

−27.82119

0.021

0.0

2.58|$^{+0.04}_{-0.04}$|

2.582

18645

53.18137

−27.77756

0.906 ± 0.041

21.045

53.18137

−27.77757

0.044

0.0002

2.92|$^{+0.06}_{-0.06}$|

—

18701

53.16061

−27.77622

0.735 ± 0.039

18.101

53.16063

−27.77628

0.228

0.0057

2.61|$^{+0.07}_{-0.05}$|

2.543^‡

22177

53.19835

−27.74788

0.922 ± 0.074

12.421

53.19830

−27.74790

0.153

0.0026

1.93|$^{+0.04}_{-0.03}$|

—

20298

53.13735

−27.76163

0.778 ± 0.086

8.785

53.13710

−27.76141

1.124

0.13

0.52|$^{+0.02}_{-0.01}$|

0.523

19033

53.13112

−27.77319

0.610 ± 0.072

8.654

53.13115

−27.77320

0.084

0.0008

2.22|$^{+0.03}_{-0.03}$|

2.225

21234

53.19656

−27.75704

0.457 ± 0.055

8.575

53.19656

−27.75708

0.123

0.0017

2.46|$^{+0.05}_{-0.05}$|

—

18912

53.17092

−27.77547

0.261 ± 0.031

8.550

53.17091

−27.77544

0.099

0.0011

2.36|$^{+0.10}_{-0.11}$|

—

21730

53.12185

−27.75278

0.635 ± 0.078

8.506

53.12186

−27.75277

0.071

0.0006

2.01|$^{+0.06}_{-0.04}$|

—

16952

53.15405

−27.79093

0.376 ± 0.049

7.378

53.15401

−27.79087

0.251

0.0069

1.88|$^{+0.04}_{-0.03}$|

1.317^‡

17733

53.14349

−27.78328

0.400 ± 0.053

7.227

53.14351

−27.78329

0.05

0.0003

1.62|$^{+0.04}_{-0.05}$|

1.415^‡

18336

53.18053

−27.77972

0.238 ± 0.035

7.178

53.18053

−27.77971

0.038

0.0002

2.67|$^{+0.11}_{-0.15}$|

—

15702

53.16692

−27.79882

0.416 ± 0.064

6.637

53.16694

−27.79881

0.082

0.0007

1.93|$^{+0.03}_{-0.03}$|

1.998

19487

53.16558

−27.76987

0.488 ± 0.065

6.491

53.16562

−27.76991

0.194

0.0041

1.61|$^{+0.08}_{-0.06}$|

1.551^‡

12438

53.20235

−27.82627

0.975 ± 0.172

5.803

53.20236

−27.82629

0.063

0.0004

1.07|$^{+0.03}_{-0.03}$|

—

14580

53.18585

−27.81004

0.387 ± 0.073

5.659

53.18585

−27.81004

0.024

0.0001

2.81|$^{+0.10}_{-0.10}$|

2.593

18270

53.14617

−27.77995

0.182 ± 0.037

5.360

53.14620

−27.77995

0.096

0.001

2.61|$^{+0.05}_{-0.06}$|

—

14146

53.18201

−27.81420

0.222 ± 0.052

4.923

53.18198

−27.81420

0.107

0.0013

2.41|$^{+0.18}_{-0.14}$|^§

—

14419

53.16144

−27.81116

0.197 ± 0.046

4.835

53.16141

−27.81114

0.115

0.0015

2.77|$^{+0.11}_{-0.10}$|

—

13714

53.14167

−27.81665

0.733 ± 0.158

4.714

53.14175

−27.81670

0.328

0.0118

2.53|$^{+0.09}_{-0.10}$|

—

14122

53.11914

−27.81402

0.318 ± 0.079

4.701

53.11911

−27.81405

0.136

0.002

3.32|$^{+0.44}_{-0.45}$|

—

14700

53.12011

−27.80834

1.768 ± 0.447

4.546

53.12018

−27.80825

0.401

0.0175

1.83|$^{+0.05}_{-0.05}$|

—

ID	RA_ZFOURGE^†	Dec_ZFOURGE^†	ID	S _ALMA	S/N_peak	RA_ALMA	Dec_ALMA	\|Δ_offset\|	p-value	\|$z$\| _photo	\|$z$\| _spec	Chandra
18658	53.18341	−27.77646	1	0.985 ± 0.036	25.995	53.18348	−27.77666	0.735	0.0578	2.83\|$^{+0.07}_{-0.08}$\|	—	Y
17856	53.11880	−27.78289	2	1.973 ± 0.075	25.625	53.11881	−27.78288	0.048	0.0003	2.38\|$^{+0.17}_{-0.10}$\|	—	Y
13086	53.14885	−27.82119	3	1.748 ± 0.070	24.008	53.14885	−27.82119	0.021	0.0	2.58\|$^{+0.04}_{-0.04}$\|	2.582	Y
18645	53.18137	−27.77756	4	0.906 ± 0.041	21.045	53.18137	−27.77757	0.044	0.0002	2.92\|$^{+0.06}_{-0.06}$\|	—
18701	53.16061	−27.77622	5	0.735 ± 0.039	18.101	53.16063	−27.77628	0.228	0.0057	2.61\|$^{+0.07}_{-0.05}$\|	2.543^‡	Y
22177	53.19835	−27.74788	6	0.922 ± 0.074	12.421	53.19830	−27.74790	0.153	0.0026	1.93\|$^{+0.04}_{-0.03}$\|	—	Y
20298	53.13735	−27.76163	7	0.778 ± 0.086	8.785	53.13710	−27.76141	1.124	0.13	0.52\|$^{+0.02}_{-0.01}$\|	0.523
19033	53.13112	−27.77319	8	0.610 ± 0.072	8.654	53.13115	−27.77320	0.084	0.0008	2.22\|$^{+0.03}_{-0.03}$\|	2.225	Y
21234	53.19656	−27.75704	9	0.457 ± 0.055	8.575	53.19656	−27.75708	0.123	0.0017	2.46\|$^{+0.05}_{-0.05}$\|	—
18912	53.17092	−27.77547	10	0.261 ± 0.031	8.550	53.17091	−27.77544	0.099	0.0011	2.36\|$^{+0.10}_{-0.11}$\|	—
21730	53.12185	−27.75278	11	0.635 ± 0.078	8.506	53.12186	−27.75277	0.071	0.0006	2.01\|$^{+0.06}_{-0.04}$\|	—	Y
16952	53.15405	−27.79093	12	0.376 ± 0.049	7.378	53.15401	−27.79087	0.251	0.0069	1.88\|$^{+0.04}_{-0.03}$\|	1.317^‡
17733	53.14349	−27.78328	13	0.400 ± 0.053	7.227	53.14351	−27.78329	0.05	0.0003	1.62\|$^{+0.04}_{-0.05}$\|	1.415^‡
18336	53.18053	−27.77972	14	0.238 ± 0.035	7.178	53.18053	−27.77971	0.038	0.0002	2.67\|$^{+0.11}_{-0.15}$\|	—	Y
15702	53.16692	−27.79882	15	0.416 ± 0.064	6.637	53.16694	−27.79881	0.082	0.0007	1.93\|$^{+0.03}_{-0.03}$\|	1.998	Y
19487	53.16558	−27.76987	16	0.488 ± 0.065	6.491	53.16562	−27.76991	0.194	0.0041	1.61\|$^{+0.08}_{-0.06}$\|	1.551^‡	Y
12438	53.20235	−27.82627	18	0.975 ± 0.172	5.803	53.20236	−27.82629	0.063	0.0004	1.07\|$^{+0.03}_{-0.03}$\|	—	Y
14580	53.18585	−27.81004	19	0.387 ± 0.073	5.659	53.18585	−27.81004	0.024	0.0001	2.81\|$^{+0.10}_{-0.10}$\|	2.593	Y
18270	53.14617	−27.77995	23	0.182 ± 0.037	5.360	53.14620	−27.77995	0.096	0.001	2.61\|$^{+0.05}_{-0.06}$\|	—	Y
14146	53.18201	−27.81420	26	0.222 ± 0.052	4.923	53.18198	−27.81420	0.107	0.0013	2.41\|$^{+0.18}_{-0.14}$\|^§	—	Y
14419	53.16144	−27.81116	29	0.197 ± 0.046	4.835	53.16141	−27.81114	0.115	0.0015	2.77\|$^{+0.11}_{-0.10}$\|	—	Y
13714	53.14167	−27.81665	31	0.733 ± 0.158	4.714	53.14175	−27.81670	0.328	0.0118	2.53\|$^{+0.09}_{-0.10}$\|	—	Y
14122	53.11914	−27.81402	33	0.318 ± 0.079	4.701	53.11911	−27.81405	0.136	0.002	3.32\|$^{+0.44}_{-0.45}$\|	—
14700	53.12011	−27.80834	44	1.768 ± 0.447	4.546	53.12018	−27.80825	0.401	0.0175	1.83\|$^{+0.05}_{-0.05}$\|	—

RA_ZFOURGE^†

Dec_ZFOURGE^†

S _ALMA

S/N_peak

RA_ALMA

Dec_ALMA

|Δ_offset|

p-value

|$z$| _photo

|$z$| _spec

Chandra

(ZFOURGE)

(°)

(ASAGAO)

(mJy)

(°)

(^″)

counterpart?

(1)

(2)

(3)

(4)

(5)

(6)

(7)

(8)

(9)

(10)

(11)

(12)

(13)

18658

53.18341

−27.77646

0.985 ± 0.036

25.995

53.18348

−27.77666

0.735

0.0578

2.83|$^{+0.07}_{-0.08}$|

—

17856

53.11880

−27.78289

1.973 ± 0.075

25.625

53.11881

−27.78288

0.048

0.0003

2.38|$^{+0.17}_{-0.10}$|

—

13086

53.14885

−27.82119

1.748 ± 0.070

24.008

53.14885

−27.82119

0.021

0.0

2.58|$^{+0.04}_{-0.04}$|

2.582

18645

53.18137

−27.77756

0.906 ± 0.041

21.045

53.18137

−27.77757

0.044

0.0002

2.92|$^{+0.06}_{-0.06}$|

—

18701

53.16061

−27.77622

0.735 ± 0.039

18.101

53.16063

−27.77628

0.228

0.0057

2.61|$^{+0.07}_{-0.05}$|

2.543^‡

22177

53.19835

−27.74788

0.922 ± 0.074

12.421

53.19830

−27.74790

0.153

0.0026

1.93|$^{+0.04}_{-0.03}$|

—

20298

53.13735

−27.76163

0.778 ± 0.086

8.785

53.13710

−27.76141

1.124

0.13

0.52|$^{+0.02}_{-0.01}$|

0.523

19033

53.13112

−27.77319

0.610 ± 0.072

8.654

53.13115

−27.77320

0.084

0.0008

2.22|$^{+0.03}_{-0.03}$|

2.225

21234

53.19656

−27.75704

0.457 ± 0.055

8.575

53.19656

−27.75708

0.123

0.0017

2.46|$^{+0.05}_{-0.05}$|

—

18912

53.17092

−27.77547

0.261 ± 0.031

8.550

53.17091

−27.77544

0.099

0.0011

2.36|$^{+0.10}_{-0.11}$|

—

21730

53.12185

−27.75278

0.635 ± 0.078

8.506

53.12186

−27.75277

0.071

0.0006

2.01|$^{+0.06}_{-0.04}$|

—

16952

53.15405

−27.79093

0.376 ± 0.049

7.378

53.15401

−27.79087

0.251

0.0069

1.88|$^{+0.04}_{-0.03}$|

1.317^‡

17733

53.14349

−27.78328

0.400 ± 0.053

7.227

53.14351

−27.78329

0.05

0.0003

1.62|$^{+0.04}_{-0.05}$|

1.415^‡

18336

53.18053

−27.77972

0.238 ± 0.035

7.178

53.18053

−27.77971

0.038

0.0002

2.67|$^{+0.11}_{-0.15}$|

—

15702

53.16692

−27.79882

0.416 ± 0.064

6.637

53.16694

−27.79881

0.082

0.0007

1.93|$^{+0.03}_{-0.03}$|

1.998

19487

53.16558

−27.76987

0.488 ± 0.065

6.491

53.16562

−27.76991

0.194

0.0041

1.61|$^{+0.08}_{-0.06}$|

1.551^‡

12438

53.20235

−27.82627

0.975 ± 0.172

5.803

53.20236

−27.82629

0.063

0.0004

1.07|$^{+0.03}_{-0.03}$|

—

14580

53.18585

−27.81004

0.387 ± 0.073

5.659

53.18585

−27.81004

0.024

0.0001

2.81|$^{+0.10}_{-0.10}$|

2.593

18270

53.14617

−27.77995

0.182 ± 0.037

5.360

53.14620

−27.77995

0.096

0.001

2.61|$^{+0.05}_{-0.06}$|

—

14146

53.18201

−27.81420

0.222 ± 0.052

4.923

53.18198

−27.81420

0.107

0.0013

2.41|$^{+0.18}_{-0.14}$|^§

—

14419

53.16144

−27.81116

0.197 ± 0.046

4.835

53.16141

−27.81114

0.115

0.0015

2.77|$^{+0.11}_{-0.10}$|

—

13714

53.14167

−27.81665

0.733 ± 0.158

4.714

53.14175

−27.81670

0.328

0.0118

2.53|$^{+0.09}_{-0.10}$|

—

14122

53.11914

−27.81402

0.318 ± 0.079

4.701

53.11911

−27.81405

0.136

0.002

3.32|$^{+0.44}_{-0.45}$|

—

14700

53.12011

−27.80834

1.768 ± 0.447

4.546

53.12018

−27.80825

0.401

0.0175

1.83|$^{+0.05}_{-0.05}$|

—

Table 1.

Open in new tab

ZFOURGE sources with ALMA counterparts.*

ID	RA_ZFOURGE^†	Dec_ZFOURGE^†	ID	S _ALMA	S/N_peak	RA_ALMA	Dec_ALMA	\|Δ_offset\|	p-value	\|$z$\| _photo	\|$z$\| _spec	Chandra
(ZFOURGE)	(°)	(°)	(ASAGAO)	(mJy)		(°)	(°)	(^″)				counterpart?
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)	(12)	(13)
18658	53.18341	−27.77646	1	0.985 ± 0.036	25.995	53.18348	−27.77666	0.735	0.0578	2.83\|$^{+0.07}_{-0.08}$\|	—	Y
17856	53.11880	−27.78289	2	1.973 ± 0.075	25.625	53.11881	−27.78288	0.048	0.0003	2.38\|$^{+0.17}_{-0.10}$\|	—	Y
13086	53.14885	−27.82119	3	1.748 ± 0.070	24.008	53.14885	−27.82119	0.021	0.0	2.58\|$^{+0.04}_{-0.04}$\|	2.582	Y
18645	53.18137	−27.77756	4	0.906 ± 0.041	21.045	53.18137	−27.77757	0.044	0.0002	2.92\|$^{+0.06}_{-0.06}$\|	—
18701	53.16061	−27.77622	5	0.735 ± 0.039	18.101	53.16063	−27.77628	0.228	0.0057	2.61\|$^{+0.07}_{-0.05}$\|	2.543^‡	Y
22177	53.19835	−27.74788	6	0.922 ± 0.074	12.421	53.19830	−27.74790	0.153	0.0026	1.93\|$^{+0.04}_{-0.03}$\|	—	Y
20298	53.13735	−27.76163	7	0.778 ± 0.086	8.785	53.13710	−27.76141	1.124	0.13	0.52\|$^{+0.02}_{-0.01}$\|	0.523
19033	53.13112	−27.77319	8	0.610 ± 0.072	8.654	53.13115	−27.77320	0.084	0.0008	2.22\|$^{+0.03}_{-0.03}$\|	2.225	Y
21234	53.19656	−27.75704	9	0.457 ± 0.055	8.575	53.19656	−27.75708	0.123	0.0017	2.46\|$^{+0.05}_{-0.05}$\|	—
18912	53.17092	−27.77547	10	0.261 ± 0.031	8.550	53.17091	−27.77544	0.099	0.0011	2.36\|$^{+0.10}_{-0.11}$\|	—
21730	53.12185	−27.75278	11	0.635 ± 0.078	8.506	53.12186	−27.75277	0.071	0.0006	2.01\|$^{+0.06}_{-0.04}$\|	—	Y
16952	53.15405	−27.79093	12	0.376 ± 0.049	7.378	53.15401	−27.79087	0.251	0.0069	1.88\|$^{+0.04}_{-0.03}$\|	1.317^‡
17733	53.14349	−27.78328	13	0.400 ± 0.053	7.227	53.14351	−27.78329	0.05	0.0003	1.62\|$^{+0.04}_{-0.05}$\|	1.415^‡
18336	53.18053	−27.77972	14	0.238 ± 0.035	7.178	53.18053	−27.77971	0.038	0.0002	2.67\|$^{+0.11}_{-0.15}$\|	—	Y
15702	53.16692	−27.79882	15	0.416 ± 0.064	6.637	53.16694	−27.79881	0.082	0.0007	1.93\|$^{+0.03}_{-0.03}$\|	1.998	Y
19487	53.16558	−27.76987	16	0.488 ± 0.065	6.491	53.16562	−27.76991	0.194	0.0041	1.61\|$^{+0.08}_{-0.06}$\|	1.551^‡	Y
12438	53.20235	−27.82627	18	0.975 ± 0.172	5.803	53.20236	−27.82629	0.063	0.0004	1.07\|$^{+0.03}_{-0.03}$\|	—	Y
14580	53.18585	−27.81004	19	0.387 ± 0.073	5.659	53.18585	−27.81004	0.024	0.0001	2.81\|$^{+0.10}_{-0.10}$\|	2.593	Y
18270	53.14617	−27.77995	23	0.182 ± 0.037	5.360	53.14620	−27.77995	0.096	0.001	2.61\|$^{+0.05}_{-0.06}$\|	—	Y
14146	53.18201	−27.81420	26	0.222 ± 0.052	4.923	53.18198	−27.81420	0.107	0.0013	2.41\|$^{+0.18}_{-0.14}$\|^§	—	Y
14419	53.16144	−27.81116	29	0.197 ± 0.046	4.835	53.16141	−27.81114	0.115	0.0015	2.77\|$^{+0.11}_{-0.10}$\|	—	Y
13714	53.14167	−27.81665	31	0.733 ± 0.158	4.714	53.14175	−27.81670	0.328	0.0118	2.53\|$^{+0.09}_{-0.10}$\|	—	Y
14122	53.11914	−27.81402	33	0.318 ± 0.079	4.701	53.11911	−27.81405	0.136	0.002	3.32\|$^{+0.44}_{-0.45}$\|	—
14700	53.12011	−27.80834	44	1.768 ± 0.447	4.546	53.12018	−27.80825	0.401	0.0175	1.83\|$^{+0.05}_{-0.05}$\|	—

ID	RA_ZFOURGE^†	Dec_ZFOURGE^†	ID	S _ALMA	S/N_peak	RA_ALMA	Dec_ALMA	\|Δ_offset\|	p-value	\|$z$\| _photo	\|$z$\| _spec	Chandra
(ZFOURGE)	(°)	(°)	(ASAGAO)	(mJy)		(°)	(°)	(^″)				counterpart?
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)	(12)	(13)
18658	53.18341	−27.77646	1	0.985 ± 0.036	25.995	53.18348	−27.77666	0.735	0.0578	2.83\|$^{+0.07}_{-0.08}$\|	—	Y
17856	53.11880	−27.78289	2	1.973 ± 0.075	25.625	53.11881	−27.78288	0.048	0.0003	2.38\|$^{+0.17}_{-0.10}$\|	—	Y
13086	53.14885	−27.82119	3	1.748 ± 0.070	24.008	53.14885	−27.82119	0.021	0.0	2.58\|$^{+0.04}_{-0.04}$\|	2.582	Y
18645	53.18137	−27.77756	4	0.906 ± 0.041	21.045	53.18137	−27.77757	0.044	0.0002	2.92\|$^{+0.06}_{-0.06}$\|	—
18701	53.16061	−27.77622	5	0.735 ± 0.039	18.101	53.16063	−27.77628	0.228	0.0057	2.61\|$^{+0.07}_{-0.05}$\|	2.543^‡	Y
22177	53.19835	−27.74788	6	0.922 ± 0.074	12.421	53.19830	−27.74790	0.153	0.0026	1.93\|$^{+0.04}_{-0.03}$\|	—	Y
20298	53.13735	−27.76163	7	0.778 ± 0.086	8.785	53.13710	−27.76141	1.124	0.13	0.52\|$^{+0.02}_{-0.01}$\|	0.523
19033	53.13112	−27.77319	8	0.610 ± 0.072	8.654	53.13115	−27.77320	0.084	0.0008	2.22\|$^{+0.03}_{-0.03}$\|	2.225	Y
21234	53.19656	−27.75704	9	0.457 ± 0.055	8.575	53.19656	−27.75708	0.123	0.0017	2.46\|$^{+0.05}_{-0.05}$\|	—
18912	53.17092	−27.77547	10	0.261 ± 0.031	8.550	53.17091	−27.77544	0.099	0.0011	2.36\|$^{+0.10}_{-0.11}$\|	—
21730	53.12185	−27.75278	11	0.635 ± 0.078	8.506	53.12186	−27.75277	0.071	0.0006	2.01\|$^{+0.06}_{-0.04}$\|	—	Y
16952	53.15405	−27.79093	12	0.376 ± 0.049	7.378	53.15401	−27.79087	0.251	0.0069	1.88\|$^{+0.04}_{-0.03}$\|	1.317^‡
17733	53.14349	−27.78328	13	0.400 ± 0.053	7.227	53.14351	−27.78329	0.05	0.0003	1.62\|$^{+0.04}_{-0.05}$\|	1.415^‡
18336	53.18053	−27.77972	14	0.238 ± 0.035	7.178	53.18053	−27.77971	0.038	0.0002	2.67\|$^{+0.11}_{-0.15}$\|	—	Y
15702	53.16692	−27.79882	15	0.416 ± 0.064	6.637	53.16694	−27.79881	0.082	0.0007	1.93\|$^{+0.03}_{-0.03}$\|	1.998	Y
19487	53.16558	−27.76987	16	0.488 ± 0.065	6.491	53.16562	−27.76991	0.194	0.0041	1.61\|$^{+0.08}_{-0.06}$\|	1.551^‡	Y
12438	53.20235	−27.82627	18	0.975 ± 0.172	5.803	53.20236	−27.82629	0.063	0.0004	1.07\|$^{+0.03}_{-0.03}$\|	—	Y
14580	53.18585	−27.81004	19	0.387 ± 0.073	5.659	53.18585	−27.81004	0.024	0.0001	2.81\|$^{+0.10}_{-0.10}$\|	2.593	Y
18270	53.14617	−27.77995	23	0.182 ± 0.037	5.360	53.14620	−27.77995	0.096	0.001	2.61\|$^{+0.05}_{-0.06}$\|	—	Y
14146	53.18201	−27.81420	26	0.222 ± 0.052	4.923	53.18198	−27.81420	0.107	0.0013	2.41\|$^{+0.18}_{-0.14}$\|^§	—	Y
14419	53.16144	−27.81116	29	0.197 ± 0.046	4.835	53.16141	−27.81114	0.115	0.0015	2.77\|$^{+0.11}_{-0.10}$\|	—	Y
13714	53.14167	−27.81665	31	0.733 ± 0.158	4.714	53.14175	−27.81670	0.328	0.0118	2.53\|$^{+0.09}_{-0.10}$\|	—	Y
14122	53.11914	−27.81402	33	0.318 ± 0.079	4.701	53.11911	−27.81405	0.136	0.002	3.32\|$^{+0.44}_{-0.45}$\|	—
14700	53.12011	−27.80834	44	1.768 ± 0.447	4.546	53.12018	−27.80825	0.401	0.0175	1.83\|$^{+0.05}_{-0.05}$\|	—

*ZFOURGE sources with ALMA counterparts in order of ALMA S/N. Columns: (1) ZFOURGE ID. (2) and (3) ZFOURGE position. (4) ASAGAO ID. (5) Spatially integrated ALMA flux density (de-boosted). (6) ALMA peak S/N. (7) and (8) ASAGAO position. (9) The positional offset between ALMA and ZFOURGE. (10) The p-Values for each ASAGAO source. (11) The photometric redshift. (12) The spectroscopic redshift. (13) Based on cross-matching with the Chandra catalog (Luo et al. 2017); “Y” is assigned if the angular separation between the ALMA and Chandra sources is less than three times their combined 1σ positional error (see also Ueda et al. 2018).

^†The systematic coordinate offsets have been corrected.

^‡The spectroscopic redshift presented by Inami et al. (2017) using MUSE.

^§The photometric redshift presented by Luo et al. (2017).

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