Candidate gravitationally lensed submillimeter galaxies in Herschel-ATLAS associated with WISE elliptical counterparts

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Table D.1.

List of candidate lensed galaxies with WISE elliptical counterparts found in H-ATLAS fields.

HATLAS_IAU_ID	θ_H (")	Isolated	z_s	z_l	χ_{r, SMG}²	χ_{r, lens}²	log(M_⋆ / M_⊙)	Rank
J085752.0+012635	3.6	110	2.5 ± 0.7	0.29 ± 0.04	0.29	9.05	11.35 ± 0.13	A
J143931.2+003339	3.2	100	2.6 ± 0.7	0.33 ± 0.04	0.44	7.79	11.34 ± 0.10	A
J144110.6−002759	4.7	100	2.1 ± 0.5	0.47 ± 0.05	0.17	9.77	11.33 ± 0.09	A
J003647.0−282001	3.7	001	1.9 ± 0.6	0.45 ± 0.05	0.29	1.11	11.68 ± 0.08	A
J004840.5−291409	2.4	001	2.4 ± 0.6	0.31 ± 0.07	0.38	1.20	11.19 ± 0.19	A
J005133.5−305926	3.6	000	2.6 ± 0.6	0.52 ± 0.04	0.30	2.76	12.11 ± 0.08	A
J012654.9−300145	2.8	000	2.5 ± 0.6	0.40 ± 0.05	0.37	4.66	12.17 ± 0.11	A
J013411.8−305646	2.4	000	3.4 ± 0.5	0.51 ± 0.08	0.32	1.64	11.70 ± 0.09	A
J014247.5−301140	3.8	000	2.1 ± 0.5	0.50 ± 0.06	0.70	0.87	11.71 ± 0.08	A
J130800.7+292913	3.8	001	2.2 ± 0.5	0.34 ± 0.04	0.06	5.15	11.28 ± 0.09	A
J131247.0+303802	1.6	000	2.0 ± 0.6	0.33 ± 0.05	0.64	5.56	11.18 ± 0.10	A
J131745.1+280958	2.9	001	1.9 ± 0.4	0.18 ± 0.03	0.16	6.42	11.07 ± 0.14	A
J134135.8+284212	1.6	000	1.9 ± 0.5	0.23 ± 0.05	0.18	8.88	11.15 ± 0.16	A
J135031.8+250444	2.0	000	1.6 ± 0.4	0.37 ± 0.05	1.53	4.38	11.27 ± 0.09	A
J232202.1−345556	1.8	000	2.1 ± 0.6	0.26 ± 0.03	0.32	1.29	11.54 ± 0.10	A
J084406.6+015336	10.9	110	2.1 ± 0.6	0.38 ± 0.06	0.01	16.14	11.92 ± 0.15	B
J090312.5−004509	2.4	111	1.7 ± 0.5	0.17 ± 0.03	0.51	14.43	11.15 ± 0.18	B
J090554.8+004011	13.8	110	1.5 ± 0.3	0.16 ± 0.03	0.59	6.50	10.97 ± 0.15	B
J091249.4−000403	5.7	100	2.0 ± 0.6	0.44 ± 0.02	0.83	1.86	11.95 ± 0.05	B
J113127.5+000317	5.5	100	2.4 ± 0.7	0.32 ± 0.03	1.52	7.89	11.40 ± 0.10	B
J113918.8−012015	3.2	101	1.6 ± 0.5	0.19 ± 0.04	0.40	11.83	11.16 ± 0.18	B
J114411.4−015154	5.5	100	1.7 ± 0.5	0.16 ± 0.05	0.24	4.56	11.10 ± 0.20	B
J114837.1−011246	0.4	100	1.8 ± 0.5	0.25 ± 0.09	0.55	14.10	11.54 ± 0.37	B
J115141.3−023223	13.1	111	2.0 ± 0.6	0.48 ± 0.04	0.19	2.13	11.55 ± 0.08	B
J115650.0−000944	0.3	101	2.3 ± 0.6	0.31 ± 0.09	0.02	12.82	11.37 ± 0.25	B
J120137.2−020121	8.2	100	2.2 ± 0.6	0.16 ± 0.03	0.16	9.79	11.20 ± 0.17	B
J120403.0+012221	7.9	100	2.2 ± 0.6	0.24 ± 0.07	0.29	12.79	11.23 ± 0.28	B
J122320.1+000959	10.3	100	2.5 ± 0.5	0.37 ± 0.04	0.01	9.78	11.47 ± 0.08	B
J140606.0−010139	10.2	100	2.6 ± 0.7	0.21 ± 0.04	0.13	10.25	11.19 ± 0.22	B
J140819.1−014708	6.0	100	2.3 ± 0.6	0.34 ± 0.04	0.15	7.75	11.28 ± 0.11	B
J141040.0+014026	4.3	101	2.3 ± 0.6	0.32 ± 0.05	0.19	10.75	11.27 ± 0.14	B
J141221.9+000430	6.8	101	2.2 ± 0.4	0.35 ± 0.08	0.56	15.29	11.59 ± 0.20	B
J141405.7−000402	7.7	110	3.7 ± 0.5	0.28 ± 0.04	0.52	5.95	11.05 ± 0.13	B
J141416.9+004010	10.7	100	1.8 ± 0.5	0.26 ± 0.07	0.13	13.04	11.45 ± 0.27	B
J141500.8+015525	11.3	100	1.8 ± 0.4	0.14 ± 0.03	0.21	6.20	10.61 ± 0.19	B
J143522.9+010616	6.2	100	2.4 ± 0.6	0.37 ± 0.04	0.09	10.76	11.44 ± 0.08	B
J143743.1−001512	0.7	101	1.9 ± 0.5	0.47 ± 0.07	0.09	17.94	11.77 ± 0.14	B
J144245.7−003913	10.2	100	1.9 ± 0.5	0.35 ± 0.04	0.08	9.12	11.23 ± 0.12	B
J144630.3−001948	5.3	101	2.3 ± 0.5	0.21 ± 0.06	0.31	11.09	10.98 ± 0.29	B
J145703.5+000707	7.8	101	2.3 ± 0.6	0.37 ± 0.04	0.45	9.67	11.23 ± 0.09	B
J145717.8−000252	9.3	100	2.8 ± 0.5	0.42 ± 0.04	0.50	7.69	11.44 ± 0.08	B
J000556.2−302334	11.8	001	2.0 ± 0.6	0.48 ± 0.04	0.32	1.42	11.77 ± 0.07	B
J000912.9−352344	12.2	000	2.7 ± 0.6	0.57 ± 0.04	0.30	2.10	12.19 ± 0.07	B
J002748.6−304411	5.7	000	2.8 ± 0.7	0.51 ± 0.04	0.29	2.05	12.18 ± 0.07	B
J004755.4−291216	5.5	000	2.2 ± 0.6	0.55 ± 0.04	0.48	2.45	12.39 ± 0.07	B
J011317.6−295330	5.4	001	2.7 ± 0.6	0.33 ± 0.07	0.43	1.46	11.49 ± 0.14	B
J012234.4−272621	10.0	000	3.0 ± 0.7	0.32 ± 0.08	1.50	1.25	11.38 ± 0.17	B
J012646.8−313110	7.7	001	1.7 ± 0.5	0.50 ± 0.06	0.01	0.45	11.91 ± 0.10	B
J124753.3+322448	8.9	000	2.2 ± 0.6	0.39 ± 0.05	0.18	13.55	11.47 ± 0.12	B
J125728.9+281034	6.3	001	2.4 ± 0.6	0.34 ± 0.11	0.72	23.00	11.92 ± 0.30	B
J125924.6+274428	9.6	001	1.9 ± 0.5	0.17 ± 0.04	0.47	10.52	11.34 ± 0.20	B
J130252.6+265612	9.3	001	2.8 ± 0.7	0.35 ± 0.04	0.49	11.13	11.26 ± 0.11	B
J130733.8+242712	10.4	000	2.2 ± 0.6	0.38 ± 0.05	0.19	12.68	11.28 ± 0.12	B
J131104.9+242249	10.7	000	2.5 ± 0.6	0.34 ± 0.04	0.81	5.19	11.29 ± 0.09	B
J131414.2+304600	5.5	000	1.4 ± 0.4	0.39 ± 0.04	1.43	4.29	11.37 ± 0.07	B
J131504.4+263249	7.2	000	2.6 ± 0.6	0.46 ± 0.05	0.73	6.15	11.48 ± 0.08	B
J131529.2+321000	10.9	001	1.8 ± 0.6	0.33 ± 0.03	0.03	8.41	11.30 ± 0.10	B
J132047.1+293551	8.3	000	2.4 ± 0.6	0.26 ± 0.06	0.06	13.76	11.50 ± 0.21	B
J132834.4+253433	5.5	000	2.1 ± 0.6	0.32 ± 0.04	0.21	11.87	11.49 ± 0.13	B
J132914.2+254748	12.3	001	2.4 ± 0.6	0.43 ± 0.03	0.04	7.31	11.50 ± 0.07	B
J133122.5+260312	14.1	000	2.6 ± 0.5	0.29 ± 0.04	0.11	6.95	11.41 ± 0.11	B
J133639.2+275249	8.6	001	2.9 ± 0.5	0.34 ± 0.04	0.35	11.72	11.48 ± 0.11	B
J134042.5+304101	5.5	000	2.6 ± 0.8	0.22 ± 0.05	0.08	17.13	11.12 ± 0.26	B
J134340.4+281940	8.9	000	2.1 ± 0.5	0.12 ± 0.03	1.39	18.60	11.07 ± 0.21	B
J225034.1−350409	6.8	000	2.6 ± 0.6	0.37 ± 0.09	0.30	1.18	11.67 ± 0.16	B
J233820.6−293755	5.1	001	1.4 ± 0.3	0.54 ± 0.06	1.50	0.76	11.72 ± 0.09	B
J234121.6−301027	5.2	000	2.0 ± 0.6	0.49 ± 0.05	0.42	2.37	12.09 ± 0.11	B
J235600.1−305633	5.3	000	1.5 ± 0.4	0.47 ± 0.06	1.54	0.74	11.81 ± 0.09	B

Notes. For each source, the following columns represent the angular separation of the candidate lenses with respect to H-ATLAS sources (θ_H); an isolation flag for the foreground galaxies (where 1 means “isolated”, and 0 that there are one or more counterparts; first digit for optical wavelengths, second for NIR, and third for WISE); the photometric redshift for the SMGs and lenses as derived by CIGALE (z_s and z_l, respectively); the goodness of fit of the models (χ_{r, SMG}², χ_{r, lens}²); the logarithm of the stellar mass of the lenses (log(M_⋆ / M_⊙)); and a lensing rank indicating the reliability of the lenses (A=best candidates, B=other candidates).

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