Table C1. Open in new tab Absorption EW...

	EW co-rotation fraction (⁠\|$f_{\rm EWcorot}$\|⁠)\|$^{a}$\|
J0351G1	0.69	0.32	0.45	0.45	–	0.65	0.45	–	–	0.68	0.76	0.73	29.8 \|$\pm$\| 8.9
J0407G1	0.57	–	–	–	–	–	–	–	0.72	–	–	0.6	–\|$^{b}$\|
J0456G1	0.78	–	–	0.8	–	0.87	0.84	–	–	0.91	0.65	0.51	\|$-$\|30.1 \|$\pm$\| 8.8
J0456G2	0.59	–	–	–	–	0.62	–	–	–	0.63	0.66	–	6.4 \|$\pm$\| 2.4
J0853G2	0.57	–	0.97	0.95	0.97	–	0.97	0.97	0.9	–	–	–	\|$-$\|6.5 \|$\pm$\| 9.9
J0914G1	0.23	–	0.23	0.14	–	0.19	–	0.07	–	–	–	0.16	\|$-$\|1.8 \|$\pm$\| 7.1
J0943G1	0.93	–	–	–	–	–	–	–	0.99	–	0.97	0.97	\|$-$\|3.0 \|$\pm$\| 1.0
J0950G1	0.29	0.04	0.1	0.09	0.05	0.16	0.06	0.07	0.21	–	–	0.1	2.4 \|$\pm$\| 5.4
PG1001G1	0.64	–	–	–	–	–	–	–	–	–	–	0.98	–\|$^{b}$\|
J1009G1	0.52	0.02	0.1	0.36	–	0.31	0.13	–	–	–	0.49	0.56	36.2 \|$\pm$\| 10.9
J1041G1	0.94	1.0	1.0	1.0	1.0	1.0	–	1.0	0.99	–	–	0.99	\|$-$\|0.9 \|$\pm$\| 0.2
PG1116G1	0.59	1.0	1.0	1.0	1.0	1.0	1.0	1.0	1.0	1.0	–	1.0	\|$-$\|0.2 \|$\pm$\| 0.1
J1133G1	1.0	–	0.99	1.0	–	0.99	0.99	–	–	–	–	1.0	0.2 \|$\pm$\| 0.4
J1139G2	0.03	–	–	–	–	0.01	–	–	0.01	–	–	0.02	–\|$^{c}$\|
J1139G3	0.46	–	–	0.81	–	–	–	–	0.55	c	–	0.6	\|$-$\|11.4 \|$\pm$\| 19.1
J1139G4	0.68	–	–	0.51–	–	0.63	–	0.63	0.68	–	–	0.68	9.4 \|$\pm$\| 7.0
PG1216G1	0.17	–	–	–	–	0.34	–	0.31	0.23	0.19	0.3	0.21	\|$-$\|7.0 \|$\pm$\| 7.0
J1233G1	0.43	–	–	0.31	–	0.44	–	–	0.31	–	–	0.24	\|$-$\|10.6 \|$\pm$\| 8.0
J1241G1	0.81	1.0	0.98	0.95	–	0.94	0.97	0.96	0.79	–	0.93	0.86	\|$-$\|8.4 \|$\pm$\| 5.3
J1241G2	0.27	–	–	–	–	0.35	–	–	0.15	–	0.21	0.24	\|$-$\|4.2 \|$\pm$\| 11.6
J1322G1	0.58	0.52	0.48	0.54	–	0.5	0.37	0.49	0.48	–	–	0.37	\|$-$\|11.4 \|$\pm$\| 4.6
J1342G1	0.39	0.21	0.21	0.27	0.24	0.28	0.25	0.26	0.27	–	–	0.3	5.6 \|$\pm$\| 2.2
J1555G1	0.64	0.92	0.83	0.85	0.83	0.87	0.91	0.91	0.82	–	–	0.76	\|$-$\|9.1 \|$\pm$\| 4.0
J2131G1	0.58	0.97	0.95	0.93	0.94	0.83	–	–	0.76	0.94	–	0.66	\|$-$\|22.4 \|$\pm$\| 6.6
J2253G1	0.45	–	0.31	0.42	–	0.3	0.27	–	–	0.33	–	0.29	\|$-$\|4.4 \|$\pm$\| 5.7
J2253G2	0.74	–	–	–	–	–	–	–	0.96	–	0.8	0.67	\|$-$\|31.4 \|$\pm$\| 0.4
J2253G3	0.01	–	0.0	–	–	0.0	–	0.0	0.0	–	0.0	0.0	–\|$^{c}$\|

EW co-rotation fraction (⁠|$f_{\rm EWcorot}$|⁠)|$^{a}$|

Galaxy

H i

Mg ii

Si ii

C ii

N ii

Si iii

Si iv

N iii

C iii

C iv

N v

O vi

|${{\rm d}{({f_{\rm EWcorot}})}}/{{\rm d}{(\rm eV)}}$|[|$\times 10^{-4}$|]

J0351G1

0.69

0.32

0.45

–

0.65

0.45

–

0.68

0.76

0.73

29.8 |$\pm$| 8.9

J0407G1

0.57

–

0.72

–

0.6

–|$^{b}$|

J0456G1

0.78

–

0.8

–

0.87

0.84

–

0.91

0.65

0.51

|$-$|30.1 |$\pm$| 8.8

J0456G2

0.59

–

0.62

–

0.63

0.66

–

6.4 |$\pm$| 2.4

J0853G2

0.57

–

0.97

0.95

0.97

–

0.97

0.9

–

|$-$|6.5 |$\pm$| 9.9

J0914G1

0.23

–

0.23

0.14

–

0.19

–

0.07

–

0.16

|$-$|1.8 |$\pm$| 7.1

J0943G1

0.93

–

0.99

–

0.97

|$-$|3.0 |$\pm$| 1.0

J0950G1

0.29

0.04

0.1

0.09

0.05

0.16

0.06

0.07

0.21

–

0.1

2.4 |$\pm$| 5.4

PG1001G1

0.64

–

0.98

–|$^{b}$|

J1009G1

0.52

0.02

0.1

0.36

–

0.31

0.13

–

0.49

0.56

36.2 |$\pm$| 10.9

J1041G1

0.94

1.0

–

1.0

0.99

–

0.99

|$-$|0.9 |$\pm$| 0.2

PG1116G1

0.59

1.0

–

1.0

|$-$|0.2 |$\pm$| 0.1

J1133G1

1.0

–

0.99

1.0

–

0.99

–

1.0

0.2 |$\pm$| 0.4

J1139G2

0.03

–

0.01

–

0.01

–

0.02

–|$^{c}$|

J1139G3

0.46

–

0.81

–

0.55

–

0.6

|$-$|11.4 |$\pm$| 19.1

J1139G4

0.68

–

0.51–

–

0.63

–

0.63

0.68

–

0.68

9.4 |$\pm$| 7.0

PG1216G1

0.17

–

0.34

–

0.31

0.23

0.19

0.3

0.21

|$-$|7.0 |$\pm$| 7.0

J1233G1

0.43

–

0.31

–

0.44

–

0.31

–

0.24

|$-$|10.6 |$\pm$| 8.0

J1241G1

0.81

1.0

0.98

0.95

–

0.94

0.97

0.96

0.79

–

0.93

0.86

|$-$|8.4 |$\pm$| 5.3

J1241G2

0.27

–

0.35

–

0.15

–

0.21

0.24

|$-$|4.2 |$\pm$| 11.6

J1322G1

0.58

0.52

0.48

0.54

–

0.5

0.37

0.49

0.48

–

0.37

|$-$|11.4 |$\pm$| 4.6

J1342G1

0.39

0.21

0.27

0.24

0.28

0.25

0.26

0.27

–

0.3

5.6 |$\pm$| 2.2

J1555G1

0.64

0.92

0.83

0.85

0.83

0.87

0.91

0.82

–

0.76

|$-$|9.1 |$\pm$| 4.0

J2131G1

0.58

0.97

0.95

0.93

0.94

0.83

–

0.76

0.94

–

0.66

|$-$|22.4 |$\pm$| 6.6

J2253G1

0.45

–

0.31

0.42

–

0.3

0.27

–

0.33

–

0.29

|$-$|4.4 |$\pm$| 5.7

J2253G2

0.74

–

0.96

–

0.8

0.67

|$-$|31.4 |$\pm$| 0.4

J2253G3

0.01

–

0.0

–

0.0

–

0.0

–

0.0

–|$^{c}$|

	EW co-rotation fraction (⁠\|$f_{\rm EWcorot}$\|⁠)\|$^{a}$\|
J0351G1	0.69	0.32	0.45	0.45	–	0.65	0.45	–	–	0.68	0.76	0.73	29.8 \|$\pm$\| 8.9
J0407G1	0.57	–	–	–	–	–	–	–	0.72	–	–	0.6	–\|$^{b}$\|
J0456G1	0.78	–	–	0.8	–	0.87	0.84	–	–	0.91	0.65	0.51	\|$-$\|30.1 \|$\pm$\| 8.8
J0456G2	0.59	–	–	–	–	0.62	–	–	–	0.63	0.66	–	6.4 \|$\pm$\| 2.4
J0853G2	0.57	–	0.97	0.95	0.97	–	0.97	0.97	0.9	–	–	–	\|$-$\|6.5 \|$\pm$\| 9.9
J0914G1	0.23	–	0.23	0.14	–	0.19	–	0.07	–	–	–	0.16	\|$-$\|1.8 \|$\pm$\| 7.1
J0943G1	0.93	–	–	–	–	–	–	–	0.99	–	0.97	0.97	\|$-$\|3.0 \|$\pm$\| 1.0
J0950G1	0.29	0.04	0.1	0.09	0.05	0.16	0.06	0.07	0.21	–	–	0.1	2.4 \|$\pm$\| 5.4
PG1001G1	0.64	–	–	–	–	–	–	–	–	–	–	0.98	–\|$^{b}$\|
J1009G1	0.52	0.02	0.1	0.36	–	0.31	0.13	–	–	–	0.49	0.56	36.2 \|$\pm$\| 10.9
J1041G1	0.94	1.0	1.0	1.0	1.0	1.0	–	1.0	0.99	–	–	0.99	\|$-$\|0.9 \|$\pm$\| 0.2
PG1116G1	0.59	1.0	1.0	1.0	1.0	1.0	1.0	1.0	1.0	1.0	–	1.0	\|$-$\|0.2 \|$\pm$\| 0.1
J1133G1	1.0	–	0.99	1.0	–	0.99	0.99	–	–	–	–	1.0	0.2 \|$\pm$\| 0.4
J1139G2	0.03	–	–	–	–	0.01	–	–	0.01	–	–	0.02	–\|$^{c}$\|
J1139G3	0.46	–	–	0.81	–	–	–	–	0.55	c	–	0.6	\|$-$\|11.4 \|$\pm$\| 19.1
J1139G4	0.68	–	–	0.51–	–	0.63	–	0.63	0.68	–	–	0.68	9.4 \|$\pm$\| 7.0
PG1216G1	0.17	–	–	–	–	0.34	–	0.31	0.23	0.19	0.3	0.21	\|$-$\|7.0 \|$\pm$\| 7.0
J1233G1	0.43	–	–	0.31	–	0.44	–	–	0.31	–	–	0.24	\|$-$\|10.6 \|$\pm$\| 8.0
J1241G1	0.81	1.0	0.98	0.95	–	0.94	0.97	0.96	0.79	–	0.93	0.86	\|$-$\|8.4 \|$\pm$\| 5.3
J1241G2	0.27	–	–	–	–	0.35	–	–	0.15	–	0.21	0.24	\|$-$\|4.2 \|$\pm$\| 11.6
J1322G1	0.58	0.52	0.48	0.54	–	0.5	0.37	0.49	0.48	–	–	0.37	\|$-$\|11.4 \|$\pm$\| 4.6
J1342G1	0.39	0.21	0.21	0.27	0.24	0.28	0.25	0.26	0.27	–	–	0.3	5.6 \|$\pm$\| 2.2
J1555G1	0.64	0.92	0.83	0.85	0.83	0.87	0.91	0.91	0.82	–	–	0.76	\|$-$\|9.1 \|$\pm$\| 4.0
J2131G1	0.58	0.97	0.95	0.93	0.94	0.83	–	–	0.76	0.94	–	0.66	\|$-$\|22.4 \|$\pm$\| 6.6
J2253G1	0.45	–	0.31	0.42	–	0.3	0.27	–	–	0.33	–	0.29	\|$-$\|4.4 \|$\pm$\| 5.7
J2253G2	0.74	–	–	–	–	–	–	–	0.96	–	0.8	0.67	\|$-$\|31.4 \|$\pm$\| 0.4
J2253G3	0.01	–	0.0	–	–	0.0	–	0.0	0.0	–	0.0	0.0	–\|$^{c}$\|

Table C1.

Open in new tab

Absorption EW co-rotation fraction.

	EW co-rotation fraction (⁠\|$f_{\rm EWcorot}$\|⁠)\|$^{a}$\|
Galaxy	H i	Mg ii	Si ii	C ii	N ii	Si iii	Si iv	N iii	C iii	C iv	N v	O vi	\|${{\rm d}{({f_{\rm EWcorot}})}}/{{\rm d}{(\rm eV)}}$\|[\|$\times 10^{-4}$\|]
J0351G1	0.69	0.32	0.45	0.45	–	0.65	0.45	–	–	0.68	0.76	0.73	29.8 \|$\pm$\| 8.9
J0407G1	0.57	–	–	–	–	–	–	–	0.72	–	–	0.6	–\|$^{b}$\|
J0456G1	0.78	–	–	0.8	–	0.87	0.84	–	–	0.91	0.65	0.51	\|$-$\|30.1 \|$\pm$\| 8.8
J0456G2	0.59	–	–	–	–	0.62	–	–	–	0.63	0.66	–	6.4 \|$\pm$\| 2.4
J0853G2	0.57	–	0.97	0.95	0.97	–	0.97	0.97	0.9	–	–	–	\|$-$\|6.5 \|$\pm$\| 9.9
J0914G1	0.23	–	0.23	0.14	–	0.19	–	0.07	–	–	–	0.16	\|$-$\|1.8 \|$\pm$\| 7.1
J0943G1	0.93	–	–	–	–	–	–	–	0.99	–	0.97	0.97	\|$-$\|3.0 \|$\pm$\| 1.0
J0950G1	0.29	0.04	0.1	0.09	0.05	0.16	0.06	0.07	0.21	–	–	0.1	2.4 \|$\pm$\| 5.4
PG1001G1	0.64	–	–	–	–	–	–	–	–	–	–	0.98	–\|$^{b}$\|
J1009G1	0.52	0.02	0.1	0.36	–	0.31	0.13	–	–	–	0.49	0.56	36.2 \|$\pm$\| 10.9
J1041G1	0.94	1.0	1.0	1.0	1.0	1.0	–	1.0	0.99	–	–	0.99	\|$-$\|0.9 \|$\pm$\| 0.2
PG1116G1	0.59	1.0	1.0	1.0	1.0	1.0	1.0	1.0	1.0	1.0	–	1.0	\|$-$\|0.2 \|$\pm$\| 0.1
J1133G1	1.0	–	0.99	1.0	–	0.99	0.99	–	–	–	–	1.0	0.2 \|$\pm$\| 0.4
J1139G2	0.03	–	–	–	–	0.01	–	–	0.01	–	–	0.02	–\|$^{c}$\|
J1139G3	0.46	–	–	0.81	–	–	–	–	0.55	c	–	0.6	\|$-$\|11.4 \|$\pm$\| 19.1
J1139G4	0.68	–	–	0.51–	–	0.63	–	0.63	0.68	–	–	0.68	9.4 \|$\pm$\| 7.0
PG1216G1	0.17	–	–	–	–	0.34	–	0.31	0.23	0.19	0.3	0.21	\|$-$\|7.0 \|$\pm$\| 7.0
J1233G1	0.43	–	–	0.31	–	0.44	–	–	0.31	–	–	0.24	\|$-$\|10.6 \|$\pm$\| 8.0
J1241G1	0.81	1.0	0.98	0.95	–	0.94	0.97	0.96	0.79	–	0.93	0.86	\|$-$\|8.4 \|$\pm$\| 5.3
J1241G2	0.27	–	–	–	–	0.35	–	–	0.15	–	0.21	0.24	\|$-$\|4.2 \|$\pm$\| 11.6
J1322G1	0.58	0.52	0.48	0.54	–	0.5	0.37	0.49	0.48	–	–	0.37	\|$-$\|11.4 \|$\pm$\| 4.6
J1342G1	0.39	0.21	0.21	0.27	0.24	0.28	0.25	0.26	0.27	–	–	0.3	5.6 \|$\pm$\| 2.2
J1555G1	0.64	0.92	0.83	0.85	0.83	0.87	0.91	0.91	0.82	–	–	0.76	\|$-$\|9.1 \|$\pm$\| 4.0
J2131G1	0.58	0.97	0.95	0.93	0.94	0.83	–	–	0.76	0.94	–	0.66	\|$-$\|22.4 \|$\pm$\| 6.6
J2253G1	0.45	–	0.31	0.42	–	0.3	0.27	–	–	0.33	–	0.29	\|$-$\|4.4 \|$\pm$\| 5.7
J2253G2	0.74	–	–	–	–	–	–	–	0.96	–	0.8	0.67	\|$-$\|31.4 \|$\pm$\| 0.4
J2253G3	0.01	–	0.0	–	–	0.0	–	0.0	0.0	–	0.0	0.0	–\|$^{c}$\|

	EW co-rotation fraction (⁠\|$f_{\rm EWcorot}$\|⁠)\|$^{a}$\|
Galaxy	H i	Mg ii	Si ii	C ii	N ii	Si iii	Si iv	N iii	C iii	C iv	N v	O vi	\|${{\rm d}{({f_{\rm EWcorot}})}}/{{\rm d}{(\rm eV)}}$\|[\|$\times 10^{-4}$\|]
J0351G1	0.69	0.32	0.45	0.45	–	0.65	0.45	–	–	0.68	0.76	0.73	29.8 \|$\pm$\| 8.9
J0407G1	0.57	–	–	–	–	–	–	–	0.72	–	–	0.6	–\|$^{b}$\|
J0456G1	0.78	–	–	0.8	–	0.87	0.84	–	–	0.91	0.65	0.51	\|$-$\|30.1 \|$\pm$\| 8.8
J0456G2	0.59	–	–	–	–	0.62	–	–	–	0.63	0.66	–	6.4 \|$\pm$\| 2.4
J0853G2	0.57	–	0.97	0.95	0.97	–	0.97	0.97	0.9	–	–	–	\|$-$\|6.5 \|$\pm$\| 9.9
J0914G1	0.23	–	0.23	0.14	–	0.19	–	0.07	–	–	–	0.16	\|$-$\|1.8 \|$\pm$\| 7.1
J0943G1	0.93	–	–	–	–	–	–	–	0.99	–	0.97	0.97	\|$-$\|3.0 \|$\pm$\| 1.0
J0950G1	0.29	0.04	0.1	0.09	0.05	0.16	0.06	0.07	0.21	–	–	0.1	2.4 \|$\pm$\| 5.4
PG1001G1	0.64	–	–	–	–	–	–	–	–	–	–	0.98	–\|$^{b}$\|
J1009G1	0.52	0.02	0.1	0.36	–	0.31	0.13	–	–	–	0.49	0.56	36.2 \|$\pm$\| 10.9
J1041G1	0.94	1.0	1.0	1.0	1.0	1.0	–	1.0	0.99	–	–	0.99	\|$-$\|0.9 \|$\pm$\| 0.2
PG1116G1	0.59	1.0	1.0	1.0	1.0	1.0	1.0	1.0	1.0	1.0	–	1.0	\|$-$\|0.2 \|$\pm$\| 0.1
J1133G1	1.0	–	0.99	1.0	–	0.99	0.99	–	–	–	–	1.0	0.2 \|$\pm$\| 0.4
J1139G2	0.03	–	–	–	–	0.01	–	–	0.01	–	–	0.02	–\|$^{c}$\|
J1139G3	0.46	–	–	0.81	–	–	–	–	0.55	c	–	0.6	\|$-$\|11.4 \|$\pm$\| 19.1
J1139G4	0.68	–	–	0.51–	–	0.63	–	0.63	0.68	–	–	0.68	9.4 \|$\pm$\| 7.0
PG1216G1	0.17	–	–	–	–	0.34	–	0.31	0.23	0.19	0.3	0.21	\|$-$\|7.0 \|$\pm$\| 7.0
J1233G1	0.43	–	–	0.31	–	0.44	–	–	0.31	–	–	0.24	\|$-$\|10.6 \|$\pm$\| 8.0
J1241G1	0.81	1.0	0.98	0.95	–	0.94	0.97	0.96	0.79	–	0.93	0.86	\|$-$\|8.4 \|$\pm$\| 5.3
J1241G2	0.27	–	–	–	–	0.35	–	–	0.15	–	0.21	0.24	\|$-$\|4.2 \|$\pm$\| 11.6
J1322G1	0.58	0.52	0.48	0.54	–	0.5	0.37	0.49	0.48	–	–	0.37	\|$-$\|11.4 \|$\pm$\| 4.6
J1342G1	0.39	0.21	0.21	0.27	0.24	0.28	0.25	0.26	0.27	–	–	0.3	5.6 \|$\pm$\| 2.2
J1555G1	0.64	0.92	0.83	0.85	0.83	0.87	0.91	0.91	0.82	–	–	0.76	\|$-$\|9.1 \|$\pm$\| 4.0
J2131G1	0.58	0.97	0.95	0.93	0.94	0.83	–	–	0.76	0.94	–	0.66	\|$-$\|22.4 \|$\pm$\| 6.6
J2253G1	0.45	–	0.31	0.42	–	0.3	0.27	–	–	0.33	–	0.29	\|$-$\|4.4 \|$\pm$\| 5.7
J2253G2	0.74	–	–	–	–	–	–	–	0.96	–	0.8	0.67	\|$-$\|31.4 \|$\pm$\| 0.4
J2253G3	0.01	–	0.0	–	–	0.0	–	0.0	0.0	–	0.0	0.0	–\|$^{c}$\|

Notes. |$^{a}$|Typical uncertainties are on the order of |$0.001{\!-\!}0.006$| as determined from a bootstrap analysis where we varied the galaxy and absorption redshifts within their error bars.

|$^{b}$|Fewer than three metal lines were detected. A slope cannot be reliably measured.

|$^{c}$|No significant co-rotation was detected for this system.

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