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TABLE
1
Baldwin
Effect
Regressions
for
the
LBQS
Emission
line
All
Data
(including
upper
limits)
Detections
only
Line
Name
N
T
ot
N
Limits
C/K/S
a
Slope
Intercept
N
C/K/S
a
Slope
Intercept
Fe
II
UV
953
294
0.00/0.00/0.00
­0.617
\Sigma0.047
20.2
\Sigma
1.4
659
0.00/0.00/0.00
­0.105
\Sigma
0.016
4.8
\Sigma
0.5
Fe
II
opt
248
110
0.00/0.00/0.00
­0.447
\Sigma
0.108
14.5
\Sigma
3.2
138
0.47/0.35/0.36
­0.007
\Sigma
0.034
1.7
\Sigma
1.0
Lfi
–1025.7+OVI
–1035
130
27
0.98/0.19/0.22
0.112
\Sigma
0.221
­2.9
\Sigma
7.0
103
0.00/0.00/0.00
­0.500
\Sigma
0.187
16.7
\Sigma
5.9
Lff
–1215.7
259
0
0.00/0.00/0.00
­0.272
\Sigma
0.067
10.3
\Sigma
2.1
259
0.00/0.00/0.00
­0.272
\Sigma
0.067
10.3
\Sigma
2.1
NV
–1241.5
259
8
0.72/0.35/0.41
­0.037
\Sigma
0.060
2.3
\Sigma
1.9
251
0.01/0.08/0.09
­0.128
\Sigma
0.068
5.2
\Sigma
2.2
O
I
–1305
259
120
0.10/0.15/0.04
­0.266
\Sigma
0.121
8.5
\Sigma
3.8
139
0.05/0.02/0.03
­0.307
\Sigma
0.114
10.1
\Sigma
3.6
Si
IV
+O
IV]
–1400
414
19
0.00/0.00/0.00
­0.300
\Sigma
0.080
10.3
\Sigma
2.4
395
0.00/0.00/0.00
­0.308
\Sigma
0.050
10.7
\Sigma
1.6
CIV
–1549
487
1
0.00/0.00/0.00
­0.227\Sigma
0.025
8.7
\Sigma
0.8
486
0.00/0.00/0.00
­0.231
\Sigma
0.044
8.8
\Sigma
1.4
He
II
–1640
487
68
0.00/0.23/0.20
­0.166
\Sigma
0.097
6.2
\Sigma
3.0
419
0.59/0.38/0.37
0.058
\Sigma
0.077
­0.7
\Sigma
2.4
Al
III
–1859
667
181
0.00/0.00/0.00
­0.229
\Sigma
0.065
7.8
\Sigma
2.0
486
0.07/0.09/0.10
­0.064
\Sigma
0.054
2.8
\Sigma
1.7
C
III]
–1909
667
26
0.00/0.07/0.06
­0.120
\Sigma
0.037
5.1
\Sigma
1.1
641
0.55/0.56/0.57
­0.034
\Sigma
0.032
2.4
\Sigma
1.0
Mg
II
–2800
677
42
0.00/0.00/0.00
­0.187
\Sigma
0.017
7.3
\Sigma
0.5
635
0.00/0.00/0.00
­0.126
\Sigma
0.023
5.4
\Sigma
0.7
[Ne
V]
–3426
488
365
0.00/0.00/0.00
­0.288
\Sigma
0.054
8.9
\Sigma
1.6
123
0.04/0.34/0.33
0.079
\Sigma
0.079
­1.7
\Sigma
2.3
[O
II]
–3728
393
272
0.00/0.00/0.00
­0.337
\Sigma
0.036
10.4
\Sigma
1.1
121
0.32/0.20/0.24
0.059
\Sigma
0.064
­1.0
\Sigma
1.9
[Ne
III]
–3869
363
259
0.00/0.00/0.00
­0.464
\Sigma
0.069
14.3
\Sigma
2.1
104
0.09/0.06/0.06
0.126
\Sigma
0.061
­3.0
\Sigma
1.8
Hffi
–4101.7
309
222
0.00/0.00/0.00
­0.392
\Sigma
0.085
12.0
\Sigma
2.6
87
**/0.14/0.14
­0.150
\Sigma
0.080
5.6
\Sigma
2.3
Hfl
–4340.5+
[O
III]
–4363
251
87
0.07/0.08/0.05
­0.146
\Sigma
0.070
5.5
\Sigma
2.1
164
0.46/0.57/0.57
­0.029
\Sigma
0.047
2.0
\Sigma
1.4
He
II
–4686.5
186
154
0.00/0.00/0.00
­0.470
\Sigma
0.091
14.5
\Sigma
2.7
32
0.11/0.49/0.43
0.091
\Sigma
0.217
­1.6
\Sigma
6.4
Hfi
–4861.3
146
16
0.07/0.08/0.09
­0.214
\Sigma
0.083
8.1
\Sigma
2.5
130
0.92/0.20/0.25
­0.071
\Sigma
0.074
3.9
\Sigma
2.2
[O
III]
–4959
146
71
0.02/0.18/0.05
­0.246
\Sigma
0.098
8.1
\Sigma
2.9
75
0.40/0.25/0.26
0.105
\Sigma
0.129
­2.1
\Sigma
3.8
[O
III]
–5007
146
52
0.01/0.03/0.01
­0.300
\Sigma
0.138
10.1
\Sigma
4.1
94
0.73/0.70/0.76
0.087
\Sigma
0.078
­1.3
\Sigma
2.3
He
I
–5875.6
33
30
0.77/0.92/0.98
0.052
\Sigma
0.138
­0.7
\Sigma
4.0
3
**/0.60/0.67
0.040
\Sigma
0.380
0.0
\Sigma
11.3
a
Correlation
probabilities
from
ASURV
for
(C)
Cox
proportional
Hazard
model,
(K)
generalized
Kendall`s
tau,
and
(S)
Spearman`s
rho.
NOTE.---Schmitt
2­D
Kaplan­Meier
regression
fits
and
errors
from
ASURV.
The
Baldwin
effect
examined
here
is
log
L
2500
/
log
W
–
(line).
Emission
line
names
shown
in
boldface
meet
our
most
stringent
significance
criteria:
P
!
1%
in
all
3
correlation
tests
using
all
data,
and
an
upper
limit
fraction
!
33%.
Correlation
probabilities
in
boldface
meet
the
former
criterion
for
the
data
tested,
regardless
of
limit
fraction.