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TABLE
3
Evolution
Regressions
for
LBQS
Emission
Lines
Emission
line
All
Data
(including
upper
limits)
Detections
only
NAME
TOT
UPP
C/K/S
a
Slope
Intercept
NUM
C/K/S
Slope
Intercept
Full
LBQS
Fe
UV
953
294
0.00/0.00/0.00
­1.312\Sigma0.101
1.13\Sigma0.03
659
0.00/0.00/0.00
­0.190\Sigma0.038
1.52\Sigma0.01
Lyff
259
0
0.00/0.00/0.00
­1.199\Sigma0.227
2.19\Sigma0.08
259
0.00/0.00/0.00
­1.216\Sigma0.226
2.20\Sigma0.08
Si
IV
+O
IV]
414
19
0.00/0.00/0.00
­1.045\Sigma0.153
1.29\Sigma0.05
395
0.00/0.00/0.00
­1.163\Sigma0.149
1.35\Sigma0.05
C
IV
487
1
0.00/0.00/0.00
­0.480\Sigma0.063
1.69\Sigma0.02
486
0.00/0.00/0.00
­0.481\Sigma0.107
1.69\Sigma0.03
Al
III
667
181
0.00/0.00/0.00
­0.788\Sigma0.185
0.75\Sigma0.03
486
0.06/0.03/0.04
­0.202\Sigma0.092
0.87\Sigma0.02
C
III]
667
26
0.00/0.01/0.01
­0.255\Sigma0.078
1.41\Sigma0.01
641
0.60/0.24/0.26
­0.045\Sigma0.069
1.40\Sigma0.01
Mg
II
677
42
0.00/0.00/0.00
­0.390\Sigma0.044
1.49\Sigma0.02
635
0.00/0.00/0.00
­0.230\Sigma0.055
1.54\Sigma0.01
Hfi
146
16
0.00/0.00/0.00
­0.834\Sigma0.228
1.26\Sigma0.13
130
0.05/0.02/0.02
­0.561\Sigma0.171
1.45\Sigma0.09
LBQS
bright
Fe
UV
777
233
0.00/0.00/0.00
­1.283\Sigma0.079
1.12\Sigma0.02
544
0.00/0.00/0.00
­0.178\Sigma0.036
1.52\Sigma0.01
Lyff
198
0
0.00/0.00/0.00
­1.071\Sigma0.270
2.14\Sigma0.09
198
0.00/0.00/0.00
­1.071\Sigma0.270
2.14\Sigma0.09
Si
IV
323
14
0.00/0.00/0.00
­0.902\Sigma0.178
1.26\Sigma0.05
309
0.00/0.00/0.00
­1.102\Sigma0.122
1.34\Sigma0.03
CIV
383
1
0.00/0.00/0.00
­0.492\Sigma0.136
1.68\Sigma0.04
382
0.00/0.00/0.00
­0.488\Sigma0.103
1.68\Sigma0.03
Al
III
529
134
0.00/0.00/0.00
­0.689\Sigma0.140
0.76\Sigma0.03
395
0.05/0.05/0.06
­0.206\Sigma0.091
0.86\Sigma0.02
Mg
II
562
33
0.00/0.00/0.00
­0.396\Sigma0.051
1.48\Sigma0.01
529
0.00/0.00/0.00
­0.248\Sigma0.058
1.53\Sigma0.01
Hfi
124
12
0.00/0.00/0.00
­0.976\Sigma0.327
1.17\Sigma0.19
112
0.05/0.02/0.01
­0.571\Sigma0.238
1.44\Sigma0.13
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
relations
examined
here
are
log
W
–
(line)
/
log
z.
Correlation
probabilities
in
boldface
meet
our
most
stringent
significance
criteria:
P
!
1%
in
all
3
correlation
tests
using
all
data,
and
an
upper
limit
fraction
!
33%.