astro-ph/9311070 🔍 (source)
|
nonlinear mass |
|
180.0 |
|
astro-ph/9603076 🔍 (source)
|
linear distance |
|
22.0 ± 0.8 Mpc |
|
astro-ph/9803214 🔍 (source)
|
mean linear spin-down rate |
\dot { P } |
5.126e-14 |
|
astro-ph/9803342 🔍 (source)
|
Ca linear depletion |
\delta ( Ca ) |
0.00028 |
|
astro-ph/9803342 🔍 (source)
|
Ca linear depletion |
\delta ( Ca ) |
0.00014 |
|
astro-ph/9805356 🔍 (source)
|
linear size of the radio structure |
|
2.0 Mpc |
|
astro-ph/9807013 🔍 (source)
|
linear polarization |
|
9.0 |
|
astro-ph/9809025 🔍 (source)
|
linear distance |
|
660.0 ± 66.0 kpc |
|
astro-ph/9810002 🔍 (source)
|
linear diameter |
|
2.5 ± 0.4 pc |
|
astro-ph/9810365 🔍 (source)
|
linear spin-down rate |
|
5.1271e-14 |
|
astro-ph/9812089 🔍 (source)
|
linear regression slope |
|
0.6 |
|
astro-ph/9906202 🔍 (source)
|
projected linear distance |
|
-0.07 ± 0.07 c |
|
astro-ph/9906202 🔍 (source)
|
projected linear distance |
|
0.3 ± 0.07 |
|
astro-ph/9906202 🔍 (source)
|
projected linear distance |
|
0.19 ± 0.27 |
|
astro-ph/9906346 🔍 (source)
|
linear polarization in the afterglow |
|
1.6 ± 0.2 % |
|
astro-ph/9911151 🔍 (source)
|
linearly extrapolated normalization |
\sigma _ { 8 } ^ { L } |
0.79 ± 0.08 |
|
astro-ph/9911196 🔍 (source)
|
linear variance per unit |
\ln k of \Delta _ { \rho } ^ { 2 } ( k ) |
0.72 ± 0.09 |
|
astro-ph/9911350 🔍 (source)
|
optical linear diameter |
|
1.4 ± 0.2 kpc |
|
astro-ph/9912244 🔍 (source)
|
linear phase |
t |
8.0 ± 7.0 day |
|
astro-ph/0002033 🔍 (source)
|
linear size of the radio structure |
|
50.0 h |
|
astro-ph/0002033 🔍 (source)
|
linear size of the radio structure |
H _ { 0 } |
50.0 |
|
astro-ph/0004334 🔍 (source)
|
linear redshift distortion parameter |
\beta |
0.41 +0.13-0.12 |
|
astro-ph/0010363 🔍 (source)
|
linear extent |
|
2.0 AU |
|
astro-ph/0010442 🔍 (source)
|
projected linear extent of the radio structure |
|
3.14 Mpc |
|
astro-ph/0103089 🔍 (source)
|
linear polarization |
\alpha |
0.275 +0.024999999999999967-0.025000000000000022 |
|
astro-ph/0104280 🔍 (source)
|
linear size |
L |
6.0 pc |
|
astro-ph/0105267 🔍 (source)
|
linear polarization levels |
|
2.3 % |
Lower |
astro-ph/0105472 🔍 (source)
|
linear correlation coefficient |
|
0.0004 ± 0.001 |
|
astro-ph/0107196 🔍 (source)
|
linear density |
\delta _ { L , R } |
0.0 |
Lower |
astro-ph/0108192 🔍 (source)
|
linear limb-darkened radii |
|
98.0 R_\odot |
|
astro-ph/0108192 🔍 (source)
|
linear limb-darkened radii |
|
56.0 R_\odot |
|
astro-ph/0108192 🔍 (source)
|
linear limb-darkened radii |
|
114.0 R_\odot |
|
astro-ph/0110158 🔍 (source)
|
linear diameter |
|
0.54 K pc |
|
astro-ph/0201116 🔍 (source)
|
projected linear size |
|
330.0 h |
|
astro-ph/0202514 🔍 (source)
|
linear size |
|
6.8e+17 cm |
|
astro-ph/0204084 🔍 (source)
|
projected linear distance |
|
17.8 h |
|
astro-ph/0204241 🔍 (source)
|
linear size |
|
1.5 kpc |
|
astro-ph/0204417 🔍 (source)
|
projected linear extent |
|
2.0 pc |
|
astro-ph/0205255 🔍 (source)
|
linear |
v \sin i _ { \mathrm { |
1.03 |
|
astro-ph/0301635 🔍 (source)
|
linear size |
|
7.7 h |
|
astro-ph/0302080 🔍 (source)
|
linear size |
|
620.0 kpc |
|
astro-ph/0302415 🔍 (source)
|
linear polarization |
|
2.0 |
|
astro-ph/0303592 🔍 (source)
|
linear bias parameter |
b |
1.37 ± 0.3 |
|
astro-ph/0303634 🔍 (source)
|
linear diameters |
D [ A ] |
1.224 ± 0.003 |
|
astro-ph/0306322 🔍 (source)
|
linear polarization |
P |
80.0 |
|
astro-ph/0306377 🔍 (source)
|
projected linear separation |
|
184.0 AU |
|
astro-ph/0306385 🔍 (source)
|
characteristic non-linear mass scale |
M |
8.7 |
|
astro-ph/0306585 🔍 (source)
|
linear bias |
b |
3.5 ± 0.3 |
|
astro-ph/0306604 🔍 (source)
|
linear diameter |
|
1.711 ± 0.013 |
|
astro-ph/0309148 🔍 (source)
|
linear diameter |
|
2.048 ± 0.025 |
|
astro-ph/0310128 🔍 (source)
|
Rosseland linear radius R |
|
86.0 ± 3.0 R_\odot |
|
astro-ph/0312068 🔍 (source)
|
linear radii |
R [ A ] |
1.224 ± 0.003 R_\odot |
|
astro-ph/0312068 🔍 (source)
|
linear radius |
|
2.048 ± 0.025 R_\odot |
|
astro-ph/0312296 🔍 (source)
|
projected linear size |
|
1.35 Mpc |
|
astro-ph/0401618 🔍 (source)
|
non-linear coupling parameter |
|
95.0 |
|
astro-ph/0402036 🔍 (source)
|
linear diameter |
|
5.25 ± 1.75 pc |
|
astro-ph/0403421 🔍 (source)
|
linear polarization |
|
10.0 |
|
astro-ph/0405525 🔍 (source)
|
linear polarization degree |
\Pi _ { GRB } |
41.0 +57.0-44.0 % |
|
astro-ph/0406036 🔍 (source)
|
linear mass-clustering amplitude |
\sigma _ { 8 } |
0.8 |
|
astro-ph/0406513 🔍 (source)
|
amplitude of the linear redshift-space distortions relative to the galaxy overdensity field |
\beta ( L _ { * } , 0 ) |
0.58 ± 0.08 |
|
astro-ph/0407416 🔍 (source)
|
linear energy |
|
2100000000000000.0 GeV |
|
astro-ph/0407377 🔍 (source)
|
linear theory power spectrum amplitude |
\Delta ^ { 2 } _ { L } ( k _ { p } |
0.009 s km-1 |
|
astro-ph/0407643 🔍 (source)
|
linear velocity gradient |
|
0.7 km s-1 pc-1 |
|
astro-ph/0407643 🔍 (source)
|
linear velocity gradient |
|
1.4 km s-1 pc-1 |
|
astro-ph/0408446 🔍 (source)
|
linear polarization |
L |
379.0 |
|
astro-ph/0408562 🔍 (source)
|
linear momentum |
|
430.0 ± 140.0 M_\odot km s-1 |
|
astro-ph/0410232 🔍 (source)
|
linear radius |
R _ { UD } ^ { K } |
2.3 ± 0.5 AU |
|
astro-ph/0411003 🔍 (source)
|
X-ray flux decayed linearly |
|
6.900000000000001e-05 ± 9.000000000000001e-07 c |
Upper |
astro-ph/0411133 🔍 (source)
|
linear radii |
|
320.0 +50.0-40.0 R_\odot |
|
astro-ph/0411531 🔍 (source)
|
linear polarization |
P / \sigma _ { P } |
3.0 |
Lower |
astro-ph/0502293 🔍 (source)
|
linear radius |
|
1570.0 ± 400.0 R_\odot |
|
astro-ph/0504402 🔍 (source)
|
linear relation |
[ X / H ] |
1.0 |
|
astro-ph/0506249 🔍 (source)
|
rms linear theory variance in spheres of radius 8 h ^ { -1 } Mpc |
\sigma _ { 8 } |
0.88 +0.12-0.1 |
|
astro-ph/0507055 🔍 (source)
|
projected linear size |
H _ { o } |
71.0 km s-1 Mpc-1 |
|
astro-ph/0507470 🔍 (source)
|
linear correlation coefficient |
r |
98.0 |
|
astro-ph/0507470 🔍 (source)
|
linear correlation coefficient |
|
0.36 |
|
astro-ph/0507583 🔍 (source)
|
linear theory matter fluctuation amplitude |
\sigma _ { 8 } |
0.77 ± 0.05 |
|
astro-ph/0509166 🔍 (source)
|
linear radius |
|
0.863 ± 0.003 R_\odot |
|
astro-ph/0510422 🔍 (source)
|
linear size |
|
0.5 pc |
|
astro-ph/0510649 🔍 (source)
|
linear ephemeris of the light maxima |
JD _ { max } |
2449862.0 |
|
astro-ph/0602105 🔍 (source)
|
linear radii |
|
0.38 |
Lower |
gr-qc/0602117 🔍 (source)
|
linear momentum flux |
\eta = \frac { m _ { 1 } m _ { 2 } } { ( m _ { 1 } + m _ { 2 } ) } ^ { 2 } |
0.2 |
|
astro-ph/0603314 🔍 (source)
|
linear function |
a _ { 0 } |
0.289 ± 0.051 |
|
astro-ph/0604341 🔍 (source)
|
position angle of linear polarization |
\theta _ { * } |
155.0 ± 15.0 |
|
astro-ph/0607378 🔍 (source)
|
linear relation |
\log ( M _ { bh } ) |
7.81 (\pm 0.08) |
|
astro-ph/0608110 🔍 (source)
|
linear function |
z |
0.05 |
Lower |
astro-ph/0610420 🔍 (source)
|
linear size of the planetary nebula |
D _ { PN } |
1.72 pc |
|
astro-ph/0611126 🔍 (source)
|
non-linearity parameter |
f _ { NL } |
1.0 |
|
astro-ph/0611779 🔍 (source)
|
maximum linear radius |
|
1.52 ± 0.15 pc |
|
astro-ph/0612723 🔍 (source)
|
linear radius |
R _ { \star } |
1.7 ± 0.1 R_\odot |
|
astro-ph/0612723 🔍 (source)
|
linear radius |
\sigma ( M _ { \star } ) |
0.15000000000000002 +0.04999999999999999-0.05000000000000002 M_\odot |
|
astro-ph/0701120 🔍 (source)
|
linear radius |
R |
2.672 ± 0.028 R_\odot |
|
astro-ph/0701275 🔍 (source)
|
linear correlation coefficient |
|
0.38 |
|
astro-ph/0702307 🔍 (source)
|
phase-averaged linear polarisation degree |
P _ { L } |
9.4 |
|
0704.1636 🔍 (source)
|
linear phase curves |
|
0.18 |
|
0704.1636 🔍 (source)
|
linear phase curves |
|
0.1 |
|
0704.3722 🔍 (source)
|
linear radius |
|
0.779 ± 0.052 |
|
0705.1311 🔍 (source)
|
ratio of the quadratic to linear biasing coefficients |
b _ { 2 } / b _ { 1 } |
-0.4 |
Lower |
0705.1311 🔍 (source)
|
ratio of the quadratic to linear biasing coefficients |
b _ { 2 } / b _ { 1 } |
-0.4 |
Lower |
0705.1615 🔍 (source)
|
non linear coupling parameter |
f _ { NL } |
-300.0 |
Lower |
0705.1615 🔍 (source)
|
non linear coupling parameter |
f _ { NL } |
-300.0 |
Lower |
0705.1843 🔍 (source)
|
linear effective bias parameter |
|
3.0 |
|
0706.0938 🔍 (source)
|
linear growth rate of perturbations |
z |
0.15 |
|
0707.2443 🔍 (source)
|
linear bias |
b |
1.74 ± 0.16 |
|
0708.3109 🔍 (source)
|
projected linear separation |
|
1.0 |
|
0708.4321 🔍 (source)
|
non-linear parameter of the curvature perturbation |
f _ { NL } |
-5.0 c |
|
0710.5273 🔍 (source)
|
projected linear separation |
|
12.3 AU |
|
0712.0680 🔍 (source)
|
Pearson linear correlation coefficient |
|
0.94 |
|
0712.2882 🔍 (source)
|
Linear polarization |
|
0.7 ± 0.1 |
|
0712.2882 🔍 (source)
|
Linear polarization |
|
1.0 ± 0.2 % |
|
0803.3731 🔍 (source)
|
linear polarisation level |
|
16.0 |
Upper |
0804.4129 🔍 (source)
|
apparent linear expansion rate for the dust shell |
|
0.35 ± 0.03 m as day-1 |
|
0805.0596 🔍 (source)
|
nonlinear fractional density contrast of the sphere |
1 + \delta |
1.76 ± 0.17 |
|
0806.2217 🔍 (source)
|
slope of this linear portion |
a |
0.41 ± 0.01 |
|
0807.1752 🔍 (source)
|
linear scale heights |
|
103.0 pc F W H |
|
0808.2742 🔍 (source)
|
projected linear size of the radio structure |
H _ { 0 } |
71.0 km s-1 Mpc-1 |
|
0809.1959 🔍 (source)
|
linear slope |
\beta |
0.05 ± 0.004 |
|
0809.2624 🔍 (source)
|
linear separation |
|
8700.0 AU |
|
0811.2223 🔍 (source)
|
non linearity parameter |
f _ { NL } |
100.0 |
|
0812.1756 🔍 (source)
|
non-linear coupling parameter |
f _ { NL } |
-94.0 |
Lower |
0901.1385 🔍 (source)
|
linearly polarized intensity |
|
3.6 |
|
0904.0005 🔍 (source)
|
linear polarisation |
|
0.09 % |
|
0904.0005 🔍 (source)
|
linear polarisation |
|
30.0 +10.0-6.0 |
|
0904.3136 🔍 (source)
|
decreases linearly |
|
-0.047 ± 0.003 dex kpc-1 |
|
0905.0499 🔍 (source)
|
linear source power spectrum |
\Delta ^ { 2 } |
0.35 +0.15000000000000002-0.14999999999999997 |
|
0906.3010 🔍 (source)
|
fractional linear polarization |
|
29.0 |
Lower |
0907.1057 🔍 (source)
|
linear cloud size |
l |
520.0 +240.0-190.0 pc |
|
0907.3052 🔍 (source)
|
nonlinearity parameter |
f _ { NL } |
3.0 |
Upper |
0907.4453 🔍 (source)
|
normalization of the linear power spectrum |
\sigma _ { 8 } |
0.9 ± 0.04 |
|
0907.4860 🔍 (source)
|
linear growth |
\alpha |
0.254 ± 0.153 |
|
0910.0004 🔍 (source)
|
linear biasing parameter |
|
1.24 ± 0.11 |
|
0910.0004 🔍 (source)
|
linear biasing parameter |
\hat { b } |
0.4 |
|
0910.0492 🔍 (source)
|
linear effective bias parameter |
|
3.0 |
|
1003.3214 🔍 (source)
|
linear bias |
b |
1.44 ± 0.22 |
|
1004.3771 🔍 (source)
|
normalization of the linear power spectrum |
\sigma _ { 8 } |
0.91 +0.07-0.08 |
|
1009.0677 🔍 (source)
|
non-linear parameter |
f _ { NL } ^ { equil } |
4.62 |
|
1011.1242 🔍 (source)
|
fractional linear polarization |
|
1.0 |
|
1011.1242 🔍 (source)
|
fractional linear polarization |
|
1.8 |
|
1011.1242 🔍 (source)
|
fractional linear polarization |
|
2.7 % |
|
1011.1498 🔍 (source)
|
non-linear mass |
|
0.2 |
|
1012.1827 🔍 (source)
|
flux of linear momentum |
|
2.5e-07 M_\odot km yr-1 s-1 |
|
1102.2235 🔍 (source)
|
linear extent |
|
1.4 Mpc |
|
1102.3918 🔍 (source)
|
linear polarization of the \lya emission |
P _ { Ly \alpha } |
2.6 ± 2.8 % |
|
1104.4122 🔍 (source)
|
linear relation |
\sigma _ { H _ { 2 } } |
-0.2 |
|
1104.5244 🔍 (source)
|
linear bias parameter |
b |
0.16 |
Lower |
1104.5551 🔍 (source)
|
linear separation |
|
4.4 Mpc |
|
1105.0944 🔍 (source)
|
best-fit linear phase function parameters |
m ( 1 , 1 , 0 ) |
15.35 ± 0.05 mag |
|
1105.4373 🔍 (source)
|
linear polarisation fraction |
P _ { L } ^ { avg } |
0.47 |
|
1108.1911 🔍 (source)
|
linear polarization |
|
2.0 |
|
1112.5723 🔍 (source)
|
linear angular power spectrum |
\Omega _ { m } |
0.31 +0.18-0.11 |
|
1203.6682 🔍 (source)
|
linear radii |
R |
33.6 ± 2.2 R_\odot |
|
1205.6669 🔍 (source)
|
linear decay rate |
|
0.94 Mm2 hr-1 |
|
1206.2167 🔍 (source)
|
projected linear separation |
|
2.6 kpc |
|
1208.1527 🔍 (source)
|
linear expansion |
\beta |
2.0 |
|
1209.0217 🔍 (source)
|
linear radiuses |
|
0.6759 ± 0.0062 m as |
|
1209.0217 🔍 (source)
|
linear radiuses |
|
1.01 ± 0.009 R_\odot |
|
1209.2420 🔍 (source)
|
linear proportion |
\alpha _ { s } |
1.0 |
|
1210.2781 🔍 (source)
|
linear polarisation |
|
10.0 ± 1.0 |
|
1210.6040 🔍 (source)
|
linear distance |
|
7.24 ± 0.03 ± 0.4 Mpc |
|
1211.3554 🔍 (source)
|
linear size |
|
3.0 pc |
|
1212.4526 🔍 (source)
|
quasar linear bias |
b _ { Q } |
1.38 ± 0.1 |
|
1302.4202 🔍 (source)
|
linear scale length |
|
25.0 |
|
1302.5014 🔍 (source)
|
linear stellar radii |
R _ { a } |
2.85 ± 0.15 R_\odot |
|
1303.5170 🔍 (source)
|
linear relation |
N _ { H } ( 10 ^ { 20 } cm ^ { -2 } ) |
0.3 +0.13-0.09 |
|
1303.5191 🔍 (source)
|
nonlinearity parameter of the local-type non-Gaussianity |
f _ { NL } |
10.0 |
|
1305.2873 🔍 (source)
|
slope of the linear relation |
|
0.3 |
|
1305.2873 🔍 (source)
|
slope of the linear relation |
|
2.6 ± 0.2 |
|
1305.2873 🔍 (source)
|
linear equation |
x |
2.3 ± 0.1 |
|
1305.6383 🔍 (source)
|
linear mass density |
M _ { l } |
600.0 M_\odot pc-1 |
|
1306.6314 🔍 (source)
|
averaged linear polarization degree |
v sin i |
45.0 ± 15.0 km s-1 |
|
1307.1706 🔍 (source)
|
linear bias |
b |
1.61 ± 0.22 |
|
1307.6585 🔍 (source)
|
median linear radius |
|
360.0 ± 100.0 R_\odot |
|
1307.7061 🔍 (source)
|
linear distance |
r _ { A - B } |
0.013999999999999999 pc |
|
1308.4096 🔍 (source)
|
linear size of the observed radio structure |
|
26.3 kpc |
|
1308.6298 🔍 (source)
|
linear density rate |
|
30.0 M_\odot Myr-1 pc-1 |
|
1309.4423 🔍 (source)
|
linear radius |
R |
2.32 ± 0.09 R_\odot |
|
1309.4272 🔍 (source)
|
linear relation |
|
-48.0 |
|
1309.4272 🔍 (source)
|
linear relation |
\Omega _ { b } / \Omega _ { 0 } |
0.02 |
|
1309.5949 🔍 (source)
|
linear correlation factor |
|
0.0086 |
|
1312.6106 🔍 (source)
|
linear density |
G \mu / c ^ { 2 } |
7.36e-07 |
Upper |
1312.7181 🔍 (source)
|
linear |
L _ { th } |
0.84 |
|
1401.2564 🔍 (source)
|
bilinear R -parity breaking |
|
8e-13 |
Upper |
1401.2719 🔍 (source)
|
linear diameters |
|
-12.5 |
Lower |
1403.1400 🔍 (source)
|
linear size |
|
1.4 Mpc |
|
1404.3189 🔍 (source)
|
maximum linear radius |
R |
123.0 ± 14.0 R_\odot |
|
1405.3994 🔍 (source)
|
linear theory bias |
|
1.7 |
|
1405.3994 🔍 (source)
|
linear theory bias |
|
2.17 ± 0.2 |
|
1405.5286 🔍 (source)
|
linear size |
|
0.03 pc |
|
1407.2246 🔍 (source)
|
linear distance |
|
10.19 ± 0.14 ± 0.56 Mpc |
|
1407.4611 🔍 (source)
|
scale height linearly |
|
550.0 pc |
|
1407.4611 🔍 (source)
|
scale height linearly |
log ( age / yr ) |
3.5 Gyr |
|
1407.4801 🔍 (source)
|
linear size |
|
1.1 Mpc |
|
1408.6620 🔍 (source)
|
linear size |
|
0.036 pc |
|
1409.2417 🔍 (source)
|
fractional linear polarization |
p |
2.1 ± 1.6 |
|
1410.3000 🔍 (source)
|
radial velocity linear trend |
\dot { \gamma } |
0.44 ± 0.04 m s-1 day-1 |
|
1411.0776 🔍 (source)
|
linear velocity gradient |
|
1.0 ± 0.1 km day s-1 |
|
1411.5688 🔍 (source)
|
large-scale linear galaxy bias |
b _ { L } ^ { HOD } |
2.82 ± 0.27 |
|
1411.5638 🔍 (source)
|
stellar linear radii |
R _ { \ast } |
1.203 ± 0.061 R_\odot |
|
1411.5638 🔍 (source)
|
stellar linear radii |
|
0.805 ± 0.016 |
|
1412.6117 🔍 (source)
|
peak-to-peak modulation in degree of linear polarization |
\Delta P |
0.000294 ± 3.5e-05 (ppm) |
|
1501.06205 🔍 (source)
|
non-linear transverse motions perpendicular to |
|
-31.0 km s-1 |
|
1503.00837 🔍 (source)
|
linear radius |
|
7.4e+16 ± 3000000000000000.0 cm |
|
1504.02270 🔍 (source)
|
average linear decay |
D |
-0.022 ± 0.002 |
|
1506.03089 🔍 (source)
|
linear distance |
|
22.49 ± 0.41 ± 1.24 Mpc |
|
1506.03089 🔍 (source)
|
linear distance |
|
21.58 ± 0.5 ± 1.19 Mpc |
|
1506.08494 🔍 (source)
|
degree of linear polarization |
P |
1.0 ± 3.4 % |
|
1507.04675 🔍 (source)
|
linear isospin splitting coefficient |
\Delta m _ { 1 } ^ { * } ( \rho _ { 0 } ) |
0.27 ± 0.15 |
|
1507.04675 🔍 (source)
|
linear isospin splitting coefficient |
\Delta m _ { 1 } ^ { * } ( \rho _ { 0 } ) |
0.33 ± 0.16 |
|
1508.00030 🔍 (source)
|
total projected linear size |
|
1.2 Mpc |
|
1508.01679 🔍 (source)
|
linear relation |
\sigma { |
0.3 dex |
|
1508.04982 🔍 (source)
|
linear scale |
|
66.0 kpc |
|
1508.04926 🔍 (source)
|
linear polarization |
|
-2.0 |
|
1509.07147 🔍 (source)
|
median linear major axis FWHM |
|
4.2 ± 0.9 kpc |
|
1510.00015 🔍 (source)
|
linear ephemeris |
BJD _ { TDB } |
2456193.29157 ± 0.00021 |
|
1510.03474 🔍 (source)
|
linearly polarized strain amplitude |
h _ { 0 } |
6.3e-25 |
|
1510.05122 🔍 (source)
|
linear polarization degrees |
P _ { max } |
30.8 |
Upper |
1510.06351 🔍 (source)
|
linear size of the system |
|
2.3 pc |
|
1511.01243 🔍 (source)
|
linear mass ratio |
|
80.0 M_\odot pc-1 |
|
1511.08330 🔍 (source)
|
projected linear distances |
|
324.0 kpc |
|
1601.01353 🔍 (source)
|
degree of linear polarization |
p _ { \text { CL } 99.73 \% } |
2.4 |
Upper |
1601.02701 🔍 (source)
|
degree of linear polarisation |
|
18.81 ± 0.02 % |
|
1601.02701 🔍 (source)
|
degree of linear polarisation |
|
17.01 ± 0.09 |
|
1602.01784 🔍 (source)
|
linear growth rate of structure |
f / b |
0.417 ± 0.089 |
|
1602.04596 🔍 (source)
|
linearly polarized flux density of the pulsar amounts |
|
1.5 ± 0.2 mJy |
|
1602.04596 🔍 (source)
|
linearly polarized flux density of the pulsar amounts |
|
2.3 ± 0.31 mJy |
|
1602.06671 🔍 (source)
|
linear mass density |
|
1600.0 M_\odot pc-1 |
|
1604.01096 🔍 (source)
|
radial projected linear distance |
|
62.0 pc |
|
1604.01987 🔍 (source)
|
linear size |
|
2.0 pc |
|
1604.03945 🔍 (source)
|
best-fit linear |
|
-76.0 ± 26.0 km s-1 |
|
1605.00653 🔍 (source)
|
linear polarisation |
|
1.09 ± 0.27 |
|
1605.00653 🔍 (source)
|
linear polarisation |
|
0.9 ± 0.17 |
|
1605.09495 🔍 (source)
|
linear diameter |
|
0.65 +0.45000000000000007-0.45 pc |
|
1607.04351 🔍 (source)
|
linear radii |
R ( A ) |
0.165 ± 0.006 R_\odot |
|
1607.06452 🔍 (source)
|
linear mass density |
|
4339.5 ± 4285.5 M_\odot pc-1 |
|
1609.01992 🔍 (source)
|
linear source size |
|
1.4 kpc |
|
1609.09501 🔍 (source)
|
linear size of the source |
|
0.5 kpc |
|
1610.06185 🔍 (source)
|
linear radii |
R _ { A } |
1.2234 ± 0.0053 R_\odot (0.43 \%) |
|
1610.07653 🔍 (source)
|
fractional linear polarization |
|
0.6 |
Upper |
1610.07783 🔍 (source)
|
projected linear size |
|
700.0 kpc |
|
1611.07046 🔍 (source)
|
linear growth rate |
f \sigma _ { 8 } |
0.296 +0.075-0.078 |
|
1701.05283 🔍 (source)
|
linear size |
|
5.0 kpc |
|
1701.05690 🔍 (source)
|
linear growth factor |
\alpha |
1.125 ± 0.125 |
|
1702.01215 🔍 (source)
|
linear velocity |
|
1374.0 km s-1 |
|
1703.01394 🔍 (source)
|
linear mass of the filaments |
|
17.92 |
|
1704.00516 🔍 (source)
|
linear size |
|
0.7 Mpc |
|
1704.05868 🔍 (source)
|
linear slope |
|
0.003 ± 0.0005 mag day-1 |
|
1706.08903 🔍 (source)
|
linear velocity gradient |
|
0.2 km s-1 pc-1 |
|
1707.01518 🔍 (source)
|
linear ephemeris |
BJD _ { TDB } |
3.474107 ± 1.9e-06 |
|
1707.01518 🔍 (source)
|
linear ephemeris |
|
2457503.120049 ± 0.00019 |
|
1708.08026 🔍 (source)
|
linear polarization |
|
10.3 |
|
1708.08026 🔍 (source)
|
linear polarization |
|
8.7 |
|
1708.09098 🔍 (source)
|
linear mass density |
|
361.5 M_\odot pc-1 |
|
1708.08876 🔍 (source)
|
linear slope |
m |
4.0999999999999996e-16 ± 4e-17 s-2 day-1 |
|
1708.08635 🔍 (source)
|
linear size of of this standard ruler |
l _ { m } |
11.03 ± 0.25 pc |
|
1708.08928 🔍 (source)
|
projected linear size |
|
1.3 Mpc |
|
1709.01603 🔍 (source)
|
linear polarization degree |
P _ { max } |
7.32 ± 0.25 % |
|
1709.09435 🔍 (source)
|
total mass and linear momentum of the fast outflow |
|
9.6e+37 g cm s-1 |
|
1709.09435 🔍 (source)
|
total mass and linear momentum of the fast outflow |
|
0.00073 M_\odot |
|
1710.05303 🔍 (source)
|
linear obscuration |
|
0.12 |
|
1710.05849 🔍 (source)
|
linear optical polarization |
P |
0.5 ± 0.07 |
|
1710.06182 🔍 (source)
|
linear size |
|
2.2 Mpc |
|
1710.11129 🔍 (source)
|
linear quantity |
10 ^ { 5 } { ( D / H ) } _ { P } |
2.527 ± 0.03 |
|
1711.00696 🔍 (source)
|
linear Holmberg diameter |
|
1.36 kpc |
|
1711.04583 🔍 (source)
|
linear bias of 2MPZ galaxies |
b _ { eff } |
1.1 +0.3-0.4 |
|
1711.06074 🔍 (source)
|
linear effective diameter |
A _ { e } |
3.0 kpc |
Lower |
1712.05054 🔍 (source)
|
linear size |
|
0.22 pc |
|
1801.03062 🔍 (source)
|
linear growth rate of structure |
f \sigma _ { 8 } ( z _ { eff } ) |
0.426 ± 0.077 |
|
1801.03537 🔍 (source)
|
linear fractional brightness change |
\sigma |
0.005 |
|
1801.06080 🔍 (source)
|
linear distance |
d |
40.7 ± 1.4 ± 1.9 Mpc |
|
1802.08257 🔍 (source)
|
fractional linear polarization |
| Q / I | |
0.19 ± 0.02 |
|
1804.01099 🔍 (source)
|
linear size |
|
550.0 kpc |
|
1804.05600 🔍 (source)
|
linear size |
|
0.3 pc |
|
1804.09178 🔍 (source)
|
linear polarization fraction |
|
84.0 ± 15.0 % |
|
1804.09178 🔍 (source)
|
linear polarization fraction |
|
6.0 rad m-2 |
|
1805.01088 🔍 (source)
|
linear speed |
|
682.0 km s-1 |
|
1806.01227 🔍 (source)
|
spectral index of the power spectrum of linear density fluctuations |
P ( k ) : N ^ { 2 } |
2.09e-10 ± 3.3e-11 |
|
1806.03261 🔍 (source)
|
linear density perturbation amplitude |
\sigma _ { 8 } |
0.792 ± 0.006 |
|
1807.07702 🔍 (source)
|
linear phase |
\beta _ { i } |
1.0 |
Lower |
1809.10161 🔍 (source)
|
linear slope |
d \log _ { 10 } M _ { \star } / dM _ { UV } |
0.44 |
|
1809.10738 🔍 (source)
|
non-linear displacement parameter |
\Sigma _ { NL } |
11.8 ± 0.3 Mpc h-1 |
|
1811.07815 🔍 (source)
|
fractional linear polarization |
GHz |
0.5 +0.19999999999999996-0.2 % |
|
1901.00900 🔍 (source)
|
linear |
M _ { vir } |
5000000000.0 M_\odot N |
|
1901.01707 🔍 (source)
|
super-linear Kennicutt-Schmidt relation |
n _ { KS } |
1.47 |
|
1901.03441 🔍 (source)
|
maximum degree of linear polarization |
|
1.16 ± 0.06 % |
|
1902.06581 🔍 (source)
|
linear bias of RLAGN |
b |
2.5 ± 0.8 |
|
1902.06955 🔍 (source)
|
linear bias |
b |
2.7 ± 0.3 |
|
1903.02994 🔍 (source)
|
nonlinear parameter |
f _ { NL } |
-1.0 |
|
1904.07261 🔍 (source)
|
linear polarization |
\Pi |
0.6 ± 0.19 |
|
1904.07261 🔍 (source)
|
linear polarization |
|
0.87 ± 0.13 |
|
1904.08111 🔍 (source)
|
linear polarization degree in the millimeter band |
|
0.27 ± 0.04 |
|
1904.10259 🔍 (source)
|
total linear size |
|
4.0 |
|
1905.11156 🔍 (source)
|
linear radius |
|
1.5 ± 0.04 R_\odot |
|
1906.06790 🔍 (source)
|
non-linear parameter |
| f _ { NL } | |
1.0 |
Upper |
1906.09760 🔍 (source)
|
cumulative linear mass |
|
12.0 |
|
1908.03232 🔍 (source)
|
linear radius |
|
2.0 ± 0.03 R_\odot |
|
1908.06080 🔍 (source)
|
projected linear size |
|
1.1 Mpc |
|
1908.10885 🔍 (source)
|
linear polarization |
|
66.0 +26.0-27.0 |
|
1910.05687 🔍 (source)
|
linear polarization upper |
| \Pi | |
12.0 |
Upper |
1910.11624 🔍 (source)
|
optical linear polarisation |
P _ { V } |
8.0 |
|
1911.03502 🔍 (source)
|
off-axis linear polarisation leakage |
|
1.4 |
Upper |
1911.13081 🔍 (source)
|
linear rotation |
|
-5.0 +1.6-1.9 km s-1 |
|
2001.10546 🔍 (source)
|
linear polarization |
| Q / I | |
0.12 ± 0.04 |
Lower |
2004.04952 🔍 (source)
|
intrinsic linear polarization of the system |
|
275.3 ± 31.9 |
|
2004.06730 🔍 (source)
|
linear fractional polarization |
\Pi _ { L } |
0.3 |
Upper |
2004.06730 🔍 (source)
|
linearly polarized intensity |
P |
97.2 Jy |
Upper |
2004.08363 🔍 (source)
|
effective linear equation |
H _ { 0 } + 30.93 w |
36.47 |
Upper |
2004.13756 🔍 (source)
|
linear size of this component |
|
4.0 kpc |
|
2006.10028 🔍 (source)
|
linear size |
\alpha |
-1.5 |
Upper |
2007.09008 🔍 (source)
|
normalisation of the linear power spectrum |
D _ { H } ( z _ { eff } ) / r _ { drag } |
20.0 +2.4-2.2 |
|
2007.09009 🔍 (source)
|
linear growth rate of structure |
f \sigma _ { 8 } ( z _ { eff } ) |
0.35 ± 0.1 |
|
2007.08999 🔍 (source)
|
linear growth rate of structure |
f ( z _ { eff } ) \sigma _ { 8 } ( z _ { eff } ) |
0.476 ± 0.047 |
|