|
astro-ph/9702199 🔍 (source)
|
relative |
|
21.5 ± 4.9 km s-1 kpc-1 |
|
|
astro-ph/9806125 🔍 (source)
|
semi-major axis A of the relative orbit |
|
10.57 ± 0.16 R_\odot |
|
|
astro-ph/9810079 🔍 (source)
|
solar motion relative to |
U _ { \odot } |
9.7 ± 0.3 km s-1 |
|
|
astro-ph/9812133 🔍 (source)
|
age of the universe relative to the Hubble time |
t _ { 0 } ^ { flat } |
14.9 +1.4-1.1 (0.63 / h) Gyr |
|
|
astro-ph/9904137 🔍 (source)
|
Fe relative to the solar |
{ [ M / H ] _ { \odot } |
-0.9 |
|
|
astro-ph/9904261 🔍 (source)
|
relative abundance |
] / [ H _ { 2 } ] |
9e-06 ± 3.5e-06 |
|
|
astro-ph/9905075 🔍 (source)
|
relative |
|
5.9 ± 0.4 m as |
|
|
astro-ph/9907195 🔍 (source)
|
relative reflected light flux |
|
5e-05 |
Upper |
|
astro-ph/0101550 🔍 (source)
|
velocities relative |
|
62.5 ± 37.5 km s-1 |
Lower |
|
astro-ph/0104466 🔍 (source)
|
overabundance relative to iron |
[ Co / Fe ] |
0.31 ± 0.05 |
|
|
astro-ph/0105292 🔍 (source)
|
mean space velocity components for the Association relative to the Sun |
U |
-3.8 ± 1.2 |
|
|
astro-ph/0105291 🔍 (source)
|
space velocity components relative |
U |
-9.8 ± 1.2 |
|
|
astro-ph/0107314 🔍 (source)
|
abundance relative to solar |
|
0.26 ± 0.15 |
|
|
astro-ph/0111006 🔍 (source)
|
relative amplitude |
\Delta \nu / \nu |
2.4000000000000003e-08 |
|
|
astro-ph/0205300 🔍 (source)
|
relative iron abundance |
\Delta { [ Fe / H ] } |
0.04 ± 0.07 |
|
|
astro-ph/0205352 🔍 (source)
|
metallicity relative to solar |
[ Zn / H ] |
-1.75 |
Upper |
|
astro-ph/0206503 🔍 (source)
|
relative transverse velocity of the lens projected into the observer plane |
\tilde { v } |
12.5 ± 1.1 km s-1 |
|
|
astro-ph/0208450 🔍 (source)
|
mean abundances relative to solar |
[ Si / H ] |
-1.26 ± 0.13 |
|
|
astro-ph/0303010 🔍 (source)
|
minimum relative inclination |
|
85.0 |
|
|
astro-ph/0305024 🔍 (source)
|
Oxygen abundances relative to hydrogen range |
Tree(positive_expression, [FunctionSymbol(LeafSymbol('log'), BinaryOperatorExpression('/', LeafSymbol('O'), LeafSymbol('H')))]) |
9.0 |
Upper |
|
astro-ph/0309302 🔍 (source)
|
lens-source relative proper motion |
\mu _ { rel } |
27.0 ± 2.0 km s-1 kpc-1 |
|
|
astro-ph/0310346 🔍 (source)
|
Oxygen abundances relative to hydrogen range |
log ( O / H ) |
9.0 |
Upper |
|
astro-ph/0404470 🔍 (source)
|
ISW effect relative to |
|
1.13 ± 0.35 |
|
|
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/0407426 🔍 (source)
|
space density relative to the thin disk |
|
0.08499999999999999 +0.065-0.06499999999999999 |
|
|
astro-ph/0407596 🔍 (source)
|
velocity of the core relative to the rest |
|
230.0 km s-1 |
|
|
astro-ph/0409204 🔍 (source)
|
projected relative position |
|
2000.0 km |
|
|
astro-ph/0409352 🔍 (source)
|
overabundant relative |
[ N / O ] |
2.5 ± 0.5 |
|
|
astro-ph/0504174 🔍 (source)
|
individual ^ { 16 } OH column densities relative to water give ratios |
[ H _ { 2 } O/OH |
0.8999999999999999 +0.30000000000000004-0.29999999999999993 |
|
|
astro-ph/0505057 🔍 (source)
|
Sun ’ s motion relative |
{ ( U , V , W ) } _ { \odot } |
10.1 |
|
|
astro-ph/0505057 🔍 (source)
|
Sun ’ s motion relative |
{ ( U , V , W ) } _ { \odot } |
4.0 |
|
|
astro-ph/0505141 🔍 (source)
|
Apparent speeds of jet components relative |
|
0.028 c |
Upper |
|
astro-ph/0505499 🔍 (source)
|
production rate ratio of HCN relative |
H _ { 2 } O |
0.0007400000000000001 ± 0.00039 |
|
|
astro-ph/0505499 🔍 (source)
|
production rate ratio of HCN relative |
H _ { 2 } O |
0.0033 ± 0.0011 |
|
|
astro-ph/0506484 🔍 (source)
|
velocity dispersion of all nine stars relative |
|
15.0 ± 4.0 km s-1 |
|
|
astro-ph/0507134 🔍 (source)
|
relative magnesium abundance |
grad _ { Z } [ Mg / Fe ] |
0.06 ± 0.02 |
|
|
astro-ph/0509812 🔍 (source)
|
lag relative to the thin disk |
|
63.0 km s-1 |
|
|
astro-ph/0509914 🔍 (source)
|
relative to |
|
1.2 ks |
|
|
astro-ph/0511553 🔍 (source)
|
error of the relative proper motions |
|
4.2 m as yr-1 |
|
|
astro-ph/0601716 🔍 (source)
|
semimajor axis of the relative orbit |
a |
29.32 ± 0.04 R_\odot |
|
|
astro-ph/0603276 🔍 (source)
|
lens-source relative proper motion |
\mu |
8.5 ± 1.5 m as yr-1 |
|
|
astro-ph/0603275 🔍 (source)
|
correlative scatter |
|
0.2 |
|
|
astro-ph/0604555 🔍 (source)
|
relative magnesium abundance |
grad _ { Z } [ Mg / Fe ] |
0.13 ± 0.02 |
|
|
astro-ph/0604592 🔍 (source)
|
mean relative abundance |
\langle [ Mn / Fe ] \rangle |
-0.37 ± 0.01 |
|
|
astro-ph/0606445 🔍 (source)
|
C/CO relative abundance |
|
0.2 |
|
|
astro-ph/0607376 🔍 (source)
|
metallicities relative to solar |
[ X / H ] |
-1.3 |
Lower |
|
astro-ph/0608111 🔍 (source)
|
relative proper motion |
|
102.0 m as yr-1 |
|
|
astro-ph/0610921 🔍 (source)
|
galaxy ’ s velocity relative to the intra-cluster medium |
|
-550.0 km s-1 |
Upper |
|
astro-ph/0611540 🔍 (source)
|
deprojected relative size |
a _ { bar } / R _ { 25 } |
0.3 ± 0.2 |
Lower |
|
astro-ph/0702570 🔍 (source)
|
relative humidity |
|
90.0 |
Lower |
|
0705.3057 🔍 (source)
|
relative proximity |
|
3.8 ± 0.6 Mpc |
|
|
0706.2900 🔍 (source)
|
relative proper motions |
|
2.7 m as yr-1 |
|
|
0706.2900 🔍 (source)
|
relative proper motions |
|
105.0 km s-1 |
|
|
0706.4093 🔍 (source)
|
relative escape fraction |
f _ { esc , rel } |
1.0 |
Upper |
|
0707.1711 🔍 (source)
|
relative disk mass |
h |
2.0 |
Upper |
|
0707.4252 🔍 (source)
|
relative abundance |
[ F / Fe ] |
2.9 |
|
|
0708.3088 🔍 (source)
|
CO abundances relative |
|
0.44 ± 0.03 % |
|
|
0801.3682 🔍 (source)
|
metallicities relative to solar |
[ X / H ] |
-1.3 |
Lower |
|
0804.0116 🔍 (source)
|
abundances relative |
|
-0.03 ± 0.12 |
|
|
0804.0116 🔍 (source)
|
abundances relative |
S |
0.16 ± 0.11 |
|
|
0804.0803 🔍 (source)
|
mean relative Compton reflection |
R |
0.9 +0.6-0.5 |
|
|
0805.0573 🔍 (source)
|
HD abundance relative |
H _ { 2 } |
1.4500000000000003e-05 +3.499999999999999e-06-3.5000000000000012e-06 |
|
|
0807.0930 🔍 (source)
|
relative abundances |
[ Si / Fe ] |
0.23 ± 0.05 |
|
|
0807.3744 🔍 (source)
|
relative distance |
|
17.0 kpc |
|
|
0809.3139 🔍 (source)
|
rest–frame relative LOS velocity |
v _ { rf } |
2000.0 km s-1 |
|
|
0904.3127 🔍 (source)
|
relative proper motion |
|
58.0 ± 1.0 m as yr-1 |
|
|
0905.0495 🔍 (source)
|
accretion rate relative to Eddington |
|
0.21 +0.06-0.1 |
|
|
0908.0529 🔍 (source)
|
source-lens relative motion |
\mu |
5.0 m as yr-1 |
|
|
0908.0733 🔍 (source)
|
timing of the X-ray blast relative to the GRB trigger time |
t _ { 0 } |
11.0 ± 417.0 s |
|
|
0908.3133 🔍 (source)
|
relative flux |
|
0.88 |
|
|
0909.0707 🔍 (source)
|
^ { 13 } CO/C ^ { 18 } O line ratio the relative abundance of the two species |
( \mathrm { [ ^ { 13 } CO ] / [ C ^ { 18 } O ] } |
7.0 |
|
|
0911.4019 🔍 (source)
|
relative |
H |
0.089 ± 0.009 |
|
|
1001.0604 🔍 (source)
|
relative depth |
|
0.00087 |
|
|
1001.3412 🔍 (source)
|
translate to relative escape fraction |
f _ { esc , rel } |
0.21 |
|
|
1001.3412 🔍 (source)
|
translate to relative escape fraction |
|
0.03 |
Upper |
|
1001.4080 🔍 (source)
|
s relative |
\Delta \mu / \mu |
5.6e-06 ± 5.5e-06 (stat) ± 2.7e-06 (sys) |
|
|
1005.2729 🔍 (source)
|
fractional abundance relative to H nuclei |
|
7.5e-10 |
|
|
1005.4080 🔍 (source)
|
relative |
|
0.07 +0.009999999999999995-0.010000000000000009 M_\odot |
|
|
1006.3664 🔍 (source)
|
relative depths |
|
0.04 |
Upper |
|
1007.1102 🔍 (source)
|
total water content ( relative to molecular hydrogen |
|
6.6e-05 |
|
|
1008.3161 🔍 (source)
|
relative to volatiles |
T _ { C } |
900.0 K |
Upper |
|
1010.2146 🔍 (source)
|
flux relative contribution |
|
0.23 ± 0.02 |
|
|
1105.0082 🔍 (source)
|
FDD relative |
|
0.85 ± 0.02 |
|
|
1105.3108 🔍 (source)
|
kinetic temperature of this relatively warm gas |
T _ { kin } |
260.0 ± 240.0 K |
|
|
1105.5920 🔍 (source)
|
fractional CH abundance relative |
H _ { 2 } |
-8.0 |
Upper |
|
1106.4301 🔍 (source)
|
average water abundance relative |
H _ { 2 } |
1.3999999999999998e-07 |
|
|
1107.1484 🔍 (source)
|
relative brightness |
\Delta { K _ { s } } |
5.09 ± 0.1 |
|
|
1107.4313 🔍 (source)
|
relative proximity |
|
60.0 kpc |
|
|
1109.2617 🔍 (source)
|
mean relative velocity |
|
235.0 km s-1 |
|
|
1204.0122 🔍 (source)
|
rate of relative mass change |
\Delta m _ { 1 } / m |
5.18e-08 yr-1 |
|
|
1205.6739 🔍 (source)
|
appreciable relative velocity |
|
42.0 km s-1 |
|
|
1206.2275 🔍 (source)
|
relative abundances |
\log ( N / O ) |
1.32 ± 0.05 |
|
|
1209.0456 🔍 (source)
|
rotational lag of the thick disk component relative |
LSR v _ { thick , lag } |
49.0 km s-1 |
|
|
1209.1043 🔍 (source)
|
degradation relative |
\Delta \chi _ { eff } ^ { 2 } |
1.0 |
Upper |
|
1210.1154 🔍 (source)
|
gas-phase relative abundance |
[ Zn / Fe ] |
1.0 |
|
|
1301.4024 🔍 (source)
|
mass density of dust grains relative to hydrogen |
\rho _ { dust } / \rho _ { H } |
120.0 |
Lower |
|
1304.2039 🔍 (source)
|
relative distances |
|
0.53 ± 0.06 |
|
|
1304.2039 🔍 (source)
|
relative distances |
|
0.53 ± 0.07 |
|
|
1305.1337 🔍 (source)
|
dimensionless gravitational potential relative |
\Delta \phi |
5e-05 |
|
|
1308.2470 🔍 (source)
|
gravitational potentials relative |
\Delta \phi |
0.1 |
|
|
1309.1371 🔍 (source)
|
proportion of dust mass relative to stellar mass |
M _ { dust } / M _ { star } |
0.02 % |
|
|
1309.2282 🔍 (source)
|
dust relative abundance |
A |
0.072 |
|
|
1310.6231 🔍 (source)
|
OH } abundances relative to total number of hydrogen atoms |
|
2.2999999999999998e-10 |
|
|
1310.8569 🔍 (source)
|
iron depleted relative |
zinc [ Zn / Fe ] |
0.45 ± 0.06 |
|
|
1311.3424 🔍 (source)
|
lens-source relative proper motion |
\mu _ { rel } |
7.6 ± 1.6 m as yr-1 |
|
|
1311.5035 🔍 (source)
|
mutual inclination relative to the belt plane |
|
29.0 |
Upper |
|
1312.3951 🔍 (source)
|
lens-source relative proper motion |
\mu _ { rel } |
19.6 ± 1.6 m as yr-1 |
|
|
1312.7297 🔍 (source)
|
lens-source relative proper motion |
|
20.0 m as |
Lower |
|
1401.1104 🔍 (source)
|
HF abundance relative |
|
0.00018 ± 5e-05 |
|
|
1401.1104 🔍 (source)
|
CH _ { 3 } OH abundances relative |
|
2.7 ± 0.3 % |
|
|
1401.1104 🔍 (source)
|
CH _ { 3 } OH abundances relative |
|
3.4 ± 0.6 % |
|
|
1403.3229 🔍 (source)
|
accretion rate relative to the Eddington |
|
3.2 |
Lower |
|
1403.5850 🔍 (source)
|
ratio of nickel to iron relative to |
|
11.0 +4.0-3.0 |
|
|
1406.4081 🔍 (source)
|
relative abundances |
|
1.1000000000000001e-08 +9e-09-9.000000000000001e-09 |
|
|
1407.2185 🔍 (source)
|
CO relative to water |
|
0.14 ± 0.03 |
|
|
1407.3714 🔍 (source)
|
High relative speed |
|
60.0 km s-1 |
|
|
1408.3534 🔍 (source)
|
1 \sigma relative error |
|
4.9999999999999996e-06 |
|
|
1410.5832 🔍 (source)
|
matter density relative |
\Omega _ { M } |
0.3 |
|
|
1410.7060 🔍 (source)
|
radial velocities relative |
|
-4.0 km s-1 |
|
|
1412.0690 🔍 (source)
|
water enrichment ( relative to solar |
|
0.75 |
Upper |
|
1412.0690 🔍 (source)
|
water enrichment ( relative to solar |
|
0.1 |
Lower |
|
1412.8318 🔍 (source)
|
CH _ { 3 } CHO relative abundance |
|
2.5e-08 ± 5e-09 |
|
|
1501.05311 🔍 (source)
|
relative |
A _ { I } / E ( V - I |
1.2899 |
|
|
1501.05311 🔍 (source)
|
relative |
\Delta \mu _ { LMC } |
10.72 ± 0.03 |
|
|
1502.06978 🔍 (source)
|
relative |
|
0.07 |
Lower |
|
1504.05702 🔍 (source)
|
inclination relative to the disk |
|
10.0 |
Upper |
|
1506.07878 🔍 (source)
|
s relative flux |
|
2.7 day |
|
|
1509.05287 🔍 (source)
|
relative velocities |
|
2.4 |
|
|
1509.05287 🔍 (source)
|
relative velocities |
\Delta v _ { O } |
4.0 km s %-1 |
|
|
1509.06555 🔍 (source)
|
relative |
A _ { tSZ - CIB } |
1.2 ± 0.3 |
|
|
1510.01329 🔍 (source)
|
mass density relative to the critical density of the Universe |
\Omega _ { C~ { } \textsc { IV } } Â |
1e-07 ± 1.5000000000000002e-08 |
|
|
1602.05098 🔍 (source)
|
Ni abundance relative to its decay product |
|
59.0 C |
|
|
1603.05677 🔍 (source)
|
lens-source relative proper motion |
\mu _ { rel } |
6.5 ± 1.1 m as yr-1 |
|
|
1604.03939 🔍 (source)
|
ISW effect signal amplitudes relative |
A |
1.0 |
|
|
1606.05873 🔍 (source)
|
velocity relative |
r _ { h } |
0.43 AU |
|
|
1606.05873 🔍 (source)
|
velocity relative |
\Delta |
0.84 AU |
|
|
1607.04325 🔍 (source)
|
logarithmic scale relative to |
[ Z ] |
-0.37 ± 0.03 |
|
|
1609.07252 🔍 (source)
|
OCS abundances relative |
|
32.0 |
|
|
1609.07440 🔍 (source)
|
microlensing magnification of B relative |
A |
1.4 |
|
|
1611.01156 🔍 (source)
|
CH _ { 3 } OH column density relative |
H _ { 2 } ( X _ { CH _ { 3 } OH } ) |
8e-09 |
|
|
1611.05473 🔍 (source)
|
relative |
|
0.2 dex |
|
|
1611.05882 🔍 (source)
|
relative escape fraction |
f _ { esc } ^ { rel } |
0.09 ± 0.04 |
|
|
1611.09373 🔍 (source)
|
separation ( relative to the stellar radius |
/ R _ { \star } |
3.5 |
|
|
1701.03112 🔍 (source)
|
average strengths of these lines relative to the far-IR continuum |
|
0.00084 ± 0.00017 |
|
|
1701.03112 🔍 (source)
|
average strengths of these lines relative to the far-IR continuum |
|
0.00035999999999999997 ± 0.00012 |
|
|
1701.03112 🔍 (source)
|
average strengths of these lines relative to the far-IR continuum |
|
0.00027 ± 0.0001 |
|
|
1702.02213 🔍 (source)
|
relative differential rotation |
\Delta \Omega / \Omega |
8.0 ± 0.9 % |
|
|
1703.05624 🔍 (source)
|
relative position |
|
46.0 ± 1.0 m as W |
|
|
1703.05491 🔍 (source)
|
mass fraction of baryons relative to the total dark matter halo |
m _ { d } |
0.05 |
Lower |
|
1703.08381 🔍 (source)
|
efficiency of transformation into dSphs relative to their |
f _ { gas } |
0.0 |
|
|
1704.03481 🔍 (source)
|
center relative |
\tau _ { dep } |
2.4 Gyr s |
|
|
1705.00964 🔍 (source)
|
relative |
|
9.7 km s-1 |
|
|
1705.03937 🔍 (source)
|
lens-source relative proper motion |
\mu _ { rel } |
11.8 ± 0.8 m as yr-1 |
|
|
1705.06355 🔍 (source)
|
LyC escape fraction relative to |
f _ { esc } |
5.6 % |
Upper |
|
1707.03880 🔍 (source)
|
relative escape fraction |
f _ { 900 } ^ { e } |
911.8 |
|
|
1707.06003 🔍 (source)
|
peak o- \mathrm { H } _ { 2 } S abundances relative |
H _ { 2 } |
2.5e-05 |
|
|
1707.06003 🔍 (source)
|
peak o- \mathrm { H } _ { 2 } S abundances relative |
|
4e-07 |
Lower |
|
1709.06991 🔍 (source)
|
maximum relative flux increase |
|
50.0 |
Lower |
|
1709.06747 🔍 (source)
|
mean relative radio emissivity |
|
0.7 ± 0.13 |
|
|
1709.08476 🔍 (source)
|
lens-source relative proper motion |
\mu |
6.0 m as yr-1 |
|
|
1803.07082 🔍 (source)
|
relative |
\langle \alpha \rangle |
1.09 ± 0.08 |
|
|
1804.09721 🔍 (source)
|
relative Lyman continuum escape fractions |
f _ { abs } ( LyC ) |
0.4 +10.1-0.4 % |
|
|
1804.10197 🔍 (source)
|
relative velocity |
|
870.0 +69.0-66.0 km s-1 |
|
|
1805.08277 🔍 (source)
|
relative proper motion |
|
80.0 ± 11.0 km s-1 |
|
|
1806.08453 🔍 (source)
|
lens-source relative proper motion |
\mu |
12.4 ± 1.1 m as yr-1 |
|
|
1809.04863 🔍 (source)
|
A relative radial forcing |
dF _ { r } |
1.5 % |
|
|
1809.09009 🔍 (source)
|
relative velocity |
|
24.7 km s-1 |
|
|
1810.05650 🔍 (source)
|
projected velocity relative |
|
38.0 ± 17.0 km s-1 |
|
|
1810.06596 🔍 (source)
|
relative radial velocity |
|
4.5 ± 5.0 km s-1 |
|
|
1812.08860 🔍 (source)
|
relative motion |
|
1.12 ± 0.15 m as yr-1 (0.61 \pm 0.09 km s ^ -1) |
|
|
1902.01826 🔍 (source)
|
relative flux |
|
2.7 % |
|
|
1904.04489 🔍 (source)
|
minimum relative amplitude |
|
0.08 ± 0.05 |
|
|
1904.04489 🔍 (source)
|
minimum relative amplitude |
\Delta \Omega / \Omega |
0.14 ± 0.05 |
|
|
1905.05369 🔍 (source)
|
CO relative abundances |
N ( CO ) / H _ { 2 } |
2e-06 |
Upper |
|
1905.08540 🔍 (source)
|
lens-source relative proper motion |
|
2.8 ± 0.5 m as |
|
|
1905.08540 🔍 (source)
|
lens-source relative proper motion |
\mu _ { rel } |
46.0 ± 8.0 m as |
|
|
1906.09827 🔍 (source)
|
rotates relative |
|
0.1 m as yr-1 |
|
|
1911.02439 🔍 (source)
|
source-lens relative proper motion |
\mu _ { rel } |
9.0 m as yr-1 |
|
|
1912.00588 🔍 (source)
|
H i abundance relative to total hydrogen |
H i ] / [ H ] |
0.0044 |
|
|
1912.03822 🔍 (source)
|
relative |
q |
4.3700000000000005e-05 |
|
|
1912.09618 🔍 (source)
|
relative intensity |
|
193.0 |
|
|
1912.09618 🔍 (source)
|
relative intensity |
|
171.0 |
|
|
1912.10213 🔍 (source)
|
relative velocity |
|
23.0 km s-1 |
|
|
2001.04975 🔍 (source)
|
average relative intensities of the first four { { } ^ { 12 } CO } J transitions |
|
0.7 |
|
|
2001.04975 🔍 (source)
|
average relative intensities of the first four { { } ^ { 12 } CO } J transitions |
|
0.92 |
|
|
2001.04975 🔍 (source)
|
average relative intensities of the first four { { } ^ { 12 } CO } J transitions |
|
0.57 |
|
|
2007.05519 🔍 (source)
|
relative escape fraction of individual galaxies |
f _ { esc , rel } |
0.16 ± 0.06 |
Upper |