astro-ph/9309040 🔍 (source)
|
spectral index of the power spectrum |
n |
-1.0 |
Upper |
astro-ph/9311056 🔍 (source)
|
slope of the power spectrum of density perturbations |
n |
-1.0 |
Upper |
astro-ph/9311068 🔍 (source)
|
spectrum |
\lambda _ { peak } |
51.0 ± 18.0 Mpc h-1 |
|
astro-ph/9402024 🔍 (source)
|
effective power spectrum index |
n _ { eff } |
1.35 |
|
astro-ph/9404009 🔍 (source)
|
spectrum |
n |
1.0 |
|
astro-ph/9512151 🔍 (source)
|
spectral parameter of the power spectrum of primordial perturbation |
n |
1.84 ± 0.29 |
|
astro-ph/9609194 🔍 (source)
|
soft intrinsic QSO spectrum |
\alpha _ { Q } |
1.9 +0.10000000000000009-0.09999999999999987 |
|
astro-ph/9610219 🔍 (source)
|
spectrum |
n |
1.0 |
Lower |
astro-ph/9611029 🔍 (source)
|
faint source spectrum |
\alpha |
0.95 +0.1-0.15 |
|
astro-ph/9612016 🔍 (source)
|
power spectrum normalisation |
\mbox { $Q _ { rms - ps } |
21.0 ± 1.6 K |
|
astro-ph/9703043 🔍 (source)
|
power spectrum normalisation |
Q _ { rms - ps } |
22.0 +10.0-6.0 K |
|
astro-ph/9703181 🔍 (source)
|
power-law index of the GRB spectrum |
s |
-1.1 ± 0.3 |
|
astro-ph/9704246 🔍 (source)
|
power spectrum |
\Omega h |
0.2 |
|
astro-ph/9705180 🔍 (source)
|
power spectrum of the density fluctuations |
k _ { c } |
0.055 +0.045000000000000005-0.045 Mpc-1 |
|
astro-ph/9706077 🔍 (source)
|
position of the dominant peak in the best-fit power spectrum |
A _ { peak } |
76.0 +3.0-7.0 K |
|
astro-ph/9706077 🔍 (source)
|
power spectrum normalization |
\ell |
10.0 |
|
astro-ph/9706118 🔍 (source)
|
steep X-ray spectrum |
\alpha _ { energy } |
1.5 |
Lower |
astro-ph/9709020 🔍 (source)
|
power spectrum |
\beta |
0.6 |
Upper |
astro-ph/9709020 🔍 (source)
|
power spectrum |
|
0.5 |
Lower |
astro-ph/9709198 🔍 (source)
|
power-law index of the power spectrum in this range |
|
-1.4 |
|
astro-ph/9712030 🔍 (source)
|
power spectrum |
\sigma _ { 8 } \Omega ^ { 0.53 } |
0.6 |
|
astro-ph/9801106 🔍 (source)
|
energy spectrum of the neutrino emission from electron-positron pair annihilation |
M |
50000.0 M_\odot |
Lower |
astro-ph/9801136 🔍 (source)
|
BAL spectrum |
|
0.4 |
Lower |
astro-ph/9802109 🔍 (source)
|
mass power-spectrum |
\sigma _ { 8 } |
0.67 |
|
astro-ph/9802299 🔍 (source)
|
spectrum |
T _ { eff } |
900.0 K |
|
astro-ph/9804019 🔍 (source)
|
spectrum |
z _ { em } |
2.22 |
|
astro-ph/9804333 🔍 (source)
|
flat-spectrum |
S _ { 5 GHz } |
25.0 |
Lower |
astro-ph/9806026 🔍 (source)
|
power spectrum |
|
-1.0 |
|
astro-ph/9807213 🔍 (source)
|
spectrum |
\Gamma |
0.8 |
|
astro-ph/9807240 🔍 (source)
|
power spectrum |
|
0.55 |
Upper |
astro-ph/9807240 🔍 (source)
|
power spectrum |
\Omega _ { 0 } |
0.1 |
Lower |
astro-ph/9807240 🔍 (source)
|
power spectrum |
\Omega _ { 0 } |
0.1 |
Lower |
astro-ph/9807240 🔍 (source)
|
slope of the power spectrum |
\Omega _ { 0 } |
0.6 |
Upper |
astro-ph/9810006 🔍 (source)
|
steep spectrum |
n |
-1.5 |
|
astro-ph/9810364 🔍 (source)
|
power spectrum |
\Omega _ { 0 } ^ { m } |
1.0 |
|
astro-ph/9810398 🔍 (source)
|
spectrum |
peak |
20.0 keV |
|
astro-ph/9811199 🔍 (source)
|
spectrum |
|
43.0 ± 7.0 |
|
astro-ph/9812245 🔍 (source)
|
power-law spectrum |
\Gamma |
2.2 |
|
astro-ph/9812247 🔍 (source)
|
power-law spectrum of index |
n |
-1.9 |
|
astro-ph/9812311 🔍 (source)
|
spectrum |
b _ { P } |
1.0 |
Upper |
astro-ph/9901061 🔍 (source)
|
spectrum |
|
-0.6 |
Lower |
astro-ph/9901351 🔍 (source)
|
power spectrum |
\beta |
0.58 ± 0.26 |
|
astro-ph/9901351 🔍 (source)
|
power spectrum |
\Gamma |
0.2 |
|
astro-ph/9901351 🔍 (source)
|
power spectrum |
\beta |
0.47 ± 0.16 |
|
astro-ph/9901393 🔍 (source)
|
power spectrum slope |
n |
0.7 |
|
astro-ph/9903146 🔍 (source)
|
spectrum |
m _ { R } |
24.4 |
|
astro-ph/9903450 🔍 (source)
|
power spectrum |
|
0.9 |
|
astro-ph/9903472 🔍 (source)
|
shape parameter of the mass power-spectrum |
\Gamma |
0.15 |
|
astro-ph/9906127 🔍 (source)
|
EUV spectrum |
|
112.5 ± 37.5 |
|
astro-ph/9909239 🔍 (source)
|
power density spectrum |
|
33.0 hr |
|
astro-ph/9909487 🔍 (source)
|
spectrum |
\sigma _ { 8 } \Omega _ { m } ^ { 0.6 } |
0.8 ± 0.2 |
|
astro-ph/9910349 🔍 (source)
|
spectrum |
z _ { e } |
1.202 |
|
astro-ph/9910484 🔍 (source)
|
power spectrum |
\Gamma |
1.2000000000000002 +0.09999999999999987-0.10000000000000009 |
|
astro-ph/9912127 🔍 (source)
|
unabsorbed reflection spectrum |
R |
0.15 |
Lower |
astro-ph/0001089 🔍 (source)
|
spectrum |
\nu |
-2.25 ± 0.18 |
|
astro-ph/0002052 🔍 (source)
|
soft spectrum ( index |
|
3.39 ± 0.24 |
|
astro-ph/0003008 🔍 (source)
|
normalisation of the mass power spectrum |
\sigma _ { 8 } |
1.5 ± 0.5 |
|
hep-ex/0003006 🔍 (source)
|
differential energy spectrum |
|
6.1e-11 ± 6.999999999999999e-12 |
|
astro-ph/0004068 🔍 (source)
|
soft X-ray spectrum |
kT |
0.5 keV |
|
astro-ph/0005335 🔍 (source)
|
plasma spectrum |
T |
0.7 keV |
|
astro-ph/0006255 🔍 (source)
|
power spectrum |
|
-2.14 ± 0.28 |
|
astro-ph/0007092 🔍 (source)
|
power spectrum |
|
2.3499999999999996 +0.050000000000000266-0.04999999999999982 |
Upper |
astro-ph/0007092 🔍 (source)
|
power spectrum |
|
1.7 |
Lower |
astro-ph/0007263 🔍 (source)
|
X-ray spectrum |
\Gamma _ { x } |
-4.0 |
|
astro-ph/0007274 🔍 (source)
|
source spectrum temperature |
T _ { 0 } |
1.15 +0.15000000000000013-0.1499999999999999 keV |
|
astro-ph/0007284 🔍 (source)
|
fluctuation spectrum |
\sigma _ { 8 } |
1.0 |
|
astro-ph/0007377 🔍 (source)
|
thermal spectrum |
kT _ { 1 } |
0.6 keV |
|
astro-ph/0008211 🔍 (source)
|
spectrum |
|
0.44 ± 0.1 (stat) |
|
astro-ph/0009110 🔍 (source)
|
Crab-like spectrum the X-ray flux |
|
2.5e-13 ± 5e-14 erg s-1 cm-2 |
|
astro-ph/0009105 🔍 (source)
|
power spectrum |
P ( k ) , |
-1.8 |
Lower |
astro-ph/0009105 🔍 (source)
|
power spectrum |
n |
-1.8 |
Lower |
astro-ph/0009110 🔍 (source)
|
Crab-like spectrum the X-ray flux |
f _ { x } |
1.25 ± 1.15 keV |
|
astro-ph/0010367 🔍 (source)
|
X-ray spectrum |
\Gamma |
1.27 ± 0.02 |
|
astro-ph/0011465 🔍 (source)
|
power spectrum index |
\beta |
1.74 |
|
astro-ph/0011469 🔍 (source)
|
power spectrum |
\ell |
197.0 ± 6.0 |
|
astro-ph/0011554 🔍 (source)
|
soft thermal spectrum |
kT |
1.3 keV |
|
astro-ph/0012066 🔍 (source)
|
amplitude of the matter power spectrum |
|
6400.0 +2800.0-1800.0 |
|
astro-ph/0012356 🔍 (source)
|
spectrum |
\alpha _ { r } |
0.7 |
Upper |
astro-ph/0101213 🔍 (source)
|
normalization of the matter power spectrum |
\sigma _ { 8 } \Omega _ { m } ^ { 0.48 } |
0.51 +0.14-0.17 |
|
astro-ph/0102163 🔍 (source)
|
power spectrum |
\Omega _ { m } |
0.3 |
|
astro-ph/0103056 🔍 (source)
|
power spectrum shape parameter |
\Gamma |
0.1 ± 0.1 |
|
astro-ph/0103084 🔍 (source)
|
column density of the CO observed in the STIS spectrum |
N ( CO ) |
71000000000000.0 ± 5000000000000.0 cm-2 |
|
astro-ph/0103227 🔍 (source)
|
local color temperature of the spectrum emerging |
T _ { c } / T _ { eff } |
1.4500000000000002 +0.34999999999999987-0.3500000000000001 |
Lower |
astro-ph/0103343 🔍 (source)
|
power law spectrum |
\alpha _ { x } |
0.92 ± 0.04 |
|
astro-ph/0103417 🔍 (source)
|
flat spectrum |
\Gamma |
1.7 |
|
astro-ph/0104139 🔍 (source)
|
spectrum |
n |
-1.0 |
|
astro-ph/0104329 🔍 (source)
|
low-resolution spectrum |
|
-0.89 ± 0.03 |
|
astro-ph/0104384 🔍 (source)
|
steep spectrum shell emission |
\alpha |
-0.57 |
|
astro-ph/0105022 🔍 (source)
|
steep power spectrum density |
f ^ |
-2.0 |
Lower |
hep-ph/0105064 🔍 (source)
|
spectrum |
m _ { \nu } |
0.26 +0.2-0.14 eV |
|
hep-ph/0105064 🔍 (source)
|
spectrum |
|
2.75 +1.28-0.97 eV |
|
astro-ph/0105131 🔍 (source)
|
thin thermal spectrum of temperature |
|
5.8 ± 0.6 keV |
|
astro-ph/0105194 🔍 (source)
|
two-point spectrum of the core emission |
\alpha _ { rx } |
0.75 |
|
astro-ph/0105450 🔍 (source)
|
power spectrum |
\Omega _ { m } h |
0.2 ± 0.03 |
|
astro-ph/0106029 🔍 (source)
|
steep X-ray spectrum |
\alpha |
1.3 ± 0.1 |
|
astro-ph/0106198 🔍 (source)
|
S/N ratio spectrum |
z _ { em } |
2.4 |
|
astro-ph/0106417 🔍 (source)
|
spectrum of photon index |
\gamma |
1.63 +0.11-0.1 |
|
astro-ph/0109016 🔍 (source)
|
power-law power-spectrum of index |
n |
-1.0 |
Upper |
astro-ph/0109114 🔍 (source)
|
power spectrum normalization |
\sigma _ { 8 } |
0.83 |
|
astro-ph/0109374 🔍 (source)
|
LETGS X-ray spectrum |
|
60.0 pc |
|
astro-ph/0110552 🔍 (source)
|
spectrum |
z _ { em } |
3.7 |
|
astro-ph/0111577 🔍 (source)
|
power-law spectrum of photon index |
|
1.45 ± 0.19 |
|
astro-ph/0201137 🔍 (source)
|
power spectrum of the image features three peaks |
\ell |
213.0 +10.0-13.0 |
|
astro-ph/0201137 🔍 (source)
|
power spectrum of the image features three peaks |
\ell |
541.0 +20.0-32.0 |
|
astro-ph/0201137 🔍 (source)
|
power spectrum of the image features three peaks |
\ell |
845.0 +12.0-25.0 |
|
astro-ph/0201267 🔍 (source)
|
power-law spectrum |
N _ { H } |
8e+22 ± 4e+21 cm-2 |
|
astro-ph/0201375 🔍 (source)
|
power spectrum |
\sigma _ { 8 } |
1.0 |
|
astro-ph/0202218 🔍 (source)
|
power spectrum |
n |
1.27 |
Upper |
astro-ph/0202290 🔍 (source)
|
Harrison-Zeldovich spectrum |
m _ { \nu } |
0.74 eV |
Upper |
astro-ph/0204239 🔍 (source)
|
power spectrum |
\Omega _ { m } h |
0.2 ± 0.03 |
|
astro-ph/0204361 🔍 (source)
|
soft spectrum |
|
0.6 keV |
|
astro-ph/0205160 🔍 (source)
|
blackbody spectrum |
T _ { eff } |
210000000.0 ± 80000000.0 K |
|
astro-ph/0207213 🔍 (source)
|
power spectrum |
\epsilon _ { 1 } |
0.057 |
Upper |
astro-ph/0207515 🔍 (source)
|
spectrum of the luminous |
L _ { bol } |
10.0 L_\odot |
|
astro-ph/0208501 🔍 (source)
|
BeppoSAX spectrum |
\alpha _ { x } |
0.7 |
|
astro-ph/0209127 🔍 (source)
|
column density spectrum |
f ( N _ { HI } ) |
-2.8 |
Lower |
astro-ph/0209244 🔍 (source)
|
velocity power spectrum index |
\beta |
1.74 |
|
astro-ph/0209478 🔍 (source)
|
spectrum |
|
-0.01 |
|
astro-ph/0209487 🔍 (source)
|
differential energy spectrum |
dN / dE |
3.3e-13 ± 9.000000000000001e-14 (stat) ± 3e-14 (syst) |
|
astro-ph/0210007 🔍 (source)
|
scale invariant spectrum |
n _ { s } |
0.97 +0.08-0.05 |
|
astro-ph/0210147 🔍 (source)
|
spectrum |
\alpha |
1.18 ± 0.02 |
|
astro-ph/0210274 🔍 (source)
|
amplitude of matter power spectrum |
\sigma _ { 8 } |
0.9 |
|
astro-ph/0210604 🔍 (source)
|
power spectrum of matter fluctuations |
{ \sigma _ { 8 } ( \Omega _ { m } / 0.3 ) } ^ { 0.57 } |
0.71 +0.12-0.16 |
|
astro-ph/0211090 🔍 (source)
|
matter power spectrum normalization |
\sigma _ { 8 } |
0.78 +0.3-0.06 |
|
astro-ph/0212165 🔍 (source)
|
peak in the power spectrum |
|
144.18 ± 0.06 s |
|
astro-ph/0301037 🔍 (source)
|
spectrum normalization parameter |
|
0.7 |
Lower |
astro-ph/0301037 🔍 (source)
|
spectrum normalization parameter |
\sigma _ { 8 } |
1.1 |
|
astro-ph/0301083 🔍 (source)
|
power spectrum |
\Gamma |
0.19 +0.13-0.04 |
|
astro-ph/0301297 🔍 (source)
|
AGN X-ray spectrum |
|
3e-07 |
|
astro-ph/0301551 🔍 (source)
|
index of primeval fluctuation spectrum |
n _ { p } |
1.0 |
|
astro-ph/0302159 🔍 (source)
|
power spectrum normalization |
C _ { 10 } |
690.0 +200.0-125.0 K2 |
|
astro-ph/0302307 🔍 (source)
|
spectral index of the positron spectrum |
\gamma _ { + } |
3.4 ± 0.06 |
|
astro-ph/0302415 🔍 (source)
|
flat spectrum |
\alpha |
0.05 ± 0.05 |
|
astro-ph/0303168 🔍 (source)
|
perturbation spectrum |
|
0.944 |
|
astro-ph/0304175 🔍 (source)
|
power spectrum |
k _ { 0 } |
0.76 |
|
astro-ph/0304175 🔍 (source)
|
power spectrum |
|
0.05 Mpc-1 |
|
astro-ph/0305600 🔍 (source)
|
steep spectrum |
\alpha |
-1.2 |
|
astro-ph/0307561 🔍 (source)
|
power law index of the relativistic electron spectrum |
p |
2.25 |
|
astro-ph/0308277 🔍 (source)
|
infrared spectrum |
B |
2.6 ± 1.0 |
|
astro-ph/0308278 🔍 (source)
|
spectrum |
T _ { |
2.17 +0.25-0.12 keV |
|
astro-ph/0310735 🔍 (source)
|
scale invariant spectrum |
|
0.95 +0.07-0.04 |
|
astro-ph/0310735 🔍 (source)
|
scale invariant spectrum |
n _ { s } |
0.97 ± 0.02 |
|
astro-ph/0311560 🔍 (source)
|
part of the spectrum the time averaged mass accretion rate |
|
5.7e-13 M_\odot yr-1 |
Lower |
astro-ph/0312357 🔍 (source)
|
mass spectrum slope |
\alpha |
1.6 |
Upper |
astro-ph/0312457 🔍 (source)
|
powerlaw spectrum |
\Gamma |
2.3 |
|
astro-ph/0401026 🔍 (source)
|
hard spectrum |
\Gamma |
1.0 |
|
astro-ph/0401111 🔍 (source)
|
thermal spectrum |
kT |
0.7 keV |
|
astro-ph/0401515 🔍 (source)
|
fluctuation power spectrum normalization |
\sigma _ { 8 } |
0.8 |
Upper |
astro-ph/0401589 🔍 (source)
|
power density spectrum |
|
1008.0 ± 120.0 s |
|
astro-ph/0403592 🔍 (source)
|
soft spectrum |
E |
-4.6 ± 0.5 |
|
astro-ph/0404072 🔍 (source)
|
index of the mass spectrum |
\alpha |
0.6 ± 0.06 |
|
astro-ph/0404132 🔍 (source)
|
scale-invariant pressure fluctuation spectrum |
|
90.0 |
Upper |
astro-ph/0405360 🔍 (source)
|
photon spectrum index |
\Gamma |
1.7 |
|
astro-ph/0406246 🔍 (source)
|
power spectrum normalization |
\sigma _ { 8 } |
0.7 |
|
astro-ph/0406340 🔍 (source)
|
spectrum |
|
21.5 ± 0.5 |
|
astro-ph/0407130 🔍 (source)
|
spectrum |
\alpha _ { 0.843 } ^ { 18 |
-0.5 |
Lower |
astro-ph/0407203 🔍 (source)
|
spectral slope of the FUSE composite spectrum |
\alpha |
-0.56 +0.38-0.28 |
|
astro-ph/0407203 🔍 (source)
|
spectral slope of the FUSE composite spectrum |
F _ { \nu } |
-0.56 +0.38-0.28 |
|
astro-ph/0407377 🔍 (source)
|
linear theory power spectrum amplitude |
\Delta ^ { 2 } _ { L } ( k _ { p } |
0.009 s km-1 |
|
astro-ph/0408549 🔍 (source)
|
unusually steep spectrum |
\alpha |
-2.1 |
Upper |
astro-ph/0409253 🔍 (source)
|
spectrum of photon index |
\Gamma |
1.3 ± 0.5 |
|
astro-ph/0410149 🔍 (source)
|
mean spectrum |
\Gamma |
1.4 ± 0.1 |
|
astro-ph/0410149 🔍 (source)
|
mean intrinsic spectrum |
\Gamma |
1.76 ± 0.08 |
|
astro-ph/0411474 🔍 (source)
|
power spectrum index |
\beta |
1.74 |
|
astro-ph/0501095 🔍 (source)
|
steep radio spectrum |
\alpha |
-0.7 |
|
astro-ph/0502064 🔍 (source)
|
spectrum |
T _ { WD } |
120000.0 K |
|
astro-ph/0502114 🔍 (source)
|
thermal X-ray spectrum |
kT |
0.4 keV |
|
astro-ph/0502243 🔍 (source)
|
amplitude of the power spectrum |
\sigma _ { 8 } |
0.81 +0.15-0.1 |
|
astro-ph/0502326 🔍 (source)
|
power-law spectrum of photon index |
|
2.02 ± 0.13 |
|
nucl-ex/0502021 🔍 (source)
|
B spectrum |
|
1.68 ± 0.06 (stat) +0.08-0.09 (syst) |
|
astro-ph/0503085 🔍 (source)
|
spectrum |
\alpha |
2.82 ± 0.15 (stat) ± 0.3 (sys) |
|
astro-ph/0503242 🔍 (source)
|
slope of the matter power spectrum at large scales |
n _ { s } |
0.98 ± 0.02 |
|
astro-ph/0503295 🔍 (source)
|
power spectrum slopes |
|
-1.3 |
Lower |
astro-ph/0503295 🔍 (source)
|
power spectrum slopes |
|
-1.5 |
|
astro-ph/0503396 🔍 (source)
|
optical spectrum |
T _ { eff } |
33.0 |
|
astro-ph/0504280 🔍 (source)
|
reflectance spectrum |
|
90377.0 |
|
astro-ph/0504279 🔍 (source)
|
} keV } spectrum |
\Gamma |
2.0 |
Lower |
astro-ph/0504647 🔍 (source)
|
synchrotron spectrum |
\alpha |
-1.0 ± 0.1 |
|
astro-ph/0505370 🔍 (source)
|
steep spectrum |
\alpha |
1.4 ± 0.2 |
|
astro-ph/0505478 🔍 (source)
|
Harrison-Zel´dovich density perturbation spectrum |
n _ { S } |
0.95 |
|
astro-ph/0506109 🔍 (source)
|
AGN spectrum |
\Gamma |
1.7999999999999998 +0.10000000000000009-0.09999999999999987 |
|
astro-ph/0506471 🔍 (source)
|
BH mass spectrum slope |
|
2.5 |
|
astro-ph/0506642 🔍 (source)
|
magnetic field power spectrum spectral index |
n |
-2.9 |
|
astro-ph/0506682 🔍 (source)
|
radio synchrotron spectrum |
|
1.73 ± 0.01 |
|
astro-ph/0507215 🔍 (source)
|
galaxy power spectrum shape |
\Gamma _ { eff } |
0.14 ± 0.02 |
|
astro-ph/0507215 🔍 (source)
|
galaxy power spectrum normalisation |
\sigma _ { 8 } b _ { K } ) ^ { 2 } |
1.36 ± 0.1 |
|
astro-ph/0507489 🔍 (source)
|
flat spectrum |
\alpha _ { 1.7 GHz } ^ { 5 GHz } |
-0.2 ± 0.1 |
|
astro-ph/0507591 🔍 (source)
|
power spectrum |
M _ { rms } |
1.0 |
|
astro-ph/0509478 🔍 (source)
|
spectrum |
n _ { s } |
0.97 |
|
gr-qc/0512100 🔍 (source)
|
spectral index of its spectrum |
n _ { 1 } |
0.9483 |
Lower |
astro-ph/0601242 🔍 (source)
|
cutoff to the spectrum |
|
1300000000.0 |
|
astro-ph/0602246 🔍 (source)
|
core mass spectrum |
\alpha |
2.1 ± 0.4 |
|
astro-ph/0602413 🔍 (source)
|
normalization of the matter power spectrum |
\sigma _ { 8 } |
1.03 +0.2-0.29 |
|
astro-ph/0602511 🔍 (source)
|
radio spectrum |
\alpha _ { thin } |
0.5 |
Upper |
astro-ph/0603146 🔍 (source)
|
power spectrum normalizations |
\sigma _ { 8 } |
0.7 |
|
astro-ph/0604335 🔍 (source)
|
power spectrum |
\sigma _ { 8 } |
0.85 ± 0.02 |
|
astro-ph/0605004 🔍 (source)
|
Harrison–Zel ’ dovich spectrum |
n _ { S } |
1.0 |
|
astro-ph/0605046 🔍 (source)
|
index of the source spectrum |
x |
2.23 ± 0.07 |
|
astro-ph/0605051 🔍 (source)
|
break frequency of the spectrum |
\nu _ { thin } |
37000000000000.0 Hz |
|
astro-ph/0606308 🔍 (source)
|
mass spectrum |
M |
1.8 M_\odot |
Lower |
astro-ph/0606384 🔍 (source)
|
spectrum |
z |
0.263 +0.012-0.01 |
|
astro-ph/0606571 🔍 (source)
|
mass power spectrum normalisation |
\sigma _ { 8 } |
0.8 ± 0.1 |
|
astro-ph/0606611 🔍 (source)
|
mass power spectrum normalisation |
\sigma _ { 8 , CDFS } |
0.52 +0.11-0.15 (stat) ± 0.07 (% sys) |
|
astro-ph/0607353 🔍 (source)
|
energy spectrum |
d \log n / d \log \varepsilon |
-2.0 |
|
astro-ph/0607394 🔍 (source)
|
power spectrum normalization |
\sigma _ { 8 } |
0.74 |
|
astro-ph/0608433 🔍 (source)
|
power spectrum spectral index |
n |
2.0 |
|
astro-ph/0610164 🔍 (source)
|
/IRS mid-infrared spectrum |
L _ { IR } |
400000000000.0 L_\odot |
|
hep-th/0610205 🔍 (source)
|
blue spectrum |
n _ { S } |
0.0 |
Upper |
astro-ph/0611349 🔍 (source)
|
HST spectrum |
|
-2.3 ± 0.1 |
|
astro-ph/0611655 🔍 (source)
|
spectrum synchrotron |
\alpha |
-0.7 |
|
astro-ph/0611655 🔍 (source)
|
flat spectrum free-free ( Bremsstrahlung |
\alpha |
0.1 |
|
astro-ph/0612594 🔍 (source)
|
powerlaw spectrum of photon index |
|
2.03 +0.51-0.36 |
|
astro-ph/0701095 🔍 (source)
|
source spectrum |
|
7e-14 ± 9e-15 erg cm-2 s-1 |
|
astro-ph/0701131 🔍 (source)
|
normalisation of the power spectrum fluctuations |
\sigma _ { 8 } |
0.74 |
|
astro-ph/0701611 🔍 (source)
|
powerlaw spectrum of photon index |
|
2.03 +0.51-0.36 |
|
astro-ph/0701776 🔍 (source)
|
spectrum |
\alpha |
0.8 |
|
astro-ph/0703083 🔍 (source)
|
spectrum |
N ( H _ { I } ) |
4.5e+20 cm-2 |
|
astro-ph/0703234 🔍 (source)
|
strain power spectrum |
|
6.1e-48 s |
|
astro-ph/0703234 🔍 (source)
|
strain power spectrum |
|
8.499999999999999e-49 s |
Lower |
astro-ph/0703802 🔍 (source)
|
power-law spectrum of a photon index |
\Gamma |
1.1 ± 0.2 |
|
0704.3851 🔍 (source)
|
power spectrum |
\boldsymbol { v } |
-1.69 |
|
0705.3611 🔍 (source)
|
spectrum |
\alpha |
0.2 |
|
0706.0517 🔍 (source)
|
suppression of the gamma-ray spectrum |
E _ { \gamma } |
-2.0 |
|
0707.3529 🔍 (source)
|
spectrum |
n _ { H } |
1.9 |
|
0707.3529 🔍 (source)
|
spectrum |
\Gamma _ { ext } |
1.9 |
|
0707.3529 🔍 (source)
|
spectrum |
\Gamma _ { comp } |
1.3 |
|
0708.2030 🔍 (source)
|
\alpha forest power spectrum |
m _ { \nu _ { s } |
1.7 keV |
Lower |
0709.2604 🔍 (source)
|
near-infrared spectrum |
T _ { eff } |
55.0 |
|
0709.4584 🔍 (source)
|
spectrum |
\Gamma _ { int } |
1.5 |
|
0709.4532 🔍 (source)
|
spectrum |
\alpha |
-1.0 |
Upper |
0709.4532 🔍 (source)
|
spectrum |
\alpha _ { 0 } |
-0.45 ± 0.12 |
|
0709.4584 🔍 (source)
|
spectrum |
\Gamma |
2.5 ± 0.19 (stat) ± 0.1 (syst) |
|
0710.5183 🔍 (source)
|
X-ray spectrum |
N _ { H } |
3e+23 cm-2 |
|
0711.2529 🔍 (source)
|
power spectrum of the flux |
|
76.8 Mpc |
Upper |
0712.1909 🔍 (source)
|
energy spectrum |
|
90.0 |
|
0712.3293 🔍 (source)
|
power spectrum normalisation |
\sigma _ { 8 } |
0.92 +0.26-0.3 |
|
0712.3293 🔍 (source)
|
power spectrum normalisation |
\Omega _ { m } |
0.92 +0.26-0.3 |
|
0801.1193 🔍 (source)
|
SFG spectrum |
log ( Z / Z _ { \odot } ) |
-0.699 s |
|
0802.1069 🔍 (source)
|
power spectrum normalization |
\sigma _ { 8 } |
0.85 |
|
0802.2961 🔍 (source)
|
power spectrum shape parameter |
\Gamma |
0.15 +0.18-0.08 |
|
0804.4007 🔍 (source)
|
X-ray spectrum |
\Gamma |
2.1 |
|
0804.4007 🔍 (source)
|
X-ray spectrum |
\Gamma |
0.8 |
|
0805.0691 🔍 (source)
|
velocity power spectrum |
n |
3.8 |
|
0805.3151 🔍 (source)
|
power spectrum of density fluctuations |
|
1.57 |
|
0805.4645 🔍 (source)
|
steeper spectrum |
\beta |
3.0 |
|
0808.0857 🔍 (source)
|
flat spectrum |
\Gamma |
1.0 |
|
0809.1321 🔍 (source)
|
turbulence energy spectrum function |
\beta |
2.0 |
|
0809.2104 🔍 (source)
|
spectral index of the primordial perturbation spectrum |
n _ { s } |
0.935 |
|
0810.2522 🔍 (source)
|
differential spectral index of the intrinsic spectrum |
|
1.28 ± 0.2 |
|
0811.1466 🔍 (source)
|
power spectrum |
|
-3.24 ± 0.03 |
|
0811.1466 🔍 (source)
|
power spectrum |
|
-3.2 |
Lower |
0811.1466 🔍 (source)
|
power spectrum |
|
-2.2 |
Upper |
0811.3759 🔍 (source)
|
steep spectrum |
\alpha |
2.7 |
|
0812.4151 🔍 (source)
|
softness of its X-ray spectrum |
kT |
117.0 ± 14.0 eV |
|
0901.4576 🔍 (source)
|
power spectrum |
n |
-2.5 |
Lower |
0901.4561 🔍 (source)
|
spectrum |
\Gamma |
1.86 ± 0.37 (stat) |
|
0901.4576 🔍 (source)
|
power spectrum |
P ( k ) \propto k ^ { n } |
-2.5 |
Lower |
0902.2927 🔍 (source)
|
spectrum |
\Gamma |
1.8 |
|
0902.4466 🔍 (source)
|
power spectrum |
|
-5.0 |
Upper |
0904.0404 🔍 (source)
|
polarization power spectrum |
\delta T |
3.3 K |
|
0904.0613 🔍 (source)
|
optical spectrum |
T _ { eff } |
7000.0 K |
|
0904.1200 🔍 (source)
|
power spectrum |
|
3.8 ± 0.6 |
|
0904.1200 🔍 (source)
|
power spectrum |
P ( k _ { \theta } |
3.9 ± 0.6 |
|
0905.0499 🔍 (source)
|
linear source power spectrum |
\Delta ^ { 2 } |
0.35 +0.15000000000000002-0.14999999999999997 |
|
0905.3176 🔍 (source)
|
power spectrum of PSF size |
\delta _ { R ^ { 2 } } |
2e-12 |
Lower |
0906.0234 🔍 (source)
|
harder X-ray spectrum |
\Gamma |
1.5 ± 0.01 |
|
0907.0486 🔍 (source)
|
primordial power spectrum |
|
0.742 |
|
0907.0486 🔍 (source)
|
primordial power spectrum |
\sigma _ { 8 } |
0.798 |
|
0907.0832 🔍 (source)
|
energy spectrum |
|
17.7 |
|
0907.1659 🔍 (source)
|
power spectrum |
\chi ^ { 2 } |
39.6 |
|
0907.1659 🔍 (source)
|
power spectrum |
\Omega _ { m } |
0.289 ± 0.019 |
|
0907.2907 🔍 (source)
|
energy spectrum exponent |
\alpha |
-2.0 |
|
0907.4453 🔍 (source)
|
normalization of the linear power spectrum |
\sigma _ { 8 } |
0.9 ± 0.04 |
|
0909.1837 🔍 (source)
|
spectrum |
|
0.42 ± 0.86 |
|
0909.5198 🔍 (source)
|
steep spectrum |
\alpha |
2.6 |
Upper |
0909.5383 🔍 (source)
|
soft X-ray spectrum |
\hat { a } |
0.56 ± 0.02 |
|
0909.5562 🔍 (source)
|
spectrum |
{ \bf E ^ { 2 } F _ { \nu } ( E ) |
2.9e-07 GeV cm-2 s-1 sr-1 |
Upper |
0910.1384 🔍 (source)
|
power spectrum of integrated intensity |
\ell |
0.16 pc |
Lower |
0911.0961 🔍 (source)
|
power spectrum |
n _ { t } |
0.0 |
|
0911.2709 🔍 (source)
|
X-ray spectrum |
\Delta \Gamma _ { X } |
0.7 |
|
1001.1655 🔍 (source)
|
power spectrum |
\Delta \nu |
3.47 ± 0.12 Hz |
|
1001.4538 🔍 (source)
|
power-law index of the primordial power spectrum |
n _ { s } |
0.968 ± 0.012 |
|
1001.4744 🔍 (source)
|
power-law index of the primordial power spectrum |
n _ { s } |
0.963 ± 0.012 |
|
1002.1815 🔍 (source)
|
radio spectrum of index |
\alpha |
-0.26 ± 0.04 |
|
1003.2911 🔍 (source)
|
spectrum of tensor-to-scalar ratio |
r |
0.001 |
|
1004.3771 🔍 (source)
|
normalization of the linear power spectrum |
\sigma _ { 8 } |
0.91 +0.07-0.08 |
|
1005.4410 🔍 (source)
|
bispectrum non-gaussianity parameter |
f _ { NL } |
10.0 |
Lower |
1005.4554 🔍 (source)
|
spectrum |
N _ { H } |
3e+22 |
|
1006.5463 🔍 (source)
|
spectrum |
\Gamma |
2.67 ± 0.1 (stat) ± 0.08 (sys) |
|
1007.3736 🔍 (source)
|
spectrum |
\beta |
0.08 |
|
1008.1068 🔍 (source)
|
power-law spectrum |
\Gamma |
1.26 |
|
1008.1218 🔍 (source)
|
power spectrum slope |
\beta |
2.8 |
|
1008.2724 🔍 (source)
|
scale invariant spectrum |
| 8 n _ { T } | / r |
1.0 |
Upper |
1008.3491 🔍 (source)
|
normalisation of the intrinsic alignment power spectrum |
|
0.077 ± 0.008 |
|
1009.6102 🔍 (source)
|
X-ray spectrum temperature |
T _ { X |
45.0 |
|
1010.1267 🔍 (source)
|
hard spectrum |
\Gamma _ { eff } |
-0.34 +0.57-0.61 |
|
1010.2636 🔍 (source)
|
power spectrum of tensor-to-scalar ratio |
r |
1.0 |
|
1010.5379 🔍 (source)
|
\nu F _ { \nu } spectrum |
E _ { p } |
240.0 keV |
|
1011.0387 🔍 (source)
|
temporal spectrum |
|
6343.0 Hz |
|
1012.2978 🔍 (source)
|
power spectrum of density fluctuations |
P _ { \delta } |
0.002 |
Lower |
1101.3581 🔍 (source)
|
late-time spectrum |
|
2.0 yr |
|
1101.5637 🔍 (source)
|
blackbody spectrum |
kT |
130.0 eV |
|
1103.5166 🔍 (source)
|
point source spectrum |
\Gamma |
1.44 ± 0.07 |
|
1104.0205 🔍 (source)
|
flatter spectrum |
\alpha |
-0.4 |
|
1105.2303 🔍 (source)
|
frequency part of the spectrum |
f |
5.05 ± 4.95 Hz |
Lower |
1105.5711 🔍 (source)
|
spectrum source |
\alpha |
-0.6 |
|
1106.0861 🔍 (source)
|
spectrum integrated flux |
|
2770000.0 ± 260000.0 (stat) ± 320000.0 (syst) cm-2 s-1 |
|
1106.3484 🔍 (source)
|
neutrino spectrum |
|
2.5e-10 cm-2 s-1 TeV-1 |
|
1108.2730 🔍 (source)
|
perturbation spectrum |
n _ { s } |
1.0 |
|
1109.1026 🔍 (source)
|
energy spectrum |
\varepsilon _ { k } |
0.0 |
|
1109.2778 🔍 (source)
|
steep blue anisotropic spectrum |
n _ { de } |
3.1 ± 1.5 |
|
1109.3261 🔍 (source)
|
spectrum |
\alpha |
210.0 |
|
1109.3261 🔍 (source)
|
spectrum |
|
1.8 |
|
1109.4038 🔍 (source)
|
spectrum |
|
-0.1 |
|
1109.4395 🔍 (source)
|
power-law spectrum |
\Gamma |
1.66 ± 0.08 |
|
1109.5706 🔍 (source)
|
blackbody spectrum |
\beta |
2.0 |
|
1111.6186 🔍 (source)
|
Fourier power spectrum |
P ( k ) |
-2.17 |
|
1112.5723 🔍 (source)
|
linear angular power spectrum |
\Omega _ { m } |
0.31 +0.18-0.11 |
|
1201.2044 🔍 (source)
|
steep spectrum |
\Gamma _ { X } |
2.25 ± 0.04999999999999982 |
|
1202.4921 🔍 (source)
|
spectrum |
T _ { eff } |
30000.0 ± 5000.0 K |
|
1203.3424 🔍 (source)
|
radio spectrum |
\alpha |
1.5 |
|
1203.6654 🔍 (source)
|
CMB trispectrum both |
\tau _ { nl } |
0.0 |
|
1204.4239 🔍 (source)
|
power-law spectrum in momentum |
p ^ |
-2.45 ± 0.4 |
|
1208.5866 🔍 (source)
|
Scoreproducessomeofthestructuresthatwereobservedinthecircumstellarabsorptionlinesinthespectrumof |
|
2e-06 ± 5e-07 M_\odot Th yr-1 |
|
1209.4068 🔍 (source)
|
spectrum |
\sigma |
0.08 ± 0.02 keV |
|
1209.5423 🔍 (source)
|
spectrum |
N _ { H , int } ( z = 1.3 ) |
2e+22 cm-2 |
|
1209.6602 🔍 (source)
|
spectrum |
\alpha |
-0.23 ± 0.2 |
|
1210.3298 🔍 (source)
|
power spectrum index |
n |
-3.0 |
|
1211.2510 🔍 (source)
|
spectrum slope parameter |
\alpha _ { ox } |
0.3838 F |
|
1212.3327 🔍 (source)
|
normalisation of the matter power spectrum |
\sigma _ { 8 } |
0.771 ± 0.041 |
|
1301.0824 🔍 (source)
|
thermal SZ power spectrum |
|
3.4 ± 1.4 K2 |
|
1302.5452 🔍 (source)
|
spectrum |
|
0.13 |
Upper |
1303.1808 🔍 (source)
|
normalisation of the matter power spectrum |
\sigma _ { 8 } |
0.799 ± 0.015 |
|
1303.3039 🔍 (source)
|
thermal infrared spectrum |
|
755.0 ± 745.0 |
|
1303.3535 🔍 (source)
|
normalization of the matter power spectrum |
\sigma _ { 8 } |
0.786 ± 0.031 |
|
1303.5081 🔍 (source)
|
power spectrum |
{ \sigma _ { 8 } ( \Omega _ { m } / 0.28 ) } ^ { 3.2 / 8.1 } |
0.784 ± 0.016 (68 % \% C) |
|
1304.1216 🔍 (source)
|
amplitude of the local-shape bispectrum |
f _ { NL } ^ { local * } |
-14.0 +22.0-21.0 |
|
1305.0572 🔍 (source)
|
photon index of the LAT spectrum |
\Gamma |
2.6 ± 0.06 |
|
1306.2172 🔍 (source)
|
spectrum |
\nu |
4.0 |
|
1306.4024 🔍 (source)
|
optical spectrum |
|
30.0 ± 210.0 K W |
|
1306.4024 🔍 (source)
|
optical spectrum |
|
12.0 |
|
1306.5475 🔍 (source)
|
transmission spectrum |
|
-0.079 ± 0.012 |
|
1306.5475 🔍 (source)
|
transmission spectrum |
|
-0.138 ± 0.013 |
|
1306.5475 🔍 (source)
|
transmission spectrum |
|
-0.059 ± 0.012 |
|
1306.5475 🔍 (source)
|
transmission spectrum |
|
-0.123 ± 0.012 |
|
1306.5475 🔍 (source)
|
transmission spectrum |
|
-0.071 ± 0.016 |
|
1306.6624 🔍 (source)
|
radio spectrum |
\alpha |
-0.24 ± 0.42 |
|
1308.5341 🔍 (source)
|
local-form bispectrum parameter |
|
5.0 |
|
1308.5968 🔍 (source)
|
power spectrum slope |
\beta |
2.3 +0.8-0.6 |
|
1309.3282 🔍 (source)
|
cross-power spectrum |
{ \sigma _ { 8 } ( \Omega _ { M } / 0.30 ) } ^ { 0.26 } |
0.8 ± 0.02 |
|
1309.5261 🔍 (source)
|
slope of the transmission spectrum constraining the quantity |
\alpha T |
-3528.0 ± 660.0 K |
|
1310.6499 🔍 (source)
|
power spectrum |
H _ { \alpha } V / R |
0.011873 day-1 |
|
1310.8287 🔍 (source)
|
spectrum |
|
1.72 +1.35-0.89 GeV |
|
1310.8617 🔍 (source)
|
‘ local ’ trispectrum shape |
g _ { NL } / 10 ^ { 5 } |
-4.1 ± 2.3 |
|
1401.8025 🔍 (source)
|
radio spectrum |
\alpha |
-0.52 ± 0.07 |
|
1403.1667 🔍 (source)
|
spectrum of high-redshift |
|
-770.0 GHz |
|
1403.5231 🔍 (source)
|
temperature power spectrum |
r _ { 0.002 } |
0.11 |
Upper |
1403.5372 🔍 (source)
|
proton spectrum |
|
2.68 ± 0.04 |
|
1403.7623 🔍 (source)
|
spectrum amplitude ratio of bounce-to-inflation |
r _ { B } |
0.71 ± 0.09 |
|
1404.0017 🔍 (source)
|
spectrum |
|
1.0 |
|
1404.3813 🔍 (source)
|
total matter power spectrum |
|
0.05 |
|
1404.3813 🔍 (source)
|
total matter power spectrum |
|
0.03 |
|
1405.1188 🔍 (source)
|
tensor spectrum |
n _ { T } |
1.0 |
Lower |
1405.2594 🔍 (source)
|
spectrum |
A _ { flux } |
1.03 ± 0.02 |
|
1405.3056 🔍 (source)
|
red-tilt spectrum |
n _ { s } |
0.96 |
|
1405.7396 🔍 (source)
|
hard spectrum |
E _ { peak } |
1.0 |
|
1405.7974 🔍 (source)
|
power spectrum |
c _ { T } ^ { 2 } |
2.33 |
Upper |
1405.7969 🔍 (source)
|
amplitude of oscillations in the power-spectrum |
\rho _ { h } / \rho _ { I } |
0.01 |
Upper |
1406.4157 🔍 (source)
|
power spectrum amplitude |
k |
0.1 |
|
1407.1836 🔍 (source)
|
bispectrum of dark matter |
k _ { i } |
0.1 h |
Upper |
1407.1897 🔍 (source)
|
spectrum |
L / L _ { Edd } |
0.008 |
|
1407.5081 🔍 (source)
|
peculiar hard spectrum |
\Gamma |
0.8 |
|
1408.2397 🔍 (source)
|
soft spectrum |
|
0.7 +0.10000000000000009-0.09999999999999998 keV |
|
1408.2397 🔍 (source)
|
soft spectrum |
kT |
2000.0 yr |
|
1408.3736 🔍 (source)
|
CMB temperature power spectrum |
\Omega _ { CDM } |
0.22 |
|
1408.5281 🔍 (source)
|
flux spectrum |
\Gamma |
1.68 +0.03-0.02 |
|
1408.5281 🔍 (source)
|
flux spectrum |
\Gamma |
1.78 +0.02-0.03 |
|
1409.2004 🔍 (source)
|
electromagnetic spectrum of PWNe in free expansion |
t _ { age } |
10.0 kyr |
Upper |
1409.5437 🔍 (source)
|
ultra-steep spectrum |
\alpha |
-1.1 |
Upper |
1410.1500 🔍 (source)
|
power-law X-ray spectrum |
\Gamma |
2.0 |
|
1411.3193 🔍 (source)
|
shear power spectrum |
\sqrt { A } |
9e-06 |
|
1412.4760 🔍 (source)
|
ratio of the spectrum |
A _ { MV } |
0.92 ± 0.14 (Stat) ± 0.08 (Sys) |
|
1501.04144 🔍 (source)
|
IRS spectrum |
|
3.0 AU |
|
1502.04501 🔍 (source)
|
GTC/CanariCam nuclear spectrum |
|
50.0 pc |
|
1506.07526 🔍 (source)
|
power spectrum |
dz| |
1.0 |
Upper |
1507.00859 🔍 (source)
|
spectrum |
\alpha |
0.0 ± 0.07 |
|
1507.02308 🔍 (source)
|
tilted spectrum of scalar perturbations |
n _ { s } |
0.96 |
|
1507.08977 🔍 (source)
|
energy spectrum |
|
2.6 ± 0.8 MeV |
|
1509.00315 🔍 (source)
|
radial velocity of the spectrum |
|
417.0 ± 4.0 km s-1 |
|
1510.02288 🔍 (source)
|
ii optical spectrum |
T _ { eff } |
24.0 |
|
1510.02681 🔍 (source)
|
power-law spectrum |
\Gamma |
1.7 +0.57-0.45 |
|
1510.05649 🔍 (source)
|
oscillation spectrum |
\omega _ { R } / \mu |
1.0 |
|
1510.08716 🔍 (source)
|
power spectrum |
c _ { T } |
1.0 |
|
1511.03283 🔍 (source)
|
steep spectrum |
\alpha |
-1.8 |
Lower |
1512.01242 🔍 (source)
|
\gamma -ray spectrum |
\Gamma |
2.78 ± 0.14 |
|
1512.04825 🔍 (source)
|
power spectrum of the source |
|
0.006500000000000001 +0.0005-0.0011 Hz |
|
1601.00660 🔍 (source)
|
radio spectrum |
\alpha |
-0.7 |
|
1601.02542 🔍 (source)
|
X-ray spectrum |
\Gamma |
0.0 |
|
1603.01226 🔍 (source)
|
flat spectrum |
\alpha |
-0.03 ± 0.03 |
|
1604.07871 🔍 (source)
|
clustering amplitude of the matter power spectrum |
\sigma _ { 8 } |
0.74 ± 0.13 |
|
1605.00016 🔍 (source)
|
power spectrum |
|
21.0 cm |
|
1605.00270 🔍 (source)
|
parallax of this flat-spectrum variable radio |
|
2.2 +0.5-0.3 kpc day |
|
1605.02403 🔍 (source)
|
suppression of the matter power spectrum |
\Delta P / P |
8.0 |
|
1605.04646 🔍 (source)
|
power spectrum of the curvature perturbations |
|
0.018 |
Upper |
1605.04788 🔍 (source)
|
spectrum |
k _ { max } |
0.5 h |
Lower |
1605.08360 🔍 (source)
|
power spectrum |
\gamma |
-2.9 ± 0.1 |
|
1606.01968 🔍 (source)
|
amplitude of the spectrum |
A _ { L } ^ { \phi \phi } |
1.15 ± 0.36 |
|
1607.06858 🔍 (source)
|
CMB power spectrum |
|
6.2 |
|
1607.06858 🔍 (source)
|
CMB power spectrum |
|
-6.0 |
Lower |
1608.01684 🔍 (source)
|
spectrum |
E |
3.54 ± 0.02 keV |
|
1608.02583 🔍 (source)
|
power-law spectrum |
\Gamma |
1.7 |
|
1608.06281 🔍 (source)
|
cosmological power spectrum |
\Delta ^ { 2 } |
27000.0 mK2 |
Upper |
1608.07012 🔍 (source)
|
slope of the velocity power spectrum |
|
22.0 |
|
1609.02518 🔍 (source)
|
spectrum |
d |
24.0 pc |
|
1609.05210 🔍 (source)
|
Grating spectrum |
|
4700.0 +2700.0-1500.0 km s-1 |
|
1609.07739 🔍 (source)
|
spectrum |
\log T _ { eff } |
3.7 |
Lower |
1610.02174 🔍 (source)
|
rotational spectrum of the formaldehyde isotopologue |
H _ { 2 } C ^ { 17 } O |
0.56 |
Lower |
1610.03504 🔍 (source)
|
spectrum |
R |
50.0 |
|
1610.03504 🔍 (source)
|
spectrum |
R |
135.0 |
|
1611.00475 🔍 (source)
|
spectrum |
Vr ( DIBs ) |
-12.0 km s-1 |
|
1612.05645 🔍 (source)
|
growth rate times the matter power spectrum normalisation parameter |
|
0.55 ± 0.12 |
|
1612.05645 🔍 (source)
|
growth rate times the matter power spectrum normalisation parameter |
f \sigma _ { 8 } |
0.4 ± 0.11 |
|
1612.06409 🔍 (source)
|
emission spectrum of the |
R |
50.0 |
|
1612.06409 🔍 (source)
|
emission spectrum of the |
R |
70.0 |
|
1702.01761 🔍 (source)
|
spectrum |
k |
-0.06 s km-1 |
|
1702.01764 🔍 (source)
|
power spectrum |
|
5.3 |
Lower |
1702.01764 🔍 (source)
|
power spectrum |
|
1.4 keV |
Lower |
1703.03103 🔍 (source)
|
flux spectrum |
|
23.4 +15.6-5.4 |
|
1703.03410 🔍 (source)
|
steep X-ray spectrum |
\Delta \Gamma |
1.8 ± 0.4 |
|
1703.06802 🔍 (source)
|
spectrum |
\alpha _ { 118 MHz } ^ { 1.78 GHz } |
1.33 ± 0.08 |
|
1703.06802 🔍 (source)
|
spectrum |
\alpha |
1.5 |
|
1703.10538 🔍 (source)
|
matter power spectrum normalization on scales 8 h ^ { -1 } Mpc |
w |
-1.0 |
|
1704.03461 🔍 (source)
|
CIP power spectrum |
A _ { CIP } |
0.017 |
Upper |
1706.08972 🔍 (source)
|
tSZ power spectrum |
\sigma _ { 8 } |
0.85 |
|
1707.05416 🔍 (source)
|
spectrum |
\alpha _ { \nu } |
-1.4 |
|
1708.00697 🔍 (source)
|
power spectrum |
w |
-1.0 ± 0.2 |
|
1708.01315 🔍 (source)
|
optical spectrum |
T _ { eff } |
56.0 |
|
1708.04694 🔍 (source)
|
amplitude of the power spectrum of this white noise |
|
9e-14 |
Upper |
1710.05852 🔍 (source)
|
spectrum |
\Gamma |
2.4 ± 0.8 |
|
1712.00788 🔍 (source)
|
primordial power spectrum |
w |
-1.1 ± 0.12 |
|
1712.07253 🔍 (source)
|
broken power-law spectrum |
E _ { break } |
200.0 keV |
|
1801.07545 🔍 (source)
|
spectral index of the density fluctuation spectrum |
|
-1.7 |
|
1802.00999 🔍 (source)
|
spectrum |
old |
5.0 Gyr |
Lower |
1802.05172 🔍 (source)
|
spectrum |
E |
3000000000000000.0 eV |
|
1803.10213 🔍 (source)
|
power-law spectral index of the X-ray spectrum |
|
2.0 |
Lower |
1804.05056 🔍 (source)
|
particle spectrum hardens |
\alpha _ { e } |
-1.8 |
|
1805.06984 🔍 (source)
|
power spectrum |
P _ { R } |
3.0000000000000004e-09 |
Upper |
1805.09942 🔍 (source)
|
spectrum |
|
6.08 ± 0.18 % |
|
1805.11168 🔍 (source)
|
spectrum |
\Gamma |
2.17 ± 0.06 |
|
1805.11168 🔍 (source)
|
spectrum |
\Gamma |
1.79 ± 0.12 |
|
1805.11607 🔍 (source)
|
amplitude of the kSZ power spectrum |
D _ { 3000 } ^ { kSZ } |
4.1 K2 |
|
1805.11396 🔍 (source)
|
optical spectrum |
[ Fe / H ] |
-0.6 ± 0.07 |
|
1806.01227 🔍 (source)
|
spectral index of the power spectrum of linear density fluctuations |
P ( k ) : N ^ { 2 } |
2.09e-10 ± 3.3e-11 |
|
1806.04194 🔍 (source)
|
power-law index of the spectrum |
s _ { cr } |
2.1500000000000004 +0.04999999999999982-0.050000000000000266 |
|
1806.06795 🔍 (source)
|
mass spectrum |
|
31.96 M_\odot |
Upper |
1806.11114 🔍 (source)
|
spectrum |
|
0.21 ± 0.05 |
|
1807.05441 🔍 (source)
|
radio spectrum of slope |
\alpha |
2.5 |
Lower |
1808.05235 🔍 (source)
|
power spectrum density |
|
1.82 ± 0.14 |
|
1808.07486 🔍 (source)
|
polarization power spectrum |
|
95.0 |
Lower |
1809.06661 🔍 (source)
|
power spectrum of redshifted 21-cm brightness temperature fluctuations |
|
22.5 ± 2.6999999999999993 |
|
1809.06661 🔍 (source)
|
21-cm power spectrum |
\Delta _ { 21 } ^ { 2 } |
14561.0 mK |
Upper |
1810.02374 🔍 (source)
|
power spectrum |
\sum m _ { \nu } |
13.0 |
|
1811.08430 🔍 (source)
|
spectrum |
\alpha |
-2.0 |
Upper |
1811.10609 🔍 (source)
|
spectrum |
k |
0.36 |
|
1812.07350 🔍 (source)
|
spectrum ( photon index |
|
1.7 ± 0.2 |
|
1904.02116 🔍 (source)
|
amplitude of the cross-spectrum |
\widehat { A } _ { lens } |
1.7 ± 0.48 |
|
1906.07792 🔍 (source)
|
diffuse steep spectrum emission |
\alpha |
-1.1 |
Upper |
1907.01997 🔍 (source)
|
\gamma -ray spectrum hardens |
\Gamma _ { \gamma } |
1.82 ± 0.04 |
|
1908.01774 🔍 (source)
|
halo bispectrum up to scales |
k _ { max } |
0.08 h Mpc-1 |
Upper |
1908.10006 🔍 (source)
|
time-averaged X-ray spectrum |
|
84.3 ± 83.7 |
Upper |
1910.02395 🔍 (source)
|
scale invariant power spectrum |
D _ { \ell \in [ 2 , 350 ] } ^ { \alpha \alpha } |
4.7100000000000006e-05 rad2 |
Upper |
1911.00531 🔍 (source)
|
ultra-steep spectrum |
\alpha _ { 144 MHz } ^ { 1.4 GHz } |
-1.84 |
Upper |
1912.00995 🔍 (source)
|
tilt of tensor power spectrum |
n _ { t } |
-0.01 ± 0.31 |
|
1912.01675 🔍 (source)
|
antiproton spectrum |
T |
0.07 |
Lower |
1912.02264 🔍 (source)
|
hard power-law spectrum |
\Gamma |
1.6 ± 0.3 |
|
2001.07138 🔍 (source)
|
ATCA spectrum |
\alpha |
-1.18 +1.04-0.88 |
|
2001.11063 🔍 (source)
|
strength of the stellar ionizing spectrum |
Z _ { \star } |
20.0 ± 5.0 |
|
2002.02575 🔍 (source)
|
spectrum |
k |
3.0 h Mpc-1 |
|
2002.11857 🔍 (source)
|
spectrum residual |
|
0.204 ± 0.011 |
|
2002.11857 🔍 (source)
|
spectrum residual |
A _ { spec } |
0.615 ± 0.068 |
|
2003.07387 🔍 (source)
|
power spectrum to permille-level precision |
\sum m _ { \nu } |
0.3 eV |
Upper |
2003.11730 🔍 (source)
|
thermal spectrum |
|
85.0 % |
|
2005.00892 🔍 (source)
|
mass spectrum parameters |
M _ { 0 } |
17.0 M_\odot |
|
2005.05401 🔍 (source)
|
magnetic energy spectrum slopes |
|
-2.9 |
Lower |
2005.05401 🔍 (source)
|
magnetic energy spectrum slopes |
n _ { B } |
-2.1 |
|
2005.05401 🔍 (source)
|
steep initial power spectrum slope |
n _ { B } |
-2.1 |
|
2006.00615 🔍 (source)
|
red-side spectrum |
\lambda _ { \text { rest } |
1290.0 |
Lower |
2006.04844 🔍 (source)
|
spectrum |
\alpha |
-1.1 |
|
2006.05222 🔍 (source)
|
synchrotron spectrum |
\alpha _ { \nu } |
0.87 +0.08-0.1 |
|
2006.08061 🔍 (source)
|
amplitude of the scale-invariant cosmic rotation power spectrum |
|
1e-05 rad2 |
Upper |
2007.08999 🔍 (source)
|
power spectrum |
z _ { eff } |
1.48 |
|
2007.09008 🔍 (source)
|
normalisation of the linear power spectrum |
D _ { H } ( z _ { eff } ) / r _ { drag } |
20.0 +2.4-2.2 |
|