|
astro-ph/9708051 🔍 (source)
|
opacity |
|
2.3 ± 0.3 |
|
|
astro-ph/9710100 🔍 (source)
|
diffuse neutral hydrogen opacity |
\tau _ { GP } |
0.3 |
|
|
astro-ph/9803346 🔍 (source)
|
frequency dependence of the dust opacity |
\beta |
0.53 +0.27-0.17 |
|
|
astro-ph/9812429 🔍 (source)
|
\ion He2 Ly \alpha opacity |
\tau |
1.88 |
|
|
astro-ph/9812429 🔍 (source)
|
average \ion He2 opacity |
\tau |
4.47 +0.48-0.33 |
|
|
astro-ph/0005315 🔍 (source)
|
X-ray opacity |
\kappa _ { X } |
40.0 cm2 g-1 |
|
|
astro-ph/0103458 🔍 (source)
|
grain opacity power law exponents |
q |
0.7 |
|
|
astro-ph/0104150 🔍 (source)
|
opacity molecular cloud |
|
3.0 |
|
|
astro-ph/0205554 🔍 (source)
|
mass opacity coefficient |
\kappa _ { o } |
0.02 cm2 g-1 |
|
|
astro-ph/0303420 🔍 (source)
|
index of the dust opacity coefficient |
|
0.5 |
Lower |
|
astro-ph/0303420 🔍 (source)
|
index of the dust opacity coefficient |
\beta |
0.7 |
|
|
astro-ph/0306350 🔍 (source)
|
free-free opacity |
v |
0.3 |
Lower |
|
astro-ph/0309631 🔍 (source)
|
opacity |
|
14.0 cm-3 |
Upper |
|
astro-ph/0312557 🔍 (source)
|
He ii opacity |
\tau |
5.0 ± 1.0 |
|
|
astro-ph/0402505 🔍 (source)
|
dust opacity index |
\beta |
1.2 |
|
|
astro-ph/0407384 🔍 (source)
|
dust opacity index |
\beta |
2.0 |
|
|
astro-ph/0407433 🔍 (source)
|
dust mass opacity |
\kappa _ { 1.3 mm } |
0.04 cm2 g-1 |
|
|
astro-ph/0411663 🔍 (source)
|
dust opacity |
A _ { I } |
2.25 ± 1.75 mag |
|
|
astro-ph/0505080 🔍 (source)
|
H i opacity |
\Delta \tau _ { max } |
0.5 ± 0.05 |
|
|
astro-ph/0506225 🔍 (source)
|
mass opacity |
|
0.03 cm2 g-1 |
|
|
astro-ph/0509555 🔍 (source)
|
dust opacity indices |
|
0.5 |
Lower |
|
astro-ph/0509555 🔍 (source)
|
dust opacity indices |
\beta |
1.6 |
Upper |
|
astro-ph/0511480 🔍 (source)
|
\gamma -ray opacity |
\kappa _ { \gamma } |
0.026000000000000002 +0.0009999999999999974-0.0010000000000000009 cm2 g-1 |
|
|
astro-ph/0605129 🔍 (source)
|
opacity |
|
1.35 +0.6499999999999999-0.6500000000000001 keV |
|
|
astro-ph/0606107 🔍 (source)
|
free-free opacity |
\tau _ { 0 } |
1.0 |
|
|
astro-ph/0609122 🔍 (source)
|
steeper opacity indices |
\beta |
1.5 |
Lower |
|
astro-ph/0611366 🔍 (source)
|
opacity spectral index |
\beta |
1.5 ± 0.3 |
|
|
0704.0463 🔍 (source)
|
mass opacity |
|
1.7 cm2 g-1 |
|
|
0704.0616 🔍 (source)
|
dust opacity |
\beta |
1.0 |
|
|
0704.2140 🔍 (source)
|
mean opacity of spiral discs |
\tau _ { B } ^ { f } |
3.8 ± 0.7 |
|
|
0708.2064 🔍 (source)
|
submm dust opacity index |
\beta |
0.3 |
Upper |
|
0708.2064 🔍 (source)
|
submm dust opacity index |
|
0.1 |
Lower |
|
0709.2310 🔍 (source)
|
central face-on B-band opacity |
\tau _ { B } ^ { f } |
4.0 |
|
|
0805.1733 🔍 (source)
|
opacity |
M _ { c } |
30.0 |
|
|
0902.4240 🔍 (source)
|
opacity of the Universe |
\langle A _ { V } \rangle |
0.03 mag |
|
|
0902.4703 🔍 (source)
|
intergalactic opacity to optical/infrared photons |
|
2.0 m |
|
|
0904.1207 🔍 (source)
|
dust opacity per gas mass |
\kappa r |
0.16 cm2 g-1 |
|
|
0906.1367 🔍 (source)
|
opacity |
\tau _ { 0 } |
0.05 |
|
|
0906.1367 🔍 (source)
|
opacity |
|
0.005 |
Lower |
|
0910.1257 🔍 (source)
|
extra optical absorber of opacity |
\kappa _ { e } |
0.05 cm2 g-1 |
|
|
0912.1193 🔍 (source)
|
maximum opacity |
( A _ { \mathrm { V } } |
20.0 mag |
|
|
1002.2462 🔍 (source)
|
exponent of dust mass opacity |
\beta |
1.0 ± 1.0 |
|
|
1007.4410 🔍 (source)
|
line opacity |
|
0.26 ± 0.05 |
|
|
1007.4410 🔍 (source)
|
line opacity |
|
0.62 ± 0.11 |
|
|
1008.1950 🔍 (source)
|
dust opacity index |
\beta |
1.1 |
|
|
1008.1950 🔍 (source)
|
opacity index |
\beta |
1.75 |
|
|
1009.2697 🔍 (source)
|
dust opacity coefficient |
|
1.3 |
Lower |
|
1009.2697 🔍 (source)
|
dust opacity coefficient |
\beta |
0.6 ± 0.1 |
|
|
1011.3817 🔍 (source)
|
millimeter dust opacity index |
\beta |
0.862 |
|
|
1012.3488 🔍 (source)
|
submillimeter opacity power-law index |
\beta _ { smm } |
2.38 +0.20000000000000018-0.19999999999999973 |
|
|
1012.3488 🔍 (source)
|
dust opacity |
\kappa _ { 850 } |
1.475 +0.29499999999999993-0.29500000000000015 |
|
|
1012.3488 🔍 (source)
|
opacity ratios |
\kappa _ { 850 } / \kappa _ { 2.2 } |
4.005 ± 0.7949999999999999 |
|
|
1101.2032 🔍 (source)
|
dust opacity in the solar neighbourhood |
\tau / N _ { H } |
9.2e-26 ± 5e-27 cm2 |
|
|
1101.3003 🔍 (source)
|
dust opacity |
\kappa ( 250 \mu { m } ) |
0.125 +0.07500000000000001-0.075 cm2 g-1 |
|
|
1106.4825 🔍 (source)
|
opacity |
\tau _ { 100 } |
0.9 ± 0.2 |
|
|
1107.3515 🔍 (source)
|
X-ray opacity of dust appreciably |
E _ { X } |
1.0 keV |
|
|
1108.2297 🔍 (source)
|
extra optical opacity |
\kappa ^ { \prime } |
0.35 +0.050000000000000044-0.04999999999999999 |
|
|
1111.5184 🔍 (source)
|
average opacity index |
\beta |
0.26 ± 0.22 |
|
|
1112.5433 🔍 (source)
|
opacity |
\sigma _ { e } ( |
1200.0 |
|
|
1202.1840 🔍 (source)
|
opacity correction factor |
|
1.34 ± 0.05 |
|
|
1202.1840 🔍 (source)
|
opacity |
\Omega _ { HI } ^ { DLA } ( z = 0 ) |
0.0005400000000000001 ± 9e-05 |
|
|
1204.3093 🔍 (source)
|
total Lyman opacity |
\tau _ { eff } ^ { Lyman } |
0.4 ± 0.15 |
|
|
1210.5094 🔍 (source)
|
dust opacity spectral index |
\beta |
1.8 |
|
|
1211.6475 🔍 (source)
|
opacity ( dust emission cross-section per H nucleon |
\sigma _ { e } |
1200.0 |
|
|
1301.6480 🔍 (source)
|
spectral opacity index |
\beta |
0.6 ± 0.5 |
|
|
1302.1141 🔍 (source)
|
extra opacity |
|
0.012 cm2 g-1 |
|
|
1303.2655 🔍 (source)
|
Rosseland mean opacity |
|
1.0 |
|
|
1305.3604 🔍 (source)
|
dust opacity spectral index |
\beta |
0.0 |
|
|
1305.6896 🔍 (source)
|
opacity index |
\beta |
0.5 ± 0.5 |
|
|
1307.6815 🔍 (source)
|
opacity spectral index |
\beta _ { mm } |
1.54 |
Lower |
|
1309.3148 🔍 (source)
|
continuum opacity |
|
395.0 |
|
|
1309.3148 🔍 (source)
|
continuum opacity |
|
398.0 |
|
|
1309.3148 🔍 (source)
|
continuum opacity |
|
1.45 |
|
|
1309.3148 🔍 (source)
|
continuum opacity |
|
1.9 |
|
|
1309.3148 🔍 (source)
|
continuum opacity |
|
1.55 |
|
|
1309.3148 🔍 (source)
|
continuum opacity |
|
2.2 |
|
|
1309.3148 🔍 (source)
|
continuum opacity |
|
1.7 |
|
|
1401.7398 🔍 (source)
|
dust opacity |
|
353.0 GHz |
|
|
1402.6702 🔍 (source)
|
opacity broadening |
M _ { s } |
1.23 ± 0.07000000000000006 |
|
|
1408.0731 🔍 (source)
|
dust opacity |
\tau |
0.44 |
|
|
1412.5965 🔍 (source)
|
dust opacity spectral index |
\beta |
1.8 |
|
|
1501.05965 🔍 (source)
|
opacity law index |
|
1.7 |
|
|
1501.07092 🔍 (source)
|
submillimetre opacity |
\tau ( 250 \mu { m } ) / \tau ( J ) |
0.004 |
|
|
1501.07092 🔍 (source)
|
opacity spectral index |
\beta |
1.8 |
|
|
1507.08353 🔍 (source)
|
opacity spectral index |
\beta |
1.0 |
Upper |
|
1508.03801 🔍 (source)
|
line opacity |
|
13.0 |
Upper |
|
1508.04423 🔍 (source)
|
opacity broadening factor |
|
2.6 +1.4-1.4000000000000001 |
|
|
1509.08023 🔍 (source)
|
median opacity spectral index |
\beta |
1.84 |
|
|
1509.08652 🔍 (source)
|
opacity |
T _ { eff } |
10.0 |
|
|
1511.09183 🔍 (source)
|
cloud opacity parameter |
|
3.5 ± 1.5 |
|
|
1512.02635 🔍 (source)
|
photoelectric absorption edge opacity |
\tau _ { HeI } |
0.047 |
Upper |
|
1605.00289 🔍 (source)
|
power-law index of the dust opacity |
\beta ( R ) |
1.7 |
|
|
1605.04842 🔍 (source)
|
dust opacity spectral index |
\beta |
1.8 |
|
|
1606.09127 🔍 (source)
|
dust opacity |
|
7.999999999999999e-22 +6.999999999999999e-22-7e-22 cm2 |
|
|
1606.09127 🔍 (source)
|
dust opacity |
\sigma _ { d } |
4.0 K |
Upper |
|
1607.06220 🔍 (source)
|
continuum opacity |
\tau _ { 100 } |
1.0 |
Lower |
|
1611.01279 🔍 (source)
|
opacity |
|
0.05 |
Upper |
|
1701.01256 🔍 (source)
|
opacity |
\log T |
5.46 |
Lower |
|
1701.01256 🔍 (source)
|
opacity |
|
5.3 |
|
|
1705.06047 🔍 (source)
|
gamma-ray opacity |
|
0.01 |
Lower |
|
1705.06047 🔍 (source)
|
gamma-ray opacity |
\kappa _ { \gamma } |
0.82 cm2 g-1 |
|
|
1706.04771 🔍 (source)
|
subtle intergalactic opacity |
|
1e-07 mag h Gpc-1 |
|
|
1710.03232 🔍 (source)
|
far-UV opacity gradient |
d \tau _ { eff } / dz |
15.0 |
Lower |
|
1710.03232 🔍 (source)
|
far-UV opacity gradient |
\log N _ { HI } |
15.0 |
Lower |
|
1711.09425 🔍 (source)
|
opacity spectral index |
\beta |
1.7 ± 0.19999999999999996 |
|
|
1711.09425 🔍 (source)
|
opacity spectral index |
\beta |
1.7 |
|
|
1801.02188 🔍 (source)
|
Rosseland Mean Opacity |
|
2110000.0 K |
|
|
1802.08177 🔍 (source)
|
IGM Lyman- \alpha opacity |
z _ { source } |
5.7 |
Lower |
|
1805.00494 🔍 (source)
|
dust opacity index |
\beta |
1.0 |
|
|
1809.00864 🔍 (source)
|
dust opacity spectral index |
\beta |
1.9 |
|
|
1809.08958 🔍 (source)
|
opacity |
\log T |
6.35 |
|
|
1902.09932 🔍 (source)
|
mm dust opacity |
\kappa _ { mm } |
2.0 cm2 g-1 |
Upper |
|
1902.09932 🔍 (source)
|
mm dust opacity |
\kappa _ { mm } |
2.0 cm2 g-1 |
|
|
1904.03043 🔍 (source)
|
opacity exponent |
\beta |
-2.0 |
|
|
1909.05102 🔍 (source)
|
B-band intergalactic opacity |
\lambda _ { B } |
0.1 ± 0.03 Gpc-1 |
|
|
1912.02327 🔍 (source)
|
cosmic opacity |
\sigma _ { \epsilon } |
0.006 |
|
|
1912.02327 🔍 (source)
|
cosmic opacity |
|
0.011 |
|
|
2001.00055 🔍 (source)
|
opacity |
|
0.55 +0.44999999999999996-0.45000000000000007 Gyr |
|
|
2005.09667 🔍 (source)
|
effective Ly \alpha opacity |
\tau _ { eff } |
2.02 |
|
|
2006.02812 🔍 (source)
|
dust opacity |
\kappa _ { 9 mm } |
0.28 cm2 g-1 |
|
|
2006.02812 🔍 (source)
|
maximum dust opacity |
\kappa _ { 1.3 mm } |
2.3 cm2 g-1 |
|
|
2006.02812 🔍 (source)
|
dust opacity index |
\beta |
0.5 |
|