|
astro-ph/9311070 🔍 (source)
|
nonlinear mass |
|
180.0 |
|
|
astro-ph/9409022 🔍 (source)
|
line-of-sight distance |
R _ { 0 } |
8.0 kpc |
|
|
astro-ph/9603076 🔍 (source)
|
linear distance |
|
22.0 ± 0.8 Mpc |
|
|
astro-ph/9605189 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma _ { * } |
15.7 ± 1.5 |
|
|
astro-ph/9606031 🔍 (source)
|
line-of-sight stellar velocity dispersion |
\sigma _ { * } |
11.4 ± 1.5 |
|
|
astro-ph/9612198 🔍 (source)
|
peak line temperature |
|
0.75 K |
|
|
astro-ph/9702080 🔍 (source)
|
line ratio |
|
0.4 |
Lower |
|
astro-ph/9702198 🔍 (source)
|
line-of-sight expansion velocity |
|
112.5 ± 37.5 km s-1 |
|
|
astro-ph/9704234 🔍 (source)
|
line-of-sight ejection velocities |
|
51.0 |
|
|
astro-ph/9706242 🔍 (source)
|
Sun-Galactic centre line |
|
28.0 ± 7.0 |
|
|
astro-ph/9709131 🔍 (source)
|
lines per unit |
\log N ( \mbox { H { \sc i } } |
12.0 |
Lower |
|
astro-ph/9710114 🔍 (source)
|
iron emission line |
|
6.7 keV |
|
|
astro-ph/9711082 🔍 (source)
|
line intensity |
|
2.8 ± 0.3 Jy km s-1 |
|
|
astro-ph/9711082 🔍 (source)
|
linewidth |
|
420.0 ± 60.0 km s-1 |
|
|
astro-ph/9711164 🔍 (source)
|
broad iron line |
|
6.58 ± 0.04 keV |
|
|
astro-ph/9711176 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma _ { los } |
164.0 km s-1 |
|
|
astro-ph/9801137 🔍 (source)
|
percentage of absorption-line galaxies |
|
84.0 ± 9.0 % |
|
|
astro-ph/9801137 🔍 (source)
|
percentage of absorption-line galaxies |
|
59.0 ± 11.0 % |
Upper |
|
astro-ph/9803137 🔍 (source)
|
rest-frame equivalent width of the emission line |
( W _ { Ly \alpha } ^ { rest } |
95.0 |
|
|
astro-ph/9803214 🔍 (source)
|
mean linear spin-down rate |
\dot { P } |
5.126e-14 |
|
|
astro-ph/9803342 🔍 (source)
|
Ca linear depletion |
\delta ( Ca ) |
0.00014 |
|
|
astro-ph/9803342 🔍 (source)
|
Ca linear depletion |
\delta ( Ca ) |
0.00028 |
|
|
astro-ph/9804194 🔍 (source)
|
Gaussian dispersion of the emission lines |
|
70.0 |
|
|
astro-ph/9804229 🔍 (source)
|
Balmer absorption-line velocities |
|
1.4 M_\odot |
|
|
astro-ph/9804290 🔍 (source)
|
line ratios |
\sigma _ { \xi } |
1.0 |
Lower |
|
astro-ph/9805356 🔍 (source)
|
linear size of the radio structure |
|
2.0 Mpc |
|
|
astro-ph/9806219 🔍 (source)
|
velocity dispersion of the emission line gas |
\sigma |
70.0 km s-1 |
|
|
astro-ph/9807004 🔍 (source)
|
line |
{ ( D / H ) } _ { Capella } |
1.5600000000000003e-05 ± 1.0000000000000002e-06 |
|
|
astro-ph/9807013 🔍 (source)
|
linear polarization |
|
9.0 |
|
|
astro-ph/9808157 🔍 (source)
|
decline rate |
\Delta m _ { 15 } |
1.11 ± 0.06 |
|
|
astro-ph/9809025 🔍 (source)
|
linear distance |
|
660.0 ± 66.0 kpc |
|
|
astro-ph/9809025 🔍 (source)
|
total line-of-sight reddening |
E ( B - V ) |
1.16 ± 0.08 mag |
|
|
astro-ph/9809098 🔍 (source)
|
rms line width |
|
0.86 keV |
|
|
astro-ph/9809103 🔍 (source)
|
velocity width of the scattered line |
{ ( m _ { p } / m _ { e } ) } ^ { 1 / 2 } |
43.0 |
|
|
astro-ph/9810002 🔍 (source)
|
linear diameter |
|
2.5 ± 0.4 pc |
|
|
astro-ph/9810018 🔍 (source)
|
iron emission line |
|
6.4 keV |
|
|
astro-ph/9810365 🔍 (source)
|
linear spin-down rate |
|
5.1271e-14 |
|
|
astro-ph/9812089 🔍 (source)
|
linear regression slope |
|
0.6 |
|
|
astro-ph/9901112 🔍 (source)
|
tachocline |
|
0.05 ± 0.03 R_\odot |
|
|
astro-ph/9901134 🔍 (source)
|
CO line ratios |
J |
0.7 |
|
|
astro-ph/9901280 🔍 (source)
|
line frequency |
N _ { HI } |
200.0 ± 40.0 |
|
|
astro-ph/9901280 🔍 (source)
|
line frequency |
d N / dz |
200.0 ± 40.0 |
|
|
astro-ph/9902231 🔍 (source)
|
line fluxes |
|
1.3e-16 erg cm-2 s-1 |
|
|
astro-ph/9902250 🔍 (source)
|
absorption line indices |
Mg _ { 2 } |
-3.0 |
Upper |
|
astro-ph/9903208 🔍 (source)
|
line intensity peak |
|
3.0 |
|
|
astro-ph/9903457 🔍 (source)
|
line-of-sight stellar velocity dispersion |
\sigma |
33.0 ± 3.0 |
|
|
astro-ph/9904397 🔍 (source)
|
decline rates |
|
0.0141 ± 0.0002 |
|
|
astro-ph/9904397 🔍 (source)
|
decline rates |
|
0.0184 ± 0.0003 |
|
|
astro-ph/9904397 🔍 (source)
|
decline rates |
|
0.0181 ± 0.0003 |
|
|
astro-ph/9906202 🔍 (source)
|
projected linear distance |
|
-0.07 ± 0.07 c |
|
|
astro-ph/9906202 🔍 (source)
|
projected linear distance |
|
0.19 ± 0.27 |
|
|
astro-ph/9906202 🔍 (source)
|
projected linear distance |
|
0.3 ± 0.07 |
|
|
astro-ph/9906346 🔍 (source)
|
linear polarization in the afterglow |
|
1.6 ± 0.2 % |
|
|
astro-ph/9907352 🔍 (source)
|
broad skewed iron line |
W _ { K \alpha } |
266.0 eV |
|
|
astro-ph/9907345 🔍 (source)
|
decline rate |
|
-18.67 ± 0.3 mag |
|
|
astro-ph/9907345 🔍 (source)
|
decline rate |
|
-18.4 ± 0.3 mag |
|
|
astro-ph/9907345 🔍 (source)
|
decline rate |
|
-18.62 ± 0.3 mag |
|
|
astro-ph/9908123 🔍 (source)
|
line-of-sight |
|
69.0 pc |
|
|
astro-ph/9908205 🔍 (source)
|
line flux |
|
0.2 |
|
|
astro-ph/9908205 🔍 (source)
|
line flux |
\phi |
0.2 |
|
|
astro-ph/9908205 🔍 (source)
|
density of the narrow line region |
\log n _ { e } |
13.4 ± 0.2 |
|
|
astro-ph/9908254 🔍 (source)
|
size of the pulsar declines |
|
440.0 ± 90.0 km |
|
|
astro-ph/9910431 🔍 (source)
|
rates of decline |
|
0.015 ± 0.001 mag yr-1 |
|
|
astro-ph/9911142 🔍 (source)
|
line |
T _ { s } |
775.0 ± 100.0 K |
|
|
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/9911299 🔍 (source)
|
Fe K line emission |
|
6.3 ± 0.2 keV |
|
|
astro-ph/9911350 🔍 (source)
|
optical linear diameter |
|
1.4 ± 0.2 kpc |
|
|
astro-ph/9912017 🔍 (source)
|
line flux ratio |
|
6717.0 |
|
|
astro-ph/9912123 🔍 (source)
|
light curve decline rate |
\Delta m _ { 15 } |
0.87 |
Lower |
|
astro-ph/9912123 🔍 (source)
|
light curve decline rate |
\Delta m _ { 15 } ( B ) |
0.87 |
Lower |
|
astro-ph/9912244 🔍 (source)
|
linear phase |
t |
8.0 ± 7.0 day |
|
|
astro-ph/9912389 🔍 (source)
|
disk line |
|
6.8 keV |
|
|
astro-ph/0001030 🔍 (source)
|
line equivalent width |
|
0.6 +0.84-0.36 keV |
|
|
astro-ph/0001107 🔍 (source)
|
line energy |
E _ { K \alpha } |
6.62 ± 0.07 keV |
|
|
astro-ph/0001127 🔍 (source)
|
line-of-sight column density |
|
2.7e+19 cm-2 |
Lower |
|
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/0002366 🔍 (source)
|
neutron capture line |
|
2.223 MeV |
|
|
astro-ph/0002484 🔍 (source)
|
line ratio |
I _ { [ CI ] } / I _ { CO } |
0.2 |
|
|
astro-ph/0003291 🔍 (source)
|
line flux |
log ( L _ { H \alpha } / L _ { bol } ) |
-4.3 |
|
|
astro-ph/0004169 🔍 (source)
|
nova line flux |
|
0.0038 ph |
Upper |
|
astro-ph/0004263 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma |
1390.0 +120.0-110.0 km s-1 |
|
|
astro-ph/0004298 🔍 (source)
|
line ratio |
n _ { e } |
4100.0 cm-3 |
|
|
astro-ph/0004334 🔍 (source)
|
linear redshift distortion parameter |
\beta |
0.41 +0.13-0.12 |
|
|
astro-ph/0005567 🔍 (source)
|
rest frame line energy |
|
6.69 ± 0.11 keV |
|
|
astro-ph/0006055 🔍 (source)
|
line energy |
|
6.73 +0.13-0.12 keV |
|
|
astro-ph/0006153 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma _ { los } |
164.0 km s-1 |
|
|
astro-ph/0006206 🔍 (source)
|
absorption-line redshift |
|
1.02 |
|
|
astro-ph/0006229 🔍 (source)
|
resonance line |
P _ { 2 } / P _ { 0 } |
0.5 |
|
|
astro-ph/0007010 🔍 (source)
|
light curve tail declines |
E _ { K } |
7e+51 erg |
|
|
astro-ph/0007326 🔍 (source)
|
emission line luminosities |
L _ { \gamma } |
0.69 ± 0.11 |
|
|
astro-ph/0008375 🔍 (source)
|
temporal baseline |
|
7.5 ± 2.5 yr |
|
|
astro-ph/0009017 🔍 (source)
|
average linewidth |
|
0.22 ± 0.03 keV |
|
|
astro-ph/0009065 🔍 (source)
|
luminosity decline rate |
\Delta m _ { B } ( 15 ) |
1.31 ± 0.08 |
|
|
astro-ph/0009083 🔍 (source)
|
sight to the broad-line region |
E _ { B - V } |
0.5 |
|
|
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/0010610 🔍 (source)
|
line-of-sight column density |
|
2.7e+19 cm-2 |
Lower |
|
astro-ph/0011030 🔍 (source)
|
radial ( line-of-sight ) thicknesses |
|
0.2 pc |
Upper |
|
astro-ph/0101060 🔍 (source)
|
line-of-sight hydrogen density column |
T |
6.6 ± 0.3 keV |
|
|
astro-ph/0103089 🔍 (source)
|
linear polarization |
\alpha |
0.275 +0.024999999999999967-0.025000000000000022 |
|
|
astro-ph/0103413 🔍 (source)
|
iron line |
EW |
50.0 |
|
|
astro-ph/0104238 🔍 (source)
|
dust temperatures decline |
T _ { d } |
7.0 K |
|
|
astro-ph/0104280 🔍 (source)
|
linear size |
L |
6.0 pc |
|
|
astro-ph/0104317 🔍 (source)
|
emission line widths |
|
44.0 ± 15.0 km s-1 |
|
|
astro-ph/0105219 🔍 (source)
|
line ratio |
T _ { ex } |
720.0 +135.0-100.0 K |
|
|
astro-ph/0105267 🔍 (source)
|
linear polarization levels |
|
2.3 % |
Lower |
|
astro-ph/0105472 🔍 (source)
|
linear correlation coefficient |
|
0.0004 ± 0.001 |
|
|
astro-ph/0105490 🔍 (source)
|
decline rate parameter |
\Delta m _ { 15 } ( B ) |
1.93 |
|
|
astro-ph/0105490 🔍 (source)
|
decline rate parameter |
|
1.9 mag |
|
|
astro-ph/0106279 🔍 (source)
|
line flux |
|
1.3500000000000002e-15 ± 3.5e-16 erg cm-2 s-1 |
|
|
astro-ph/0107189 🔍 (source)
|
Balmer line intensities |
Y _ { p } ( Tree(positive_expression, [LeafSymbol('Hc')]) ) |
0.2384 ± 0.0025 |
|
|
astro-ph/0107196 🔍 (source)
|
linear density |
\delta _ { L , R } |
0.0 |
Lower |
|
astro-ph/0107468 🔍 (source)
|
line flux |
|
1.9e-05 ± 9e-06 ph cm-2 s-1 |
|
|
astro-ph/0108100 🔍 (source)
|
line-of-sight velocity dispersion |
|
10.7 km s-1 |
|
|
astro-ph/0108100 🔍 (source)
|
line-of-sight velocity dispersion |
|
8.5 km s-1 |
|
|
astro-ph/0108192 🔍 (source)
|
linear limb-darkened radii |
|
98.0 R_\odot |
|
|
astro-ph/0108192 🔍 (source)
|
linear limb-darkened radii |
|
114.0 R_\odot |
|
|
astro-ph/0108192 🔍 (source)
|
linear limb-darkened radii |
|
56.0 R_\odot |
|
|
astro-ph/0108345 🔍 (source)
|
line-of-sight velocity |
|
26.0 ± 0.5 km s-1 |
|
|
astro-ph/0109100 🔍 (source)
|
median line-width parameter |
b |
27.0 km s-1 |
|
|
astro-ph/0110158 🔍 (source)
|
linear diameter |
|
0.54 K pc |
|
|
astro-ph/0110265 🔍 (source)
|
rapid decline |
t _ { 3 } |
9.0 day |
|
|
astro-ph/0111268 🔍 (source)
|
hyperfine ratio of the two OH lines |
\tau _ { 1667 } / \tau _ { 1665 } |
2.6 ± 0.8 |
|
|
astro-ph/0111413 🔍 (source)
|
line-of-sight optical depths |
\tau _ { 0.3 \mu } |
35.0 ± 5.0 |
|
|
astro-ph/0112400 🔍 (source)
|
rotational lines |
T |
600.0 K g as |
|
|
astro-ph/0201016 🔍 (source)
|
rate of decline |
\Delta m _ { 15 } ( B ) |
2.21 |
|
|
astro-ph/0201116 🔍 (source)
|
projected linear size |
|
330.0 h |
|
|
astro-ph/0201194 🔍 (source)
|
emission line |
I _ { \tiny AB } |
25.4 |
|
|
astro-ph/0201194 🔍 (source)
|
\alpha line flux |
|
3e-17 erg cm-2 s-1 |
|
|
astro-ph/0201319 🔍 (source)
|
} emission line flux |
|
0.00019 L_\odot |
|
|
astro-ph/0201496 🔍 (source)
|
line intensity |
|
8.199999999999999e-15 erg s-1 cm-2 |
|
|
astro-ph/0202043 🔍 (source)
|
line flux |
|
3.6e-05 ph |
|
|
astro-ph/0202083 🔍 (source)
|
emission line |
E |
6.415 ± 0.007 keV |
|
|
astro-ph/0202093 🔍 (source)
|
intrinsic line width |
\sigma |
32.0 ± 7.0 eV |
|
|
astro-ph/0202227 🔍 (source)
|
line fluxes |
|
5000.0 |
|
|
astro-ph/0202227 🔍 (source)
|
line fluxes |
T |
20000.0 K |
Upper |
|
astro-ph/0202514 🔍 (source)
|
linear size |
|
6.8e+17 cm |
|
|
astro-ph/0203091 🔍 (source)
|
line-free |
|
2.6000000000000002e-30 ± 7e-31 erg cm-2 |
|
|
astro-ph/0204084 🔍 (source)
|
projected linear distance |
|
17.8 h |
|
|
astro-ph/0204241 🔍 (source)
|
linear size |
|
1.5 kpc |
|
|
astro-ph/0204300 🔍 (source)
|
width of the iron fluorescent line |
|
2.0 keV |
|
|
astro-ph/0204417 🔍 (source)
|
projected linear extent |
|
2.0 pc |
|
|
astro-ph/0205161 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma |
20.2 ± 0.5 |
|
|
astro-ph/0205255 🔍 (source)
|
linear |
v \sin i _ { \mathrm { |
1.03 |
|
|
astro-ph/0205347 🔍 (source)
|
line |
{ Fe |
6.8 |
|
|
astro-ph/0206087 🔍 (source)
|
line ratio |
|
0.34 ± 40.0 % |
|
|
astro-ph/0206077 🔍 (source)
|
intrinsic linewidth |
\langle \Deltav _ { int } |
15.0 km s-1 |
|
|
astro-ph/0206276 🔍 (source)
|
total line-of-sight velocity dispersion |
|
1.1 ± 0.2 km s-1 |
|
|
astro-ph/0206276 🔍 (source)
|
dynamical line-of-sight velocity dispersion |
|
0.7 km s-1 |
Upper |
|
astro-ph/0206276 🔍 (source)
|
total line-of-sight velocity dispersion |
|
0.9 ± 0.2 km s-1 |
|
|
astro-ph/0206276 🔍 (source)
|
dynamical line-of-sight velocity dispersion |
|
0.32 |
|
|
astro-ph/0206415 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma _ { v } |
1330.0 km s-1 |
|
|
astro-ph/0207072 🔍 (source)
|
HHT-KittPeak baseline |
|
190.0 km |
|
|
astro-ph/0207303 🔍 (source)
|
broad line width |
\Delta v _ { FWHM } |
340.0 km s-1 |
|
|
astro-ph/0207562 🔍 (source)
|
line widths |
b |
48.5 ± 32.5 km s-1 |
|
|
astro-ph/0208531 🔍 (source)
|
linewidth |
\Delta v |
0.8 km s-1 |
|
|
astro-ph/0209087 🔍 (source)
|
oxygen line emission |
N / O |
9.0 |
Lower |
|
astro-ph/0209507 🔍 (source)
|
flux decline rates before flattening |
|
0.127 ± 0.005 |
|
|
astro-ph/0209507 🔍 (source)
|
flux decline rates before flattening |
|
0.082 ± 0.001 |
|
|
astro-ph/0209507 🔍 (source)
|
flux decline rates before flattening |
|
0.074 ± 0.001 |
|
|
astro-ph/0209507 🔍 (source)
|
flux decline rates before flattening |
|
0.062 ± 0.001 |
|
|
astro-ph/0209507 🔍 (source)
|
flux decline rates before flattening |
|
0.04 ± 0.001 mag day-1 |
|
|
astro-ph/0209536 🔍 (source)
|
line–of–sight velocity dispersion |
\mathrm { \sigma _ { v } |
1325.0 ± 75.0 km |
|
|
astro-ph/0210071 🔍 (source)
|
line width |
|
0.24 ± 0.07 km s-1 |
|
|
astro-ph/0210397 🔍 (source)
|
line-profile |
|
-43.3 ± 0.7 |
|
|
astro-ph/0210654 🔍 (source)
|
emission line flux |
|
2.46e-16 ± 5e-17 erg s-1 cm-2 |
|
|
astro-ph/0211180 🔍 (source)
|
nonthermal line width |
|
0.78 km s-1 |
|
|
astro-ph/0211465 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma _ { e } |
400.0 km s-1 |
Upper |
|
astro-ph/0211476 🔍 (source)
|
luminosity decline |
|
0.625 M_\odot c |
|
|
astro-ph/0212407 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma _ { \| } |
530.0 +190.0-90.0 km s-1 |
|
|
astro-ph/0212506 🔍 (source)
|
column density sightline |
D I / O I |
0.032400000000000005 +0.0327-0.0206 |
|
|
astro-ph/0212543 🔍 (source)
|
B -band decline rate |
\Delta m _ { 15 } ( B ) |
0.93 |
|
|
astro-ph/0301297 🔍 (source)
|
Fe-K line |
EW |
382.0 eV |
Upper |
|
astro-ph/0301333 🔍 (source)
|
angle to the line-of-sight |
v |
0.997 |
|
|
astro-ph/0301322 🔍 (source)
|
baseline |
I |
15.1 |
|
|
astro-ph/0301333 🔍 (source)
|
angle to the line-of-sight |
v |
0.992 |
|
|
astro-ph/0301511 🔍 (source)
|
line |
|
0.22 |
Lower |
|
astro-ph/0301635 🔍 (source)
|
linear size |
|
7.7 h |
|
|
astro-ph/0302080 🔍 (source)
|
linear size |
|
620.0 kpc |
|
|
astro-ph/0302116 🔍 (source)
|
line flux |
|
2.9999999999999997e-20 W m-2 |
|
|
astro-ph/0302319 🔍 (source)
|
NIII line |
|
991.0 |
|
|
astro-ph/0302415 🔍 (source)
|
linear polarization |
|
2.0 |
|
|
astro-ph/0303051 🔍 (source)
|
line width |
\sigma |
3.4 ± 0.5 eV |
|
|
astro-ph/0303134 🔍 (source)
|
line widths |
|
80.0 ± 5.0 km s-1 |
|
|
astro-ph/0303554 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma |
530.0 +190.0-90.0 km s-1 |
|
|
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/0305129 🔍 (source)
|
broad line region size |
|
3.0 ± 1.5 |
|
|
astro-ph/0305571 🔍 (source)
|
line-of-sight column density |
N _ { H } |
4.0000000000000003e+23 cm-2 |
|
|
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/0306421 🔍 (source)
|
total baseline |
|
2.5 |
|
|
astro-ph/0306585 🔍 (source)
|
linear bias |
b |
3.5 ± 0.3 |
|
|
astro-ph/0306601 🔍 (source)
|
snow line |
|
1.0 AU |
|
|
astro-ph/0306604 🔍 (source)
|
linear diameter |
|
1.711 ± 0.013 |
|
|
astro-ph/0306621 🔍 (source)
|
median line flux ratio |
F _ { [ OII ] } / F _ { H \alpha } |
0.23 |
|
|
astro-ph/0308432 🔍 (source)
|
line-of-sight size |
L |
0.25 pc |
|
|
astro-ph/0309160 🔍 (source)
|
ion-to-neutral linewidth ratio |
|
0.82 ± 0.04 |
|
|
astro-ph/0309148 🔍 (source)
|
linear diameter |
|
2.048 ± 0.025 |
|
|
astro-ph/0309214 🔍 (source)
|
line ratios |
r _ { 31 } |
1.72 |
|
|
astro-ph/0309214 🔍 (source)
|
line ratios |
r _ { 31 } |
0.22 |
Lower |
|
astro-ph/0309214 🔍 (source)
|
line ratios |
r _ { 31 } |
0.66 |
|
|
astro-ph/0309484 🔍 (source)
|
intrinsic line width |
|
2.95 +0.45-0.51 keV |
|
|
astro-ph/0310037 🔍 (source)
|
mean decline rate |
|
1.1 mag day-1 |
|
|
astro-ph/0310128 🔍 (source)
|
Rosseland linear radius R |
|
86.0 ± 3.0 R_\odot |
|
|
astro-ph/0310267 🔍 (source)
|
broad-line quasars |
L _ { bol } / L _ { Edd } |
1.0 |
|
|
astro-ph/0310466 🔍 (source)
|
flux decline rate |
|
0.11 mag day-1 |
|
|
astro-ph/0310553 🔍 (source)
|
neutral iron line |
|
94.0 |
Lower |
|
astro-ph/0310553 🔍 (source)
|
neutral iron line |
|
887.0 eV |
|
|
astro-ph/0311379 🔍 (source)
|
emission line strength |
M _ { b _ { J } |
-19.5 |
Upper |
|
astro-ph/0311497 🔍 (source)
|
line–of–sight velocity dispersion |
\sigma _ { v } |
1438.0 +109.0-86.0 km s-1 |
|
|
astro-ph/0312068 🔍 (source)
|
linear radius |
|
2.048 ± 0.025 R_\odot |
|
|
astro-ph/0312068 🔍 (source)
|
linear radii |
R [ A ] |
1.224 ± 0.003 R_\odot |
|
|
astro-ph/0312296 🔍 (source)
|
projected linear size |
|
1.35 Mpc |
|
|
astro-ph/0401051 🔍 (source)
|
total line flux |
|
2.7999999999999996e-16 ± 3e-17 erg cm-2 s-1 |
|
|
astro-ph/0401510 🔍 (source)
|
diffuse sightline ratio |
|
161.0 ± 17.0 c |
|
|
astro-ph/0401510 🔍 (source)
|
average hydrogen density along the sightline |
n ( H ) |
8.5 ± 5.5 cm-3 |
|
|
astro-ph/0401618 🔍 (source)
|
non-linear coupling parameter |
|
95.0 |
|
|
astro-ph/0402036 🔍 (source)
|
linear diameter |
|
5.25 ± 1.75 pc |
|
|
astro-ph/0402272 🔍 (source)
|
time baseline |
\Delta t |
1.3 yr |
|
|
astro-ph/0403161 🔍 (source)
|
\alpha line luminosity |
|
1.1 |
Lower |
|
astro-ph/0403243 🔍 (source)
|
H _ { \beta } emission line luminosity |
R ( light - days |
24.05 |
|
|
astro-ph/0403421 🔍 (source)
|
linear polarization |
|
10.0 |
|
|
astro-ph/0403497 🔍 (source)
|
sky-projected baseline length |
|
45.8 m |
|
|
astro-ph/0403665 🔍 (source)
|
emission line velocity amplitude |
|
58.2 ± 3.7 km s-1 |
|
|
astro-ph/0403688 🔍 (source)
|
metal lines absorb |
|
2.3 ± 0.5 % |
|
|
astro-ph/0403715 🔍 (source)
|
line-of-sight velocity dispersions |
|
962.0 km s-1 |
|
|
astro-ph/0404263 🔍 (source)
|
line width |
\sigma _ { K \alpha } |
0.18 keV |
Upper |
|
astro-ph/0405501 🔍 (source)
|
keV line flux |
|
7.3e-05 ± 9e-06 ph cm-2 s-1 |
|
|
astro-ph/0405525 🔍 (source)
|
linear polarization degree |
\Pi _ { GRB } |
41.0 +57.0-44.0 % |
|
|
astro-ph/0405530 🔍 (source)
|
line width |
|
4.5 ± 1.5 km s-1 |
|
|
astro-ph/0405539 🔍 (source)
|
rms line width |
|
20.0 eV |
|
|
astro-ph/0406036 🔍 (source)
|
linear mass-clustering amplitude |
\sigma _ { 8 } |
0.8 |
|
|
astro-ph/0406151 🔍 (source)
|
P \alpha /P \beta line flux ratio |
|
1.05 ± 0.2 |
|
|
astro-ph/0406462 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma _ { rad } |
20.0 km s-1 |
|
|
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/0406577 🔍 (source)
|
Line ratios |
T |
30.0 ± 10.0 K |
|
|
astro-ph/0407123 🔍 (source)
|
\alpha line luminosity |
|
44.0 |
Upper |
|
astro-ph/0407123 🔍 (source)
|
\alpha line luminosity |
|
-1.0 |
|
|
astro-ph/0407123 🔍 (source)
|
\alpha line luminosity |
|
2.4 keV |
|
|
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/0407521 🔍 (source)
|
O vi line width |
|
2100.0 ± 200.0 km s-1 |
|
|
astro-ph/0407643 🔍 (source)
|
linear velocity gradient |
|
1.4 km s-1 pc-1 |
|
|
astro-ph/0407643 🔍 (source)
|
linear velocity gradient |
|
0.7 km s-1 pc-1 |
|
|
astro-ph/0408031 🔍 (source)
|
Lyman- \alpha line flux |
|
2.2000000000000003e-17 erg cm-2 s-1 |
|
|
astro-ph/0408392 🔍 (source)
|
high-ionization forbidden emission line |
|
4227.0 |
|
|
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/0409036 🔍 (source)
|
decline rate parameters |
\Delta m _ { 15 } |
1.1 |
|
|
astro-ph/0409054 🔍 (source)
|
velocity integrated line luminosity |
L _ { HCN } ^ { \prime } |
6700000000.0 ± 2200000000.0 K km pc2 s-1 |
|
|
astro-ph/0409153 🔍 (source)
|
line width |
\Delta v _ { FWHM } |
4.9 km s-1 |
|
|
astro-ph/0409305 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma _ { los } |
162.0 +44.0-30.0 km s-1 |
|
|
astro-ph/0409305 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma _ { los } |
136.0 +26.0-20.0 km s-1 |
|
|
astro-ph/0409305 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma _ { los } |
150.0 +55.0-38.0 km s-1 |
|
|
astro-ph/0409494 🔍 (source)
|
luminosity decline rate |
\Delta m _ { 15 } ( B ) |
1.04 ± 0.04 mag |
|
|
astro-ph/0410232 🔍 (source)
|
linear radius |
R _ { UD } ^ { K } |
2.3 ± 0.5 AU |
|
|
astro-ph/0410247 🔍 (source)
|
line center |
|
330.0 ± 100.0 km s-1 |
|
|
astro-ph/0410385 🔍 (source)
|
Fe xxvi X-ray absorption lines |
|
6.97 ± 0.05 keV |
|
|
astro-ph/0410372 🔍 (source)
|
emission line |
|
4.45 ± 0.05 keV |
|
|
hep-ph/0410283 🔍 (source)
|
baseline |
L |
60.0 ± 10.0 km |
|
|
astro-ph/0411003 🔍 (source)
|
X-ray flux decayed linearly |
|
6.900000000000001e-05 ± 9.000000000000001e-07 c |
Upper |
|
astro-ph/0411085 🔍 (source)
|
velocity-integrated line flux |
|
0.81 ± 0.12 Jy km s-1 |
|
|
astro-ph/0411133 🔍 (source)
|
linear radii |
|
320.0 +50.0-40.0 R_\odot |
|
|
astro-ph/0411252 🔍 (source)
|
emission line properties |
H \beta ) |
1710.0 km s-1 |
|
|
astro-ph/0411252 🔍 (source)
|
emission line properties |
H \beta ) |
0.32 |
|
|
astro-ph/0411351 🔍 (source)
|
width of the annihilation line |
|
2.37 ± 0.25 keV |
|
|
astro-ph/0411351 🔍 (source)
|
line energy |
|
510.954 ± 0.075 keV |
|
|
astro-ph/0411328 🔍 (source)
|
line velocity width |
\sigma |
60.0 eV |
|
|
astro-ph/0411531 🔍 (source)
|
linear polarization |
P / \sigma _ { P } |
3.0 |
Lower |
|
astro-ph/0412053 🔍 (source)
|
dust temperature and the molecular line properties |
L _ { sub } / L _ { bol } |
1.0 |
|
|
astro-ph/0412557 🔍 (source)
|
line width parameter |
b _ { \sigma } |
1.4 |
|
|
astro-ph/0412583 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma _ { H } |
88.0 ± 20.0 km s-1 |
|
|
astro-ph/0501037 🔍 (source)
|
frequency of emission-line galaxies |
W _ { \lambda } |
20.0 |
Lower |
|
astro-ph/0501161 🔍 (source)
|
line-of-sight magnetic field strength |
|
3.0 ± 0.3 m |
|
|
astro-ph/0501253 🔍 (source)
|
emission line ratios |
|
0.8 |
Lower |
|
astro-ph/0501545 🔍 (source)
|
line-of-sight extinction |
E ( B - V ) |
1.41 ± 0.04 |
|
|
astro-ph/0501545 🔍 (source)
|
line-of-sight extinction |
E ( B - V ) |
1.32 ± 0.04 |
|
|
astro-ph/0501664 🔍 (source)
|
common decline rate |
\Delta m _ { 15 } |
1.1 |
|
|
astro-ph/0502011 🔍 (source)
|
baseline rms |
|
50.0 mK |
|
|
astro-ph/0502011 🔍 (source)
|
baseline rms |
\sigma _ { rms } |
2.6 km s-1 |
|
|
astro-ph/0502128 🔍 (source)
|
line |
|
6.2 keV |
|
|
astro-ph/0502293 🔍 (source)
|
linear radius |
|
1570.0 ± 400.0 R_\odot |
|
|
astro-ph/0502482 🔍 (source)
|
line-of-sight velocity dispersion |
\Delta v |
650.0 km s-1 |
|
|
astro-ph/0503055 🔍 (source)
|
median CO line luminosity |
\langle L _ { \tiny { CO } } ^ { \prime } \rangle |
38000000000.0 ± 20000000000.0 K km pc2 s-1 |
|
|
astro-ph/0503055 🔍 (source)
|
median CO fwhm linewidth |
\langle fwhm \rangle |
780.0 ± 320.0 km s-1 |
|
|
astro-ph/0503205 🔍 (source)
|
line-of-sight |
\tau _ { 2.2 } |
5.3 |
|
|
astro-ph/0503250 🔍 (source)
|
line-of-sight cluster magnetic |
B _ { \| } |
2.1 |
|
|
astro-ph/0503320 🔍 (source)
|
\alpha line |
f _ { Ly \alpha,TOT } |
1.94e-12 erg s-1 cm-2 |
|
|
astro-ph/0503482 🔍 (source)
|
outburst decline time scale |
|
1.2 day mag-1 |
|
|
astro-ph/0503623 🔍 (source)
|
Fe xxv emission line |
|
6.71 +0.03-0.02 keV |
|
|
astro-ph/0503623 🔍 (source)
|
iron line |
|
6.5 +0.3-0.2 keV |
|
|
astro-ph/0503623 🔍 (source)
|
iron line width |
\sigma |
32.0 +13.0-14.0 eV |
|
|
astro-ph/0504106 🔍 (source)
|
Fe xi electron density diagnostic line intensity ratio |
|
184.8 |
|
|
astro-ph/0504137 🔍 (source)
|
blueshifted iron line |
v / c |
0.18 |
|
|
astro-ph/0504402 🔍 (source)
|
linear relation |
[ X / H ] |
1.0 |
|
|
astro-ph/0504494 🔍 (source)
|
line-of-sight |
D _ { \sun } |
7.2 ± 1.0 kpc |
|
|
astro-ph/0504555 🔍 (source)
|
line-of-sight rotation speed of the star |
v \sin I _ { \star } |
4.7 ± 0.16 km s-1 |
|
|
astro-ph/0504604 🔍 (source)
|
line widths |
\Delta v _ { FWHM } |
500.0 ± 130.0 km s-1 |
|
|
astro-ph/0506026 🔍 (source)
|
keV line flux |
|
0.0010500000000000002 ± 6e-05 ph cm-2 s-1 |
|
|
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/0506590 🔍 (source)
|
emission line |
|
19.19 +0.05-0.09 |
|
|
astro-ph/0507055 🔍 (source)
|
projected linear size |
H _ { o } |
71.0 km s-1 Mpc-1 |
|
|
astro-ph/0507094 🔍 (source)
|
emission line width |
\sigma |
320.0 km s-1 |
|
|
astro-ph/0507163 🔍 (source)
|
HCN/ ^ { 12 } CO line intensity ratio |
|
0.25 |
|
|
astro-ph/0507470 🔍 (source)
|
linear correlation coefficient |
|
0.36 |
|
|
astro-ph/0507470 🔍 (source)
|
linear correlation coefficient |
r |
98.0 |
|
|
astro-ph/0507583 🔍 (source)
|
linear theory matter fluctuation amplitude |
\sigma _ { 8 } |
0.77 ± 0.05 |
|
|
astro-ph/0507653 🔍 (source)
|
H \beta linewidth |
\sigma |
27.0 km s-1 |
|
|
astro-ph/0507653 🔍 (source)
|
H i FWHM linewidth |
|
33.0 +60.0-12.0 |
|
|
astro-ph/0507706 🔍 (source)
|
/H \alpha line ratio |
[ S II ] / H \alpha |
0.4 |
Upper |
|
astro-ph/0508656 🔍 (source)
|
absorption-line frequency |
W _ { \lambda } ( { CIII } |
12.0 +3.0-2.0 |
|
|
astro-ph/0508656 🔍 (source)
|
absorption-line frequency |
d N _ { CIII } / dz |
12.0 +3.0-2.0 |
|
|
astro-ph/0509166 🔍 (source)
|
linear radius |
|
0.863 ± 0.003 R_\odot |
|
|
astro-ph/0509589 🔍 (source)
|
line intensity |
\int T _ { A } d |
28.0 mK km s-1 |
|
|
astro-ph/0509648 🔍 (source)
|
line-strength ratios |
f ( 1370 Å ) |
0.0588 ± 0.006 |
|
|
astro-ph/0509827 🔍 (source)
|
inclination of Alderamin to the line |
i |
88.2 +1.8-13.3 |
|
|
astro-ph/0510099 🔍 (source)
|
line ratio |
O ii ] I ( 3729 ) |
3726.0 |
|
|
astro-ph/0510395 🔍 (source)
|
line-of-sight magnetic field |
|
-220.0 ± 38.0 |
|
|
astro-ph/0510422 🔍 (source)
|
linear size |
|
0.5 pc |
|
|
astro-ph/0510542 🔍 (source)
|
line luminosity |
L _ { HCN ( J = 5 - 4 ) } ^ { \prime } |
40000000000.0 ± 5000000000.0 K km pc2 s-1 |
|
|
astro-ph/0510649 🔍 (source)
|
linear ephemeris of the light maxima |
JD _ { max } |
2449862.0 |
|
|
astro-ph/0511065 🔍 (source)
|
maximum baseline length |
|
480.0 km |
|
|
astro-ph/0511387 🔍 (source)
|
line energy |
|
6.51 +0.21-0.12 keV |
|
|
astro-ph/0511667 🔍 (source)
|
H \delta line strength |
d H \delta / dr _ { p } |
0.35 ± 0.06 |
|
|
astro-ph/0601465 🔍 (source)
|
decline rate |
|
0.018 |
|
|
astro-ph/0602105 🔍 (source)
|
linear radii |
|
0.38 |
Lower |
|
astro-ph/0602181 🔍 (source)
|
emission lines |
|
54.0 ± 8.0 km s-1 |
|
|
astro-ph/0602217 🔍 (source)
|
snow line |
|
1.7000000000000002 +0.09999999999999987-0.10000000000000009 AU |
|
|
gr-qc/0602117 🔍 (source)
|
linear momentum flux |
\eta = \frac { m _ { 1 } m _ { 2 } } { ( m _ { 1 } + m _ { 2 } ) } ^ { 2 } |
0.2 |
|
|
astro-ph/0603192 🔍 (source)
|
line–of–sight ( LOS ) velocity dispersion |
\sigma _ { V } |
1767.0 +121.0-99.0 km s-1 |
|
|
astro-ph/0603244 🔍 (source)
|
line fluxes |
|
2.5 |
Lower |
|
astro-ph/0603244 🔍 (source)
|
line fluxes |
|
-2.0 |
Upper |
|
astro-ph/0603314 🔍 (source)
|
linear function |
a _ { 0 } |
0.289 ± 0.051 |
|
|
astro-ph/0603392 🔍 (source)
|
decline rate |
\Delta m _ { 15 } |
4.37 ± 0.25 |
|
|
astro-ph/0603654 🔍 (source)
|
optical emission-line flux ratios |
\left \langle ICF \right \rangle |
1.08 ± 0.09 |
Lower |
|
astro-ph/0604341 🔍 (source)
|
position angle of linear polarization |
\theta _ { * } |
155.0 ± 15.0 |
|
|
astro-ph/0604541 🔍 (source)
|
temporal baseline |
|
2.8 |
Lower |
|
astro-ph/0605277 🔍 (source)
|
crystalline silicates |
T _ { gr } |
445.0 ± 155.0 K |
|
|
astro-ph/0605437 🔍 (source)
|
HCO ^ { + } line luminosity |
L ^ { \prime } _ { HCO ^ { + } } |
3500000000.0 K km pc2 s-1 |
|
|
astro-ph/0606210 🔍 (source)
|
\alpha line |
EW _ { Ly \alpha } ^ { rest } |
46.0 ± 5.0 |
|
|
astro-ph/0606502 🔍 (source)
|
extended emission-line |
|
2.5000000000000002e+57 erg |
|
|
astro-ph/0606543 🔍 (source)
|
line-of-sight absorption column |
|
1.2e+23 cm-2 |
|
|
astro-ph/0606736 🔍 (source)
|
line flux |
|
2.5e-05 ± 3e-06 cm-2 s-1 |
|
|
astro-ph/0607267 🔍 (source)
|
line luminosity |
L _ { H _ { 2 } O } ^ { \prime } |
18000000000.0 K km pc2 s-1 |
Upper |
|
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/0608301 🔍 (source)
|
metal-line absorber |
Z / Z _ { \sun } |
-0.3 |
Upper |
|
astro-ph/0608406 🔍 (source)
|
emission-line time delay |
\tau _ { cent } |
3.73 ± 0.75 day |
|
|
astro-ph/0608598 🔍 (source)
|
fast decline |
t _ { 2 } |
11.0 day |
|
|
astro-ph/0609360 🔍 (source)
|
steep decline |
dN _ { cluster } / d \tau |
10.0 |
Upper |
|
astro-ph/0609405 🔍 (source)
|
line polarization features |
P |
0.5 |
Upper |
|
astro-ph/0609611 🔍 (source)
|
line-of-sight turbulent velocity |
|
0.37 ± 0.08 km s-1 |
|
|
astro-ph/0609774 🔍 (source)
|
line-of-sight velocity dispersions |
|
17.0 km s-1 |
|
|
astro-ph/0610092 🔍 (source)
|
phantom divide line |
w |
-1.0 |
|
|
astro-ph/0610273 🔍 (source)
|
median line width |
|
6.5 km s-1 |
|
|
astro-ph/0610420 🔍 (source)
|
linear size of the planetary nebula |
D _ { PN } |
1.72 pc |
|
|
astro-ph/0610824 🔍 (source)
|
linewidths |
\sigma |
125.0 km s-1 |
Upper |
|
astro-ph/0611126 🔍 (source)
|
non-linearity parameter |
f _ { NL } |
1.0 |
|
|
astro-ph/0611547 🔍 (source)
|
line of sight |
i |
15.0 |
|
|
astro-ph/0611779 🔍 (source)
|
maximum linear radius |
|
1.52 ± 0.15 pc |
|
|
astro-ph/0612409 🔍 (source)
|
Fe ii line equivalent width |
|
1.72 ± 0.25 |
|
|
astro-ph/0612409 🔍 (source)
|
Fe ii line equivalent width |
|
0.28 ± 0.21 |
|
|
astro-ph/0612409 🔍 (source)
|
Fe ii line equivalent width |
|
0.96 ± 0.21 |
Lower |
|
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/0701140 🔍 (source)
|
line-of-sight depth |
\sigma _ { los } |
1.5 ± 0.2 kpc |
|
|
astro-ph/0701275 🔍 (source)
|
linear correlation coefficient |
|
0.38 |
|
|
astro-ph/0702191 🔍 (source)
|
CO line luminosity |
L \arcmin _ { CO } |
690000000.0 K km pc2 s-1 |
|
|
astro-ph/0702307 🔍 (source)
|
phase-averaged linear polarisation degree |
P _ { L } |
9.4 |
|
|
astro-ph/0702523 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma _ { v } |
433.0 +152.0-74.0 km s-1 |
|
|
astro-ph/0702566 🔍 (source)
|
post–maximum decline |
\Delta { m _ { 15 } ( B ) } _ { true } |
1.12 |
|
|
astro-ph/0702663 🔍 (source)
|
Ca line equivalent |
width ( EW ) |
165.0 ± 4.0 m |
|
|
0704.0603 🔍 (source)
|
line-of-sight velocity |
\log \tau _ { 5 } |
-0.4 |
|
|
0704.1636 🔍 (source)
|
linear phase curves |
|
0.1 |
|
|
0704.1636 🔍 (source)
|
linear phase curves |
|
0.18 |
|
|
0704.3722 🔍 (source)
|
linear radius |
|
0.779 ± 0.052 |
|
|
0705.0726 🔍 (source)
|
rms intrinsic scatter of the decline-rate-corrected SN rise time |
|
0.96 +0.52-0.25 day |
|
|
0705.0726 🔍 (source)
|
light-curve decline rate |
|
18.81 ± 0.36 day |
|
|
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 |
|
|
0705.2381 🔍 (source)
|
decline rates |
|
0.17 ± 0.11 |
|
|
0705.2381 🔍 (source)
|
decline rates |
|
0.19 ± 0.1 |
|
|
0705.2772 🔍 (source)
|
effective line-of-sight extent of the gas |
|
10.1 kpc |
|
|
0705.2772 🔍 (source)
|
effective line-of-sight extent of the gas |
|
3.4 (1.0) |
|
|
0705.3181 🔍 (source)
|
phantom divide line |
w |
-1.0 |
|
|
0706.0938 🔍 (source)
|
linear growth rate of perturbations |
z |
0.15 |
|
|
0706.0987 🔍 (source)
|
mean velocity of the UV lines |
|
-16.0 ± 4.0 km s-1 |
|
|
0706.1828 🔍 (source)
|
line-of-sight absorption |
N _ { H } |
1e+22 ± 1e+22 cm-2 |
|
|
0707.2339 🔍 (source)
|
line |
|
0.72 ± 0.09 mJy |
|
|
0707.2425 🔍 (source)
|
narrow iron line width |
\sigma |
22.0 eV |
Upper |
|
0707.2339 🔍 (source)
|
line |
|
610.0 ± 110.0 km s-1 |
|
|
0707.2443 🔍 (source)
|
linear bias |
b |
1.74 ± 0.16 |
|
|
0708.0010 🔍 (source)
|
line-of-sight velocities |
|
2.5 km s-1 |
|
|
0708.1045 🔍 (source)
|
line ratio |
R _ { \mathrm { HCN } / \mathrm { HCO } + } |
1.0 |
Upper |
|
0708.2863 🔍 (source)
|
mean line-width |
|
0.38 km s-1 |
|
|
0708.3109 🔍 (source)
|
projected linear separation |
|
1.0 |
|
|
0708.3258 🔍 (source)
|
line of sight velocity dispersion |
|
580.0 ± 140.0 km s-1 |
|
|
0708.3377 🔍 (source)
|
recombination-line velocity |
|
76.1 ± 0.6 km s-1 |
|
|
0708.3377 🔍 (source)
|
recombination-line velocity |
|
82.7 ± 2.0 km s-1 |
|
|
0708.3377 🔍 (source)
|
recombination-line velocities |
|
89.6 ± 2.1 km s-1 |
|
|
0708.3377 🔍 (source)
|
recombination-line velocities |
|
103.0 ± 0.5 km s-1 |
|
|
0708.4321 🔍 (source)
|
non-linear parameter of the curvature perturbation |
f _ { NL } |
-5.0 c |
|
|
0709.0523 🔍 (source)
|
\cotracer linewidths |
{ { \Delta } v |
0.4 km |
|
|
0709.1136 🔍 (source)
|
decline rate of the radio emission steepens |
t ^ { + \beta } ) \beta |
-0.7 |
|
|
0709.4030 🔍 (source)
|
O vi absorber line frequency |
d N / dz |
40.0 +14.0-8.0 |
|
|
0710.1634 🔍 (source)
|
line width |
\log M _ { BH } / M _ { \odot } |
8.44 ± 0.14 |
|
|
0710.4525 🔍 (source)
|
HCN line luminosity |
L _ { HCN } ^ { \prime } |
3300000000.0 K km pc2 s-1 |
Upper |
|
0710.5273 🔍 (source)
|
projected linear separation |
|
12.3 AU |
|
|
0710.5701 🔍 (source)
|
value of decline |
t _ { 2 } |
6.5 ± 1.0 day |
|
|
0711.1904 🔍 (source)
|
mean He II Ly \alpha line transmission |
\bar { F } |
0.304 ± 0.002 |
|
|
0711.1999 🔍 (source)
|
line width |
|
4.3 km s-1 |
|
|
0711.2215 🔍 (source)
|
emission line |
|
52.594 |
|
|
0711.4822 🔍 (source)
|
Galactic line-of-sight column density |
N _ { H } |
5.7e+19 cm-2 |
|
|
0712.0680 🔍 (source)
|
Pearson linear correlation coefficient |
|
0.94 |
|
|
0712.2882 🔍 (source)
|
Linear polarization |
|
1.0 ± 0.2 % |
|
|
0712.2882 🔍 (source)
|
Linear polarization |
|
0.7 ± 0.1 |
|
|
0801.2258 🔍 (source)
|
line-of-sight velocity dispersion |
|
250.0 km s-1 |
|
|
0801.2379 🔍 (source)
|
fast decline |
t _ { 2 } |
9.0 ± 0.5 day |
|
|
0801.2534 🔍 (source)
|
sightline |
[ { Z / H } |
-1.7 |
Lower |
|
0801.3729 🔍 (source)
|
broad line region mass |
|
0.35 +0.050000000000000044-0.04999999999999999 M_\odot |
|
|
0801.4338 🔍 (source)
|
iron line equivalent |
|
3.7000000000000002e+22 |
|
|
0801.4338 🔍 (source)
|
iron line equivalent |
N _ { H } |
6.1e+23 cm-2 |
|
|
0802.0698 🔍 (source)
|
line-of-sight distance |
|
794.0 ± 40.0 kpc |
|
|
0803.2473 🔍 (source)
|
emission line star |
|
215.0 |
|
|
0803.3731 🔍 (source)
|
linear polarisation level |
|
16.0 |
Upper |
|
0804.1226 🔍 (source)
|
line-of-sight velocity dispersion |
{ \sigma _ { v } |
1268.0 +93.0-84.0 km s-1 |
|
|
0804.1871 🔍 (source)
|
line-of-sight velocities |
|
56.0 km s-1 |
Upper |
|
0804.4129 🔍 (source)
|
apparent linear expansion rate for the dust shell |
|
0.35 ± 0.03 m as day-1 |
|
|
0804.4439 🔍 (source)
|
luminosity decline rate |
\Delta m _ { 15 } ( B ) |
1.17 ± 0.12 mag |
|
|
0805.0596 🔍 (source)
|
nonlinear fractional density contrast of the sphere |
1 + \delta |
1.76 ± 0.17 |
|
|
0805.2293 🔍 (source)
|
{ 13 } CO/ ^ { 12 } CO line ratio |
|
0.1 J |
|
|
0806.2217 🔍 (source)
|
slope of this linear portion |
a |
0.41 ± 0.01 |
|
|
0806.2969 🔍 (source)
|
line–of–sight velocity dispersion of galaxies |
\sigma _ { V } |
560.0 ± 140.0 km s-1 |
|
|
0807.1185 🔍 (source)
|
line-of-sight velocity |
|
220.0 km s-1 |
|
|
0807.1752 🔍 (source)
|
linear scale heights |
|
103.0 pc F W H |
|
|
0807.2860 🔍 (source)
|
line intensity ratio |
|
1299999.9999999998 +100000.00000000009-99999.99999999987 K |
|
|
0807.2899 🔍 (source)
|
} CO line ratio |
|
1.7 |
|
|
0807.3686 🔍 (source)
|
line of sight |
\langle n _ { e } \rangle |
0.018 ± 0.002 cm-3 |
|
|
0808.2193 🔍 (source)
|
fast decline rate |
|
0.042 mag day-1 |
|
|
0808.2742 🔍 (source)
|
projected linear size of the radio structure |
H _ { 0 } |
71.0 km s-1 Mpc-1 |
|
|
0808.2796 🔍 (source)
|
apparent line variation |
|
0.04 |
|
|
0809.0327 🔍 (source)
|
line-of-sight velocity dispersion |
|
3.9 ± 0.3 km s-1 |
|
|
0809.1066 🔍 (source)
|
line-of-sight stellar velocity dispersion |
\sigma _ { \star } |
43.0 ± 3.0 km s-1 |
|
|
0809.1426 🔍 (source)
|
rate of incline |
{ ( 1 + z ) } ^ { n } , n |
5.0 ± 0.4 |
|
|
0809.1959 🔍 (source)
|
linear slope |
\beta |
0.05 ± 0.004 |
|
|
0809.2624 🔍 (source)
|
linear separation |
|
8700.0 AU |
|
|
0809.2780 🔍 (source)
|
integrated line flux |
|
0.106 ± 0.012 Jy km s-1 |
|
|
0809.4177 🔍 (source)
|
line ratio HCN |
|
0.07 |
Lower |
|
0809.4177 🔍 (source)
|
line ratio HCN |
( 1–0 ) / ^ { 12 } CO ( 1–0 |
0.12 |
|
|
0810.0635 🔍 (source)
|
slow luminosity decline |
\gamma _ { R } |
237.0 |
|
|
0810.1712 🔍 (source)
|
mean line width |
|
0.48 km s-1 |
|
|
0810.2424 🔍 (source)
|
H \alpha emission line |
EW _ { obs } |
85.0 ± 35.0 |
|
|
0810.3405 🔍 (source)
|
integrated line flux |
|
0.66 Jy |
|
|
0811.0118 🔍 (source)
|
line-of-sight velocity ( median error |
|
2.1 km s-1 |
|
|
0811.1205 🔍 (source)
|
luminosity decline rate |
\Delta m _ { 15 } ( B ) |
1.05 ± 0.03 mag |
|
|
0811.1382 🔍 (source)
|
frequency along quasar lines of sight |
{ [ dN / dz ] } _ { QSO } |
0.24 |
|
|
0811.2223 🔍 (source)
|
non linearity parameter |
f _ { NL } |
100.0 |
|
|
0811.3929 🔍 (source)
|
decline rate |
|
56.0 C |
Upper |
|
0812.0379 🔍 (source)
|
HI line width |
( W _ { 20 } /2 |
238.0 km s-1 |
|
|
0812.1580 🔍 (source)
|
median line-of-sight velocity dispersion |
\sigma _ { LOS } |
230.0 km s-1 |
|
|
0812.1756 🔍 (source)
|
non-linear coupling parameter |
f _ { NL } |
-94.0 |
Lower |
|
0812.2975 🔍 (source)
|
iron K \alpha emission line |
|
6.39 ± 0.03 keV |
|
|
0812.3409 🔍 (source)
|
integrated line intensity |
|
1.2 ± 0.2 Jy km s-1 |
|
|
0812.3409 🔍 (source)
|
line width |
|
410.0 ± 120.0 km s-1 |
|
|
0812.3409 🔍 (source)
|
line intensity |
|
1.0 ± 0.1 Jy km s-1 |
|
|
0812.3409 🔍 (source)
|
line width |
|
280.0 ± 50.0 km s-1 |
|
|
0901.0642 🔍 (source)
|
/H \alpha emission line ratio |
|
0.42 |
|
|
0901.1138 🔍 (source)
|
total line-of-sight depth |
|
2.0 +0.4-0.6 Mpc |
|
|
0901.1385 🔍 (source)
|
linearly polarized intensity |
|
3.6 |
|
|
0901.3097 🔍 (source)
|
total line-of-sight reddening |
E ( V - I ) |
0.07 ± 0.04 mag |
|
|
0901.4627 🔍 (source)
|
Ly \alpha line flux |
|
1.47e-17 erg s-1 cm-2 |
|
|
0902.1125 🔍 (source)
|
distribution of line-of-sight velocities on the surface |
\log \tau _ { 5 } |
-1.0 |
|
|
0902.2131 🔍 (source)
|
line-of-sight peculiar velocity |
v _ { r } |
-140.0 ± 460.0 km s-1 |
|
|
0903.3583 🔍 (source)
|
full-width-half-maximum velocity of the broad iron line |
v |
0.37 c |
Lower |
|
0903.4002 🔍 (source)
|
line-of-sight velocity |
\delta _ { p , tri } |
10.0 |
Upper |
|
0903.4698 🔍 (source)
|
H beta line width |
|
79000000.0 M_\odot |
|
|
0904.0005 🔍 (source)
|
linear polarisation |
|
0.09 % |
|
|
0904.0005 🔍 (source)
|
linear polarisation |
|
30.0 +10.0-6.0 |
|
|
0904.0196 🔍 (source)
|
lithium line Li i |
\lambda |
6707.8 |
|
|
0904.1007 🔍 (source)
|
least-squares best-fit line |
Z ( z ) / Z _ { \odot } |
0.46 ± 0.05 |
|
|
0904.3136 🔍 (source)
|
decreases linearly |
|
-0.047 ± 0.003 dex kpc-1 |
|
|
0904.4901 🔍 (source)
|
mean HVC column density per sight line |
\langle \log { N } _ { SiIII } \rangle |
13.42 ± 0.21 |
|
|
0905.0499 🔍 (source)
|
linear source power spectrum |
\Delta ^ { 2 } |
0.35 +0.15000000000000002-0.14999999999999997 |
|
|
0905.1041 🔍 (source)
|
iron line |
EW |
0.7 |
|
|
0905.1958 🔍 (source)
|
line-of-sight velocity dispersion |
\beta |
0.4 |
|
|
0905.4742 🔍 (source)
|
line ratio |
|
0.8 |
|
|
0906.0823 🔍 (source)
|
SiO line width |
|
15.0 km s-1 |
|
|
0906.1532 🔍 (source)
|
line unit |
|
2.66 +0.37-0.3 |
|
|
0906.3010 🔍 (source)
|
fractional linear polarization |
|
29.0 |
Lower |
|
0906.3347 🔍 (source)
|
absorber line density |
d N _ { C IV } / d X |
4.1 +0.7-0.6 |
|
|
0906.3347 🔍 (source)
|
absorber line density |
\log N ( C ^ { Tree(positive_expression, [LeafNumber('3')]) } ) |
4.1 +0.7-0.6 |
|
|
0906.4600 🔍 (source)
|
line-of-sight velocity |
|
42.0 km s-1 |
|
|
0907.0171 🔍 (source)
|
narrow H i line widths |
v _ { FWHM } |
1.8 |
Lower |
|
0907.1057 🔍 (source)
|
linear cloud size |
l |
520.0 +240.0-190.0 pc |
|
|
0907.1087 🔍 (source)
|
} O line luminosities |
L _ { H _ { 2 } O } |
7470.0 L_\odot |
Upper |
|
0907.1661 🔍 (source)
|
HI column density sightline |
N _ { HI } |
3.2e+19 cm-2 |
Upper |
|
0907.2240 🔍 (source)
|
line-of-sight extinction |
A _ { V } |
2.0 mag |
Lower |
|
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 |
|
|
0908.0537 🔍 (source)
|
B -band decline-rate parameter |
\Delta m _ { 15 } ( B ) |
1.61 ± 0.02 |
|
|
0908.2059 🔍 (source)
|
decline rate of the light curve |
\Delta m _ { 15 } ( B ) |
0.65 ± 0.03 |
|
|
0908.3893 🔍 (source)
|
sight line of the QSO to a point source |
U _ { AB } |
28.0 |
|
|
0909.0464 🔍 (source)
|
broad-line AGNs |
|
1.47 ± 0.03 |
|
|
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 |
|
|
0909.1607 🔍 (source)
|
absorption line |
|
6.961 ± 0.002 keV |
|
|
0909.5049 🔍 (source)
|
longitude of the line of nodes |
\Omega _ { 1 } |
48.0 ± 2.0 |
|
|
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 |
|
|
0910.1913 🔍 (source)
|
decline rate |
\Delta m _ { 15 } ( B ) ( true ) |
1.33 ± 0.09 mag |
|
|
0910.2244 🔍 (source)
|
emission line fluxes |
F _ { Ly \alpha } |
2e-17 |
Lower |
|
0910.2986 🔍 (source)
|
line luminosity |
L ( Pa \alpha ) |
2.05e+42 ± 3.3000000000000004e+41 erg s-1 |
|
|
0911.2004 🔍 (source)
|
CO line luminosity |
L _ { CO } ^ { \prime } |
3000000000.0 K km s-1 pc-2 |
|
|
0912.1067 🔍 (source)
|
high-excitation line ratios |
T _ { eff } |
39000.0 K |
|
|
0912.1603 🔍 (source)
|
line frequency |
{ ( d N / dz ) } _ { BLA } |
18.0 ± 11.0 |
|
|
1001.0356 🔍 (source)
|
line |
|
6.396 +0.009-0.007 keV |
|
|
1001.0356 🔍 (source)
|
line |
|
7.08 ± 0.05 keV |
|
|
1001.2204 🔍 (source)
|
A ^ { 12 } CO line broadening |
|
32.0 km s-1 |
|
|
1001.4836 🔍 (source)
|
line flux upper |
|
2.55e-09 +1.9500000000000005e-09-1.9499999999999997e-09 cm-2 s-1 |
|
|
1002.4991 🔍 (source)
|
QSO H \beta emission line |
\sigma _ { * } ( M _ { BH } ) |
124.0 ± 47.0 km s-1 |
|
|
1003.2369 🔍 (source)
|
line luminosity |
L _ { CO ( 3 - 2 ) } ^ { \prime } |
25250000000.0 +12450000000.000002-12449999999.999998 K km pc2 s-1 |
|
|
1003.3214 🔍 (source)
|
linear bias |
b |
1.44 ± 0.22 |
|
|
1003.4622 🔍 (source)
|
Balmer-line absorption troughs |
|
5370.0 km s-1 |
|
|
1004.3771 🔍 (source)
|
normalization of the linear power spectrum |
\sigma _ { 8 } |
0.91 +0.07-0.08 |
|
|
1005.0840 🔍 (source)
|
line-of-sight velocity |
|
33.78 ± 0.18 km s-1 |
|
|
1005.2729 🔍 (source)
|
H ^ { 37 } Cl J =1-0 integrated line-intensity ratio |
|
35.0 C |
|
|
1005.3498 🔍 (source)
|
Gaussian emission line |
|
6.4 +0.2-0.3 keV |
|
|
1005.3755 🔍 (source)
|
average line centroid |
|
6.67 ± 0.02 keV |
|
|
1005.4727 🔍 (source)
|
H \alpha emission line galaxies |
|
0.1125 ± 0.023500000000000007 M_\odot yr-1 Mpc-3 |
|
|
1005.5287 🔍 (source)
|
iv line |
width |
0.08 dex |
|
|
1006.2458 🔍 (source)
|
abundance baseline |
\alpha |
-3.34 ± 0.08 |
|
|
1006.3552 🔍 (source)
|
line strength |
|
7.000000000000001e-05 M_\odot |
|
|
1006.3691 🔍 (source)
|
line-integrated brightness temperature ratio |
J |
2.5 ± 0.5 |
|
|
1006.4564 🔍 (source)
|
peak line strength integrated |
|
17.8 mJy |
|
|
1007.0905 🔍 (source)
|
line-of-sight velocity |
|
0.06 km s-1 |
|
|
1007.1420 🔍 (source)
|
} J =1–0 line frequency |
\nu |
835137.0 ± 3.0 MHz |
|
|
1007.4410 🔍 (source)
|
line opacity |
|
0.62 ± 0.11 |
|
|
1007.4410 🔍 (source)
|
line opacity |
|
0.26 ± 0.05 |
|
|
1008.1578 🔍 (source)
|
CII ] line luminosity |
L _ { [ CII ] } |
16399999999.999998 ± 2600000000.0 L_\odot |
|
|
1008.4089 🔍 (source)
|
time baseline |
|
240.0 day |
|
|
1008.4126 🔍 (source)
|
slow decline rate |
\Delta m _ { 15 } ( B ) |
0.95 |
|
|
1008.4842 🔍 (source)
|
\alpha line luminosity |
L ( Ly \alpha ) |
9.2e+42 erg s-1 |
|
|
1009.0677 🔍 (source)
|
non-linear parameter |
f _ { NL } ^ { equil } |
4.62 |
|
|
1009.0749 🔍 (source)
|
median line width ratio |
\sigma _ { 1 - 0 } / \sigma _ { 3 - 2 } |
1.15 ± 0.06 |
|
|
1009.1455 🔍 (source)
|
line-to-continuum flux ratio |
|
0.2 +0.09999999999999998-0.1 |
|
|
1009.1896 🔍 (source)
|
average line widths |
|
341.0 ± 38.0 km s-1 |
|
|
1009.4857 🔍 (source)
|
line-of-sight velocities |
|
2.0 km s-1 |
|
|
1010.0191 🔍 (source)
|
inclination angle of the system to the line |
|
22.5 day |
|
|
1010.0191 🔍 (source)
|
inclination angle of the system to the line |
|
17.0 |
|
|
1010.1563 🔍 (source)
|
line-of-sight velocity dispersion |
|
18.0 km s-1 |
|
|
1010.2754 🔍 (source)
|
line |
S / N |
7.0 |
Upper |
|
1011.0750 🔍 (source)
|
absorber line density |
G |
1.0 |
|
|
1011.0991 🔍 (source)
|
CO line emission |
|
2.0 |
|
|
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 |
|
|
1012.0267 🔍 (source)
|
short-baseline |
\sin ^ { 2 } 2 \vartheta _ { \mu \mu } |
0.1 |
Lower |
|
1012.0267 🔍 (source)
|
short-baseline |
\bar { \nu } _ { \mu } |
0.2 |
Lower |
|
1012.1827 🔍 (source)
|
flux of linear momentum |
|
2.5e-07 M_\odot km yr-1 s-1 |
|
|
1012.2127 🔍 (source)
|
heliocentric line-of-sight velocities |
V _ { los } |
-200.0 km s-1 |
|
|
1012.2371 🔍 (source)
|
CO line formation height varies |
z |
425.0 |
Lower |
|
1012.2471 🔍 (source)
|
emission-line flux ratio |
( [ O iii ] |
57.21 |
|
|
1012.5791 🔍 (source)
|
time baseline |
|
25.0 yr |
|
|
1101.2122 🔍 (source)
|
HNC/HCN line ratios |
|
0.5 |
Upper |
|
1101.2447 🔍 (source)
|
line–of–sight velocity dispersion |
\sigma _ { v } |
1000.0 km s-1 |
|
|
1101.4226 🔍 (source)
|
crystalline dust content |
|
1.5 ± 0.5 AU |
Upper |
|
1101.4226 🔍 (source)
|
crystalline dust content |
|
10.0 AU |
Upper |
|
1101.4399 🔍 (source)
|
line-of-sight number density |
\ell ( X ) |
0.25 +0.21-0.13 |
|
|
1101.5624 🔍 (source)
|
CO line luminosities |
L _ { CO } ^ { \prime } |
10825000000.0 +10175000000.0-10174999999.999998 K km pc2 s-1 |
|
|
1102.2235 🔍 (source)
|
linear extent |
|
1.4 Mpc |
|
|
1102.3264 🔍 (source)
|
maximum baseline length |
|
12.0 |
|
|
1102.3918 🔍 (source)
|
linear polarization of the \lya emission |
P _ { Ly \alpha } |
2.6 ± 2.8 % |
|
|
1102.5330 🔍 (source)
|
total time baseline |
|
2.0 yr s |
|
|
1103.0660 🔍 (source)
|
Narrow-Line Regions |
n _ { H } |
0.32 |
Lower |
|
1103.0660 🔍 (source)
|
Narrow-Line Regions |
r _ { FHIL } |
0.32 |
Lower |
|
1103.1927 🔍 (source)
|
narrow Fe K \alpha line width |
|
2.6 +0.9-0.4 |
|
|
1103.2350 🔍 (source)
|
peak line brightness |
|
100.25 ± 99.75 K km pc2 s-1 |
|
|
1103.2350 🔍 (source)
|
integrated line luminosity |
|
1.35 +1.15-1.1500000000000001 |
|
|
1104.2276 🔍 (source)
|
intrinsic luminosity of the He ii \lambda 4686 emission line |
L |
310.0 L_\odot |
|
|
1104.3608 🔍 (source)
|
emission-line fluxes |
|
7.5e-17 ± 2.5e-17 erg s-1 cm-2 |
|
|
1104.4122 🔍 (source)
|
linear relation |
\sigma _ { H _ { 2 } } |
-0.2 |
|
|
1104.4116 🔍 (source)
|
CO line luminosities |
L _ { CO ( 1 - 0 ) } ^ { \prime } |
4.17 ± 0.41 |
|
|
1104.4348 🔍 (source)
|
line brightness temperature ratios |
r _ { 31 |
0.37 ± 0.1 |
|
|
1104.4348 🔍 (source)
|
line brightness temperature ratios |
|
0.39 ± 0.09 |
|
|
1104.4498 🔍 (source)
|
crystalline substructure |
|
16.1 |
|
|
1104.4498 🔍 (source)
|
crystalline substructure |
|
18.8 |
|
|
1104.4498 🔍 (source)
|
crystalline substructure |
|
23.6 |
|
|
1104.4498 🔍 (source)
|
crystalline mass fractions |
|
0.17 |
|
|
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 |
|
|
1105.1677 🔍 (source)
|
Line Region |
|
0.0025299999999999997 +0.00035-0.0015500000000000002 |
|
|
1105.4373 🔍 (source)
|
linear polarisation fraction |
P _ { L } ^ { avg } |
0.47 |
|
|
1106.0044 🔍 (source)
|
position angle of the kinematic line of nodes |
\theta |
142.0 ± 5.0 |
|
|
1106.0746 🔍 (source)
|
line-of-sight velocity separation |
|
350.0 km s-1 |
|
|
1106.0745 🔍 (source)
|
rotation declines dramatically |
v / \sigma |
0.7 |
|
|
1106.3968 🔍 (source)
|
decline-rate parameter |
\Delta m _ { 15 } ( B ) |
0.68 ± 0.05 mag |
|
|
1106.4818 🔍 (source)
|
line fluxes |
|
44.3 ± 0.7 W m-2 |
|
|
1106.4818 🔍 (source)
|
line fluxes |
|
39.9 ± 0.8 W m-2 |
|
|
1107.4598 🔍 (source)
|
cross the phantom line |
w _ { D } |
-1.0 |
|
|
1107.1673 🔍 (source)
|
line-of sight |
|
88.0 ± 6.0 day |
|
|
1107.4011 🔍 (source)
|
H \alpha emission line nebula |
L _ { H \alpha } |
2.2000000000000004e+40 erg s-1 |
|
|
1107.4177 🔍 (source)
|
line width |
|
1.5 ± 0.5 km s-1 |
|
|
1108.0769 🔍 (source)
|
line of sight |
|
21.1 ± 10.1 day |
|
|
1108.1911 🔍 (source)
|
linear polarization |
|
2.0 |
|
|
1108.2757 🔍 (source)
|
optical forbidden lines |
[ N ii ] \lambda~ { |
6583.0 |
|
|
1108.3088 🔍 (source)
|
lines |
|
62.0 ± 9.0 |
|
|
1108.3088 🔍 (source)
|
lines |
|
0.18 |
Upper |
|
1108.4924 🔍 (source)
|
line-force parameter |
\alpha |
0.6 |
Lower |
|
1109.3157 🔍 (source)
|
inclination angle of the rotation axis to our line-of-sight |
|
70.0 ± 10.0 |
|
|
1109.4651 🔍 (source)
|
relativistically broad Fe K \alpha line |
EW |
26.0 eV |
Upper |
|
1109.4647 🔍 (source)
|
K \alpha line intensity of the warm-hot intergalactic medium |
|
1.5 |
|
|
1110.0507 🔍 (source)
|
Paschen line |
|
8598.0 |
|
|
1110.1765 🔍 (source)
|
integrated Galactic H I line emission |
N _ { HI } |
5e+18 cm-2 |
|
|
1110.4679 🔍 (source)
|
line-of-sight average magnetic field |
B _ { \parallel } |
36.0 ± 6.0 |
|
|
1110.5648 🔍 (source)
|
broad-line AGNs |
log ( M _ { DMH } / [ h ^ { -1 } M _ { \odot } ] ) |
12.9 ± 0.5 |
|
|
1110.5708 🔍 (source)
|
disk emission line shift |
|
200.0 km s-1 |
|
|
1110.6179 🔍 (source)
|
H \beta \lambda 4861 broad emission line |
|
13.9 ± 0.9 day |
|
|
1111.2630 🔍 (source)
|
line-of-sight extinction |
A _ { V } |
45.0 |
|
|
1111.4961 🔍 (source)
|
intensity of the line-of-sight component of the magnetic |
|
1.2 |
|
|
1112.0035 🔍 (source)
|
H \alpha line |
|
56.0 N |
|
|
1112.3648 🔍 (source)
|
absorption line |
|
6.91 ± 0.01 keV |
|
|
1112.3648 🔍 (source)
|
absorption line |
|
9300.0 +500.0-400.0 km s-1 |
|
|
1112.3656 🔍 (source)
|
restframe line width of the extended component |
|
21.0 ± 7.0 |
|
|
1112.3656 🔍 (source)
|
restframe line width of the extended component |
|
52.0 ± 4.0 |
|
|
1112.5007 🔍 (source)
|
time baseline |
|
57.0 yr A |
|
|
1112.5723 🔍 (source)
|
linear angular power spectrum |
\Omega _ { m } |
0.31 +0.18-0.11 |
|
|
1201.1487 🔍 (source)
|
line width |
|
110.0 km s-1 |
|
|
1201.2941 🔍 (source)
|
para-H _ { 2 } ^ { 35 } Cl ^ { + } line strengths |
H _ { 2 } |
1.0 |
Lower |
|
1202.0087 🔍 (source)
|
line flux |
|
1.8000000000000003e-17 erg s-1 cm-2 |
|
|
1202.3554 🔍 (source)
|
secular decline |
|
0.2 +0.12-0.09 W m-2 |
|
|
1202.5301 🔍 (source)
|
fast decline |
\Delta m _ { 15 } ( B ) |
1.69 ± 0.05 mag |
|
|
1203.2084 🔍 (source)
|
H \beta emission line flux variations |
|
21.1 ± 1.9 day |
|
|
1203.5844 🔍 (source)
|
line luminosity |
|
1200000000.0 ± 200000000.0 L_\odot |
|
|
1203.6682 🔍 (source)
|
linear radii |
R |
33.6 ± 2.2 R_\odot |
|
|
1204.0041 🔍 (source)
|
line |
|
192.8 |
|
|
1204.1862 🔍 (source)
|
broad emission line region |
L |
47.0 erg |
Upper |
|
1204.3234 🔍 (source)
|
\alpha line flux |
F _ { Ly \alpha } |
6.900000000000001e-18 erg s-1 cm-2 |
|
|
1204.3234 🔍 (source)
|
line flux |
F _ { Ly \alpha } |
4.4000000000000005e-18 erg s-1 cm-2 |
Upper |
|
1204.3897 🔍 (source)
|
CO J =2-1 line luminosities |
|
6080000000.0 |
Upper |
|
1204.3897 🔍 (source)
|
CO J =2-1 line luminosities |
L _ { CO } ^ { \prime } |
6630000000.0 K km pc2 s-1 |
Upper |
|
1204.3897 🔍 (source)
|
CO line luminosity |
L _ { CO } ^ { \prime } |
19400000000.0 ± 3500000000.0 K km pc2 s-1 |
|
|
1204.5475 🔍 (source)
|
post-break decline rates |
\alpha _ { X , 1 } |
-0.78 |
|
|
1205.0052 🔍 (source)
|
line-of-sight proper velocity |
v _ { z } |
3600.0 +3440.0-2160.0 km s-1 |
|
|
1205.1526 🔍 (source)
|
line ratio |
|
0.05 ± 0.01 |
|
|
1205.3779 🔍 (source)
|
3 \sigma line flux |
|
8e-18 erg cm-2 s-1 |
|
|
1205.4872 🔍 (source)
|
decline rate by two magnitude |
|
6.2 ± 0.3 day |
|
|
1205.4872 🔍 (source)
|
decline rate by two magnitude |
|
14.3 ± 0.7 day |
|
|
1205.6669 🔍 (source)
|
linear decay rate |
|
0.94 Mm2 hr-1 |
|
|
1206.2167 🔍 (source)
|
projected linear separation |
|
2.6 kpc |
|
|
1206.2762 🔍 (source)
|
{ 12 } CO line intensity ratio |
R _ { I _ { CO ( 3 - 2 ) } / I _ { CO ( 2 - 1 ) } } |
1.14 |
|
|
1206.2762 🔍 (source)
|
{ 12 } CO line intensity ratio |
|
0.7 |
Lower |
|
1207.1573 🔍 (source)
|
magnitudes of line-of-sight extinction |
EW ( 5780 ) |
0.61 |
|
|
1207.2042 🔍 (source)
|
broad line region size |
r _ { s } |
24.0 +22.0-15.0 |
|
|
1208.1150 🔍 (source)
|
average line energy |
|
6.32 ± 0.04 keV |
|
|
1208.1527 🔍 (source)
|
linear expansion |
\beta |
2.0 |
|
|
1208.4003 🔍 (source)
|
H \alpha line |
[ O i ] 6300 |
6427.0 |
|
|
1208.4848 🔍 (source)
|
thermal linewidth |
|
2000000000000000.0 cm-2 |
|
|
1208.5866 🔍 (source)
|
Scoreproducessomeofthestructuresthatwereobservedinthecircumstellarabsorptionlinesinthespectrumof |
|
2e-06 ± 5e-07 M_\odot Th yr-1 |
|
|
1209.0217 🔍 (source)
|
linear radiuses |
|
0.6759 ± 0.0062 m as |
|
|
1209.0217 🔍 (source)
|
linear radiuses |
|
1.01 ± 0.009 R_\odot |
|
|
1209.0983 🔍 (source)
|
line-of-sight velocity |
s |
14.0 km |
Upper |
|
1209.2092 🔍 (source)
|
FWHM linewidth |
|
0.497 km s-1 |
|
|
1209.2420 🔍 (source)
|
linear proportion |
\alpha _ { s } |
1.0 |
|
|
1210.1154 🔍 (source)
|
emission-line redshift |
z _ { e } |
2.5125 |
|
|
1210.1573 🔍 (source)
|
fast decline |
t _ { 2 } |
3.5 ± 0.3 day |
|
|
1210.1954 🔍 (source)
|
\sigma line-of-sight depth |
\sigma _ { int } |
5.3 ± 0.4 kpc |
|
|
1210.2781 🔍 (source)
|
linear polarisation |
|
10.0 ± 1.0 |
|
|
1210.6040 🔍 (source)
|
linear distance |
|
7.24 ± 0.03 ± 0.4 Mpc |
|
|
1210.6434 🔍 (source)
|
width of the forbidden red emission line |
Fe x |
6374.0 |
|
|
1211.3452 🔍 (source)
|
spectral line profile |
|
187.0 ± 46.0 km s-1 |
|
|
1211.3452 🔍 (source)
|
effective spectral line velocity width |
|
418.0 ± 20.0 km s-1 |
|
|
1211.3453 🔍 (source)
|
inclination of the axis to the line of sight |
i |
15.0 ± 5.0 day |
|
|
1211.3554 🔍 (source)
|
linear size |
|
3.0 pc |
|
|
1211.6722 🔍 (source)
|
line ratio |
[ O i ] / [ C ii ] |
7.2 |
Upper |
|
1212.1622 🔍 (source)
|
-ray line emission |
E _ { \gamma } |
5.05 ± 4.95 MeV |
|
|
1212.2662 🔍 (source)
|
ice line temperature |
T _ { Ice } |
160.0 ± 10.0 K |
|
|
1212.4526 🔍 (source)
|
quasar linear bias |
b _ { Q } |
1.38 ± 0.1 |
|
|
1301.0631 🔍 (source)
|
average line ratio |
r _ { 31 } |
0.46 ± 0.07 |
|
|
1301.5839 🔍 (source)
|
effective fraction of absorbing dust along the line of sight |
f _ { d } |
0.3 |
|
|
1301.6761 🔍 (source)
|
line flux ratio He |
i 5875 / H \alpha |
0.81 ± 0.04 |
|
|
1301.6966 🔍 (source)
|
line broadening |
|
278.7 km s-1 |
|
|
1302.0738 🔍 (source)
|
line-of-sight density of the warm molecular gas |
n _ { CO } |
2035.0 ± 1965.0 cm-3 |
|
|
1302.1905 🔍 (source)
|
mean time baseline |
|
6.35 yr s |
|
|
1302.4202 🔍 (source)
|
linear scale length |
|
25.0 |
|
|
1302.5014 🔍 (source)
|
linear stellar radii |
R _ { a } |
2.85 ± 0.15 R_\odot |
|
|
1302.5435 🔍 (source)
|
line flux ratio |
|
0.03 |
|
|
1303.1978 🔍 (source)
|
line-of-sight |
|
3.4 pc |
|
|
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 |
|
|
1303.6281 🔍 (source)
|
average line-of-sight metal-filling fraction |
c _ { L } |
0.1 |
|
|
1304.3414 🔍 (source)
|
line-of-sight velocity dispersions |
\sigma _ { los } |
42.5 ± 32.5 km s-1 |
|
|
1305.2873 🔍 (source)
|
slope of the linear relation |
|
2.6 ± 0.2 |
|
|
1305.2873 🔍 (source)
|
linear equation |
x |
2.3 ± 0.1 |
|
|
1305.2873 🔍 (source)
|
slope of the linear relation |
|
0.3 |
|
|
1305.6383 🔍 (source)
|
linear mass density |
M _ { l } |
600.0 M_\odot pc-1 |
|
|
1305.6469 🔍 (source)
|
CO line luminosity |
L ^ { \prime } ( CO ) |
894999999.9999999 ± 79000000.0 K km pc2 s-1 |
Lower |
|
1306.0042 🔍 (source)
|
line width |
|
26.0 km s-1 |
|
|
1306.3387 🔍 (source)
|
decline |
|
2.9 ± 0.5 (stat) ± 1.0 (sys) |
|
|
1306.3387 🔍 (source)
|
A temperature decline |
|
2.25 ± 1.25 % |
|
|
1306.4272 🔍 (source)
|
line-of-sight |
|
68.0 ± 10.0 |
|
|
1306.6314 🔍 (source)
|
averaged linear polarization degree |
v sin i |
45.0 ± 15.0 km s-1 |
|
|
1307.0854 🔍 (source)
|
broad line region |
|
1.6 pc |
|
|
1307.1133 🔍 (source)
|
H _ { 2 } O line contrast ratio |
|
0.0013000000000000002 ± 0.0002 |
|
|
1307.1706 🔍 (source)
|
linear bias |
b |
1.61 ± 0.22 |
|
|
1307.1595 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma _ { V } |
1000.0 km s-1 |
|
|
1307.6585 🔍 (source)
|
median linear radius |
|
360.0 ± 100.0 R_\odot |
|
|
1307.7061 🔍 (source)
|
linear distance |
r _ { A - B } |
0.013999999999999999 pc |
|
|
1308.0593 🔍 (source)
|
angle of the bar-bulge to the line-of-sight |
|
27.0 ± 2.0 |
|
|
1308.4096 🔍 (source)
|
linear size of the observed radio structure |
|
26.3 kpc |
|
|
1308.4149 🔍 (source)
|
line width |
|
3.3 km s-1 |
|
|
1308.6298 🔍 (source)
|
linear density rate |
|
30.0 M_\odot Myr-1 pc-1 |
|
|
1309.1144 🔍 (source)
|
{ 12 } CO/ ^ { 13 } CO line ratio |
|
25.0 |
Lower |
|
1309.1144 🔍 (source)
|
line ratio |
|
0.6 |
|
|
1309.1477 🔍 (source)
|
transverse sightline separations |
\langle d _ { \perp } \rangle |
3.6 |
Lower |
|
1309.4013 🔍 (source)
|
decline rate of the radio emission |
|
2.2 |
|
|
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 |
|
|
1309.4788 🔍 (source)
|
emission line |
|
-4.5 Myr |
|
|
1309.4788 🔍 (source)
|
emission line |
|
2.0 |
|
|
1309.5949 🔍 (source)
|
linear correlation factor |
|
0.0086 |
|
|
1310.1399 🔍 (source)
|
intensity of the absorption line |
EW |
162.0 keV |
Upper |
|
1310.4824 🔍 (source)
|
line-of-sight depth |
|
23.0 kpc |
|
|
1311.1054 🔍 (source)
|
line ratio |
|
50.0 |
|
|
1311.5969 🔍 (source)
|
decline rate |
|
25.0 ± 15.0 % |
|
|
1312.3680 🔍 (source)
|
line-of-sight velocity |
|
3200.0 km s-1 |
|
|
1312.3680 🔍 (source)
|
best-fit line-of-sight velocity |
v _ { z } |
3450.0 ± 900.0 km s-1 |
|
|
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 |
|
1401.3228 🔍 (source)
|
line luminosity |
|
1056000000.0 L_\odot |
|
|
1401.4678 🔍 (source)
|
line-of-sight |
|
87.0 ± 11.0 day |
|
|
1401.5160 🔍 (source)
|
decline rate of the light curve |
\Delta m _ { 15 } ( B ) |
1.39 ± 0.05 mag |
|
|
1401.4962 🔍 (source)
|
width of radio recombination line |
|
43.2 |
|
|
1401.4962 🔍 (source)
|
width of radio recombination line |
|
-1.0 |
|
|
1402.6714 🔍 (source)
|
line-of-sight velocity dispersion |
\langle \sigma _ { cmp } \rangle |
225.0 ± 25.0 km s-1 |
|
|
1403.0398 🔍 (source)
|
post-maximum decline rate |
\Delta m _ { 15 } ( B ) |
0.85 ± 0.05 mag |
|
|
1403.1400 🔍 (source)
|
linear size |
|
1.4 Mpc |
|
|
1403.6071 🔍 (source)
|
line width |
|
140.0 km s-1 |
|
|
1403.6071 🔍 (source)
|
line width |
|
190.0 km s-1 |
|
|
1403.6056 🔍 (source)
|
mass-loss rate declined |
|
-9.0 |
|
|
1403.6056 🔍 (source)
|
mass-loss rate declined |
\log ( \dot { M } / M _ { \odot } yr ^ { -1 } |
-11.6 |
Upper |
|
1403.6603 🔍 (source)
|
temperature in the forbidden lines region |
\log N _ { e } |
4.5 ± 0.5 |
|
|
1404.1930 🔍 (source)
|
line ratio |
I _ { H \alpha } ^ { c } |
1.0 |
|
|
1404.3189 🔍 (source)
|
maximum linear radius |
R |
123.0 ± 14.0 R_\odot |
|
|
1404.4434 🔍 (source)
|
intensity of spectral lines Fe xxvi |
|
1.51 |
|
|
1404.4434 🔍 (source)
|
intensity of spectral lines Fe xxvi |
|
1.78 |
|
|
1404.6094 🔍 (source)
|
Ba vii line |
|
993.41 |
|
|
1404.7393 🔍 (source)
|
line brightness temperature ratios |
R _ { 21 } |
0.7 ± 0.16 |
|
|
1404.7575 🔍 (source)
|
jet efficiency line |
R |
25.0 |
|
|
1405.3332 🔍 (source)
|
line fluxes |
|
0.62 ± 0.13 |
|
|
1405.3994 🔍 (source)
|
linear theory bias |
|
2.17 ± 0.2 |
|
|
1405.3970 🔍 (source)
|
decline parameter |
\Delta m _ { 15 } |
1.11 ± 0.02 mag |
|
|
1405.3994 🔍 (source)
|
linear theory bias |
|
1.7 |
|
|
1405.4707 🔍 (source)
|
line-of-sight ( LOS ) velocity dispersion |
\sigma _ { V } |
1500.0 km s-1 |
|
|
1405.5286 🔍 (source)
|
linear size |
|
0.03 pc |
|
|
1405.6198 🔍 (source)
|
line flux |
|
1e-16 |
Lower |
|
1405.7180 🔍 (source)
|
line broadening |
|
35.0 |
Lower |
|
1405.7933 🔍 (source)
|
intrinsic linewidth |
|
18.0 K |
|
|
1406.3052 🔍 (source)
|
line-of-sight filling fraction |
|
0.6 +0.14-0.13999999999999996 |
|
|
1406.6139 🔍 (source)
|
decline rate |
\Delta { m _ { 15 } ( B ) } _ { true } |
0.92 ± 0.04 mag |
|
|
1406.7052 🔍 (source)
|
emission line widths |
|
100.0 ± 30.0 km s-1 |
|
|
1407.1028 🔍 (source)
|
iron K \alpha line |
|
6.426 ± 0.008 keV |
|
|
1407.2045 🔍 (source)
|
line direction |
|
-2.4 km |
|
|
1407.2246 🔍 (source)
|
linear distance |
|
10.19 ± 0.14 ± 0.56 Mpc |
|
|
1407.2944 🔍 (source)
|
line |
|
0.11 |
|
|
1407.3235 🔍 (source)
|
linewidth |
|
5.5 km s-1 |
|
|
1407.4458 🔍 (source)
|
line-of-sight velocity |
V _ { GSR } |
50.0 km s-1 |
|
|
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 |
|
|
1409.3376 🔍 (source)
|
line-of-sight velocity |
\sigma _ { B } |
35.0 |
Upper |
|
1409.8304 🔍 (source)
|
effective logarithmic extinction of the H \beta emission line |
c _ { H \beta } |
0.5 |
|
|
1410.0135 🔍 (source)
|
broad iron line |
|
6.65 ± 0.25 keV |
|
|
1410.2893 🔍 (source)
|
line-of-sight velocity difference |
|
69.0 ± 190.0 km s-1 |
|
|
1410.3000 🔍 (source)
|
radial velocity linear trend |
\dot { \gamma } |
0.44 ± 0.04 m s-1 day-1 |
|
|
1410.6171 🔍 (source)
|
line |
|
6.7 keV |
|
|
1410.7134 🔍 (source)
|
baseline |
|
543.0 ± 7.0 m |
|
|
1411.0050 🔍 (source)
|
emission line |
|
3.59 ± 0.02 keV |
|
|
1410.8731 🔍 (source)
|
\gamma -line |
|
50.0 |
Lower |
|
1411.0709 🔍 (source)
|
line ratios |
f } |
0.52 ± 0.02 |
Lower |
|
1411.0776 🔍 (source)
|
linear velocity gradient |
|
1.0 ± 0.1 km day s-1 |
|
|
1411.4632 🔍 (source)
|
narrow-line component |
CO / HCN |
40.0 ± 5.0 |
|
|
1411.4745 🔍 (source)
|
narrow absorption line |
|
5.46 ± 0.1 keV |
|
|
1411.5688 🔍 (source)
|
large-scale linear galaxy bias |
b _ { L } ^ { HOD } |
2.82 ± 0.27 |
|
|
1411.5638 🔍 (source)
|
stellar linear radii |
|
0.805 ± 0.016 |
|
|
1411.5638 🔍 (source)
|
stellar linear radii |
R _ { \ast } |
1.203 ± 0.061 R_\odot |
|
|
1412.2757 🔍 (source)
|
integrated line flux |
|
0.16 Jy km s-1 |
|
|
1412.6117 🔍 (source)
|
peak-to-peak modulation in degree of linear polarization |
\Delta P |
0.000294 ± 3.5e-05 (ppm) |
|
|
1501.00790 🔍 (source)
|
emission line |
|
5.44 ± 0.05 keV |
|
|
1501.01638 🔍 (source)
|
Balmer line ratio H |
\alpha / H \beta |
7.5 ± 4.4 |
|
|
1501.02751 🔍 (source)
|
line-of-sight speeds |
|
52.0 |
Lower |
|
1501.05694 🔍 (source)
|
{ 17 } O isotopic line ratio |
|
350.0 |
Lower |
|
1501.05439 🔍 (source)
|
line |
|
1.6 km s-1 |
|
|
1501.06205 🔍 (source)
|
non-linear transverse motions perpendicular to |
|
-31.0 km s-1 |
|
|
1501.07289 🔍 (source)
|
H _ { 2 } /Br \gamma line ratio |
|
2.3 +1.7000000000000002-1.6999999999999997 |
|
|
1502.06771 🔍 (source)
|
broad-line H \alpha velocity width |
|
1020.0 km s-1 |
|
|
1503.00837 🔍 (source)
|
linear radius |
|
7.4e+16 ± 3000000000000000.0 cm |
|
|
1503.07164 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma _ { LOS } ^ { gas } |
127.0 ± 32.0 km s-1 |
|
|
1503.09037 🔍 (source)
|
column density line |
N ( H _ { 2 } ) |
1e+22 cm-2 |
|
|
1504.00262 🔍 (source)
|
linewidth |
|
1.3 km s-1 |
|
|
1504.01401 🔍 (source)
|
angle to the line-of-sight |
|
30.5 ± 2.5 |
|
|
1504.01734 🔍 (source)
|
line width |
|
386.0 ± 30.0 km s-1 |
|
|
1504.02270 🔍 (source)
|
average linear decay |
D |
-0.022 ± 0.002 |
|
|
1504.02889 🔍 (source)
|
line-of-sight integral of the dark matter density squared |
\log _ { 10 } ( J ) |
18.8 ± 0.6 GeV2 cm-5 |
|
|
1504.03697 🔍 (source)
|
line-of-sight velocity |
v _ { p , los } ^ { obs } |
-30.0 ± 30.0 km s-1 |
|
|
1504.03697 🔍 (source)
|
line-of-sight velocity |
v _ { p , los } |
-51.0 +17.0-14.0 km s-1 |
|
|
1504.05604 🔍 (source)
|
SFRs decline exponentially on quenching time-scales |
|
1.73 ± 0.25 Gyr |
|
|
1504.07723 🔍 (source)
|
narrow-line map the exponent |
|
-1.9 ± 0.1 |
|
|
1505.01593 🔍 (source)
|
rate of decline of the light curve |
( \Delta m _ { 15 } ( B ) |
1.6 ± 0.1 mag |
|
|
1505.02623 🔍 (source)
|
line strength |
|
0.8 Jy km s-1 |
|
|
1506.01547 🔍 (source)
|
line-of-sight velocity difference |
v _ { \perp } |
1880.0 ± 210.0 km s-1 |
|
|
1506.03089 🔍 (source)
|
linear distance |
|
21.58 ± 0.5 ± 1.19 Mpc |
|
|
1506.03089 🔍 (source)
|
linear distance |
|
22.49 ± 0.41 ± 1.24 Mpc |
|
|
1506.08034 🔍 (source)
|
line width |
|
0.54 km s-1 |
|
|
1506.08494 🔍 (source)
|
degree of linear polarization |
P |
1.0 ± 3.4 % |
|
|
1506.09002 🔍 (source)
|
width of the line |
EW |
230.0 eV |
|
|
1507.01945 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma |
17.0 km s-1 |
|
|
1507.03742 🔍 (source)
|
line mass |
|
26.0 ± 5.0 M_\odot pc-1 |
|
|
1507.04675 🔍 (source)
|
linear isospin splitting coefficient |
\Delta m _ { 1 } ^ { * } ( \rho _ { 0 } ) |
0.33 ± 0.16 |
|
|
1507.04675 🔍 (source)
|
linear isospin splitting coefficient |
\Delta m _ { 1 } ^ { * } ( \rho _ { 0 } ) |
0.27 ± 0.15 |
|
|
1507.07234 🔍 (source)
|
line-of-sight velocity dispersion |
|
1004.0 km s-1 |
|
|
1507.07480 🔍 (source)
|
snowline |
|
55.0 AU |
|
|
1508.00030 🔍 (source)
|
total projected linear size |
|
1.2 Mpc |
|
|
1508.00288 🔍 (source)
|
silicate crystalline mass fraction |
|
0.2 +0.3-0.1 |
|
|
1508.01679 🔍 (source)
|
linear relation |
\sigma { |
0.3 dex |
|
|
1508.03801 🔍 (source)
|
line opacity |
|
13.0 |
Upper |
|
1508.04982 🔍 (source)
|
linear scale |
|
66.0 kpc |
|
|
1508.04926 🔍 (source)
|
linear polarization |
|
-2.0 |
|
|
1508.06323 🔍 (source)
|
/H \alpha emission-line ratios |
|
0.93 ± 0.01 |
|
|
1508.06323 🔍 (source)
|
/H \alpha emission-line ratios |
|
0.66 ± 0.02 |
|
|
1508.06409 🔍 (source)
|
line-of-sight velocity dispersion |
\beta |
-0.24 |
|
|
1508.07685 🔍 (source)
|
line-of-sight column density |
|
9.02e+23 +1.2e+22-1.3e+22 cm-2 |
|
|
1509.02950 🔍 (source)
|
ICM line of sight peculiar velocity |
v _ { pec } |
-1040.0 +870.0-840.0 km s-1 |
|
|
1509.04277 🔍 (source)
|
line ratio |
L _ { HeII 4686 } / L _ { H \alpha } |
5.0 |
Lower |
|
1509.05431 🔍 (source)
|
decline indices |
|
-1.71 ± 0.02 |
|
|
1509.05431 🔍 (source)
|
decline indices |
|
-3.36 ± 0.14 |
|
|
1509.05626 🔍 (source)
|
baseline |
Tycho 2 |
100.0 yr |
|
|
1509.07147 🔍 (source)
|
median linear major axis FWHM |
|
4.2 ± 0.9 kpc |
|
|
1510.00015 🔍 (source)
|
linear ephemeris |
BJD _ { TDB } |
2456193.29157 ± 0.00021 |
|
|
1510.01414 🔍 (source)
|
temporal baseline |
|
4.2 yr |
|
|
1510.02106 🔍 (source)
|
emission line fluxes |
|
1.5e-17 erg s-1 cm-2 |
|
|
1510.03474 🔍 (source)
|
linearly polarized strain amplitude |
h _ { 0 } |
6.3e-25 |
|
|
1510.04816 🔍 (source)
|
line-of-sight velocity dispersion |
M _ { dyn } |
16000000000000.0 ± 3000000000000.0 M_\odot |
|
|
1510.05122 🔍 (source)
|
linear polarization degrees |
P _ { max } |
30.8 |
Upper |
|
1510.06234 🔍 (source)
|
X-ray line |
|
5.44 ± 0.05 keV |
|
|
1510.06351 🔍 (source)
|
linear size of the system |
|
2.3 pc |
|
|
1511.01243 🔍 (source)
|
linear mass ratio |
|
80.0 M_\odot pc-1 |
|
|
1511.02522 🔍 (source)
|
line-of-sight velocity |
\Delta V _ { rf } |
-1700.0 km s-1 |
|
|
1511.08330 🔍 (source)
|
projected linear distances |
|
324.0 kpc |
|
|
1511.09424 🔍 (source)
|
keV line |
|
9.199999999999999e+39 |
|
|
1511.09424 🔍 (source)
|
keV line |
|
1.6e+39 ph |
|
|
1512.00246 🔍 (source)
|
\sigma emission-line surface brightness |
|
1e-19 erg s-1 cm-2 |
|
|
1512.00325 🔍 (source)
|
keV line intensity amounts |
|
0.0027400000000000002 ± 0.00025 ph cm-2 s-1 |
|
|
1512.00325 🔍 (source)
|
keV line intensity |
|
0.00096 ± 7.000000000000001e-05 ph cm-2 s-1 |
|
|
1512.00325 🔍 (source)
|
line intensity |
|
0.00166 ± 0.00035 ph cm-2 s-1 |
|
|
1512.01050 🔍 (source)
|
line-of-sight length |
L _ { temp } |
20.0 kpc |
Upper |
|
1512.01350 🔍 (source)
|
gradual decline of the mass-loss rate |
|
1.6000000000000003e-05 M_\odot yr-1 |
|
|
1512.03995 🔍 (source)
|
post-maximum decline rate |
\Delta m _ { 15 } ( B ) |
0.92 ± 0.03 mag |
|
|
1512.09291 🔍 (source)
|
broad-line H |
\alpha / H \beta ratio |
2.72 ± 0.04 |
|
|
1601.00805 🔍 (source)
|
decline rate parameter |
\Delta m _ { 15 } ( B ) |
1.08 ± 0.03 |
|
|
1601.01353 🔍 (source)
|
degree of linear polarization |
p _ { \text { CL } 99.73 \% } |
2.4 |
Upper |
|
1601.02701 🔍 (source)
|
degree of linear polarisation |
|
17.01 ± 0.09 |
|
|
1601.02701 🔍 (source)
|
degree of linear polarisation |
|
18.81 ± 0.02 % |
|
|
1601.05425 🔍 (source)
|
line dispersion |
|
0.104 |
|
|
1601.05425 🔍 (source)
|
line dispersion |
\sigma _ { l } |
0.12 |
|
|
1602.01008 🔍 (source)
|
sightline |
\delta _ { b } |
550.0 ± 450.0 |
|
|
1602.01008 🔍 (source)
|
sightline |
L |
5.5 ± 4.5 Mpc |
|
|
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 |
|
2.3 ± 0.31 mJy |
|
|
1602.04596 🔍 (source)
|
linearly polarized flux density of the pulsar amounts |
|
1.5 ± 0.2 mJy |
|
|
1602.05262 🔍 (source)
|
line ratio |
|
0.71 ± 0.04 |
|
|
1602.06671 🔍 (source)
|
linear mass density |
|
1600.0 M_\odot pc-1 |
|
|
1603.00042 🔍 (source)
|
orbital period of this post snow-line planet |
|
1071.2323 ± 0.0006 day |
|
|
1603.00947 🔍 (source)
|
iron emission line |
E _ { rest } |
6.62 ± 0.04 keV |
|
|
1603.07084 🔍 (source)
|
post-maximum decline-rate |
\Delta m _ { 15 } ( B ) |
1.76 ± 0.15 mag |
|
|
1603.08520 🔍 (source)
|
CO snowline |
|
20.0 ± 3.0 |
|
|
1604.01096 🔍 (source)
|
radial projected linear distance |
|
62.0 pc |
|
|
1604.01987 🔍 (source)
|
linear size |
|
2.0 pc |
|
|
1604.03624 🔍 (source)
|
linewidth |
|
1.36 km s-1 |
|
|
1604.03624 🔍 (source)
|
linewidth |
|
0.3 km s-1 |
|
|
1604.03945 🔍 (source)
|
best-fit linear |
|
-76.0 ± 26.0 km s-1 |
|
|
1604.07433 🔍 (source)
|
line-of-sight field strength |
|
-687.0 ± 420.0 |
|
|
1605.00653 🔍 (source)
|
linear polarisation |
|
1.09 ± 0.27 |
|
|
1605.00653 🔍 (source)
|
linear polarisation |
|
0.9 ± 0.17 |
|
|
1605.01058 🔍 (source)
|
line-of-sight velocity dispersion |
v / \sigma |
5.0 ± 2.0 |
|
|
1605.06519 🔍 (source)
|
Lyman- \alpha  line flux |
|
1.06e-17 ± 1.9000000000000003e-18 erg s-1 cm-2 |
|
|
1605.08041 🔍 (source)
|
line-of-sight column density |
N _ { H } |
3e+24 cm-2 |
|
|
1605.09495 🔍 (source)
|
linear diameter |
|
0.65 +0.45000000000000007-0.45 pc |
|
|
1606.00528 🔍 (source)
|
H \alpha emission-line integrated velocity dispersions |
\sigma _ { int } |
140.0 ± 90.0 km s-1 |
|
|
1606.05649 🔍 (source)
|
line-of-sight column |
N _ { H } |
5.0000000000000006e+23 cm-2 |
|
|
1607.03915 🔍 (source)
|
median stellar mass of these LINERs |
|
65000000000.0 ± 5000000000.0 M_\odot |
|
|
1607.04351 🔍 (source)
|
linear radii |
R ( A ) |
0.165 ± 0.006 R_\odot |
|
|
1607.06322 🔍 (source)
|
baseline time-scale |
|
2.4 yr |
|
|
1607.06452 🔍 (source)
|
linear mass density |
|
4339.5 ± 4285.5 M_\odot pc-1 |
|
|
1607.08060 🔍 (source)
|
H \beta line dispersion |
|
3124.0 ± 302.0 km s-1 |
|
|
1607.08060 🔍 (source)
|
broad-line region |
f _ { BLR } |
6.3 ± 1.5 |
|
|
1608.01229 🔍 (source)
|
H \beta emission line |
\tau |
5.3 ± 1.8 day |
|
|
1608.01316 🔍 (source)
|
decline rate |
|
2.7 yr |
|
|
1608.01569 🔍 (source)
|
pre-flare baseline flux |
|
3.8999999999999995e-11 ph cm-2 s-1 |
|
|
1608.01930 🔍 (source)
|
exponential decline time scale |
|
96.0 ± 3.0 day |
|
|
1609.01992 🔍 (source)
|
linear source size |
|
1.4 kpc |
|
|
1609.03271 🔍 (source)
|
CO line width |
|
107.0 ± 20.0 km s-1 |
|
|
1609.04465 🔍 (source)
|
decline rate |
\Delta m _ { 15 } ( B ) |
1.35 ± 0.03 mag |
|
|
1609.04423 🔍 (source)
|
broad line flux |
|
4.75 ± 0.5 |
|
|
1609.05897 🔍 (source)
|
\sigma line flux |
|
4e-17 erg s-1 cm-2 |
|
|
1609.06487 🔍 (source)
|
broad emission line |
|
64.0 +52.0-15.0 km |
|
|
1609.09501 🔍 (source)
|
linear size of the source |
|
0.5 kpc |
|
|
1610.01498 🔍 (source)
|
sSFR of the entire cluster population declines |
|
0.48 ± 0.06 Gyr-1 |
Lower |
|
1610.01498 🔍 (source)
|
sSFR of the entire cluster population declines |
|
0.043 ± 0.009 Gyr-1 |
Upper |
|
1610.05548 🔍 (source)
|
line |
|
61.0 K |
|
|
1610.05548 🔍 (source)
|
line |
|
46.0 ± 9.0 K A |
|
|
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 |
|
|
1611.00006 🔍 (source)
|
luminosity of the line |
L _ { Br \alpha } |
3.3 |
|
|
1611.05516 🔍 (source)
|
line-of-sight peculiar velocities |
|
-66.0 km s-1 |
|
|
1611.07046 🔍 (source)
|
linear growth rate |
f \sigma _ { 8 } |
0.296 +0.075-0.078 |
|
|
1611.08446 🔍 (source)
|
line-of-sight velocities |
v _ { los } ( r _ { h } ) |
16.0 ± 3.0 km s-1 |
|
|
1611.09712 🔍 (source)
|
baseline energy resolution |
\sigma _ { E } |
91.0 eV |
|
|
1612.00447 🔍 (source)
|
/H \alpha emission line ratio |
\Delta log ( O/H ) / \Delta R= |
-0.026 ± 0.008 dex kpc-1 |
|
|
1612.06398 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma _ { v _ { los } } |
2.7 ± 0.3 km s-1 |
|
|
1612.09307 🔍 (source)
|
warm lines peak |
|
-14.0 km s-1 |
|
|
1701.00043 🔍 (source)
|
[ Nii ] 205 \mu m emission line ratio |
L _ { [ Cii ] } / L _ { [ Nii ] } |
55.0 |
Lower |
|
1701.01604 🔍 (source)
|
line ratios |
|
150000.0 ± 40000.0 cm-3 |
|
|
1701.01604 🔍 (source)
|
line ratios |
|
35.0 |
Lower |
|
1701.01604 🔍 (source)
|
line ratios |
|
63.0 K |
|
|
1701.01604 🔍 (source)
|
line ratios |
|
47.0 ± 5.0 K |
|
|
1701.01604 🔍 (source)
|
line ratios |
|
165000.0 ± 125000.0 cm-3 |
|
|
1701.03112 🔍 (source)
|
average strengths of these lines relative to the far-IR continuum |
|
0.00027 ± 0.0001 |
|
|
1701.03032 🔍 (source)
|
baseline length |
|
15.0 km |
|
|
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 |
|
0.00084 ± 0.00017 |
|
|
1701.04116 🔍 (source)
|
optical emission-line spectroscopic period |
|
98.413 ± 0.004 min |
|
|
1701.05283 🔍 (source)
|
linear size |
|
5.0 kpc |
|
|
1701.05690 🔍 (source)
|
linear growth factor |
\alpha |
1.125 ± 0.125 |
|
|
1701.07932 🔍 (source)
|
line intensity |
|
8.8e-07 ± 2.9e-07 ph cm-2 s-1 |
|
|
1701.08885 🔍 (source)
|
line polarisation |
p |
1.25 ± 0.25 |
|
|
1701.09026 🔍 (source)
|
time to decline two magnitudes |
|
2.1 |
Lower |
|
1702.01215 🔍 (source)
|
linear velocity |
|
1374.0 km s-1 |
|
|
1702.03852 🔍 (source)
|
] line flux |
F _ { [ CII ] } |
1.11 ± 0.1 Jy km s-1 |
|
|
1702.05107 🔍 (source)
|
isophotal area of emission lines |
|
1.2e-18 erg s-1 cm-2 kpc-2 |
|
|
1703.01394 🔍 (source)
|
line width |
|
0.85 |
|
|
1703.01394 🔍 (source)
|
linear mass of the filaments |
|
17.92 |
|
|
1703.02969 🔍 (source)
|
line luminosities |
L _ { HCN ( J = 2 \to 1 ) } ^ { \prime } |
9000000000.0 ± 3000000000.0 K km pc2 s-1 |
|
|
1703.02969 🔍 (source)
|
line luminosity ratio |
L _ { HCN } ^ { \prime } / L _ { CO } ^ { \prime } |
0.17 ± 0.07 |
|
|
1703.05764 🔍 (source)
|
FWHM line width |
|
750.0 ± 41.0 km s-1 |
|
|
1704.00516 🔍 (source)
|
linear size |
|
0.7 Mpc |
|
|
1704.05868 🔍 (source)
|
linear slope |
|
0.003 ± 0.0005 mag day-1 |
|
|
1704.06278 🔍 (source)
|
number of clumps per sightline |
f _ { c } |
1000.0 |
|
|
1704.08621 🔍 (source)
|
narrow line-widths |
|
2.5 ± 0.5 km s-1 |
|
|
1705.03370 🔍 (source)
|
age distribution of clusters declines |
dN / d \tau |
-0.3 |
Upper |
|
1705.06280 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma _ { v , los } |
160.0 km |
|
|
1705.07671 🔍 (source)
|
line-to-continuum ratio |
|
0.01 |
Lower |
|
1706.01366 🔍 (source)
|
line |
|
569.0 |
|
|
1706.01366 🔍 (source)
|
line |
|
3.6 ± 0.3 Jy km s-1 |
|
|
1706.03289 🔍 (source)
|
decline rate parameter |
\Delta m _ { 15 } ( B ) |
1.32 ± 0.1 |
|
|
1706.08903 🔍 (source)
|
linear velocity gradient |
|
0.2 km s-1 pc-1 |
|
|
1706.09944 🔍 (source)
|
linewidth |
\Delta v |
21.7 km s-1 |
|
|
1707.01518 🔍 (source)
|
linear ephemeris |
|
2457503.120049 ± 0.00019 |
|
|
1707.01518 🔍 (source)
|
linear ephemeris |
BJD _ { TDB } |
3.474107 ± 1.9e-06 |
|
|
1707.04363 🔍 (source)
|
CO line flux ( dust flux density |
|
71.0 ± 7.0 mJy |
|
|
1707.04363 🔍 (source)
|
CO line flux ( dust flux density |
|
180.0 ± 18.0 Jy km s-1 |
|
|
1707.07003 🔍 (source)
|
line luminosity |
|
2.7e+42 ± 1e+41 erg s-1 |
|
|
1707.07077 🔍 (source)
|
line |
|
8.3 ± 0.9 |
|
|
1708.00473 🔍 (source)
|
line-force parameters |
|
1.5 |
Lower |
|
1708.01605 🔍 (source)
|
H \alpha narrow-line full-width |
W _ { NL } |
54.8 ± 1.8 km s-1 |
|
|
1708.02727 🔍 (source)
|
ratio of the separation to the snow-line distance |
a _ { \perp } / a _ { sl } |
15.4 |
|
|
1708.03158 🔍 (source)
|
line-of-sight velocity |
|
38.3 ± 5.1 km s-1 |
|
|
1708.08026 🔍 (source)
|
linear polarization |
|
8.7 |
|
|
1708.08026 🔍 (source)
|
linear polarization |
|
10.3 |
|
|
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 |
|
|
1708.08928 🔍 (source)
|
projected linear size |
|
1.3 Mpc |
|
|
1708.08635 🔍 (source)
|
linear size of of this standard ruler |
l _ { m } |
11.03 ± 0.25 pc |
|
|
1709.01603 🔍 (source)
|
linear polarization degree |
P _ { max } |
7.32 ± 0.25 % |
|
|
1709.04084 🔍 (source)
|
mean line widths |
|
0.7 ± 0.2 km s-1 |
|
|
1709.06096 🔍 (source)
|
line–of–sight velocity difference |
|
560.0 km s-1 |
|
|
1709.06564 🔍 (source)
|
spectral line broadening |
|
150.0 ± 50.0 km |
|
|
1709.06564 🔍 (source)
|
spectral line broadening |
\sigma _ { v, { los } |
-1.0 |
|
|
1709.07694 🔍 (source)
|
2 } CO line ratios |
|
62.0 ± 2.0 K |
|
|
1709.08926 🔍 (source)
|
neutral iron line |
|
5247.1 |
|
|
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 |
|
|
1710.00129 🔍 (source)
|
H \beta line dispersion |
\sigma _ { line } |
668.0 ± 44.0 km s-1 |
|
|
1710.03002 🔍 (source)
|
3 \sigma emission line |
|
3.1e-19 erg s-1 cm-2 |
|
|
1710.05303 🔍 (source)
|
linear obscuration |
|
0.12 |
|
|
1710.05849 🔍 (source)
|
linear optical polarization |
P |
0.5 ± 0.07 |
|
|
1710.05856 🔍 (source)
|
line-of-sight peculiar velocity |
v _ { pec } |
307.0 ± 230.0 km s-1 |
|
|
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 |
|
|
1711.00628 🔍 (source)
|
intrinsic decline rate parameter |
\Delta { m _ { 15 } ( B ) } _ { true } |
1.27 ± 0.05 |
|
|
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 |
|
1711.10012 🔍 (source)
|
line ratios |
|
4450000.0 +3850000.0000000005-3850000.0 cm-3 |
|
|
1711.11449 🔍 (source)
|
emission-line flux ratio |
O _ { 32 } |
11.5 |
|
|
1712.03511 🔍 (source)
|
sight line of the background quasar |
z _ { q } |
1.5266 |
|
|
1712.03958 🔍 (source)
|
line of sight to |
|
28.0 day |
Upper |
|
1712.04540 🔍 (source)
|
/CO line ratio |
|
0.19 ± 0.07 |
|
|
1712.05054 🔍 (source)
|
linear size |
|
0.22 pc |
|
|
1801.01264 🔍 (source)
|
line-of-sight velocity |
|
-129.0 ± 3.0 km s-1 |
|
|
1801.02141 🔍 (source)
|
line-of-sight magnetic field strengths |
|
-2.0 |
Lower |
|
1801.02141 🔍 (source)
|
line-of-sight magnetic field strengths |
|
-5.0 m |
Upper |
|
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 |
|
|
1801.08897 🔍 (source)
|
crystalline water ice |
{ E _ { des } |
4930.0 K |
|
|
1802.03447 🔍 (source)
|
well-delineated decline |
A ( Li ) |
1.25 |
|
|
1802.04432 🔍 (source)
|
line-of-sight velocity |
Fe |
10747.0 |
|
|
1802.07043 🔍 (source)
|
mean line width |
|
0.71 km s-1 |
|
|
1802.08257 🔍 (source)
|
fractional linear polarization |
| Q / I | |
0.19 ± 0.02 |
|
|
1802.09280 🔍 (source)
|
total integrated line flux |
|
730.0 ± 73.0 mJy km s-1 |
|
|
1803.04854 🔍 (source)
|
line-of-sight rotation velocity |
|
71.0 km s-1 |
|
|
1804.01099 🔍 (source)
|
linear size |
|
550.0 kpc |
|
|
1804.01828 🔍 (source)
|
fluorescent line |
|
6.4 keV |
|
|
1804.01789 🔍 (source)
|
spectral lines Si |
|
1082.7 nm |
|
|
1804.01789 🔍 (source)
|
spectral lines Si |
|
1083.0 nm |
|
|
1804.04666 🔍 (source)
|
average lifetime of a BAL along our line |
sight |
90.0 ± 10.0 yr |
|
|
1804.04666 🔍 (source)
|
rest-frame time baseline |
|
0.28 |
Lower |
|
1804.04666 🔍 (source)
|
rest-frame time baseline |
|
4.9 yr |
|
|
1804.05600 🔍 (source)
|
linear size |
|
0.3 pc |
|
|
1804.07765 🔍 (source)
|
line-of-nodes position angle |
\theta |
149.23 +6.43-8.35 day |
|
|
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 |
|
|
1805.01008 🔍 (source)
|
decline of the accretion fraction |
|
6.0 ± 4.0 Myr |
|
|
1805.02721 🔍 (source)
|
declines |
|
-0.01 ± 0.03 dex |
|
|
1805.03670 🔍 (source)
|
line masses of the two filaments |
|
120.0 M_\odot pc-1 |
|
|
1805.04079 🔍 (source)
|
line-of-sight rotation |
V _ { rot } |
-206.0 ± 86.0 |
|
|
1805.09932 🔍 (source)
|
rapid-decline type novae |
M _ { WD } |
1.3775 +0.007500000000000062-0.00749999999999984 M_\odot |
|
|
1806.01474 🔍 (source)
|
line-emitting gas temperature |
|
2300000.0 K |
|
|
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 |
|
|
1806.10150 🔍 (source)
|
two X-ray line peaks |
\Delta v |
0.06 c |
|
|
1807.00706 🔍 (source)
|
optical light-curve decline |
t _ { 2 } |
2.9 day |
Upper |
|
1807.00657 🔍 (source)
|
line-of-sight stellar rotation axis inclination |
|
162.4 +3.8-4.3 day |
|
|
1807.00657 🔍 (source)
|
line-of-sight stellar rotation axis inclination |
|
18.6 +4.3-3.8 day |
|
|
1807.04029 🔍 (source)
|
line |
|
80.0 |
|
|
1807.04029 🔍 (source)
|
line |
|
6.4 |
Upper |
|
1807.05309 🔍 (source)
|
line luminosity |
|
8e+35 ± 1e+35 erg s-1 |
|
|
1807.05994 🔍 (source)
|
line of sight |
|
2.3 km s-1 |
Upper |
|
1807.07702 🔍 (source)
|
linear phase |
\beta _ { i } |
1.0 |
Lower |
|
1807.08895 🔍 (source)
|
line luminosity |
L _ { CO ( 3 - 2 ) } ^ { \prime } |
55300000000.0 ± 6899999999.999999 K km pc %2 s-1 |
|
|
1808.04133 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma _ { V } |
1100.0 km s-1 |
|
|
1808.04372 🔍 (source)
|
total CO line brightness |
|
0.45 ± 0.2 K |
|
|
1808.06311 🔍 (source)
|
line-of-sight extinction |
A _ { v } |
1.9 ± 0.6 mag |
|
|
1808.09373 🔍 (source)
|
line-of-sight velocity |
v |
0.3 c |
|
|
1809.01053 🔍 (source)
|
transverse line-of-sight separation |
|
0.7 kpc |
|
|
1809.01288 🔍 (source)
|
snowline |
a _ { sl } |
2.1 AU |
|
|
1809.05269 🔍 (source)
|
broad line region of size |
|
0.08 pc |
|
|
1809.07598 🔍 (source)
|
line mass |
|
38.5 ± 2.5 M_\odot pc-1 |
|
|
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 |
|
|
1810.03693 🔍 (source)
|
core line depth |
\Delta F |
0.007 |
Upper |
|
1810.06179 🔍 (source)
|
line intensity ratio |
|
1.2 ± 0.4 |
|
|
1810.08507 🔍 (source)
|
line width |
\Delta { v _ { FWHM } } |
5.0 km s-1 |
Upper |
|
1811.00412 🔍 (source)
|
line flux |
|
9.5 ± 3.6 mJy km s-1 |
|
|
1811.03627 🔍 (source)
|
number of detectable line-of-sight haloes rises |
\mu _ { l } |
9.0 ± 3.0 |
|
|
1811.05986 🔍 (source)
|
line width ( Doppler parameter |
b |
3.2 km s-1 |
Upper |
|
1811.07815 🔍 (source)
|
fractional linear polarization |
GHz |
0.5 +0.19999999999999996-0.2 % |
|
|
1812.02645 🔍 (source)
|
line-of-sight peculiar velocity |
v _ { pec } |
650.0 km s-1 |
|
|
1901.00906 🔍 (source)
|
maximum baseline length |
|
25.0 km |
|
|
1901.00900 🔍 (source)
|
linear |
M _ { vir } |
5000000000.0 M_\odot N |
|
|
1901.01353 🔍 (source)
|
post-maximum decline rate |
\Delta m _ { 15 } ( B ) |
1.0 ± 0.05 mag |
|
|
1901.01707 🔍 (source)
|
super-linear Kennicutt-Schmidt relation |
n _ { KS } |
1.47 |
|
|
1901.02877 🔍 (source)
|
decline |
|
0.6 +0.54-1.54 Gyr |
|
|
1901.03441 🔍 (source)
|
maximum degree of linear polarization |
|
1.16 ± 0.06 % |
|
|
1901.04488 🔍 (source)
|
line-of-sight velocity dispersion of these |
\sigma _ { group } |
230.0 km s-1 |
|
|
1901.04488 🔍 (source)
|
line-of-sight velocity offset |
\Delta v _ { group } |
181.0 km s-1 |
|
|
1901.07108 🔍 (source)
|
Fe K \alpha emission line |
EW _ { \textnormal { rest } |
0.5 |
Lower |
|
1901.07586 🔍 (source)
|
line width |
|
3.2 km s-1 |
|
|
1901.08020 🔍 (source)
|
line |
|
33.0 |
|
|
1902.01863 🔍 (source)
|
line-of-sight column densities |
N _ { CO } |
2e+17 +3e+17-1e+17 |
|
|
1902.02251 🔍 (source)
|
prominent H \alpha emission line |
L _ { H \alpha } |
2.2e+38 ± 2.0000000000000001e+37 erg s-1 |
|
|
1902.02720 🔍 (source)
|
iceline |
R _ { CO } |
30.0 |
|
|
1902.05007 🔍 (source)
|
CO line width |
\sigma _ { HWHM } |
4.6 ± 0.9 km s-1 |
|
|
1902.05007 🔍 (source)
|
H i line width |
\sigma _ { HWHM } |
6.6 ± 0.1 km s-1 |
|
|
1902.05007 🔍 (source)
|
median line width ratio of the line-of-sight line widths |
|
0.56 ± 0.01 |
|
|
1902.05822 🔍 (source)
|
temperature line ratio |
|
0.5 |
|
|
1902.05960 🔍 (source)
|
\sigma line flux |
|
3.1e-19 erg s-1 cm-2 |
|
|
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 |
|
|
1904.03095 🔍 (source)
|
inclination to the line of sight |
i |
27.2 ± 0.7 |
|
|
1904.07306 🔍 (source)
|
line-of-sight velocity |
\log ( \tau ) |
0.0 |
|
|
1904.07261 🔍 (source)
|
linear polarization |
|
0.87 ± 0.13 |
|
|
1904.07261 🔍 (source)
|
linear polarization |
\Pi |
0.6 ± 0.19 |
|
|
1904.08111 🔍 (source)
|
linear polarization degree in the millimeter band |
|
0.27 ± 0.04 |
|
|
1904.08946 🔍 (source)
|
H \beta broad line region ( BLR ) radius |
R _ { \text { H } \beta, \text { BLR } |
26.0 |
|
|
1904.10356 🔍 (source)
|
line peak velocities |
v _ { LSR } |
10.7 ± 0.2 km s-1 |
|
|
1904.10259 🔍 (source)
|
total linear size |
|
4.0 |
|
|
1904.11028 🔍 (source)
|
K \alpha line |
EW |
2.3 ± 0.3 keV |
|
|
1905.00145 🔍 (source)
|
H \alpha line-of-sight velocity dispersion |
\sigma _ { line } |
426.0 ± 1.0 km s-1 |
|
|
1905.01315 🔍 (source)
|
optical emission lines |
|
94.0 ± 4.0 c-1 |
|
|
1905.01245 🔍 (source)
|
average line-of-sight |
|
1.1 ± 0.6 km s-1 |
|
|
1905.01800 🔍 (source)
|
radial velocity of the radio recombination line |
|
10.0 km s-1 |
|
|
1905.02035 🔍 (source)
|
line-of-sight velocities range |
|
12.5 ± 7.5 km s-1 |
|
|
1905.05509 🔍 (source)
|
snow line distance |
a _ { snow } |
2.7 |
|
|
1905.07950 🔍 (source)
|
line width |
|
2.5 km s-1 |
|
|
1905.09285 🔍 (source)
|
line-of-sight magnetic strengths |
B _ { \parallel, \text { |
-15.0 |
|
|
1905.09496 🔍 (source)
|
cyclotron line energy |
E _ { cyc } |
47.7 ± 0.8 keV |
|
|
1905.11156 🔍 (source)
|
linear radius |
|
1.5 ± 0.04 R_\odot |
|
|
1906.03268 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma |
7.8 +5.2-2.2 km s-1 |
|
|
1906.06790 🔍 (source)
|
non-linear parameter |
| f _ { NL } | |
1.0 |
Upper |
|
1906.06889 🔍 (source)
|
line-of-sight velocities |
|
150.0 |
|
|
1906.06889 🔍 (source)
|
line-of-sight velocities |
v - v _ { sys } |
200.0 km s-1 |
Upper |
|
1906.09760 🔍 (source)
|
cumulative linear mass |
|
12.0 |
|
|
1906.11106 🔍 (source)
|
ortho-H _ { 2 } O line flux |
|
7.5e-20 W m-2 |
|
|
1906.11106 🔍 (source)
|
ortho-H _ { 2 } O line flux |
|
1.1999999999999999e-19 W m-2 |
|
|
1907.03854 🔍 (source)
|
line emission |
|
661.0 km s-1 |
|
|
1907.03524 🔍 (source)
|
line masses |
|
36.0 ± 24.0 M_\odot pc-1 |
|
|
1907.10078 🔍 (source)
|
stellar mean line profiles |
|
1.22 ± 0.02 |
|
|
1908.03232 🔍 (source)
|
linear radius |
|
2.0 ± 0.03 R_\odot |
|
|
1908.06080 🔍 (source)
|
projected linear size |
|
1.1 Mpc |
|
|
1908.06538 🔍 (source)
|
line flux ratio |
F ( B ) / F ( N ) |
1.35 |
|
|
1908.08293 🔍 (source)
|
emission line |
|
0.66 ± 0.01 keV |
|
|
1908.09269 🔍 (source)
|
line-of-sight velocity |
|
85.0 km s-1 |
|
|
1908.10885 🔍 (source)
|
linear polarization |
|
66.0 +26.0-27.0 |
|
|
1909.04545 🔍 (source)
|
rapid decline rate |
|
0.48 ± 0.03 mag day-1 |
|
|
1909.05267 🔍 (source)
|
decline rate |
\Delta m _ { 15 } ( B ) |
1.77 mag |
|
|
1910.05068 🔍 (source)
|
Paschen emission lines |
|
260.0 ± 20.0 km s-1 |
|
|
1910.05431 🔍 (source)
|
line flux |
F _ { H \sc i } |
2.0 Jy km s-1 |
|
|
1910.05687 🔍 (source)
|
linear polarization upper |
| \Pi | |
12.0 |
Upper |
|
1910.11624 🔍 (source)
|
optical linear polarisation |
P _ { V } |
8.0 |
|
|
1911.00380 🔍 (source)
|
average line depth |
|
2.02 ± 0.17 |
|
|
1911.00380 🔍 (source)
|
average line depth |
|
0.78 ± 0.04 |
|
|
1911.03502 🔍 (source)
|
off-axis linear polarisation leakage |
|
1.4 |
Upper |
|
1911.07713 🔍 (source)
|
line-of-sight radial velocity amplitude |
|
12.0 ± 10.0 km s-1 |
|
|
1911.11953 🔍 (source)
|
line-of-sight separation |
D _ { LS } |
1.21 +0.96-0.63 kpc |
|
|
1911.11399 🔍 (source)
|
decline rate in the impact parameter |
d b / d t |
-0.011 yr-1 |
|
|
1911.13108 🔍 (source)
|
line-of-sight velocity increase |
|
480.0 ± 210.0 |
|
|
1911.13081 🔍 (source)
|
linear rotation |
|
-5.0 +1.6-1.9 km s-1 |
|
|
1912.06565 🔍 (source)
|
line ratio |
|
0.58 |
Lower |
|
1912.06565 🔍 (source)
|
line ratio |
r _ { 21 } |
0.15 |
|
|
2001.01853 🔍 (source)
|
line luminosity ratio |
L _ { [ O _ { I \hskip { -1.0 pt } I |
10.0 |
Lower |
|
2001.04581 🔍 (source)
|
line-of-sight accelerations |
|
4.4 km s-1 yr-1 |
|
|
2001.04707 🔍 (source)
|
line-of-sight velocity dispersion |
\sigma _ { v } |
1300.0 km s-1 |
|
|
2001.08221 🔍 (source)
|
H \alpha line width |
|
1950.0 km F W H s-1 |
|
|
2001.08900 🔍 (source)
|
median column density of LINERs |
|
22.68 ± 0.75 |
|
|
2001.10103 🔍 (source)
|
mean field line length |
L |
135.0 ± 35.0 Mm |
|
|
2001.10546 🔍 (source)
|
linear polarization |
| Q / I | |
0.12 ± 0.04 |
Lower |
|
2002.00393 🔍 (source)
|
post-maximum decline rate |
\Delta m _ { 15 } ( g ) |
1.66 ± 0.15 mag |
|
|
2002.04816 🔍 (source)
|
line width |
|
343.0 ± 40.0 km s-1 |
|
|
2002.05806 🔍 (source)
|
average line velocity |
|
-230.0 km s-1 |
|
|
2002.06207 🔍 (source)
|
line-of-sight velocity dispersion |
z _ { mean } |
2.23224 ± 0.00101 |
|
|
2002.08028 🔍 (source)
|
the H \alpha emission line |
|
55.0 +27.0-31.0 |
|
|
2002.08028 🔍 (source)
|
the H \alpha emission line |
|
122.0 +33.0-67.0 min |
Upper |
|
2002.08028 🔍 (source)
|
the H \alpha emission line |
|
49.0 +15.0-14.0 |
|
|
2002.08516 🔍 (source)
|
total line-of-sight CGM metallicity |
[ Si / H ] |
-1.5 +0.4-0.3 |
|
|
2002.08379 🔍 (source)
|
line contrast |
Na D _ { 1 } |
1.09 ± 0.16 % |
|
|
2002.09829 🔍 (source)
|
line ratios |
|
0.9 |
Lower |
|
2003.01397 🔍 (source)
|
broad line region luminosity |
L _ { BLR } |
1.4999999999999999e+46 erg s-1 |
|
|
2003.07576 🔍 (source)
|
line-of-sight velocity |
|
-20.0 km s-1 |
|
|
2004.04952 🔍 (source)
|
intrinsic linear polarization of the system |
|
275.3 ± 31.9 |
|
|
2004.06730 🔍 (source)
|
linearly polarized intensity |
P |
97.2 Jy |
Upper |
|
2004.06730 🔍 (source)
|
linear fractional polarization |
\Pi _ { L } |
0.3 |
Upper |
|
2004.08363 🔍 (source)
|
effective linear equation |
H _ { 0 } + 30.93 w |
36.47 |
Upper |
|
2004.13065 🔍 (source)
|
line-of-sight gas density |
|
2.61 |
Upper |
|
2004.13756 🔍 (source)
|
linear size of this component |
|
4.0 kpc |
|
|
2005.03901 🔍 (source)
|
Balmer lines |
\langle f _ { H \beta } \rangle |
0.43 ± 0.2 |
|
|
2005.09653 🔍 (source)
|
line brightness temperature ratio |
r _ { |
31.0 |
|
|
2005.10001 🔍 (source)
|
lag of the broad He ii line |
|
26.0 ± 8.0 day |
|
|
2006.04168 🔍 (source)
|
mean line width |
\Delta \upsilon |
0.39 km F W H s-1 |
|
|
2006.10028 🔍 (source)
|
linear size |
\alpha |
-1.5 |
Upper |
|
2006.11543 🔍 (source)
|
line-of-sight |
M _ { 200 } |
1600000000000000.0 M_\odot |
Upper |
|
2007.08221 🔍 (source)
|
line-of-sight magnetic |
B _ { || } |
26.0 ± 5.0 |
|
|
2007.09009 🔍 (source)
|
linear growth rate of structure |
f \sigma _ { 8 } ( z _ { eff } ) |
0.35 ± 0.1 |
|
|
2007.09008 🔍 (source)
|
normalisation of the linear power spectrum |
D _ { H } ( z _ { eff } ) / r _ { drag } |
20.0 +2.4-2.2 |
|
|
2007.08999 🔍 (source)
|
linear growth rate of structure |
f ( z _ { eff } ) \sigma _ { 8 } ( z _ { eff } ) |
0.476 ± 0.047 |
|
|
2007.14289 🔍 (source)
|
baseline energy resolution |
\sigma _ { E } |
4.92 ± 0.01 eV |
|
|
2007.13337 🔍 (source)
|
brightness decline |
t _ { 2 , V } |
3.0 |
|