|
astro-ph/9705018 🔍 (source)
|
bolometric luminosity ratio |
\log ( L _ { x } / L _ { bol } ) |
-3.1 ± 0.14 |
|
|
astro-ph/9811423 🔍 (source)
|
the mass-to-luminosity ratio of visible stellar population |
M / L _ { B } |
4.0 ± 1.4 |
|
|
astro-ph/9907384 🔍 (source)
|
Volume galaxies their total mass-to- luminosity ratio |
|
3.0 M_\odot L_\odot-1 |
|
|
astro-ph/0008513 🔍 (source)
|
luminosity ratio |
SSRQs ( LN/LG |
3.8 ± 3.2 |
|
|
astro-ph/0010148 🔍 (source)
|
virial mass-to-luminosity ratio |
|
56.0 M_\odot L_\odot-1 |
|
|
astro-ph/0105015 🔍 (source)
|
luminosity ratio |
log ( L _ { x } / L _ { bol } ) |
-7.0 |
|
|
astro-ph/0201245 🔍 (source)
|
bulge to disk luminosity ratio |
|
0.6 |
Lower |
|
astro-ph/0201245 🔍 (source)
|
bulge to disk luminosity ratio |
L _ { bulge } / L _ { disk } |
22.0 |
|
|
astro-ph/0202307 🔍 (source)
|
logarithm of the bulge-to-disk luminosity ratio |
\log ( B / D ) |
0.22 |
|
|
astro-ph/0210360 🔍 (source)
|
luminosity ratio |
\log { ( L _ { X } / L _ { bol } ) } |
-6.28 |
Upper |
|
astro-ph/0210414 🔍 (source)
|
orbital mass-to-luminosity ratio |
|
88.0 M_\odot L_\odot-1 |
|
|
astro-ph/0303025 🔍 (source)
|
X-ray to bolometric luminosity ratio |
L _ { X } / L _ { bol } |
10.0 |
Lower |
|
astro-ph/0405077 🔍 (source)
|
luminosity ratios |
log ( L _ { X } / L _ { bol } ) |
-2.07 |
|
|
astro-ph/0409711 🔍 (source)
|
luminosity ratio |
|
0.2 |
|
|
astro-ph/0410458 🔍 (source)
|
X-ray to optical luminosity ratio |
L _ { X } / L _ { B } |
170.0 |
Lower |
|
astro-ph/0501008 🔍 (source)
|
mass to luminosity ratio |
|
2.5 ± 0.5 |
|
|
astro-ph/0506608 🔍 (source)
|
X-ray to far-infrared luminosity ratio |
L _ { X } \over { L _ { FIR } } |
0.004 |
|
|
astro-ph/0603252 🔍 (source)
|
nucleus-to-galaxy luminosity ratio |
\langle \log _ { 10 } \eta \rangle |
-2.49 ± 0.09 dex |
|
|
astro-ph/0604351 🔍 (source)
|
total mass-to-infrared-luminosity ratio |
|
52.0 M_\odot L_\odot-1 |
|
|
astro-ph/0604351 🔍 (source)
|
total mass-to-infrared-luminosity ratio |
|
49.0 M_\odot L_\odot-1 |
|
|
astro-ph/0605437 🔍 (source)
|
HCO ^ { + } /CO luminosity ratio |
|
0.08 |
|
|
astro-ph/0605437 🔍 (source)
|
HCO ^ { + } /HCN luminosity ratio |
|
0.8 |
|
|
astro-ph/0606543 🔍 (source)
|
luminosity ratio |
L _ { X } / L _ { K } |
0.0008 |
|
|
astro-ph/0611599 🔍 (source)
|
luminosity ratio |
L _ { pwn } / L _ { psr } ^ { nonth } |
4.0 |
|
|
astro-ph/0612443 🔍 (source)
|
luminosity ratios |
L / L _ { Edd } |
0.003 |
Upper |
|
astro-ph/0612546 🔍 (source)
|
bulge to disk luminosity ratio |
b / d ) |
1.1 |
|
|
0705.3338 🔍 (source)
|
CO/CN luminosity ratio |
|
9.3 ± 1.9 |
|
|
0705.3338 🔍 (source)
|
HCN/CN luminosity ratio |
|
0.95 ± 0.15 |
|
|
0708.3870 🔍 (source)
|
bulge-to-total luminosity ratio |
|
0.05 |
|
|
0709.1737 🔍 (source)
|
bulge-to-total luminosity ratio |
B / T ) |
0.2 |
Lower |
|
0710.4525 🔍 (source)
|
HCN/CO luminosity ratio |
L _ { HCN } ^ { \prime } / L _ { CO } ^ { \prime } |
0.13 |
Upper |
|
0711.0238 🔍 (source)
|
bulge-to-total luminosity ratio |
B / T ) |
0.2 |
Lower |
|
0810.0720 🔍 (source)
|
typical infrared to X-ray luminosity ratio |
|
4.8e-06 ± 1.1e-06 Mpc-3 |
|
|
0812.0984 🔍 (source)
|
luminosity ratio |
R _ { ir / x } |
30.0 |
Upper |
|
0901.0909 🔍 (source)
|
bolometric luminosity ratios |
L _ { IR } / L _ { \star } |
0.0079 |
|
|
0901.3378 🔍 (source)
|
Eddington luminosity ratios |
|
0.7 |
Upper |
|
0907.1198 🔍 (source)
|
luminosity ratio |
L _ { p } / L _ { s } |
0.5 ± 0.15 |
|
|
0909.3842 🔍 (source)
|
X-ray luminosity ratios |
|
4.7 +10.2-2.0 |
|
|
0909.3842 🔍 (source)
|
X-ray luminosity ratios |
L _ { IR } / L _ { X } |
12.7 +7.1-2.6 |
|
|
1002.3354 🔍 (source)
|
X/K luminosity ratios |
|
2.45e+27 +7.500000000000001e+26-7.500000000000002e+26 erg s-1 |
|
|
1002.3740 🔍 (source)
|
luminosity ratio |
|
50.05 +49.95-49.949999999999996 GeV |
Lower |
|
1005.1647 🔍 (source)
|
pseudobulge-to-total luminosity ratio of the galaxy |
PB / T |
0.06 ± 0.01 |
|
|
1006.2383 🔍 (source)
|
luminosity ratio |
L _ { 2 } / L _ { 1 } |
0.2 |
|
|
1006.3273 🔍 (source)
|
H i mass to luminosity ratio |
M _ { H I } / L _ { B } |
1.6 |
|
|
1006.3438 🔍 (source)
|
luminosity ratio |
HCO ^ { + } |
0.015 |
|
|
1006.3438 🔍 (source)
|
luminosity ratio |
|
0.0034 |
|
|
1006.3438 🔍 (source)
|
luminosity ratio |
|
0.004900000000000001 |
|
|
1006.3438 🔍 (source)
|
luminosity ratio |
|
0.035 |
|
|
1008.1578 🔍 (source)
|
CII ] -to-FIR luminosity ratio |
|
0.00053 ± 8e-05 |
|
|
1009.0172 🔍 (source)
|
luminosity ratio |
L _ { flare } / L _ { steep } |
4.7 |
|
|
1102.0798 🔍 (source)
|
Eddington luminosity ratio |
\lambda _ { crit } |
0.01 |
|
|
1102.1837 🔍 (source)
|
mass to luminosity ratio |
M / L |
300.0 M_\odot L_\odot-1 |
|
|
1104.4116 🔍 (source)
|
luminosity ratios |
r _ { |
31.0 |
|
|
1108.5897 🔍 (source)
|
X-ray-to-bolometric luminosity ratio |
log L _ { X } / L _ { bol } |
-0.1 +0.2-0.3 |
|
|
1111.6774 🔍 (source)
|
MIR-to-X luminosity ratio |
|
7.5 ± 2.5 |
|
|
1203.2084 🔍 (source)
|
Eddington luminosity ratio |
L _ { bol } / L _ { Edd } |
0.01 |
|
|
1205.3498 🔍 (source)
|
luminosity ratio |
L _ { [ CII ] } / L _ { FIR } |
0.0008300000000000001 ± 0.00012 |
|
|
1206.1346 🔍 (source)
|
luminosity ratios |
\log ( L _ { 0.1 - 100 GeV } / L _ { 1.4 GHz } ) |
1.7 ± 0.1 (() s |
|
|
1209.2414 🔍 (source)
|
IR-to-UV luminosity ratio |
IRX _ { z |
7.1 ± 1.1 |
|
|
1302.4154 🔍 (source)
|
luminosity ratios |
|
0.0004 +0.00010999999999999996-0.00011000000000000002 |
|
|
1303.2477 🔍 (source)
|
orbital mass-to-luminosity ratio |
|
49.0 M_\odot L_\odot-1 |
|
|
1303.2477 🔍 (source)
|
orbital mass-to-luminosity ratio |
|
0.22 |
|
|
1305.3701 🔍 (source)
|
mass–luminosity ratio |
M / L _ { B } |
30.0 |
|
|
1307.0335 🔍 (source)
|
luminosity ratio |
L ( CO ) / L _ { FIR } |
0.0002 ± 0.0001 |
|
|
1307.7061 🔍 (source)
|
total stellar luminosity ratio |
L _ { X } / L _ { Bol } |
1e-05 |
|
|
1402.4811 🔍 (source)
|
bolometric luminosity ratio |
|
8.5 ± 6.5 % |
|
|
1506.01425 🔍 (source)
|
luminosity ratio |
r _ { 8 - 7 / 5 - 4 } |
0.3 ± 0.04 |
|
|
1511.05069 🔍 (source)
|
luminosity ratio |
M _ { HI } / L _ { V } |
0.026000000000000002 M_\odot L_\odot-1 |
Upper |
|
1512.05907 🔍 (source)
|
total mass-to-blue luminosity ratio |
|
162.0 M_\odot L_\odot-1 |
|
|
1512.08793 🔍 (source)
|
luminosity ratio |
L _ { B } / L _ { A } |
0.81 +0.1299999999999999-0.13 |
|
|
1601.06783 🔍 (source)
|
luminosity ratio |
|
0.23 |
|
|
1602.07289 🔍 (source)
|
radio to X-ray luminosity ratio |
log ( L _ { R } / L _ { X } ) |
-5.0 |
|
|
1605.03194 🔍 (source)
|
Ly \alpha to X-ray luminosity ratio |
L _ { Ly \alpha } / L _ { X } |
505.0 ± 495.0 |
Lower |
|
1605.03194 🔍 (source)
|
Ly \alpha to X-ray luminosity ratio |
|
0.3 |
|
|
1607.03038 🔍 (source)
|
dust-to-star luminosity ratio |
|
4.599999999999999e-06 ± 4e-07 |
|
|
1610.05324 🔍 (source)
|
luminosity ratio |
B / T |
0.2 |
Lower |
|
1611.04532 🔍 (source)
|
X-ray to gamma-ray luminosity ratio |
L _ { X } / L _ { \gamma } |
0.0005 |
Upper |
|
1702.07523 🔍 (source)
|
luminosity ratio |
K _ { ep } |
0.008 |
Lower |
|
1703.02969 🔍 (source)
|
line luminosity ratio |
L _ { HCN } ^ { \prime } / L _ { CO } ^ { \prime } |
0.17 ± 0.07 |
|
|
1705.09672 🔍 (source)
|
photon luminosity ratios |
|
0.012 |
|
|
1705.09672 🔍 (source)
|
photon luminosity ratios |
|
0.12 |
|
|
1807.03313 🔍 (source)
|
infrared-to-radio luminosity ratio |
q |
1.8 |
|
|
1808.10331 🔍 (source)
|
luminosity ratio |
|
2.0 |
|
|
1903.11234 🔍 (source)
|
luminosity ratio |
L _ { [ OIII ] } / L _ { [ NII ] } |
6.4 ± 2.2 |
|
|
1904.13155 🔍 (source)
|
mean orbital-mass-to-K-band luminosity ratio |
|
20.0 ± 3.0 |
|
|
2001.01853 🔍 (source)
|
line luminosity ratio |
L _ { [ O _ { I \hskip { -1.0 pt } I |
10.0 |
Lower |
|
2002.00961 🔍 (source)
|
[ CII ] -to-FIR luminosity ratio |
log ( L _ { [ CII ] } / L _ { FIR } ) |
-2.5 |
|
|
2007.01182 🔍 (source)
|
luminosity ratio |
|
16.1 ± 2.5 |
|
|
2007.01182 🔍 (source)
|
luminosity ratio |
|
2.5 ± 0.6 |
|