|
astro-ph/9303016 🔍 (source)
|
mean ratio of Lyman \alpha to Lyman \beta absorption |
|
0.476 ± 0.054 |
|
|
astro-ph/9510061 🔍 (source)
|
H \alpha luminosity |
\alpha |
-1.3 ± 0.2 |
|
|
astro-ph/9512017 🔍 (source)
|
H \alpha emission of surface brightness |
|
0.37 ± 0.02 |
|
|
astro-ph/9512017 🔍 (source)
|
H \alpha emission of surface brightness |
|
0.21 ± 0.04 |
|
|
astro-ph/9512017 🔍 (source)
|
H \alpha emission of surface brightness |
|
0.2 ± 0.02 |
|
|
astro-ph/9512165 🔍 (source)
|
Ly \alpha flux |
|
1.5e-16 erg cm-2 s-1 |
|
|
astro-ph/9604179 🔍 (source)
|
\alpha -element enhancement |
\alpha /Fe ] |
0.5 |
|
|
astro-ph/9605114 🔍 (source)
|
H \alpha |
\lambda |
6583.0 |
|
|
astro-ph/9605114 🔍 (source)
|
H \alpha |
|
6548.0 |
|
|
astro-ph/9703128 🔍 (source)
|
H \alpha emissions |
|
1.26 +0.45-0.32 MJy sr-1 |
|
|
astro-ph/9709109 🔍 (source)
|
\alpha -forest baryon density |
J _ { 0 } |
1.1000000000000001e-23 ± 4.0000000000000004e-24 erg cm-2 sr-1 |
|
|
astro-ph/9710373 🔍 (source)
|
{ Ly } \alpha flux |
|
1.8500000000000002e-13 ± 5.3e-14 erg cm-2 s-1 |
|
|
astro-ph/9710373 🔍 (source)
|
{ Ly } \alpha flux |
|
1.25e-12 ± 5.1e-13 erg cm-2 s-1 |
|
|
astro-ph/9801004 🔍 (source)
|
\alpha |
log N _ { HI } |
12.8 |
Lower |
|
astro-ph/9802220 🔍 (source)
|
H \alpha |
_ { LSR } |
130.0 km |
|
|
astro-ph/9802220 🔍 (source)
|
H \alpha |
|
0.27 +0.02999999999999997-0.030000000000000027 |
|
|
astro-ph/9807063 🔍 (source)
|
H \alpha luminosity |
|
5.6e+37 erg s-1 |
|
|
astro-ph/9810407 🔍 (source)
|
H \alpha flux |
|
1.3000000000000002e-15 ± 2.0000000000000002e-16 erg cm-2 s-1 |
|
|
astro-ph/9812429 🔍 (source)
|
\ion He2 Ly \alpha opacity |
\tau |
1.88 |
|
|
astro-ph/9901280 🔍 (source)
|
Ly \alpha -forest baryon density |
\Omega _ { b } |
0.008 ± 0.004 h |
|
|
astro-ph/9904227 🔍 (source)
|
total H \alpha flux |
|
1.5000000000000002e-13 erg s-1 cm-2 |
|
|
astro-ph/9904227 🔍 (source)
|
H \alpha luminosity |
|
2.3999999999999998e+38 erg s-1 |
|
|
astro-ph/9905290 🔍 (source)
|
\alpha luminosity |
|
8.0 |
|
|
astro-ph/9912376 🔍 (source)
|
Ly \alpha luminosity |
L _ { Ly \alpha } |
1.8e+42 ± 8e+41 erg s-1 |
|
|
astro-ph/0001156 🔍 (source)
|
Ly \alpha luminosity |
|
1700000000.0 |
|
|
astro-ph/0001201 🔍 (source)
|
OVII-OVIII K \alpha, \beta emission feature |
|
0.54 +0.07-0.06 keV |
|
|
astro-ph/0001522 🔍 (source)
|
\alpha blobs |
|
3.4e-05 h3 Mpc-3 |
|
|
astro-ph/0006301 🔍 (source)
|
H \alpha flux |
|
-0.7 M_\odot yr-1 |
|
|
astro-ph/0007374 🔍 (source)
|
H \alpha luminosity of the nebula |
|
1.75e+35 +4.500000000000002e+34-4.499999999999999e+34 erg s-1 |
|
|
astro-ph/0008122 🔍 (source)
|
\alpha +N V emission |
|
69.0 |
|
|
astro-ph/0009435 🔍 (source)
|
Fe~ { } K \alpha |
EW } |
300.0 eV |
Upper |
|
astro-ph/0105399 🔍 (source)
|
\alpha luminosities |
\Omega _ { m } |
0.3 |
|
|
astro-ph/0105507 🔍 (source)
|
Shakura-Sunyaev \alpha parameter |
|
0.1 |
|
|
astro-ph/0105507 🔍 (source)
|
Shakura-Sunyaev \alpha parameter |
|
0.01 |
|
|
astro-ph/0107250 🔍 (source)
|
H \alpha intensity |
|
1.1 pc cm-6 |
|
|
astro-ph/0109401 🔍 (source)
|
narrow Fe K \alpha |
|
1720.0 ± 360.0 km s-1 |
|
|
astro-ph/0110177 🔍 (source)
|
extinction-corrected H \alpha luminosity density |
|
5.4e+39 ± 1.1e+39 erg s-1 Mpc-3 |
|
|
astro-ph/0111511 🔍 (source)
|
halo H \alpha luminosity |
L _ { H \alpha } |
4e+38 |
|
|
astro-ph/0112500 🔍 (source)
|
H \alpha emission toward the direction |
\ell |
148.0 |
|
|
astro-ph/0201058 🔍 (source)
|
NeIX _ { K \alpha |
|
13.448 +0.022-0.024 |
|
|
astro-ph/0201194 🔍 (source)
|
\alpha line flux |
|
3e-17 erg cm-2 s-1 |
|
|
astro-ph/0202047 🔍 (source)
|
H \alpha luminosity |
|
1.3999999999999997e+39 ± 1e+38 erg s-1 |
|
|
astro-ph/0202397 🔍 (source)
|
\alpha -enhancement |
[ \alpha /Fe ] > |
0.1 ± 0.04 |
|
|
astro-ph/0206426 🔍 (source)
|
H \alpha |
|
0.05332 ± 2e-05 day |
|
|
astro-ph/0209258 🔍 (source)
|
absolute H \alpha emission |
|
4.9500000000000003e-17 +3.850000000000001e-17-3.8500000000000003e-17 erg s-1 cm-2 |
|
|
astro-ph/0301471 🔍 (source)
|
H \alpha flux |
SFR |
0.05 M_\odot yr-1 |
|
|
astro-ph/0302243 🔍 (source)
|
H \alpha radial velocities |
K _ { 1 } |
14.0 km s-1 |
|
|
astro-ph/0302432 🔍 (source)
|
Ly \alpha emission |
\theta |
1.0 |
Upper |
|
astro-ph/0306261 🔍 (source)
|
extinction-corrected H _ { \alpha } luminosity |
|
1.25 M_\odot yr-1 |
|
|
astro-ph/0308345 🔍 (source)
|
Pa \alpha emission |
|
1745.0 ± 40.0 km s-1 |
|
|
astro-ph/0308432 🔍 (source)
|
\alpha absorber |
\log N ( H i ) |
19.88 ± 0.05 |
|
|
astro-ph/0312653 🔍 (source)
|
Ly \alpha Gunn-Peterson trough |
z _ { gp } |
7.0 ± 1.0 |
|
|
astro-ph/0403161 🔍 (source)
|
\alpha line luminosity |
|
1.1 |
Lower |
|
astro-ph/0405187 🔍 (source)
|
uncorrected { H \alpha } star-formation rates |
|
42.0 ± 18.0 M_\odot yr-1 |
|
|
astro-ph/0406151 🔍 (source)
|
P \alpha /P \beta line flux ratio |
|
1.05 ± 0.2 |
|
|
astro-ph/0406307 🔍 (source)
|
Ly \alpha flux |
|
5.400000000000001e-17 +2e-17-8e-18 erg s-1 cm-2 |
|
|
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/0407352 🔍 (source)
|
\alpha absorbers |
d N / dz |
170.0 |
|
|
astro-ph/0407352 🔍 (source)
|
\alpha absorbers |
N _ { HI } |
170.0 |
|
|
astro-ph/0407507 🔍 (source)
|
[ S II ] /H \alpha flux ratios |
|
9.0 +3.0-4.0 |
|
|
astro-ph/0407521 🔍 (source)
|
H \alpha width |
|
2290.0 ± 80.0 km s-1 |
|
|
astro-ph/0408031 🔍 (source)
|
Lyman- \alpha line flux |
|
2.2000000000000003e-17 erg cm-2 s-1 |
|
|
astro-ph/0409010 🔍 (source)
|
K \alpha absorption |
|
650.9 +0.8-1.9 eV |
|
|
astro-ph/0410672 🔍 (source)
|
H \alpha rotation curves |
|
20.9 +6.2-5.2 km s-1 |
|
|
astro-ph/0410672 🔍 (source)
|
H \alpha rotation curves |
|
34.8 ± 3.8 km s-1 |
|
|
astro-ph/0410672 🔍 (source)
|
H \alpha rotation curves |
|
30.9 ± 7.2 km s-1 |
|
|
astro-ph/0410672 🔍 (source)
|
H \alpha rotation curves |
|
16.0 +6.1-5.4 km s-1 |
|
|
astro-ph/0410695 🔍 (source)
|
\alpha -enhancement |
[ \alpha / Fe ] |
0.3 |
|
|
astro-ph/0411072 🔍 (source)
|
Ly \alpha effective optical depth |
|
0.9 ± 0.3 |
|
|
astro-ph/0411152 🔍 (source)
|
effective Ly \alpha optical depth |
\tau _ { eff } |
14.3 |
Upper |
|
astro-ph/0501259 🔍 (source)
|
Ly \alpha emission |
\beta |
-1.09 |
|
|
astro-ph/0502066 🔍 (source)
|
H \alpha fluxes |
|
1.7e-16 erg s-1 cm-2 |
Upper |
|
astro-ph/0502066 🔍 (source)
|
H \alpha fluxes |
|
9.0 |
Lower |
|
astro-ph/0502384 🔍 (source)
|
H \alpha emission |
L _ { H \alpha } / L _ { bol } |
2e-07 |
Upper |
|
astro-ph/0503241 🔍 (source)
|
A Ly \alpha luminosity |
|
5.599999999999999e+43 erg s-1 |
|
|
astro-ph/0503320 🔍 (source)
|
\alpha line |
f _ { Ly \alpha,TOT } |
1.94e-12 erg s-1 cm-2 |
|
|
astro-ph/0503570 🔍 (source)
|
Fe K \alpha |
|
1700.0 +410.0-390.0 km s-1 |
|
|
astro-ph/0504187 🔍 (source)
|
\alpha |
cz |
3046.0 ± 12.0 km s-1 |
|
|
astro-ph/0505453 🔍 (source)
|
\alpha /Fe abundance ratios |
[ \alpha /Fe ] Â |
0.47 ± 0.06 dex |
|
|
astro-ph/0507689 🔍 (source)
|
H \alpha emission |
|
-1600.0 km s-1 |
|
|
astro-ph/0507706 🔍 (source)
|
/H \alpha line ratio |
[ S II ] / H \alpha |
0.4 |
Upper |
|
astro-ph/0510374 🔍 (source)
|
H \alpha scale lengths of the field galaxies |
|
1.14 ± 0.07 |
|
|
astro-ph/0510368 🔍 (source)
|
\alpha absorber |
\log { N _ { H i } } |
22.6 ± 0.3 |
|
|
astro-ph/0602523 🔍 (source)
|
net escape fraction of Ly \alpha photon |
f _ { Ly \alpha } |
0.1 |
Upper |
|
astro-ph/0605019 🔍 (source)
|
\alpha emitting |
|
1.0 |
Lower |
|
astro-ph/0606210 🔍 (source)
|
\alpha line |
EW _ { Ly \alpha } ^ { rest } |
46.0 ± 5.0 |
|
|
astro-ph/0607036 🔍 (source)
|
\alpha absorption |
|
340.0 km s-1 |
|
|
astro-ph/0608432 🔍 (source)
|
H \alpha luminosity in the nebular phase |
|
56.0 N |
|
|
astro-ph/0610761 🔍 (source)
|
total Ly \alpha luminosity |
|
2e+43 erg s-1 |
|
|
astro-ph/0701645 🔍 (source)
|
H \alpha flux |
|
8e-15 erg s-1 cm-2 |
Lower |
|
astro-ph/0703461 🔍 (source)
|
Fe K \alpha complex |
z |
0.27 ± 0.01 |
|
|
astro-ph/0703522 🔍 (source)
|
total Lyman- \alpha luminosity |
|
2.1000000000000003e+44 erg s-1 |
|
|
0704.1116 🔍 (source)
|
total Ly \alpha luminosities |
|
1.85e+44 +1.5500000000000002e+44-1.55e+44 erg s-1 |
|
|
0705.1544 🔍 (source)
|
H \alpha -derived star formation rate of the inner |
N ( WR ) / N ( O ) |
0.04 |
|
|
0706.1083 🔍 (source)
|
fluorescent iron K \alpha emission |
|
6.97 keV |
|
|
0706.1801 🔍 (source)
|
Ly \alpha survival fraction |
\alpha _ { esc } \epsilon ^ { 1 / \gamma } |
0.030000000000000002 +0.02-0.020000000000000004 |
|
|
0707.3161 🔍 (source)
|
\alpha luminosity |
|
3e+42 erg s-1 |
|
|
0708.2030 🔍 (source)
|
\alpha forest power spectrum |
m _ { \nu _ { s } |
1.7 keV |
Lower |
|
0708.2790 🔍 (source)
|
\alpha -element-to-iron abundance ratios |
|
0.0 |
|
|
0708.2790 🔍 (source)
|
\alpha -element-to-iron abundance ratios |
[ \alpha / Fe ] |
0.4 |
|
|
0709.1009 🔍 (source)
|
H \alpha luminosity density |
|
2.7e+39 +6.999999999999999e+38-5.9999999999999995e+38 erg s-1 Mpc-3 |
|
|
0709.1009 🔍 (source)
|
angular two-point correlation function of H \alpha emitting galaxies |
\log L ( H \alpha ) |
39.8 |
Lower |
|
0710.0547 🔍 (source)
|
\alpha /Fe ] abundance ratio |
|
0.31 ± 0.09 |
|
|
0711.1904 🔍 (source)
|
mean He II Ly \alpha line transmission |
\bar { F } |
0.304 ± 0.002 |
|
|
0802.0228 🔍 (source)
|
Ly \alpha photons |
|
0.1 |
|
|
0802.0228 🔍 (source)
|
Ly \alpha photons |
f _ { Ly \alpha } |
0.15 |
|
|
0803.2489 🔍 (source)
|
\alpha -element abundance |
[ \alpha / Fe ] |
-0.11 |
|
|
0806.3218 🔍 (source)
|
slight \alpha -element overabundance |
[ \alpha / Fe ] |
0.1 |
|
|
0807.0101 🔍 (source)
|
H \alpha luminosity density |
|
4.45e+39 +2.9599999999999995e+39-1.7499999999999998e+39 erg s-1 Mpc-3 |
|
|
0808.1414 🔍 (source)
|
\alpha enhancement |
[ \alpha / Fe ] |
0.39 ± 0.05 dex |
|
|
0810.2424 🔍 (source)
|
H \alpha emission line |
EW _ { obs } |
85.0 ± 35.0 |
|
|
0811.1662 🔍 (source)
|
H \alpha emission |
H \alpha - r |
-0.88 ± 0.02 |
|
|
0812.2975 🔍 (source)
|
iron K \alpha emission line |
|
6.39 ± 0.03 keV |
|
|
0901.0642 🔍 (source)
|
/H \alpha emission line ratio |
|
0.42 |
|
|
0901.4627 🔍 (source)
|
Ly \alpha line flux |
|
1.47e-17 erg s-1 cm-2 |
|
|
0902.0736 🔍 (source)
|
H \alpha luminosity |
|
4.4 |
|
|
0902.2716 🔍 (source)
|
H \alpha velocity profile of the starburst region |
\sigma |
33.5 ± 1.5 km s-1 |
|
|
0905.1329 🔍 (source)
|
Ly \alpha emission |
EW _ { Ly \alpha } |
60.0 |
|
|
0906.1532 🔍 (source)
|
O viii Lyman \alpha emission |
|
9.98 +1.1-1.99 |
|
|
0906.4785 🔍 (source)
|
He ii /Ly \alpha ratio |
|
0.12 ± 0.04 |
|
|
0907.4989 🔍 (source)
|
\alpha escape fraction |
f _ { \alpha } |
0.1 |
|
|
0908.4283 🔍 (source)
|
\alpha, \gamma ) ^ { 16 } O reaction rates of the production |
|
44.0 T |
|
|
0909.3844 🔍 (source)
|
\alpha -element enhancement |
|
-0.1 ± 0.04 dex-1 |
|
|
0910.2244 🔍 (source)
|
median Ly \alpha luminosity |
L _ { Ly \alpha } |
1.3000000000000001e+42 |
|
|
0910.3521 🔍 (source)
|
H \alpha to FUV flux ratio |
Log f ( H \alpha ) / f ( FUV ) |
1.1 ± 0.34 |
|
|
0910.5590 🔍 (source)
|
\alpha -elements overabundant |
\alpha / Fe ] |
0.2 |
|
|
0911.3400 🔍 (source)
|
column density of the Ly- \alpha absorbers |
log _ { 10 } ( N _ { HI } ( cm ^ { -2 } ) ) |
13.2 |
Lower |
|
0911.5566 🔍 (source)
|
{ L } \alpha surface brightness profile |
r |
-1.2 |
|
|
1001.2825 🔍 (source)
|
median AGN H \alpha luminosity |
|
7.1e+39 erg s-1 |
|
|
1002.0839 🔍 (source)
|
intrinsic Ly \alpha -to-continuum luminosity |
|
1.5 |
|
|
1002.0839 🔍 (source)
|
intrinsic Ly \alpha -to-continuum luminosity |
f _ { \alpha } / f _ { c } |
3.7 |
Upper |
|
1002.2973 🔍 (source)
|
disc \alpha coefficient |
( \alpha |
0.1 |
Upper |
|
1003.0039 🔍 (source)
|
Lyman- \alpha emission |
|
135.6 ± 20.3 |
|
|
1003.0463 🔍 (source)
|
\alpha luminosity |
|
0.02 |
|
|
1004.4318 🔍 (source)
|
H \alpha flux surface density |
|
0.79 ± 0.19 |
|
|
1005.1841 🔍 (source)
|
\alpha emission |
|
-10.0 |
Lower |
|
1005.3829 🔍 (source)
|
Ly \alpha quasar density |
|
2.7e-06 +6.2e-06-2.2e-06 Mpc-3 |
|
|
1005.3829 🔍 (source)
|
escape fraction of Ly \alpha photons |
f _ { esc,Ly \alpha } |
6.5 ± 3.5 |
Lower |
|
1005.4727 🔍 (source)
|
H \alpha emission line galaxies |
|
0.1125 ± 0.023500000000000007 M_\odot yr-1 Mpc-3 |
|
|
1007.5357 🔍 (source)
|
H \alpha flux |
|
9.000000000000001e-18 erg s-1 cm-2 |
|
|
1008.4842 🔍 (source)
|
\alpha line luminosity |
L ( Ly \alpha ) |
9.2e+42 erg s-1 |
|
|
1009.1395 🔍 (source)
|
\alpha luminosity |
|
2e+41 erg s-1 |
Upper |
|
1011.4239 🔍 (source)
|
Ly \alpha absorber |
log ( N _ { H \sc I } / cm ^ { -2 } ) |
21.9 ± 0.1 |
|
|
1102.1509 🔍 (source)
|
escape fractions of Lyman- \alpha photons |
f _ { esc } |
0.07500000000000001 +0.024999999999999994-0.02500000000000001 |
|
|
1103.0233 🔍 (source)
|
\alpha -elements enhancement |
|
0.39 ± 0.02 dex |
|
|
1103.1927 🔍 (source)
|
narrow Fe K \alpha line width |
|
2.6 +0.9-0.4 |
|
|
1106.2811 🔍 (source)
|
average Ly \alpha escape fraction |
f _ { Ly \alpha } ^ { Esc } |
28.0 % |
Lower |
|
1106.5731 🔍 (source)
|
iron K \alpha equivalent |
width |
0.85 ± 0.35 keV |
|
|
1107.3159 🔍 (source)
|
fraction of Ly \alpha -emitting galaxies |
|
25.0 |
Lower |
|
1107.3159 🔍 (source)
|
fraction of Ly \alpha -emitting galaxies |
EW _ { 0 } ^ { Ly \alpha } |
24.0 |
Lower |
|
1107.4011 🔍 (source)
|
H \alpha emission line nebula |
L _ { H \alpha } |
2.2000000000000004e+40 erg s-1 |
|
|
1109.0023 🔍 (source)
|
\alpha luminosity |
|
3e+43 erg s-1 |
|
|
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 |
|
|
1111.0958 🔍 (source)
|
H \alpha -derived O star |
N ( WR ) / N ( O ) |
0.03 |
|
|
1111.1393 🔍 (source)
|
extinction-corrected H \alpha luminosity |
L ( H \alpha ) |
7.27e+41 erg s-1 |
|
|
1112.0035 🔍 (source)
|
H \alpha line |
|
56.0 N |
|
|
1112.3656 🔍 (source)
|
Ly \alpha luminosity |
|
1.7e+43 ± 1e+42 erg s-1 |
|
|
1202.1822 🔍 (source)
|
median H \alpha effective radius |
r _ { e } ( H \alpha ) |
4.2 ± 0.1 kpc |
|
|
1202.2884 🔍 (source)
|
Ly \alpha transmissivity |
T _ { \alpha } ^ { LAE } |
0.25 |
|
|
1203.1919 🔍 (source)
|
escape fraction of resonantly-scattered Ly \alpha photons |
f _ { esc } |
0.08 |
Upper |
|
1204.3234 🔍 (source)
|
\alpha line flux |
F _ { Ly \alpha } |
6.900000000000001e-18 erg s-1 cm-2 |
|
|
1205.1493 🔍 (source)
|
total Lyman- \alpha intensity ( times frequency |
|
2.5e-08 +1.0699999999999998e-08-1.0700000000000002e-08 erg s-1 cm-2 sr-1 |
|
|
1205.2697 🔍 (source)
|
Ly- \alpha population |
N _ { HI } |
-75.0 ± 12.0 c-1 |
|
|
1205.5452 🔍 (source)
|
average H \alpha velocity dispersion |
\langle \sigma \rangle |
220.0 ± 80.0 km s-1 |
|
|
1206.4930 🔍 (source)
|
\alpha luminosity |
|
-4.6 |
Lower |
|
1208.0714 🔍 (source)
|
\alpha -spectroscopic factor |
S _ { \alpha } |
6.356 MeV |
|
|
1208.3529 🔍 (source)
|
mean rest-frame H \alpha equivalent width |
|
3.8 |
Lower |
|
1208.4003 🔍 (source)
|
H \alpha line |
[ O i ] 6300 |
6427.0 |
|
|
1209.3679 🔍 (source)
|
H \alpha equivalent width |
|
-125.0 ± 15.0 |
|
|
1210.0531 🔍 (source)
|
Ly \alpha absorption |
|
7.5 ± 1.8 |
|
|
1210.3496 🔍 (source)
|
H \alpha emitting |
|
5800000.0 M_\odot |
|
|
1303.1937 🔍 (source)
|
Ly \alpha forest redshift distortion factor |
\beta _ { F } |
1.1 ± 0.15 |
|
|
1305.1399 🔍 (source)
|
H \alpha flux |
|
2e-16 erg s-1 cm-2 |
|
|
1306.3949 🔍 (source)
|
mean Ly \alpha transmission fraction |
|
0.2 |
Upper |
|
1306.3994 🔍 (source)
|
average proper motion of H \alpha filaments |
|
0.1 ± 0.02 |
|
|
1306.3994 🔍 (source)
|
average proper motion of H \alpha filaments |
|
1200.0 ± 200.0 km s-1 |
|
|
1307.3556 🔍 (source)
|
H \alpha extinctions |
A _ { H \alpha } |
1.0 ± 0.2 mag |
|
|
1310.7020 🔍 (source)
|
NII ] \lambda 6584/H \alpha ratio |
|
0.27 ± 0.01 |
|
|
1311.1653 🔍 (source)
|
H \alpha luminosities |
|
1.3e+38 |
Lower |
|
1311.1653 🔍 (source)
|
H \alpha luminosities |
|
4e+41 erg-1 |
Upper |
|
1311.5534 🔍 (source)
|
\alpha emission |
z _ { em } |
3.115 ± 0.003 |
|
|
1312.6299 🔍 (source)
|
Ly \alpha fluxes |
|
2.8e-18 erg-1 cm-2 |
|
|
1401.6201 🔍 (source)
|
\alpha escape fraction |
|
0.7 ± 0.4 |
|
|
1401.7597 🔍 (source)
|
\alpha scale |
) N _ { eff } |
3.5 ± 0.4 |
|
|
1401.7668 🔍 (source)
|
H \alpha emission |
EW ( H \alpha ) |
290.0 |
|
|
1402.0493 🔍 (source)
|
fraction of H \alpha luminosity due to star formation and AGN activity |
|
35.0 ± 2.0 % |
|
|
1402.6328 🔍 (source)
|
\mathrm { \alpha } |
[ Fe / H ] |
-2.5 c |
|
|
1402.6697 🔍 (source)
|
\alpha luminosity |
|
6.3e+43 erg s-1 |
|
|
1404.2297 🔍 (source)
|
\alpha emission |
EW _ { 0 } |
100.0 |
|
|
1404.7126 🔍 (source)
|
broad Iron K \alpha |
|
-11.0 |
|
|
1404.7486 🔍 (source)
|
Fe K \alpha |
E _ { rest } |
6.46 +0.08-0.07 keV |
|
|
1405.7405 🔍 (source)
|
effective optical depth of He ii Ly \alpha absorption |
z |
2.3 |
Lower |
|
1405.7405 🔍 (source)
|
effective optical depth of He ii Ly \alpha absorption |
\tau _ { eff , HeII } |
2.3 |
Lower |
|
1407.1028 🔍 (source)
|
iron K \alpha line |
|
6.426 ± 0.008 keV |
|
|
1408.1629 🔍 (source)
|
\alpha -element abundance |
[ \alpha / Fe ] |
0.25 dex |
|
|
1409.8304 🔍 (source)
|
volumetric Ly \alpha escape fraction |
|
4.4 +2.1-1.2 |
|
|
1409.8131 🔍 (source)
|
\alpha /Fe ratio |
[ Si ii / Fe ii ] |
0.5 |
|
|
1409.8347 🔍 (source)
|
Ly \alpha  luminosity |
L _ { Ly \alpha } |
1.3000000000000001e+42 |
|
|
1410.4288 🔍 (source)
|
prominent H \alpha emission |
\langle \log _ { 10 } L _ { H \alpha } / L _ { bol } \rangle |
-4.68 ± 0.06 |
|
|
1410.7476 🔍 (source)
|
\alpha, \gamma ) ^ { 16 } O reaction rates on the production of supernova |
|
25.0 M_\odot |
|
|
1411.3357 🔍 (source)
|
H \alpha luminosity |
|
41.3 +5.700000000000003-5.699999999999996 M_\odot yr-1 |
|
|
1411.3443 🔍 (source)
|
H \alpha luminosity |
L _ { H \alpha } |
4.2e+37 ± 4e+36 erg s-1 |
|
|
1501.07210 🔍 (source)
|
\alpha |
|
-0.21 ± 0.22 |
|
|
1502.05403 🔍 (source)
|
Lyman- \alpha /H- \alpha photon ratio |
\langle R ( L \alpha / H \alpha ) \rangle |
17.0 |
|
|
1502.06771 🔍 (source)
|
broad-line H \alpha velocity width |
|
1020.0 km s-1 |
|
|
1502.07579 🔍 (source)
|
H \alpha emitting region |
|
10.4 ± 0.5 R_\odot |
|
|
1503.02661 🔍 (source)
|
\alpha -element abundances |
[ Mg / Fe ] |
0.3 |
Lower |
|
1503.03929 🔍 (source)
|
H \alpha luminosity |
SFR |
7.5e-42 ± 1.3000000000000002e-42 |
|
|
1503.06635 🔍 (source)
|
Ly \alpha~ { } equivalent width distribution |
EW |
100.0 |
Lower |
|
1504.05592 🔍 (source)
|
H \alpha flux sensitivity |
|
1.6e-16 erg cm-2 s-1 |
Lower |
|
1504.06619 🔍 (source)
|
Lyman- \alpha escape fraction |
f _ { esc } |
0.5 |
|
|
1504.06881 🔍 (source)
|
CIV/Ly \alpha flux ratio |
f _ { CIV } / f _ { Ly \alpha } |
0.3 |
|
|
1504.07916 🔍 (source)
|
\alpha -enhanced to |
[ \alpha / Fe ] |
0.4 dex |
|
|
1507.06648 🔍 (source)
|
Lyman- \alpha escape fraction |
( \mathrm { f } _ { \mathrm { esc } } \mathrm { ( Ly \alpha ) } |
0.78 |
Lower |
|
1508.05103 🔍 (source)
|
\alpha -element |
[ \alpha /Fe ] ) |
9.5 Gyr |
Upper |
|
1508.05067 🔍 (source)
|
Ly \alpha absorption |
\lambda _ { obs } |
8426.0 |
Upper |
|
1508.06323 🔍 (source)
|
/H \alpha emission-line ratios |
|
0.66 ± 0.02 |
|
|
1508.06323 🔍 (source)
|
/H \alpha emission-line ratios |
|
0.93 ± 0.01 |
|
|
1509.04345 🔍 (source)
|
H \alpha emission |
log [ N ii ] / H \alpha |
0.6 ± 0.2 |
|
|
1509.08663 🔍 (source)
|
H \alpha emission |
full-width-half-maximum FWHM |
2700.0 ± 280.0 km s-1 |
|
|
1512.01854 🔍 (source)
|
Ly \alpha luminosity range |
\log L _ { Ly \alpha } |
43.05 +1.3500000000000014-1.3499999999999943 erg s-1 |
|
|
1512.03063 🔍 (source)
|
\alpha escape |
\Omega _ { Ly \alpha } |
2.4 ± 0.8 s |
|
|
1512.09208 🔍 (source)
|
total H \alpha luminosity amounts |
L _ { H \alpha } |
1.6e+42 erg s-1 |
|
|
1602.02160 🔍 (source)
|
rest-frame Ly \alpha equivalent width |
EW ( Ly \alpha ) |
15.6 +5.9-3.6 |
|
|
1602.02933 🔍 (source)
|
\alpha emission region |
R _ { d } / R _ { * } |
5.0 |
|
|
1603.00461 🔍 (source)
|
Ly \alpha break redshifted |
{ z _ { \mathrm { grism } } |
11.09 +0.08-0.12 |
|
|
1603.06295 🔍 (source)
|
H \alpha -derived star formation rates |
|
1.0 |
Upper |
|
1603.07832 🔍 (source)
|
broad H \alpha emission |
|
2100000.0 M_\odot |
|
|
1604.03941 🔍 (source)
|
H \alpha detection rate |
|
9.2 +3.5-2.1 % |
|
|
1604.06074 🔍 (source)
|
\alpha -elements |
\alpha /Fe ] |
0.4 |
|
|
1605.03194 🔍 (source)
|
Ly \alpha to X-ray luminosity ratio |
|
0.3 |
|
|
1605.03194 🔍 (source)
|
Ly \alpha to X-ray luminosity ratio |
L _ { Ly \alpha } / L _ { X } |
505.0 ± 495.0 |
Lower |
|
1605.05771 🔍 (source)
|
intrinsic Ly \alpha luminosity |
|
1.3000000000000001e+42 erg s-1 |
|
|
1605.05771 🔍 (source)
|
\alpha equivalent width |
|
74.0 ± 15.0 |
|
|
1605.06519 🔍 (source)
|
Lyman- \alpha  line flux |
|
1.06e-17 ± 1.9000000000000003e-18 erg s-1 cm-2 |
|
|
1606.00528 🔍 (source)
|
H \alpha emission-line integrated velocity dispersions |
\sigma _ { int } |
140.0 ± 90.0 km s-1 |
|
|
1606.07073 🔍 (source)
|
Ly \alpha escape fraction |
f _ { ESC } ^ { Ly \alpha } |
40.0 % |
Upper |
|
1607.04126 🔍 (source)
|
H \alpha luminosity |
L ( H \alpha ) |
1.67e-31 erg s-1 |
|
|
1608.08756 🔍 (source)
|
\alpha viscous stress parameter |
\alpha |
0.002 |
|
|
1609.04021 🔍 (source)
|
diffuse Ly \alpha nebular luminosity |
L _ { nebula } |
5.1e+44 ± 1.0000000000000001e+43 erg s-1 |
|
|
1609.05897 🔍 (source)
|
escape fraction of Ly \alpha photons |
|
5.1 ± 0.2 % |
|
|
1610.00013 🔍 (source)
|
\alpha emitting region |
|
0.21 |
Upper |
|
1611.00777 🔍 (source)
|
median Ly \alpha escape fraction |
f _ { esc } ^ { Ly \alpha } |
0.68 ± 0.3 |
|
|
1611.05506 🔍 (source)
|
polarization of the Ly \alpha emission |
P _ { \%, { Ly } \alpha } |
5.0 kpc |
|
|
1612.00447 🔍 (source)
|
/H \alpha emission line ratio |
\Delta log ( O/H ) / \Delta R= |
-0.026 ± 0.008 dex kpc-1 |
|
|
1612.01996 🔍 (source)
|
Fe K \alpha equivalent width |
EW |
2.5 +2.6-1.0 keV |
|
|
1701.06721 🔍 (source)
|
H \alpha -emitting portion |
|
-9.0 |
Upper |
|
1702.05280 🔍 (source)
|
Fe K \alpha emission |
|
6.6850000000000005 +0.28499999999999925-0.28500000000000014 keV |
|
|
1703.04544 🔍 (source)
|
\alpha emission |
|
-125.0 |
Lower |
|
1703.05756 🔍 (source)
|
\alpha absorbers |
N _ { HI } |
20.0 cm-2 |
Lower |
|
1703.05756 🔍 (source)
|
\alpha absorbers |
log N _ { HI } |
20.0 cm-2 |
Lower |
|
1703.07410 🔍 (source)
|
Fe K \alpha equivalent width |
|
0.18 +0.17-0.12 |
Lower |
|
1703.07410 🔍 (source)
|
Fe K \alpha equivalent width |
EW |
0.61 +0.27-0.25 keV |
|
|
1703.07778 🔍 (source)
|
dust-corrected { H \alpha } star formation rates |
|
-7.0 M_\odot yr-1 |
Upper |
|
1703.08901 🔍 (source)
|
mean broad H \alpha luminosity |
log L _ { H \alpha } |
40.73 ± 0.32 erg s-1 |
|
|
1706.04863 🔍 (source)
|
\alpha -elements abundance |
\alpha / M ] \right \rangle |
-0.1 ± 0.08 dex |
|
|
1708.01605 🔍 (source)
|
H \alpha narrow-line full-width |
W _ { NL } |
54.8 ± 1.8 km s-1 |
|
|
1708.05683 🔍 (source)
|
\alpha -to-proton temperature ratio |
|
5.25 ± 0.04999999999999982 |
|
|
1709.08228 🔍 (source)
|
average Ly \alpha surface brightness |
SB _ { Ly \alpha } |
6.04e-18 erg s-1 cm-2 |
|
|
1710.01784 🔍 (source)
|
effective Ly \alpha escape fraction |
f _ { esc } ^ { eff } ( Ly \alpha ) |
0.23 +0.36-0.17 |
|
|
1710.01784 🔍 (source)
|
IGM transmission to Ly \alpha photons |
T _ { IGM } |
0.2 |
Lower |
|
1710.10184 🔍 (source)
|
Ly \alpha spatial extent |
\alpha _ { ext } |
5.7 kpc |
Upper |
|
1711.07418 🔍 (source)
|
Fe K \alpha emission region |
|
98.0 pc |
|
|
1711.11449 🔍 (source)
|
extinction-corrected Ly \alpha /H \beta flux ratio |
f _ { esc } ( Ly \alpha ) |
98.0 c-1 |
|
|
1712.03964 🔍 (source)
|
H \alpha emission |
( EW _ { \mathrm { H } \alpha } |
560.0 ± 82.0 |
|
|
1802.08177 🔍 (source)
|
IGM Lyman- \alpha opacity |
z _ { source } |
5.7 |
Lower |
|
1803.09557 🔍 (source)
|
Ly \alpha rest-frame equivalent width |
|
52.0 ± 22.0 |
|
|
1804.03831 🔍 (source)
|
\alpha modulation |
|
308.0 +26.0-23.0 day |
|
|
1805.11621 🔍 (source)
|
Ly \alpha peak separation |
|
220.0 ± 20.0 km s-1 |
|
|
1805.11621 🔍 (source)
|
\alpha emission |
r _ |
50.0 |
|
|
1806.00316 🔍 (source)
|
\alpha -element abundances |
|
-0.2 |
Lower |
|
1806.01191 🔍 (source)
|
Ly \alpha luminosity |
|
5.7e+42 erg s-1 |
|
|
1807.03785 🔍 (source)
|
H \alpha emission |
EW _ { REST } |
40.0 |
|
|
1808.02801 🔍 (source)
|
H \alpha star formation rate |
|
0.0047 M_\odot yr-1 |
|
|
1808.05247 🔍 (source)
|
optical depth of \ion He2 Ly \alpha absorption |
\tau _ { eff } |
2.54 |
Lower |
|
1808.05247 🔍 (source)
|
optical depth of \ion He2 Ly \alpha absorption |
z |
2.54 |
Lower |
|
1811.00823 🔍 (source)
|
median H \alpha velocity dispersion |
\sigma |
27.0 km s-1 |
|
|
1811.00823 🔍 (source)
|
H \alpha luminosity |
L _ { H \alpha } |
4e+38 erg s-1 |
|
|
1811.03662 🔍 (source)
|
\alpha emission |
EW _ { 0 } |
150.0 |
Lower |
|
1901.07108 🔍 (source)
|
Fe K \alpha emission line |
EW _ { \textnormal { rest } |
0.5 |
Lower |
|
1902.02251 🔍 (source)
|
prominent H \alpha emission line |
L _ { H \alpha } |
2.2e+38 ± 2.0000000000000001e+37 erg s-1 |
|
|
1902.09555 🔍 (source)
|
Ly \alpha luminosity |
\log ( L _ { Ly \alpha } / [ erg s ^ { -1 } ] ) |
43.0 |
|
|
1903.03131 🔍 (source)
|
total Ly \alpha luminosity |
|
2.5000000000000002e+44 erg s-1 |
|
|
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 |
|
|
1905.12491 🔍 (source)
|
H \alpha absorption depth |
|
0.68 ± 0.05 |
|
|
1905.12491 🔍 (source)
|
H \alpha absorption depth |
|
0.59 ± 0.07 |
|
|
1907.01158 🔍 (source)
|
\alpha ) ^ { 13 } N rate |
|
4000000000.0 ± 1000000000.0 K |
|
|
1907.01158 🔍 (source)
|
\alpha ) ^ { 13 } N rate |
|
0.5 |
|
|
1907.07666 🔍 (source)
|
\alpha -element enhancement |
[ \alpha / Fe ] |
0.2 ± 0.2 |
|
|
1909.06376 🔍 (source)
|
\alpha equivalent width |
EW _ { 0 } |
38.0 |
|
|
1909.10518 🔍 (source)
|
Ly \alpha absorption |
\log ( N _ { H I } / cm ^ { -2 } ) |
13.7 |
Upper |
|
1910.00269 🔍 (source)
|
H \alpha activity |
|
-4.16 |
Lower |
|
1910.00269 🔍 (source)
|
H \alpha activity |
( log \mathrm { ( L _ { H \alpha } / L _ { bol } } ) |
-4.31 |
Upper |
|
1910.03593 🔍 (source)
|
median Ly \alpha flux |
|
10.0 |
|
|
1910.04771 🔍 (source)
|
Ly \alpha fluxes |
F _ { \lambda } |
7e-18 erg s-1 cm-2 |
Lower |
|
1911.02284 🔍 (source)
|
Fe \hbox { K } \alpha~ { |
|
7.8 |
|
|
2001.03619 🔍 (source)
|
Ly \alpha luminosity |
L |
2.8e+40 erg s-1 |
Upper |
|
2001.08206 🔍 (source)
|
\alpha partial widths |
E _ { x } |
11.171 MeV |
|
|
2001.08206 🔍 (source)
|
\alpha partial widths |
E _ { x } |
11.112 |
|
|
2001.08206 🔍 (source)
|
\alpha partial widths |
E _ { x } |
11.163 |
|
|
2001.08206 🔍 (source)
|
\alpha partial widths |
E _ { x } |
11.169 |
|
|
2001.08221 🔍 (source)
|
H \alpha line width |
|
1950.0 km F W H s-1 |
|
|
2002.05179 🔍 (source)
|
Ly \alpha flux |
F _ { Ly \alpha } |
1.56e-16 ± 1e-17 erg s-1 cm-2 |
|
|
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 |
|
|
2003.01397 🔍 (source)
|
\ion H \alpha broad emission |
z _ { sys } |
2.213 ± 0.0004 |
|
|
2005.09667 🔍 (source)
|
effective Ly \alpha opacity |
\tau _ { eff } |
2.02 |
|
|
2005.14482 🔍 (source)
|
Ne ( \alpha,n ) ^ { |
|
25.0 |
|
|
2006.02234 🔍 (source)
|
H \alpha luminosity |
|
1.1000000000000001e+36 erg s-1 |
Upper |
|
2007.03691 🔍 (source)
|
H \alpha emission |
( t _ { \text { over } } |
1.7 Myr |
Upper |
|
2007.12712 🔍 (source)
|
\alpha -enhancement |
\alpha /Fe ] |
0.24 ± 0.1 |
|