Suggested: Dimensionless
Exclude
Name/Symbol Condition
Name: spectrum
Mean: 340 ± 4.38e+03
Median: 1
Range: -3.53e+03 ‒ 9.04e+04
492 results.
arXiv Name Symbol Parsed Bound
astro-ph/9309040 🔍 (source) spectral index of the power spectrum n
-1.0
Upper
astro-ph/9311056 🔍 (source) slope of the power spectrum of density perturbations n
-1.0
Upper
astro-ph/9311068 🔍 (source) spectrum \lambda _ { peak }
51.0 ± 18.0 Mpc h-1
astro-ph/9402024 🔍 (source) effective power spectrum index n _ { eff }
1.35
astro-ph/9404009 🔍 (source) spectrum n
1.0
astro-ph/9512151 🔍 (source) spectral parameter of the power spectrum of primordial perturbation n
1.84 ± 0.29
astro-ph/9609194 🔍 (source) soft intrinsic QSO spectrum \alpha _ { Q }
1.9 +0.10000000000000009-0.09999999999999987
astro-ph/9610219 🔍 (source) spectrum n
1.0
Lower
astro-ph/9611029 🔍 (source) faint source spectrum \alpha
0.95 +0.1-0.15
astro-ph/9612016 🔍 (source) power spectrum normalisation \mbox { $Q _ { rms - ps }
21.0 ± 1.6 K
astro-ph/9703043 🔍 (source) power spectrum normalisation Q _ { rms - ps }
22.0 +10.0-6.0 K
astro-ph/9703181 🔍 (source) power-law index of the GRB spectrum s
-1.1 ± 0.3
astro-ph/9704246 🔍 (source) power spectrum \Omega h
0.2
astro-ph/9705180 🔍 (source) power spectrum of the density fluctuations k _ { c }
0.055 +0.045000000000000005-0.045 Mpc-1
astro-ph/9706077 🔍 (source) position of the dominant peak in the best-fit power spectrum A _ { peak }
76.0 +3.0-7.0 K
astro-ph/9706077 🔍 (source) power spectrum normalization \ell
10.0
astro-ph/9706118 🔍 (source) steep X-ray spectrum \alpha _ { energy }
1.5
Lower
astro-ph/9709020 🔍 (source) power spectrum \beta
0.6
Upper
astro-ph/9709020 🔍 (source) power spectrum
0.5
Lower
astro-ph/9709198 🔍 (source) power-law index of the power spectrum in this range
-1.4
astro-ph/9712030 🔍 (source) power spectrum \sigma _ { 8 } \Omega ^ { 0.53 }
0.6
astro-ph/9801106 🔍 (source) energy spectrum of the neutrino emission from electron-positron pair annihilation M
50000.0 M_\odot
Lower
astro-ph/9801136 🔍 (source) BAL spectrum
0.4
Lower
astro-ph/9802109 🔍 (source) mass power-spectrum \sigma _ { 8 }
0.67
astro-ph/9802299 🔍 (source) spectrum T _ { eff }
900.0 K
astro-ph/9804019 🔍 (source) spectrum z _ { em }
2.22
astro-ph/9804333 🔍 (source) flat-spectrum S _ { 5 GHz }
25.0
Lower
astro-ph/9806026 🔍 (source) power spectrum
-1.0
astro-ph/9807213 🔍 (source) spectrum \Gamma
0.8
astro-ph/9807240 🔍 (source) power spectrum
0.55
Upper
astro-ph/9807240 🔍 (source) power spectrum \Omega _ { 0 }
0.1
Lower
astro-ph/9807240 🔍 (source) power spectrum \Omega _ { 0 }
0.1
Lower
astro-ph/9807240 🔍 (source) slope of the power spectrum \Omega _ { 0 }
0.6
Upper
astro-ph/9810006 🔍 (source) steep spectrum n
-1.5
astro-ph/9810364 🔍 (source) power spectrum \Omega _ { 0 } ^ { m }
1.0
astro-ph/9810398 🔍 (source) spectrum peak
20.0 keV
astro-ph/9811199 🔍 (source) spectrum
43.0 ± 7.0
astro-ph/9812245 🔍 (source) power-law spectrum \Gamma
2.2
astro-ph/9812247 🔍 (source) power-law spectrum of index n
-1.9
astro-ph/9812311 🔍 (source) spectrum b _ { P }
1.0
Upper
astro-ph/9901061 🔍 (source) spectrum
-0.6
Lower
astro-ph/9901351 🔍 (source) power spectrum \beta
0.58 ± 0.26
astro-ph/9901351 🔍 (source) power spectrum \Gamma
0.2
astro-ph/9901351 🔍 (source) power spectrum \beta
0.47 ± 0.16
astro-ph/9901393 🔍 (source) power spectrum slope n
0.7
astro-ph/9903146 🔍 (source) spectrum m _ { R }
24.4
astro-ph/9903450 🔍 (source) power spectrum
0.9
astro-ph/9903472 🔍 (source) shape parameter of the mass power-spectrum \Gamma
0.15
astro-ph/9906127 🔍 (source) EUV spectrum
112.5 ± 37.5
astro-ph/9909239 🔍 (source) power density spectrum
33.0 hr
astro-ph/9909487 🔍 (source) spectrum \sigma _ { 8 } \Omega _ { m } ^ { 0.6 }
0.8 ± 0.2
astro-ph/9910349 🔍 (source) spectrum z _ { e }
1.202
astro-ph/9910484 🔍 (source) power spectrum \Gamma
1.2000000000000002 +0.09999999999999987-0.10000000000000009
astro-ph/9912127 🔍 (source) unabsorbed reflection spectrum R
0.15
Lower
astro-ph/0001089 🔍 (source) spectrum \nu
-2.25 ± 0.18
astro-ph/0002052 🔍 (source) soft spectrum ( index
3.39 ± 0.24
astro-ph/0003008 🔍 (source) normalisation of the mass power spectrum \sigma _ { 8 }
1.5 ± 0.5
hep-ex/0003006 🔍 (source) differential energy spectrum
6.1e-11 ± 6.999999999999999e-12
astro-ph/0004068 🔍 (source) soft X-ray spectrum kT
0.5 keV
astro-ph/0005335 🔍 (source) plasma spectrum T
0.7 keV
astro-ph/0006255 🔍 (source) power spectrum
-2.14 ± 0.28
astro-ph/0007092 🔍 (source) power spectrum
2.3499999999999996 +0.050000000000000266-0.04999999999999982
Upper
astro-ph/0007092 🔍 (source) power spectrum
1.7
Lower
astro-ph/0007263 🔍 (source) X-ray spectrum \Gamma _ { x }
-4.0
astro-ph/0007274 🔍 (source) source spectrum temperature T _ { 0 }
1.15 +0.15000000000000013-0.1499999999999999 keV
astro-ph/0007284 🔍 (source) fluctuation spectrum \sigma _ { 8 }
1.0
astro-ph/0007377 🔍 (source) thermal spectrum kT _ { 1 }
0.6 keV
astro-ph/0008211 🔍 (source) spectrum
0.44 ± 0.1 (stat)
astro-ph/0009110 🔍 (source) Crab-like spectrum the X-ray flux
2.5e-13 ± 5e-14 erg s-1 cm-2
astro-ph/0009105 🔍 (source) power spectrum P ( k ) ,
-1.8
Lower
astro-ph/0009105 🔍 (source) power spectrum n
-1.8
Lower
astro-ph/0009110 🔍 (source) Crab-like spectrum the X-ray flux f _ { x }
1.25 ± 1.15 keV
astro-ph/0010367 🔍 (source) X-ray spectrum \Gamma
1.27 ± 0.02
astro-ph/0011465 🔍 (source) power spectrum index \beta
1.74
astro-ph/0011469 🔍 (source) power spectrum \ell
197.0 ± 6.0
astro-ph/0011554 🔍 (source) soft thermal spectrum kT
1.3 keV
astro-ph/0012066 🔍 (source) amplitude of the matter power spectrum
6400.0 +2800.0-1800.0
astro-ph/0012356 🔍 (source) spectrum \alpha _ { r }
0.7
Upper
astro-ph/0101213 🔍 (source) normalization of the matter power spectrum \sigma _ { 8 } \Omega _ { m } ^ { 0.48 }
0.51 +0.14-0.17
astro-ph/0102163 🔍 (source) power spectrum \Omega _ { m }
0.3
astro-ph/0103056 🔍 (source) power spectrum shape parameter \Gamma
0.1 ± 0.1
astro-ph/0103084 🔍 (source) column density of the CO observed in the STIS spectrum N ( CO )
71000000000000.0 ± 5000000000000.0 cm-2
astro-ph/0103227 🔍 (source) local color temperature of the spectrum emerging T _ { c } / T _ { eff }
1.4500000000000002 +0.34999999999999987-0.3500000000000001
Lower
astro-ph/0103343 🔍 (source) power law spectrum \alpha _ { x }
0.92 ± 0.04
astro-ph/0103417 🔍 (source) flat spectrum \Gamma
1.7
astro-ph/0104139 🔍 (source) spectrum n
-1.0
astro-ph/0104329 🔍 (source) low-resolution spectrum
-0.89 ± 0.03
astro-ph/0104384 🔍 (source) steep spectrum shell emission \alpha
-0.57
astro-ph/0105022 🔍 (source) steep power spectrum density f ^
-2.0
Lower
hep-ph/0105064 🔍 (source) spectrum m _ { \nu }
0.26 +0.2-0.14 eV
hep-ph/0105064 🔍 (source) spectrum
2.75 +1.28-0.97 eV
astro-ph/0105131 🔍 (source) thin thermal spectrum of temperature
5.8 ± 0.6 keV
astro-ph/0105194 🔍 (source) two-point spectrum of the core emission \alpha _ { rx }
0.75
astro-ph/0105450 🔍 (source) power spectrum \Omega _ { m } h
0.2 ± 0.03
astro-ph/0106029 🔍 (source) steep X-ray spectrum \alpha
1.3 ± 0.1
astro-ph/0106198 🔍 (source) S/N ratio spectrum z _ { em }
2.4
astro-ph/0106417 🔍 (source) spectrum of photon index \gamma
1.63 +0.11-0.1
astro-ph/0109016 🔍 (source) power-law power-spectrum of index n
-1.0
Upper
astro-ph/0109114 🔍 (source) power spectrum normalization \sigma _ { 8 }
0.83
astro-ph/0109374 🔍 (source) LETGS X-ray spectrum
60.0 pc
astro-ph/0110552 🔍 (source) spectrum z _ { em }
3.7
astro-ph/0111577 🔍 (source) power-law spectrum of photon index
1.45 ± 0.19
astro-ph/0201137 🔍 (source) power spectrum of the image features three peaks \ell
213.0 +10.0-13.0
astro-ph/0201137 🔍 (source) power spectrum of the image features three peaks \ell
541.0 +20.0-32.0
astro-ph/0201137 🔍 (source) power spectrum of the image features three peaks \ell
845.0 +12.0-25.0
astro-ph/0201267 🔍 (source) power-law spectrum N _ { H }
8e+22 ± 4e+21 cm-2
astro-ph/0201375 🔍 (source) power spectrum \sigma _ { 8 }
1.0
astro-ph/0202218 🔍 (source) power spectrum n
1.27
Upper
astro-ph/0202290 🔍 (source) Harrison-Zeldovich spectrum m _ { \nu }
0.74 eV
Upper
astro-ph/0204239 🔍 (source) power spectrum \Omega _ { m } h
0.2 ± 0.03
astro-ph/0204361 🔍 (source) soft spectrum
0.6 keV
astro-ph/0205160 🔍 (source) blackbody spectrum T _ { eff }
210000000.0 ± 80000000.0 K
astro-ph/0207213 🔍 (source) power spectrum \epsilon _ { 1 }
0.057
Upper
astro-ph/0207515 🔍 (source) spectrum of the luminous L _ { bol }
10.0 L_\odot
astro-ph/0208501 🔍 (source) BeppoSAX spectrum \alpha _ { x }
0.7
astro-ph/0209127 🔍 (source) column density spectrum f ( N _ { HI } )
-2.8
Lower
astro-ph/0209244 🔍 (source) velocity power spectrum index \beta
1.74
astro-ph/0209478 🔍 (source) spectrum
-0.01
astro-ph/0209487 🔍 (source) differential energy spectrum dN / dE
3.3e-13 ± 9.000000000000001e-14 (stat) ± 3e-14 (syst)
astro-ph/0210007 🔍 (source) scale invariant spectrum n _ { s }
0.97 +0.08-0.05
astro-ph/0210147 🔍 (source) spectrum \alpha
1.18 ± 0.02
astro-ph/0210274 🔍 (source) amplitude of matter power spectrum \sigma _ { 8 }
0.9
astro-ph/0210604 🔍 (source) power spectrum of matter fluctuations { \sigma _ { 8 } ( \Omega _ { m } / 0.3 ) } ^ { 0.57 }
0.71 +0.12-0.16
astro-ph/0211090 🔍 (source) matter power spectrum normalization \sigma _ { 8 }
0.78 +0.3-0.06
astro-ph/0212165 🔍 (source) peak in the power spectrum
144.18 ± 0.06 s
astro-ph/0301037 🔍 (source) spectrum normalization parameter
0.7
Lower
astro-ph/0301037 🔍 (source) spectrum normalization parameter \sigma _ { 8 }
1.1
astro-ph/0301083 🔍 (source) power spectrum \Gamma
0.19 +0.13-0.04
astro-ph/0301297 🔍 (source) AGN X-ray spectrum
3e-07
astro-ph/0301551 🔍 (source) index of primeval fluctuation spectrum n _ { p }
1.0
astro-ph/0302159 🔍 (source) power spectrum normalization C _ { 10 }
690.0 +200.0-125.0 K2
astro-ph/0302307 🔍 (source) spectral index of the positron spectrum \gamma _ { + }
3.4 ± 0.06
astro-ph/0302415 🔍 (source) flat spectrum \alpha
0.05 ± 0.05
astro-ph/0303168 🔍 (source) perturbation spectrum
0.944
astro-ph/0304175 🔍 (source) power spectrum k _ { 0 }
0.76
astro-ph/0304175 🔍 (source) power spectrum
0.05 Mpc-1
astro-ph/0305600 🔍 (source) steep spectrum \alpha
-1.2
astro-ph/0307561 🔍 (source) power law index of the relativistic electron spectrum p
2.25
astro-ph/0308277 🔍 (source) infrared spectrum B
2.6 ± 1.0
astro-ph/0308278 🔍 (source) spectrum T _ {
2.17 +0.25-0.12 keV
astro-ph/0310735 🔍 (source) scale invariant spectrum
0.95 +0.07-0.04
astro-ph/0310735 🔍 (source) scale invariant spectrum n _ { s }
0.97 ± 0.02
astro-ph/0311560 🔍 (source) part of the spectrum the time averaged mass accretion rate
5.7e-13 M_\odot yr-1
Lower
astro-ph/0312357 🔍 (source) mass spectrum slope \alpha
1.6
Upper
astro-ph/0312457 🔍 (source) powerlaw spectrum \Gamma
2.3
astro-ph/0401026 🔍 (source) hard spectrum \Gamma
1.0
astro-ph/0401111 🔍 (source) thermal spectrum kT
0.7 keV
astro-ph/0401515 🔍 (source) fluctuation power spectrum normalization \sigma _ { 8 }
0.8
Upper
astro-ph/0401589 🔍 (source) power density spectrum
1008.0 ± 120.0 s
astro-ph/0403592 🔍 (source) soft spectrum E
-4.6 ± 0.5
astro-ph/0404072 🔍 (source) index of the mass spectrum \alpha
0.6 ± 0.06
astro-ph/0404132 🔍 (source) scale-invariant pressure fluctuation spectrum
90.0
Upper
astro-ph/0405360 🔍 (source) photon spectrum index \Gamma
1.7
astro-ph/0406246 🔍 (source) power spectrum normalization \sigma _ { 8 }
0.7
astro-ph/0406340 🔍 (source) spectrum
21.5 ± 0.5
astro-ph/0407130 🔍 (source) spectrum \alpha _ { 0.843 } ^ { 18
-0.5
Lower
astro-ph/0407203 🔍 (source) spectral slope of the FUSE composite spectrum \alpha
-0.56 +0.38-0.28
astro-ph/0407203 🔍 (source) spectral slope of the FUSE composite spectrum F _ { \nu }
-0.56 +0.38-0.28
astro-ph/0407377 🔍 (source) linear theory power spectrum amplitude \Delta ^ { 2 } _ { L } ( k _ { p }
0.009 s km-1
astro-ph/0408549 🔍 (source) unusually steep spectrum \alpha
-2.1
Upper
astro-ph/0409253 🔍 (source) spectrum of photon index \Gamma
1.3 ± 0.5
astro-ph/0410149 🔍 (source) mean spectrum \Gamma
1.4 ± 0.1
astro-ph/0410149 🔍 (source) mean intrinsic spectrum \Gamma
1.76 ± 0.08
astro-ph/0411474 🔍 (source) power spectrum index \beta
1.74
astro-ph/0501095 🔍 (source) steep radio spectrum \alpha
-0.7
astro-ph/0502064 🔍 (source) spectrum T _ { WD }
120000.0 K
astro-ph/0502114 🔍 (source) thermal X-ray spectrum kT
0.4 keV
astro-ph/0502243 🔍 (source) amplitude of the power spectrum \sigma _ { 8 }
0.81 +0.15-0.1
astro-ph/0502326 🔍 (source) power-law spectrum of photon index
2.02 ± 0.13
nucl-ex/0502021 🔍 (source) B spectrum
1.68 ± 0.06 (stat) +0.08-0.09 (syst)
astro-ph/0503085 🔍 (source) spectrum \alpha
2.82 ± 0.15 (stat) ± 0.3 (sys)
astro-ph/0503242 🔍 (source) slope of the matter power spectrum at large scales n _ { s }
0.98 ± 0.02
astro-ph/0503295 🔍 (source) power spectrum slopes
-1.3
Lower
astro-ph/0503295 🔍 (source) power spectrum slopes
-1.5
astro-ph/0503396 🔍 (source) optical spectrum T _ { eff }
33.0
astro-ph/0504280 🔍 (source) reflectance spectrum
90377.0
astro-ph/0504279 🔍 (source) } keV } spectrum \Gamma
2.0
Lower
astro-ph/0504647 🔍 (source) synchrotron spectrum \alpha
-1.0 ± 0.1
astro-ph/0505370 🔍 (source) steep spectrum \alpha
1.4 ± 0.2
astro-ph/0505478 🔍 (source) Harrison-Zel´dovich density perturbation spectrum n _ { S }
0.95
astro-ph/0506109 🔍 (source) AGN spectrum \Gamma
1.7999999999999998 +0.10000000000000009-0.09999999999999987
astro-ph/0506471 🔍 (source) BH mass spectrum slope
2.5
astro-ph/0506642 🔍 (source) magnetic field power spectrum spectral index n
-2.9
astro-ph/0506682 🔍 (source) radio synchrotron spectrum
1.73 ± 0.01
astro-ph/0507215 🔍 (source) galaxy power spectrum shape \Gamma _ { eff }
0.14 ± 0.02
astro-ph/0507215 🔍 (source) galaxy power spectrum normalisation \sigma _ { 8 } b _ { K } ) ^ { 2 }
1.36 ± 0.1
astro-ph/0507489 🔍 (source) flat spectrum \alpha _ { 1.7 GHz } ^ { 5 GHz }
-0.2 ± 0.1
astro-ph/0507591 🔍 (source) power spectrum M _ { rms }
1.0
astro-ph/0509478 🔍 (source) spectrum n _ { s }
0.97
gr-qc/0512100 🔍 (source) spectral index of its spectrum n _ { 1 }
0.9483
Lower
astro-ph/0601242 🔍 (source) cutoff to the spectrum
1300000000.0
astro-ph/0602246 🔍 (source) core mass spectrum \alpha
2.1 ± 0.4
astro-ph/0602413 🔍 (source) normalization of the matter power spectrum \sigma _ { 8 }
1.03 +0.2-0.29
astro-ph/0602511 🔍 (source) radio spectrum \alpha _ { thin }
0.5
Upper
astro-ph/0603146 🔍 (source) power spectrum normalizations \sigma _ { 8 }
0.7
astro-ph/0604335 🔍 (source) power spectrum \sigma _ { 8 }
0.85 ± 0.02
astro-ph/0605004 🔍 (source) Harrison–Zel ’ dovich spectrum n _ { S }
1.0
astro-ph/0605046 🔍 (source) index of the source spectrum x
2.23 ± 0.07
astro-ph/0605051 🔍 (source) break frequency of the spectrum \nu _ { thin }
37000000000000.0 Hz
astro-ph/0606308 🔍 (source) mass spectrum M
1.8 M_\odot
Lower
astro-ph/0606384 🔍 (source) spectrum z
0.263 +0.012-0.01
astro-ph/0606571 🔍 (source) mass power spectrum normalisation \sigma _ { 8 }
0.8 ± 0.1
astro-ph/0606611 🔍 (source) mass power spectrum normalisation \sigma _ { 8 , CDFS }
0.52 +0.11-0.15 (stat) ± 0.07 (% sys)
astro-ph/0607353 🔍 (source) energy spectrum d \log n / d \log \varepsilon
-2.0
astro-ph/0607394 🔍 (source) power spectrum normalization \sigma _ { 8 }
0.74
astro-ph/0608433 🔍 (source) power spectrum spectral index n
2.0
astro-ph/0610164 🔍 (source) /IRS mid-infrared spectrum L _ { IR }
400000000000.0 L_\odot
hep-th/0610205 🔍 (source) blue spectrum n _ { S }
0.0
Upper
astro-ph/0611349 🔍 (source) HST spectrum
-2.3 ± 0.1
astro-ph/0611655 🔍 (source) spectrum synchrotron \alpha
-0.7
astro-ph/0611655 🔍 (source) flat spectrum free-free ( Bremsstrahlung \alpha
0.1
astro-ph/0612594 🔍 (source) powerlaw spectrum of photon index
2.03 +0.51-0.36
astro-ph/0701095 🔍 (source) source spectrum
7e-14 ± 9e-15 erg cm-2 s-1
astro-ph/0701131 🔍 (source) normalisation of the power spectrum fluctuations \sigma _ { 8 }
0.74
astro-ph/0701611 🔍 (source) powerlaw spectrum of photon index
2.03 +0.51-0.36
astro-ph/0701776 🔍 (source) spectrum \alpha
0.8
astro-ph/0703083 🔍 (source) spectrum N ( H _ { I } )
4.5e+20 cm-2
astro-ph/0703234 🔍 (source) strain power spectrum
6.1e-48 s
astro-ph/0703234 🔍 (source) strain power spectrum
8.499999999999999e-49 s
Lower
astro-ph/0703802 🔍 (source) power-law spectrum of a photon index \Gamma
1.1 ± 0.2
0704.3851 🔍 (source) power spectrum \boldsymbol { v }
-1.69
0705.3611 🔍 (source) spectrum \alpha
0.2
0706.0517 🔍 (source) suppression of the gamma-ray spectrum E _ { \gamma }
-2.0
0707.3529 🔍 (source) spectrum n _ { H }
1.9
0707.3529 🔍 (source) spectrum \Gamma _ { ext }
1.9
0707.3529 🔍 (source) spectrum \Gamma _ { comp }
1.3
0708.2030 🔍 (source) \alpha forest power spectrum m _ { \nu _ { s }
1.7 keV
Lower
0709.2604 🔍 (source) near-infrared spectrum T _ { eff }
55.0
0709.4584 🔍 (source) spectrum \Gamma _ { int }
1.5
0709.4532 🔍 (source) spectrum \alpha
-1.0
Upper
0709.4532 🔍 (source) spectrum \alpha _ { 0 }
-0.45 ± 0.12
0709.4584 🔍 (source) spectrum \Gamma
2.5 ± 0.19 (stat) ± 0.1 (syst)
0710.5183 🔍 (source) X-ray spectrum N _ { H }
3e+23 cm-2
0711.2529 🔍 (source) power spectrum of the flux
76.8 Mpc
Upper
0712.1909 🔍 (source) energy spectrum
90.0
0712.3293 🔍 (source) power spectrum normalisation \sigma _ { 8 }
0.92 +0.26-0.3
0712.3293 🔍 (source) power spectrum normalisation \Omega _ { m }
0.92 +0.26-0.3
0801.1193 🔍 (source) SFG spectrum log ( Z / Z _ { \odot } )
-0.699 s
0802.1069 🔍 (source) power spectrum normalization \sigma _ { 8 }
0.85
0802.2961 🔍 (source) power spectrum shape parameter \Gamma
0.15 +0.18-0.08
0804.4007 🔍 (source) X-ray spectrum \Gamma
2.1
0804.4007 🔍 (source) X-ray spectrum \Gamma
0.8
0805.0691 🔍 (source) velocity power spectrum n
3.8
0805.3151 🔍 (source) power spectrum of density fluctuations
1.57
0805.4645 🔍 (source) steeper spectrum \beta
3.0
0808.0857 🔍 (source) flat spectrum \Gamma
1.0
0809.1321 🔍 (source) turbulence energy spectrum function \beta
2.0
0809.2104 🔍 (source) spectral index of the primordial perturbation spectrum n _ { s }
0.935
0810.2522 🔍 (source) differential spectral index of the intrinsic spectrum
1.28 ± 0.2
0811.1466 🔍 (source) power spectrum
-3.24 ± 0.03
0811.1466 🔍 (source) power spectrum
-3.2
Lower
0811.1466 🔍 (source) power spectrum
-2.2
Upper
0811.3759 🔍 (source) steep spectrum \alpha
2.7
0812.4151 🔍 (source) softness of its X-ray spectrum kT
117.0 ± 14.0 eV
0901.4576 🔍 (source) power spectrum n
-2.5
Lower
0901.4561 🔍 (source) spectrum \Gamma
1.86 ± 0.37 (stat)
0901.4576 🔍 (source) power spectrum P ( k ) \propto k ^ { n }
-2.5
Lower
0902.2927 🔍 (source) spectrum \Gamma
1.8
0902.4466 🔍 (source) power spectrum
-5.0
Upper
0904.0404 🔍 (source) polarization power spectrum \delta T
3.3 K
0904.0613 🔍 (source) optical spectrum T _ { eff }
7000.0 K
0904.1200 🔍 (source) power spectrum
3.8 ± 0.6
0904.1200 🔍 (source) power spectrum P ( k _ { \theta }
3.9 ± 0.6
0905.0499 🔍 (source) linear source power spectrum \Delta ^ { 2 }
0.35 +0.15000000000000002-0.14999999999999997
0905.3176 🔍 (source) power spectrum of PSF size \delta _ { R ^ { 2 } }
2e-12
Lower
0906.0234 🔍 (source) harder X-ray spectrum \Gamma
1.5 ± 0.01
0907.0486 🔍 (source) primordial power spectrum
0.742
0907.0486 🔍 (source) primordial power spectrum \sigma _ { 8 }
0.798
0907.0832 🔍 (source) energy spectrum
17.7
0907.1659 🔍 (source) power spectrum \chi ^ { 2 }
39.6
0907.1659 🔍 (source) power spectrum \Omega _ { m }
0.289 ± 0.019
0907.2907 🔍 (source) energy spectrum exponent \alpha
-2.0
0907.4453 🔍 (source) normalization of the linear power spectrum \sigma _ { 8 }
0.9 ± 0.04
0909.1837 🔍 (source) spectrum
0.42 ± 0.86
0909.5198 🔍 (source) steep spectrum \alpha
2.6
Upper
0909.5383 🔍 (source) soft X-ray spectrum \hat { a }
0.56 ± 0.02
0909.5562 🔍 (source) spectrum { \bf E ^ { 2 } F _ { \nu } ( E )
2.9e-07 GeV cm-2 s-1 sr-1
Upper
0910.1384 🔍 (source) power spectrum of integrated intensity \ell
0.16 pc
Lower
0911.0961 🔍 (source) power spectrum n _ { t }
0.0
0911.2709 🔍 (source) X-ray spectrum \Delta \Gamma _ { X }
0.7
1001.1655 🔍 (source) power spectrum \Delta \nu
3.47 ± 0.12 Hz
1001.4538 🔍 (source) power-law index of the primordial power spectrum n _ { s }
0.968 ± 0.012
1001.4744 🔍 (source) power-law index of the primordial power spectrum n _ { s }
0.963 ± 0.012
1002.1815 🔍 (source) radio spectrum of index \alpha
-0.26 ± 0.04
1003.2911 🔍 (source) spectrum of tensor-to-scalar ratio r
0.001
1004.3771 🔍 (source) normalization of the linear power spectrum \sigma _ { 8 }
0.91 +0.07-0.08
1005.4410 🔍 (source) bispectrum non-gaussianity parameter f _ { NL }
10.0
Lower
1005.4554 🔍 (source) spectrum N _ { H }
3e+22
1006.5463 🔍 (source) spectrum \Gamma
2.67 ± 0.1 (stat) ± 0.08 (sys)
1007.3736 🔍 (source) spectrum \beta
0.08
1008.1068 🔍 (source) power-law spectrum \Gamma
1.26
1008.1218 🔍 (source) power spectrum slope \beta
2.8
1008.2724 🔍 (source) scale invariant spectrum | 8 n _ { T } | / r
1.0
Upper
1008.3491 🔍 (source) normalisation of the intrinsic alignment power spectrum
0.077 ± 0.008
1009.6102 🔍 (source) X-ray spectrum temperature T _ { X
45.0
1010.1267 🔍 (source) hard spectrum \Gamma _ { eff }
-0.34 +0.57-0.61
1010.2636 🔍 (source) power spectrum of tensor-to-scalar ratio r
1.0
1010.5379 🔍 (source) \nu F _ { \nu } spectrum E _ { p }
240.0 keV
1011.0387 🔍 (source) temporal spectrum
6343.0 Hz
1012.2978 🔍 (source) power spectrum of density fluctuations P _ { \delta }
0.002
Lower
1101.3581 🔍 (source) late-time spectrum
2.0 yr
1101.5637 🔍 (source) blackbody spectrum kT
130.0 eV
1103.5166 🔍 (source) point source spectrum \Gamma
1.44 ± 0.07
1104.0205 🔍 (source) flatter spectrum \alpha
-0.4
1105.2303 🔍 (source) frequency part of the spectrum f
5.05 ± 4.95 Hz
Lower
1105.5711 🔍 (source) spectrum source \alpha
-0.6
1106.0861 🔍 (source) spectrum integrated flux
2770000.0 ± 260000.0 (stat) ± 320000.0 (syst) cm-2 s-1
1106.3484 🔍 (source) neutrino spectrum
2.5e-10 cm-2 s-1 TeV-1
1108.2730 🔍 (source) perturbation spectrum n _ { s }
1.0
1109.1026 🔍 (source) energy spectrum \varepsilon _ { k }
0.0
1109.2778 🔍 (source) steep blue anisotropic spectrum n _ { de }
3.1 ± 1.5
1109.3261 🔍 (source) spectrum \alpha
210.0
1109.3261 🔍 (source) spectrum
1.8
1109.4038 🔍 (source) spectrum
-0.1
1109.4395 🔍 (source) power-law spectrum \Gamma
1.66 ± 0.08
1109.5706 🔍 (source) blackbody spectrum \beta
2.0
1111.6186 🔍 (source) Fourier power spectrum P ( k )
-2.17
1112.5723 🔍 (source) linear angular power spectrum \Omega _ { m }
0.31 +0.18-0.11
1201.2044 🔍 (source) steep spectrum \Gamma _ { X }
2.25 ± 0.04999999999999982
1202.4921 🔍 (source) spectrum T _ { eff }
30000.0 ± 5000.0 K
1203.3424 🔍 (source) radio spectrum \alpha
1.5
1203.6654 🔍 (source) CMB trispectrum both \tau _ { nl }
0.0
1204.4239 🔍 (source) power-law spectrum in momentum p ^
-2.45 ± 0.4
1208.5866 🔍 (source) Scoreproducessomeofthestructuresthatwereobservedinthecircumstellarabsorptionlinesinthespectrumof
2e-06 ± 5e-07 M_\odot Th yr-1
1209.4068 🔍 (source) spectrum \sigma
0.08 ± 0.02 keV
1209.5423 🔍 (source) spectrum N _ { H , int } ( z = 1.3 )
2e+22 cm-2
1209.6602 🔍 (source) spectrum \alpha
-0.23 ± 0.2
1210.3298 🔍 (source) power spectrum index n
-3.0
1211.2510 🔍 (source) spectrum slope parameter \alpha _ { ox }
0.3838 F
1212.3327 🔍 (source) normalisation of the matter power spectrum \sigma _ { 8 }
0.771 ± 0.041
1301.0824 🔍 (source) thermal SZ power spectrum
3.4 ± 1.4 K2
1302.5452 🔍 (source) spectrum
0.13
Upper
1303.1808 🔍 (source) normalisation of the matter power spectrum \sigma _ { 8 }
0.799 ± 0.015
1303.3039 🔍 (source) thermal infrared spectrum
755.0 ± 745.0
1303.3535 🔍 (source) normalization of the matter power spectrum \sigma _ { 8 }
0.786 ± 0.031
1303.5081 🔍 (source) power spectrum { \sigma _ { 8 } ( \Omega _ { m } / 0.28 ) } ^ { 3.2 / 8.1 }
0.784 ± 0.016 (68 % \% C)
1304.1216 🔍 (source) amplitude of the local-shape bispectrum f _ { NL } ^ { local * }
-14.0 +22.0-21.0
1305.0572 🔍 (source) photon index of the LAT spectrum \Gamma
2.6 ± 0.06
1306.2172 🔍 (source) spectrum \nu
4.0
1306.4024 🔍 (source) optical spectrum
30.0 ± 210.0 K W
1306.4024 🔍 (source) optical spectrum
12.0
1306.5475 🔍 (source) transmission spectrum
-0.079 ± 0.012
1306.5475 🔍 (source) transmission spectrum
-0.138 ± 0.013
1306.5475 🔍 (source) transmission spectrum
-0.059 ± 0.012
1306.5475 🔍 (source) transmission spectrum
-0.123 ± 0.012
1306.5475 🔍 (source) transmission spectrum
-0.071 ± 0.016
1306.6624 🔍 (source) radio spectrum \alpha
-0.24 ± 0.42
1308.5341 🔍 (source) local-form bispectrum parameter
5.0
1308.5968 🔍 (source) power spectrum slope \beta
2.3 +0.8-0.6
1309.3282 🔍 (source) cross-power spectrum { \sigma _ { 8 } ( \Omega _ { M } / 0.30 ) } ^ { 0.26 }
0.8 ± 0.02
1309.5261 🔍 (source) slope of the transmission spectrum constraining the quantity \alpha T
-3528.0 ± 660.0 K
1310.6499 🔍 (source) power spectrum H _ { \alpha } V / R
0.011873 day-1
1310.8287 🔍 (source) spectrum
1.72 +1.35-0.89 GeV
1310.8617 🔍 (source) ‘ local ’ trispectrum shape g _ { NL } / 10 ^ { 5 }
-4.1 ± 2.3
1401.8025 🔍 (source) radio spectrum \alpha
-0.52 ± 0.07
1403.1667 🔍 (source) spectrum of high-redshift
-770.0 GHz
1403.5231 🔍 (source) temperature power spectrum r _ { 0.002 }
0.11
Upper
1403.5372 🔍 (source) proton spectrum
2.68 ± 0.04
1403.7623 🔍 (source) spectrum amplitude ratio of bounce-to-inflation r _ { B }
0.71 ± 0.09
1404.0017 🔍 (source) spectrum
1.0
1404.3813 🔍 (source) total matter power spectrum
0.05
1404.3813 🔍 (source) total matter power spectrum
0.03
1405.1188 🔍 (source) tensor spectrum n _ { T }
1.0
Lower
1405.2594 🔍 (source) spectrum A _ { flux }
1.03 ± 0.02
1405.3056 🔍 (source) red-tilt spectrum n _ { s }
0.96
1405.7396 🔍 (source) hard spectrum E _ { peak }
1.0
1405.7974 🔍 (source) power spectrum c _ { T } ^ { 2 }
2.33
Upper
1405.7969 🔍 (source) amplitude of oscillations in the power-spectrum \rho _ { h } / \rho _ { I }
0.01
Upper
1406.4157 🔍 (source) power spectrum amplitude k
0.1
1407.1836 🔍 (source) bispectrum of dark matter k _ { i }
0.1 h
Upper
1407.1897 🔍 (source) spectrum L / L _ { Edd }
0.008
1407.5081 🔍 (source) peculiar hard spectrum \Gamma
0.8
1408.2397 🔍 (source) soft spectrum
0.7 +0.10000000000000009-0.09999999999999998 keV
1408.2397 🔍 (source) soft spectrum kT
2000.0 yr
1408.3736 🔍 (source) CMB temperature power spectrum \Omega _ { CDM }
0.22
1408.5281 🔍 (source) flux spectrum \Gamma
1.68 +0.03-0.02
1408.5281 🔍 (source) flux spectrum \Gamma
1.78 +0.02-0.03
1409.2004 🔍 (source) electromagnetic spectrum of PWNe in free expansion t _ { age }
10.0 kyr
Upper
1409.5437 🔍 (source) ultra-steep spectrum \alpha
-1.1
Upper
1410.1500 🔍 (source) power-law X-ray spectrum \Gamma
2.0
1411.3193 🔍 (source) shear power spectrum \sqrt { A }
9e-06
1412.4760 🔍 (source) ratio of the spectrum A _ { MV }
0.92 ± 0.14 (Stat) ± 0.08 (Sys)
1501.04144 🔍 (source) IRS spectrum
3.0 AU
1502.04501 🔍 (source) GTC/CanariCam nuclear spectrum
50.0 pc
1506.07526 🔍 (source) power spectrum dz|
1.0
Upper
1507.00859 🔍 (source) spectrum \alpha
0.0 ± 0.07
1507.02308 🔍 (source) tilted spectrum of scalar perturbations n _ { s }
0.96
1507.08977 🔍 (source) energy spectrum
2.6 ± 0.8 MeV
1509.00315 🔍 (source) radial velocity of the spectrum
417.0 ± 4.0 km s-1
1510.02288 🔍 (source) ii optical spectrum T _ { eff }
24.0
1510.02681 🔍 (source) power-law spectrum \Gamma
1.7 +0.57-0.45
1510.05649 🔍 (source) oscillation spectrum \omega _ { R } / \mu
1.0
1510.08716 🔍 (source) power spectrum c _ { T }
1.0
1511.03283 🔍 (source) steep spectrum \alpha
-1.8
Lower
1512.01242 🔍 (source) \gamma -ray spectrum \Gamma
2.78 ± 0.14
1512.04825 🔍 (source) power spectrum of the source
0.006500000000000001 +0.0005-0.0011 Hz
1601.00660 🔍 (source) radio spectrum \alpha
-0.7
1601.02542 🔍 (source) X-ray spectrum \Gamma
0.0
1603.01226 🔍 (source) flat spectrum \alpha
-0.03 ± 0.03
1604.07871 🔍 (source) clustering amplitude of the matter power spectrum \sigma _ { 8 }
0.74 ± 0.13
1605.00016 🔍 (source) power spectrum
21.0 cm
1605.00270 🔍 (source) parallax of this flat-spectrum variable radio
2.2 +0.5-0.3 kpc day
1605.02403 🔍 (source) suppression of the matter power spectrum \Delta P / P
8.0
1605.04646 🔍 (source) power spectrum of the curvature perturbations
0.018
Upper
1605.04788 🔍 (source) spectrum k _ { max }
0.5 h
Lower
1605.08360 🔍 (source) power spectrum \gamma
-2.9 ± 0.1
1606.01968 🔍 (source) amplitude of the spectrum A _ { L } ^ { \phi \phi }
1.15 ± 0.36
1607.06858 🔍 (source) CMB power spectrum
6.2
1607.06858 🔍 (source) CMB power spectrum
-6.0
Lower
1608.01684 🔍 (source) spectrum E
3.54 ± 0.02 keV
1608.02583 🔍 (source) power-law spectrum \Gamma
1.7
1608.06281 🔍 (source) cosmological power spectrum \Delta ^ { 2 }
27000.0 mK2
Upper
1608.07012 🔍 (source) slope of the velocity power spectrum
22.0
1609.02518 🔍 (source) spectrum d
24.0 pc
1609.05210 🔍 (source) Grating spectrum
4700.0 +2700.0-1500.0 km s-1
1609.07739 🔍 (source) spectrum \log T _ { eff }
3.7
Lower
1610.02174 🔍 (source) rotational spectrum of the formaldehyde isotopologue H _ { 2 } C ^ { 17 } O
0.56
Lower
1610.03504 🔍 (source) spectrum R
50.0
1610.03504 🔍 (source) spectrum R
135.0
1611.00475 🔍 (source) spectrum Vr ( DIBs )
-12.0 km s-1
1612.05645 🔍 (source) growth rate times the matter power spectrum normalisation parameter
0.55 ± 0.12
1612.05645 🔍 (source) growth rate times the matter power spectrum normalisation parameter f \sigma _ { 8 }
0.4 ± 0.11
1612.06409 🔍 (source) emission spectrum of the R
50.0
1612.06409 🔍 (source) emission spectrum of the R
70.0
1702.01761 🔍 (source) spectrum k
-0.06 s km-1
1702.01764 🔍 (source) power spectrum
5.3
Lower
1702.01764 🔍 (source) power spectrum
1.4 keV
Lower
1703.03103 🔍 (source) flux spectrum
23.4 +15.6-5.4
1703.03410 🔍 (source) steep X-ray spectrum \Delta \Gamma
1.8 ± 0.4
1703.06802 🔍 (source) spectrum \alpha _ { 118 MHz } ^ { 1.78 GHz }
1.33 ± 0.08
1703.06802 🔍 (source) spectrum \alpha
1.5
1703.10538 🔍 (source) matter power spectrum normalization on scales 8 h ^ { -1 } Mpc w
-1.0
1704.03461 🔍 (source) CIP power spectrum A _ { CIP }
0.017
Upper
1706.08972 🔍 (source) tSZ power spectrum \sigma _ { 8 }
0.85
1707.05416 🔍 (source) spectrum \alpha _ { \nu }
-1.4
1708.00697 🔍 (source) power spectrum w
-1.0 ± 0.2
1708.01315 🔍 (source) optical spectrum T _ { eff }
56.0
1708.04694 🔍 (source) amplitude of the power spectrum of this white noise
9e-14
Upper
1710.05852 🔍 (source) spectrum \Gamma
2.4 ± 0.8
1712.00788 🔍 (source) primordial power spectrum w
-1.1 ± 0.12
1712.07253 🔍 (source) broken power-law spectrum E _ { break }
200.0 keV
1801.07545 🔍 (source) spectral index of the density fluctuation spectrum
-1.7
1802.00999 🔍 (source) spectrum old
5.0 Gyr
Lower
1802.05172 🔍 (source) spectrum E
3000000000000000.0 eV
1803.10213 🔍 (source) power-law spectral index of the X-ray spectrum
2.0
Lower
1804.05056 🔍 (source) particle spectrum hardens \alpha _ { e }
-1.8
1805.06984 🔍 (source) power spectrum P _ { R }
3.0000000000000004e-09
Upper
1805.09942 🔍 (source) spectrum
6.08 ± 0.18 %
1805.11168 🔍 (source) spectrum \Gamma
2.17 ± 0.06
1805.11168 🔍 (source) spectrum \Gamma
1.79 ± 0.12
1805.11607 🔍 (source) amplitude of the kSZ power spectrum D _ { 3000 } ^ { kSZ }
4.1 K2
1805.11396 🔍 (source) optical spectrum [ Fe / H ]
-0.6 ± 0.07
1806.01227 🔍 (source) spectral index of the power spectrum of linear density fluctuations P ( k ) : N ^ { 2 }
2.09e-10 ± 3.3e-11
1806.04194 🔍 (source) power-law index of the spectrum s _ { cr }
2.1500000000000004 +0.04999999999999982-0.050000000000000266
1806.06795 🔍 (source) mass spectrum
31.96 M_\odot
Upper
1806.11114 🔍 (source) spectrum
0.21 ± 0.05
1807.05441 🔍 (source) radio spectrum of slope \alpha
2.5
Lower
1808.05235 🔍 (source) power spectrum density
1.82 ± 0.14
1808.07486 🔍 (source) polarization power spectrum
95.0
Lower
1809.06661 🔍 (source) power spectrum of redshifted 21-cm brightness temperature fluctuations
22.5 ± 2.6999999999999993
1809.06661 🔍 (source) 21-cm power spectrum \Delta _ { 21 } ^ { 2 }
14561.0 mK
Upper
1810.02374 🔍 (source) power spectrum \sum m _ { \nu }
13.0
1811.08430 🔍 (source) spectrum \alpha
-2.0
Upper
1811.10609 🔍 (source) spectrum k
0.36
1812.07350 🔍 (source) spectrum ( photon index
1.7 ± 0.2
1904.02116 🔍 (source) amplitude of the cross-spectrum \widehat { A } _ { lens }
1.7 ± 0.48
1906.07792 🔍 (source) diffuse steep spectrum emission \alpha
-1.1
Upper
1907.01997 🔍 (source) \gamma -ray spectrum hardens \Gamma _ { \gamma }
1.82 ± 0.04
1908.01774 🔍 (source) halo bispectrum up to scales k _ { max }
0.08 h Mpc-1
Upper
1908.10006 🔍 (source) time-averaged X-ray spectrum
84.3 ± 83.7
Upper
1910.02395 🔍 (source) scale invariant power spectrum D _ { \ell \in [ 2 , 350 ] } ^ { \alpha \alpha }
4.7100000000000006e-05 rad2
Upper
1911.00531 🔍 (source) ultra-steep spectrum \alpha _ { 144 MHz } ^ { 1.4 GHz }
-1.84
Upper
1912.00995 🔍 (source) tilt of tensor power spectrum n _ { t }
-0.01 ± 0.31
1912.01675 🔍 (source) antiproton spectrum T
0.07
Lower
1912.02264 🔍 (source) hard power-law spectrum \Gamma
1.6 ± 0.3
2001.07138 🔍 (source) ATCA spectrum \alpha
-1.18 +1.04-0.88
2001.11063 🔍 (source) strength of the stellar ionizing spectrum Z _ { \star }
20.0 ± 5.0
2002.02575 🔍 (source) spectrum k
3.0 h Mpc-1
2002.11857 🔍 (source) spectrum residual
0.204 ± 0.011
2002.11857 🔍 (source) spectrum residual A _ { spec }
0.615 ± 0.068
2003.07387 🔍 (source) power spectrum to permille-level precision \sum m _ { \nu }
0.3 eV
Upper
2003.11730 🔍 (source) thermal spectrum
85.0 %
2005.00892 🔍 (source) mass spectrum parameters M _ { 0 }
17.0 M_\odot
2005.05401 🔍 (source) magnetic energy spectrum slopes
-2.9
Lower
2005.05401 🔍 (source) magnetic energy spectrum slopes n _ { B }
-2.1
2005.05401 🔍 (source) steep initial power spectrum slope n _ { B }
-2.1
2006.00615 🔍 (source) red-side spectrum \lambda _ { \text { rest }
1290.0
Lower
2006.04844 🔍 (source) spectrum \alpha
-1.1
2006.05222 🔍 (source) synchrotron spectrum \alpha _ { \nu }
0.87 +0.08-0.1
2006.08061 🔍 (source) amplitude of the scale-invariant cosmic rotation power spectrum
1e-05 rad2
Upper
2007.08999 🔍 (source) power spectrum z _ { eff }
1.48
2007.09008 🔍 (source) normalisation of the linear power spectrum D _ { H } ( z _ { eff } ) / r _ { drag }
20.0 +2.4-2.2