1 | active galactic nucleus | AGN | 2443 | 99 | 2.004922 | 1407.1154,1407.3583,etc |
2 | spectral energy distribution | SED | 1132 | 99 | 1.001868 | 1407.1783,1407.8260,etc |
3 | cosmic microwave background | CMB | 1077 | 95 | 2.002538 | 1407.7123,1407.4639,etc |
4 | point spread function | PSF | 869 | 72 | 2.003605 | 1407.1154,1407.7546,etc |
5 | interstellar medium | ISM | 525 | 65 | 1.001894 | 1407.4745,1407.8306,etc |
6 | signal to noise ratio | SNR | 463 | 64 | 1.001139 | 1407.7516,1407.4804,etc |
7 | sloan digital sky survey | SDSS | 956 | 55 | 2.002246 | 1407.3276,1407.0307,etc |
8 | star formation rate | SFR | 1504 | 53 | 2.00382 | 1407.0706,1407.0307,etc |
9 | initial mass function | IMF | 595 | 52 | 1.003037 | 1407.4804,1407.1510,etc |
10 | field of view | FoV | 239 | 48 | 1.00096 | 1407.4605,1407.6282,etc |
11 | dark matter | DM | 1367 | 42 | 1.006898 | 1407.0034,1407.4530,etc |
12 | nasa/ipac extragalactic database | NED | 103 | 41 | 1.000388 | 1407.1154,1407.0307,etc |
13 | supernova | SN | 2532 | 40 | 1.009689 | 1407.5797,1407.0034,etc |
14 | near infrared | NIR | 511 | 38 | 2.002249 | 1407.2011,1407.0262,etc |
15 | full width at half maximum | FWHM | 163 | 36 | 2.000735 | 1407.7527,1407.4151,etc |
16 | markov chain monte carlo | MCMC | 174 | 35 | 1.000788 | 1407.7516,1407.4808,etc |
17 | equivalent width | EW | 656 | 32 | 2.002293 | 1407.1154,1407.4804,etc |
18 | ultraviolet | UV | 450 | 31 | 1.003104 | 1407.8228,1407.2956,etc |
19 | infrared | IR | 1180 | 30 | 2.005777 | 1407.1154,1407.8214,etc |
20 | cold dark matter | CDM | 348 | 30 | 2.002525 | 1407.3276,1407.7561,etc |
21 | gamma ray burst | GRB | 1287 | 29 | 2.0061 | 1407.8117,1407.0584,etc |
22 | smoothed particle hydrodynamics | SPH | 224 | 29 | 1.001054 | 1407.5797,1407.0034,etc |
23 | radial velocity | RV | 598 | 28 | 2.004012 | 1407.7516,1407.4457,etc |
24 | white dwarf | WD | 975 | 27 | 2.007568 | 1407.6231,1407.3798,etc |
25 | asymptotic giant branch | AGB | 820 | 27 | 1.003931 | 1407.8306,1407.0584,etc |
26 | polycyclic aromatic hydrocarbon | PAH | 691 | 26 | 2.005768 | 1407.1154,1407.8307,etc |
27 | adaptive optics | AO | 522 | 25 | 2.005961 | 1407.8205,1407.1154,etc |
28 | hubble space telescope | HST | 171 | 24 | 2.001034 | 1407.2011,1407.0584,etc |
29 | signal to noise | S/N | 133 | 24 | 1.000855 | 1407.1154,1407.8366,etc |
30 | main sequence | MS | 488 | 24 | 2.002613 | 1407.8214,1407.6212,etc |
31 | magnetohydrodynamic | MHD | 251 | 23 | 2.001884 | 1407.2381,1407.8228,etc |
32 | intergalactic medium | IGM | 206 | 23 | 1.001326 | 1407.0034,1407.7561,etc |
33 | black hole | BH | 1069 | 23 | 2.008469 | 1407.0034,1407.2405,etc |
34 | color magnitude diagram | CMD | 251 | 22 | 1.001684 | 1407.2011,1407.0020,etc |
35 | red giant branch | RGB | 277 | 22 | 2.003291 | 1407.2011,1407.0584,etc |
36 | supernova remnant | SNR | 940 | 22 | 2.009099 | 1407.6231,1407.8260,etc |
37 | general relativity | GR | 342 | 22 | 2.001743 | 1407.7293,1407.7561,etc |
38 | equation of state | EOS | 135 | 22 | 2.00154 | 1407.7672,1407.2130,etc |
39 | large magellanic cloud | LMC | 302 | 22 | 2.003168 | 1407.6366,1407.6468,etc |
40 | gemini planet imager | GPI | 693 | 20 | 2.004395 | 1407.2313,1407.2555,etc |
41 | very large array | VLA | 199 | 20 | 1.001548 | 1407.0706,1407.2653,etc |
42 | globular cluster | GC | 1215 | 20 | 2.005395 | 1407.1510,1407.6468,etc |
43 | star formation history | SFH | 122 | 20 | 1.002031 | 1407.8366,1407.2405,etc |
44 | coronal mass ejection | CME | 1167 | 19 | 1.010025 | 1407.8117,1407.4385,etc |
45 | probability density function | PDF | 165 | 19 | 2.001527 | 1407.4457,1407.7549,etc |
46 | cosmic ray | CR | 575 | 19 | 2.003991 | 1407.2243,1407.4530,etc |
47 | three dimensional | 3D | 150 | 18 | 1.001146 | 1407.6039,1407.8456,etc |
48 | line of sight | LOS | 161 | 18 | 2.000791 | 1407.3171,1407.7477,etc |
49 | local thermodynamic equilibrium | LTE | 111 | 18 | 1.000514 | 1407.7477,1407.2215,etc |
50 | supermassive black hole | SMBH | 265 | 18 | 2.003883 | 1407.2243,1407.6468,etc |
51 | neutron star | NS | 413 | 17 | 2.003741 | 1407.3163,1407.2405,etc |
52 | standard model | SM | 191 | 17 | 2.002236 | 1407.0688,1407.2848,etc |
53 | very large telescope | VLT | 96 | 17 | 1.000787 | 1407.8306,1407.4804,etc |
54 | kolmogorov smirnov | KS | 70 | 17 | 1.000471 | 1407.3276,1407.6212,etc |
55 | milky way | MW | 242 | 16 | 1.002509 | 1407.2011,1407.0024,etc |
56 | integral field spectrograph | IFS | 92 | 16 | 1.000824 | 1407.2313,1407.2555,etc |
57 | adaptive mesh refinement | AMR | 53 | 16 | 1.000456 | 1407.7561,1407.7124,etc |
58 | canada france hawaii telescope | CFHT | 117 | 16 | 2.00072 | 1407.7868,1407.7764,etc |
59 | two dimensional | 2D | 110 | 15 | 1.001106 | 1407.6039,1407.1154,etc |
60 | max planck institute for astronomy | MPIA | 16 | 15 | 1.00003 | 1407.3276,1407.0706,etc |
61 | brightest cluster galaxy | BCG | 722 | 15 | 2.007843 | 1407.0262,1407.4693,etc |
62 | baryon acoustic oscillations | BAO | 184 | 15 | 1.002337 | 1407.3583,1407.2274,etc |
63 | square kilometre array | SKA | 95 | 15 | 1.002284 | 1407.6366,1407.0034,etc |
64 | max planck institute for astrophysics | MPA | 18 | 14 | 1.000054 | 1407.3276,1407.0706,etc |
65 | large scale structure | LSS | 56 | 14 | 1.001503 | 1407.0376,1407.2950,etc |
66 | star formation | SF | 831 | 14 | 2.00345 | 1407.5797,1407.4731,etc |
67 | two micron all sky survey | 2MASS | 57 | 14 | 1.000398 | 1407.4820,1407.8502,etc |
68 | australia telescope compact array | ATCA | 106 | 14 | 1.000737 | 1407.2653,1407.5482,etc |
69 | luminosity function | LF | 467 | 13 | 2.003606 | 1407.2011,1407.1510,etc |
70 | planetary nebula | PN | 918 | 13 | 2.011675 | 1407.6231,1407.0109,etc |
71 | giant molecular cloud | GMC | 241 | 13 | 2.002919 | 1407.5062,1407.6468,etc |
72 | wilkinson microwave anisotropy probe | WMAP | 35 | 13 | 1.000763 | 1407.3544,1407.7561,etc |
73 | big bang nucleosynthesis | BBN | 239 | 13 | 2.00445 | 1407.3544,1407.7465,etc |
74 | zero age main sequence | ZAMS | 46 | 13 | 2.000225 | 1407.7549,1407.2405,etc |
75 | large area telescope | LAT | 166 | 13 | 2.0019 | 1407.0862,1407.2243,etc |
76 | simple stellar population | SSP | 96 | 13 | 2.000881 | 1407.7543,1407.3129,etc |
77 | probability distribution function | PDF | 574 | 13 | 2.006011 | 1407.4693,1407.2637,etc |
78 | far infrared | far-IR | 154 | 13 | 2.001226 | 1407.4579,1407.5482,etc |
79 | radio frequency interference | RFI | 53 | 12 | 1.000651 | 1407.4385,1407.7543,etc |
80 | japan society for the promotion of science | JSPS | 19 | 12 | 1.000112 | 1407.2848,1407.7676,etc |
81 | cataclysmic variable | CV | 719 | 12 | 2.008454 | 1407.3707,1407.4526,etc |
82 | low mass x ray binary | LMXB | 141 | 12 | 1.002106 | 1407.8109,1407.3150,etc |
83 | extremely large telescope | ELT | 34 | 11 | 1.000708 | 1407.2011,1407.7123,etc |
84 | horizontal branch | HB | 240 | 11 | 2.007566 | 1407.2011,1407.3129,etc |
85 | intracluster medium | ICM | 150 | 11 | 2.001488 | 1407.7527,1407.7868,etc |
86 | local standard of rest | LSR | 29 | 11 | 1.000248 | 1407.4808,1407.5375,etc |
87 | submillimeter array | SMA | 125 | 11 | 2.001614 | 1407.8228,1407.8453,etc |
88 | gravitational wave | GW | 553 | 11 | 2.006033 | 1407.2882,1407.7549,etc |
89 | lyman break galaxy | LBG | 414 | 11 | 2.006106 | 1407.7316,1407.2944,etc |
90 | inverse compton | IC | 38 | 11 | 1.000435 | 1407.6717,1407.5482,etc |
91 | flat spectrum radio quasar | FSRQ | 99 | 11 | 2.002514 | 1407.2500,1407.8502,etc |
92 | friends of friends | FoF | 63 | 11 | 2.000689 | 1407.7040,1407.4168,etc |
93 | california institute of technology | Caltech | 16 | 10 | 1.000481 | 1407.1979,1407.0617,etc |
94 | deutsche forschungsgemeinschaft | DFG | 10 | 10 | 1.000041 | 1407.7516,1407.6150,etc |
95 | photomultiplier tube | PMT | 146 | 10 | 1.004005 | 1407.8117,1407.4151,etc |
96 | baryon acoustic oscillation | BAO | 68 | 10 | 1.001587 | 1407.7123,1407.1512,etc |
97 | dispersion measure | DM | 104 | 10 | 2.001584 | 1407.4745,1407.4605,etc |
98 | integral field unit | IFU | 131 | 10 | 1.001647 | 1407.1154,1407.2939,etc |
99 | friedmann robertson walker | FRW | 73 | 10 | 2.001467 | 1407.3905,1407.4058,etc |
100 | lyman werner | LW | 92 | 10 | 1.001317 | 1407.0034,1407.7561,etc |