1 | active galactic nucleus | AGN | 2579 | 113 | 2.005306 | 1410.4837,1410.2823,etc |
2 | spectral energy distribution | SED | 957 | 93 | 2.0022 | 1410.2711,1410.8101,etc |
3 | point spread function | PSF | 948 | 77 | 2.001918 | 1410.7771,1410.4544,etc |
4 | interstellar medium | ISM | 780 | 77 | 2.001431 | 1410.4504,1410.2655,etc |
5 | sloan digital sky survey | SDSS | 1728 | 73 | 1.003078 | 1410.6050,1410.2271,etc |
6 | cosmic microwave background | CMB | 897 | 68 | 2.002437 | 1410.2250,1410.3284,etc |
7 | signal to noise ratio | S/N | 319 | 55 | 2.001106 | 1410.5216,1410.3835,etc |
8 | initial mass function | IMF | 539 | 54 | 1.002414 | 1410.0100,1410.2711,etc |
9 | dark matter | DM | 2581 | 53 | 2.008605 | 1410.3607,1410.8529,etc |
10 | star formation rate | SFR | 1302 | 46 | 1.003093 | 1410.7464,1410.7389,etc |
11 | supernova | SN | 1755 | 44 | 1.006388 | 1410.0100,1410.2774,etc |
12 | markov chain monte carlo | MCMC | 274 | 41 | 1.001759 | 1410.4837,1410.2544,etc |
13 | nasa/ipac extragalactic database | NED | 72 | 40 | 1.000192 | 1410.4837,1410.7464,etc |
14 | full width at half maximum | FWHM | 131 | 32 | 2.000362 | 1410.8013,1410.1879,etc |
15 | asymptotic giant branch | AGB | 589 | 31 | 2.005088 | 1410.6797,1410.4504,etc |
16 | black hole | BH | 1155 | 31 | 2.006565 | 1410.4250,1410.3563,etc |
17 | general relativity | GR | 646 | 31 | 2.003913 | 1410.7392,1410.0207,etc |
18 | near infrared | NIR | 577 | 30 | 2.002155 | 1410.7389,1410.6792,etc |
19 | red giant branch | RGB | 401 | 30 | 1.002562 | 1410.3823,1410.4564,etc |
20 | hubble space telescope | HST | 175 | 30 | 1.000581 | 1410.0536,1410.5560,etc |
21 | main sequence | MS | 1111 | 28 | 2.0051 | 1410.0100,1410.5883,etc |
22 | field of view | FOV | 133 | 27 | 1.00069 | 1410.2711,1410.4050,etc |
23 | kolmogorov smirnov | KS | 227 | 27 | 2.001868 | 1410.5216,1410.7515,etc |
24 | gamma ray burst | GRB | 859 | 26 | 2.005413 | 1410.3960,1410.2776,etc |
25 | very large array | VLA | 367 | 25 | 1.002998 | 1410.2558,1410.2743,etc |
26 | equation of state | EoS | 502 | 25 | 2.003541 | 1410.6479,1410.3747,etc |
27 | intergalactic medium | IGM | 397 | 24 | 2.003658 | 1410.2250,1410.7132,etc |
28 | gravitational wave | GW | 604 | 24 | 2.003647 | 1410.6606,1410.7392,etc |
29 | probability distribution function | PDF | 320 | 24 | 2.002199 | 1410.2774,1410.6479,etc |
30 | line of sight | LOS | 140 | 23 | 1.000858 | 1410.2250,1410.2774,etc |
31 | supermassive black hole | SMBH | 476 | 23 | 2.00386 | 1410.4837,1410.7515,etc |
32 | infrared | IR | 603 | 23 | 2.002992 | 1410.2408,1410.6117,etc |
33 | magnetohydrodynamic | MHD | 221 | 22 | 1.002781 | 1410.6547,1410.3757,etc |
34 | equivalent width | EW | 249 | 21 | 1.001605 | 1410.4250,1410.1551,etc |
35 | milky way | MW | 188 | 21 | 2.001985 | 1410.3563,1410.0842,etc |
36 | globular cluster | GC | 1285 | 21 | 2.006528 | 1410.4564,1410.7503,etc |
37 | color magnitude diagram | CMD | 314 | 21 | 1.001737 | 1410.4564,1410.7503,etc |
38 | neutron star | NS | 476 | 20 | 2.006179 | 1410.0100,1410.1569,etc |
39 | supernova remnant | SNR | 762 | 20 | 2.00609 | 1410.7239,1410.2655,etc |
40 | signal to noise | S/N | 80 | 20 | 1.000721 | 1410.7389,1410.0684,etc |
41 | standard model | SM | 164 | 20 | 2.002659 | 1410.0410,1410.6620,etc |
42 | local thermodynamic equilibrium | LTE | 171 | 20 | 1.004792 | 1410.4418,1410.6610,etc |
43 | inverse compton | IC | 195 | 20 | 1.002814 | 1410.2743,1410.7639,etc |
44 | ultraviolet | UV | 558 | 20 | 1.00417 | 1410.2408,1410.2093,etc |
45 | white dwarf | WD | 1079 | 19 | 1.009592 | 1410.6119,1410.4898,etc |
46 | star formation history | SFH | 276 | 19 | 2.001608 | 1410.1551,1410.5430,etc |
47 | large area telescope | LAT | 327 | 19 | 2.002656 | 1410.0358,1410.6462,etc |
48 | adaptive mesh refinement | AMR | 77 | 18 | 2.000686 | 1410.0959,1410.6479,etc |
49 | radial velocity | RV | 294 | 18 | 2.005247 | 1410.2604,1410.7379,etc |
50 | canada france hawaii telescope | CFHT | 186 | 18 | 2.003475 | 1410.1551,1410.0017,etc |
51 | weakly interacting massive particle | WIMP | 259 | 18 | 1.003202 | 1410.3925,1410.2589,etc |
52 | large scale structure | LSS | 64 | 17 | 1.000757 | 1410.2250,1410.2544,etc |
53 | coronal mass ejection | CME | 1155 | 17 | 2.009415 | 1410.8013,1410.5490,etc |
54 | cold dark matter | CDM | 326 | 17 | 2.004028 | 1410.3845,1410.4559,etc |
55 | position angle | PA | 277 | 17 | 1.002881 | 1410.3570,1410.0196,etc |
56 | polycyclic aromatic hydrocarbon | PAH | 390 | 16 | 2.008545 | 1410.4504,1410.6158,etc |
57 | cosmic ray | CR | 765 | 16 | 2.005254 | 1410.2655,1410.7639,etc |
58 | planetary nebula | PN | 402 | 16 | 2.005166 | 1410.6662,1410.6119,etc |
59 | large magellanic cloud | LMC | 563 | 16 | 2.004506 | 1410.3692,1410.7783,etc |
60 | young stellar object | YSO | 369 | 16 | 1.001993 | 1410.3377,1410.2947,etc |
61 | wolf rayet | WR | 238 | 16 | 1.008765 | 1410.0842,1410.2768,etc |
62 | atacama large millimeter/submillimeter array | ALMA | 280 | 16 | 2.001756 | 1410.0172,1410.2093,etc |
63 | friends of friends | FoF | 128 | 15 | 1.002952 | 1410.6050,1410.4270,etc |
64 | zero age main sequence | ZAMS | 106 | 15 | 2.001109 | 1410.0100,1410.5575,etc |
65 | smoothed particle hydrodynamics | SPH | 215 | 15 | 1.003335 | 1410.0959,1410.4222,etc |
66 | far infrared | FIR | 143 | 15 | 1.000972 | 1410.1569,1410.0006,etc |
67 | full width half maximum | FWHM | 57 | 15 | 1.000452 | 1410.0842,1410.3706,etc |
68 | brightest cluster galaxy | BCG | 231 | 14 | 1.002562 | 1410.7887,1410.6050,etc |
69 | intracluster medium | ICM | 264 | 14 | 2.002158 | 1410.7887,1410.1955,etc |
70 | principal component analysis | PCA | 102 | 14 | 2.000802 | 1410.1551,1410.2743,etc |
71 | two micron all sky survey | 2MASS | 105 | 14 | 2.001234 | 1410.8394,1410.0110,etc |
72 | mid infrared | mid-IR | 80 | 13 | 1.000779 | 1410.4504,1410.6792,etc |
73 | friedmann robertson walker | FRW | 46 | 13 | 1.00102 | 1410.1562,1410.0207,etc |
74 | wide field camera 3 | WFC3 | 78 | 13 | 2.001147 | 1410.3702,1410.7611,etc |
75 | submillimeter array | SMA | 117 | 13 | 2.001883 | 1410.2269,1410.0172,etc |
76 | burst alert telescope | BAT | 63 | 12 | 2.001724 | 1410.7771,1410.5216,etc |
77 | probability density function | PDF | 170 | 12 | 1.002876 | 1410.1586,1410.3537,etc |
78 | fast fourier transform | FFT | 60 | 12 | 2.000412 | 1410.4544,1410.2544,etc |
79 | max planck institute for astronomy | MPIA | 12 | 12 | 1.000091 | 1410.7464,1410.2743,etc |
80 | very long baseline array | VLBA | 104 | 12 | 2.001745 | 1410.8101,1410.0196,etc |
81 | adaptive optics | AO | 143 | 12 | 1.001863 | 1410.4634,1410.2768,etc |
82 | low mass x ray binary | LMXB | 169 | 12 | 2.002436 | 1410.1569,1410.5471,etc |
83 | william herschel telescope | WHT | 36 | 12 | 1.000356 | 1410.3702,1410.5575,etc |
84 | horizontal branch | HB | 371 | 12 | 1.006118 | 1410.4564,1410.7456,etc |
85 | active region | AR | 244 | 12 | 2.004071 | 1410.8696,1410.7994,etc |
86 | extragalactic background light | EBL | 81 | 12 | 2.001405 | 1410.0497,1410.8810,etc |
87 | broad line region | BLR | 350 | 11 | 2.003884 | 1410.4837,1410.2743,etc |
88 | max planck institute for astrophysics | MPA | 18 | 11 | 1.000169 | 1410.7464,1410.2743,etc |
89 | halo occupation distribution | HOD | 97 | 11 | 2.001788 | 1410.3563,1410.2805,etc |
90 | very long baseline interferometry | VLBI | 140 | 11 | 2.004145 | 1410.8101,1410.0196,etc |
91 | star formation | SF | 262 | 11 | 2.005785 | 1410.0959,1410.3824,etc |
92 | core collapse supernova | CCSN | 103 | 11 | 2.001844 | 1410.1569,1410.5431,etc |
93 | flat spectrum radio quasar | FSRQ | 192 | 11 | 2.002968 | 1410.2743,1410.0358,etc |
94 | early type galaxy | ETG | 522 | 11 | 2.005891 | 1410.5430,1410.1469,etc |
95 | three dimensional | 3D | 127 | 11 | 2.002015 | 1410.2776,1410.1789,etc |
96 | pre main sequence | PMS | 173 | 11 | 1.001588 | 1410.5883,1410.4238,etc |
97 | very large telescope | VLT | 40 | 11 | 2.000408 | 1410.7503,1410.5732,etc |
98 | x ray telescope | XRT | 41 | 10 | 1.000588 | 1410.4250,1410.4050,etc |
99 | colour magnitude diagram | CMD | 113 | 10 | 2.001472 | 1410.4504,1410.8352,etc |
100 | electromagnetic | EM | 108 | 10 | 1.001254 | 1410.7392,1410.3563,etc |