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http://astro.uni-altai.ru/HC/eclipses/Y-227-SE.html.
http://astro.uni-altai.ru/HC/eclipses/Y-227-SE.html.
181. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/gregg_stds.coord
... 8.30 0.960 7.59 0.71 -1.8 "hd9051" 1 28 46.5 -24 20 25.4 ! 8.93 0.820 11.18 -1.6 "hd16031" 2 34 11.0 -12 23 03.5 ! ... 8.04 0.486 2.94 5.10 d -2.0 "HD26169" 04 00 52.5 -75 36 11.4 ! ... 7.46 1.088 9.46 -2.00 -1.7 "hd29574" 4 38 55.7 -13 20 48.1 ! 8.33 1.304 10.90 -2.57 -1.9 "hd36702" 5 31 52.2 -38 33 24.0 ! ... 8.00 0.703 5.67 2.33 d -1.5 "hd55496" 7 12 11.4 -22 59 00.6 ! ... 8.33 1.015 8.54 -0.21 -1.5 "ltt4364" 11 45 43 -64 50 24 ! 11.51 0.190 DC(C2) Hamuy "g13-35" 12 25 35.0 01 17 02.3 ! ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/gregg_stds.coord -- 3.3 Кб -- 21.01.2009
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182. http://www.naic.edu/~phil/cals/cal.datR8
telescope. # new diodes were installed 13feb04 # installed 14mar04. backdated to 13feb04 # !2004 44 3012.5 11.780 1.368 11.360 1.319 9.023 1.023 9.757 1.086 3037.5 11.350 1.325 11.270 1.324 9.144 1.035 10.105 1.143 3062.5 11.130 1.314 11.130 1.312 9.289 1.054 10.391 1.169 3087.5 11.070 1.316 11.040 1.316 9.550 1.084 10.669 1.206 3112.5 11.130 1.332 11.070 1.330 9.822 1.112 10.870 1.235 3137.5 11.260 1.350 11.180 1.351 9.889 1.127 ...
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Ссылки http://www.naic.edu/~phil/cals/cal.datR8 -- 7.8 Кб -- 06.11.2011
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183. http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/spie7013-132.pdf
... The AR coating has mean reflection losses of less than 0.5%. ... PATH A-B C-B D-E F-B C-G C-H Wavelength () Ks H Ks H Ks H Ks H Ks H Ks H 1640 2140 1640 2140 1640 2140 1640 2140 1640 2140 1640 2140 V 0.940 0.940 1.000 1.000 0.982 0.982 0.980 0.978 0.939 0.939 0.976 0.978 Vi de a l V/Vi de a l VI 0.701 0.703 0.492 0.493 0.403 0.406 0.401 0.398 0.677 0.681 0.395 0.398 PATH A-B C-B D-E F-B C-G C-H Wavelength () Ks H Ks H Ks H Ks H Ks H Ks H 1640 2140 1640 ...
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Ссылки http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/spie7013-132.pdf -- 992.5 Кб -- 20.02.2013
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184. http://www.stsci.edu/hst/wfc3/documents/ISRs/WFC3-2008-15.pdf
ST-ECF Instrument Science Report WFC3-2008-15 The TV2 ground calibrations of the WFC3 NIR grisms H. Kuntschner, H. Bushouse, J. R. Walsh, M. KЭmmel July 08, 2008 ABS TRACT Based on thermal vacuum tests (TV2; June - August 2007), the performance of the WFC3 near-IR G102 and G141 grisms has been assessed. ... The setup for G141 is identical. ... 10 ST-ECF Instrument Science Report WFC3-2008-15 Figure 5: Instrument efficiency of various orders for the WFC3 G141 grism as function of wavelength. ...
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Ссылки http://www.stsci.edu/hst/wfc3/documents/ISRs/WFC3-2008-15.pdf -- 1953.1 Кб -- 16.07.2008
[ Текст ] Ссылки http://www.stecf.org/documents/isr/WFC3-2008-15.pdf -- 1953.1 Кб -- 14.08.2008
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[ Текст ] Ссылки http://www.stecf.org/documents/isr/WFC3-2008-15.pdf -- 1953.1 Кб -- 14.08.2008
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185. http://www.accuracy.puldb.ru/200704/C000.HTM
... USNO 104 Italy, San 0.40 21 x 21' 2.5" 43 136 0.390 0.535 Marccello 2.0 GSC 106 Slovenia, 0.36 36 x 36' 2.0" 886 3773 0.384 0.418 Crni vrh 2.4 USNO 113 Germany, 0.50 13 x 10' 2" 18 71 0.274 0.299 Schonbrunn 2.3 USNO 118 Slovakia, 0.57 14 x 10' 1.7" 10 64 0.073 0.058 Modra 3.3 USNO 122 France, 0.40 No data 99 676 0.374 0.300 Pises Obs. ... 1.8 UCAC A20 Sogel, 0.25 11 x 8' 1.0 1 3 0.939 0.951 Germany 2.0 USNO A24 New Millennium 0.36 12 x 12' 1.4 104 1974 0.415 0.344 Obs., ... Germany. ...
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Ссылки http://www.accuracy.puldb.ru/200704/C000.HTM -- 42.4 Кб -- 18.10.2007
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186. http://www.jsc.nasa.gov/history/suddenly_tomorrow/chapters/Chpt12.pdf
CHAPTER 12: Lead Center Space Center personnel began work on the Space Shuttle under the cloud of reductions in force, tightening budgets, growing public apathy or outright criticism, and unclear and changing program directives. ... Budgetary constraints contributed to the decision to establish a lead center management approach for the Shuttle and affected program development. ... Now, as Shuttle Program Manager, Thompson had overall responsibility for the development of the Shuttle. ...
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Ссылки http://www.jsc.nasa.gov/history/suddenly_tomorrow/chapters/Chpt12.pdf -- 323.0 Кб -- 10.11.2004
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187. http://www.2dfquasar.org/Papers/2002MNRAS.337..275C.pdf
... 337, 275292 (2002) The correlation of line strength with luminosity and redshift from composite quasi-stellar object spectra S. M. Croom,1 K. Rhook,1 E. A. Corbett,1 B. J. Boyle,1 H. Netzer,2 N. S. Loaring,3 L ... We measure highly significant Baldwin effects for most broad emission lines (C IV 1549, C III] 1909, Mg II 2798, H ,H ) and show that they are predominantly caused by correlations with luminosity, not redshift. ... The correlations of log W with log(1 + z ) for each line. ...
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Ссылки http://www.2dfquasar.org/Papers/2002MNRAS.337..275C.pdf -- 831.9 Кб -- 04.03.2004
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