... Name Designation ff ffi J (ffi J ) H (ffi H ) K (ffi K ) J \Gamma K H \Gamma K Nights a AS01­0 FS02 00 55 09.9 00 43 13 10.716 ( 0.005 ) 10.507 ( 0.010 ) 10.470 (0.003) 0.25 0.04 6,6,6 AS02­0 SAO054271 00 55 58.6 39 10 09 8.775 (0.006) 8.771 ( 0.012 ) 8.770 ( 0.009 ) 0.01 0.00 5,6,6 AS03­0 FS03 01 04 21.6 04 13 39 12.606 ( 0.011 ) 12.729 ( 0.008 ) 12.827 ( 0.013 ) ­0.22 ­0.10 6,6,6 AS04­0 FS04 01 54 37.6 00 43 01 10.555 (0.004) 10.301 ( ...

F(6 cm) Other Name ct/s erg cm -2 s -1 µJy FX/FR mJy # r B R Class z Catalogs WGAJ0011.2- 3620 0.002 1.73E - 14 0.003 -12.73 96 0.12 21.3 FSRQ 2.324 WGAJ0012.5- 1629 0.097 1.28E - 12 0.29 -10.53 50 0.62 17.7 FSRQ 0.151 1 WGAJ0015.5+ 3052 0.019 2.82E - 13 0.083 -11.37 89 0.62 16.3 17.2 FSRQ 1.619 0.023 3.16E - 13 0.095 WGAJ0029.0+ 0509 0.006 6.33E - 14 0.014 -12.71 377 0.00 19.3 18.1 FSRQ 1.633 WGAJ0032.5- 2849 ...

... The designations are given for each object along with J2000.0 coordinates, followed by three columns for each filter, containing the magnitude, the first standard deviation or scatter among data points, and the number of measurements N. The values reported for the magnitudes are weighted averages, using 1/(sigma)^2 weighting, where the sigmas are the internal photometric errors of individual measurements." ... 0.005 . ... 0.008 . ... 0.006 . ... 0.007 . ...

wmap7_spt_bao_h0 +clusters, stat. sys. omegabh2 0.02263 +- 0.00044 0.02247 +- 0.00043 +- 0.00005 ns 0.980 +- 0.012 0.975 +- 0.012 +- 0.002 logA 3.173 +- 0.036 3.153 +- 0.035 +- 0.007 omegal 0.729 +- 0.014 0.7478 +- 0.0076 +- 0.0068 omegadmh2 0.1133 +- 0.0032 0.1087 +- 0.0013 +- 0.0017 age 13.681 +- 0.086 13.707 +- 0.084 +- 0.008 omegam 0.271 +- 0.014 0.2522 +- 0.0076 +- 0.0068 sigma8 0.833 +- 0.024 0.798 +- 0.010 +- ...

Peremennye Zvezdy ( Variable Stars ) 28 , No. ... We present the results of our long-term ( 13 years) J and K photometry of the X-ray binary Cyg X-1. ... From the analysis of these observations together with optical photometry of Cyg X-1, we concluded that the variations of the binary's J and K brightness were ellipsoidal. ... 0.007 . ... 0.008 . ... 0.009 . ... Figure 2 displays variations of the J and K brightness of Cyg X-1 versus the orbital phase, from observations of 1995-2007. ...

... Digital systems . ... Standard Stars - CCD Photometry, Transformations and Comparisons . ... Figure 2: A typical sample of transformation relations to the Landolt standard system (1996 Nov. ... 0.006 . ... Landolt's natural GaAs u - b system is not very close to the standard U - B system and so it is likely that, because the transformations were made using a U - B colour term alone, systematic U - B differences exist for some kinds of stars namely, A-F stars, reddened B-A stars and giant A-F stars. ...

... 0.039 0.009 . ... 0.043 0.006 . 0.059 0.005 . 0.039 0.002 . 0.063 0.002 . 0.053 0.003 . 0.069 0.003 . 0.093 0.005 . 0.054 0.003 . 0.076 0.003 . ... 0.078 0.004 . ... 0.235 0.014 . ... 0.029 0.007 . ... 0.014 0.002 . ... 0.006 0.002 . ... 0.007 0.002 . ... 0.005 0.002 . ... 0.014 0.003 . ... 0.009 0.005 . ... 0.009 0.003 . ... 0.009 0.002 . ... 0.007 0.003 . ... 0.014 0.005 . ... 0.014 0.006 . ... 0.003 0.002 . ... 0.004 0.002 . ... 0.006 0.003 . ... 0.007 0.004 . ...

Minor Planet 2000 EW70 Date UT R.A. (2000) Dec. ... 2000 Mar 16 0h 12 25.30 - 7 12.5 0.051 1.044 166.4 15.8 Vir 2000 Mar 16 6h 12 24.62 - 6 48.1 0.049 1.043 167.1 15.7 Vir 2000 Mar 16 12h 12 23.90 - 6 22.3 0.048 1.042 167.7 15.6 Vir 2000 Mar 16 18h 12 23.14 - 5 55.0 0.047 1.041 168.4 15.5 Vir 2000 Mar 17 0h 12 22.33 - 5 25.9 0.045 1.039 169.1 15.4 Vir 2000 Mar 17 6h 12 21.47 - 4 54.9 0.044 1.038 169.8 15.3 Vir ...

... Nearly all the sources have com­ plete data at 2.3, 3.9, 7.7 and 11.2 GHz; 40 sources have 21.7 GHz flux densities. ... Fluxes of the sources in the NCP region Name, S 0.325 # t S 1.4 # t S 2.3 # t S 3.9 # t S 7.7 # t S 11.2 # t S 21.7 # t Sp. index NVSS Jy, WENSS Jy, NVSS Jy Jy Jy Jy Jy # 0.325/11.2 J000943+772440 2.059 0.082 0.628 0.021 0.447 0.04 0.267 0.017 0.161 0.007 0.14 0.016 -- -- 0.76 J001236+854313 1.605 0.064 0.691 0.023 0.539 0.048 0.246 0.018 0.148 ...