... C N Maximum number of axes in a GDS set INTEGER MAXAXES PARAMETER ( MAXAXES = 10) N Maximum number of subsets INTEGER MAXSUBS PARAMETER (MAXSUBS = 2048) N Size of internal data buffer INTEGER MAXDATA PARAMETER (MAXDATA = 4096) N Names of input and output set CHARACTER*80 SET1 , SET2 N Dimension of subsets INTEGER SUBDIM N Number of subsets INTEGER NSUBS N Array containing axis permutation INTEGER AXPERM1( ... 0) CFOR CALL FINIS STOP END . ...

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• This 10 min exposure shows star trails clearly defining the south celestial

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MIC Discussion Discussion of the Maximal Information Coefficient Alexander W Blocker http://www.awblocker.com/ Feb 21 2012 MIC Discussion Outline Outline 1 Defining MIC Subtleties technical issues Simon Tibshirani's response Broader concerns lessons 2 3 4 MIC Discussion Defining MIC Outline 1 Defining MIC Subtleties technical issues ... MIC Discussion Broader concerns & lessons Note Concerns here are not particular to the Reshef et al. paper. ...

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Astronomy Picture of the Day . ... 1.01.2001 . ... During millennium two , humanity continually redefined its concept of "Universe": first as spheres centered on the Earth , in mid-millennium as the Solar System , a few centuries ago as the Galaxy , and within the last century as the matter emanating from the Big Bang . ... 2001 2002 . ... NASA Web Site Statements, Warnings, and Disclaimers . ... Publications with keywords: universe - millennium . Publications with words: universe - millennium . ...

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... Previous: The ACSIS Data Reduction System . ... The AST library supports the attachment of astrometric calibrations to astronomical datasets, the processing of this information, and generation of associated graphical output. ... In this paper we outline some more recent developments and applications, which include a set of efficient data re-gridding algorithms for curvilinear coordinate systems, improved FITS support, user-defined coordinate transformations, and pin-cushion/barrel distortion. ...

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PRO read_ apo _red, w, t, s ; define the wavelength scale ; define_logw , 6000 , 1.17 , 1200 , w define_logw , 6000 , 7000, 1000 , w ; Initialise the data accumulation arrays IF keyword_set(t) THEN t(0) = -1 read_frame , ' apo ', ' 140502 ', ' APO _0002R', w, t, s read_frame , ' apo ', ' 140502 ', ' APO _0005R', w, t, s read_frame , ' apo ', ' 140502 ', ' APO _0007R', w, t, s read_frame , ' ...

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Copyright (c) 1999-2003 Smithsonian Astrophysical Observatory */ /* Define as 1 if you have string.h */ # undef HAVE_STRING_H /* Define as 1 if you have stdlib.h */ # undef HAVE_STDLIB_H /* Define as 1 if you have malloc.h */ # undef HAVE_MALLOC_H /* Define as 1 if you have unistd.h */ # undef HAVE_UNISTD_H /* Define as 1 if you have getopt.h */ # undef HAVE_GETOPT_H /* Define as 1 if you have pwd.h */ # ...

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Stellarium 0.12.3 . ... Classes . ... ClassљList . ... ClassљMembers . elsetrec Member List . This is the complete list of members for elsetrec , including all inherited members. a (defined in elsetrec ) . ... alta (defined in elsetrec ) . ... altp (defined in elsetrec ) . ... argpdot (defined in elsetrec ) . ... argpo (defined in elsetrec ) . ... atime (defined in elsetrec ) . ... aycof (defined in elsetrec ) . ... Generated on Sat Aug 10 2013 17:12:44 for Stellarium by љ 1.8.3.1 ...

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Jeff Mock # 2030 Gough # San Francisco, CA 94109 # jeff@mock.com # (c) 2004 # include ../ src /Makefile.defs N = ${ PREFIX } PER = 17.1 LO = 10 NOISE = 0.001 PHASE = 100 XMIX = gen /${ PREFIX }.v DEBUG = 1 AMP = 0.99 plot0.png: ${N}.f ${TBV} ${SRCV} ${XMIX} sig1.mem fft rm -rf wave.vcd ${CVER} -w -f ${N}.f ./ fft \ --wi=${ WIDTH } \ --wo=${ OWIDTH } \ --fi= sig1.mem \ --fo=mix.out \ --out= fft .out \ --n=1024 perl ${ ...

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... It?s needs solution satellite?s orientation problem for defining location of sources of ionospheric emissions above Earth?s surface with necessary accuracy. There is possibility to define orientation of photometric devices by using TV images of star background. The CCD TV camera is designed for recording of images of star sky, Earth? limb and adjoining part of Earth? surface to fix the orbit point coordinates during the measurements by FAGOT and SICH-F devices. ...

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Lord Carrington determined the solar rotation rate by watching low-latitude sunspots back in the 1850s. He defined a fixed solar coordinate system that rotates in a sidereal frame every 25.38 days. ... Carrington coordinates are heliographic and measured in latitude and longitude in that rotating frame. Carrington Time is the rotation and longitude of the point on the Sun that is at the sub-terrestrial point. ... Bartels defined his calendar based on observations of daily geomagnetic activity. ...

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... The perceptron structure, on the basis of which the database is built, is defined by a number of the input and output parameters and a required accuracy. ... The output perceptron data are the expansion coefficients of the scattering matrix elements in series of the generalized spherical functions. ... As the cluster structure depends on the generation conditions the expansion coefficients were averaged over 5--7 realizations of the clusters (for N . ... is the coefficient number. ...

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