lsst.tcc љ 1.2.2-3-g89ecb63 . ... Files . ... python . ... axis . coordConvWithFP.py . ... 22 љ def coordConvWithFP (fromCoordSys, fromPVTPair, fromPxPMRadVel, fromDir, toCoordSys, obj, inst, zeroPM, useGSWavelen): . 23 љ """!Convert a coord from one coordinate system to another . ... 35 љ @param[in] obj object block computed at desired desired TAI date of conversion . ... 50 љ obj = tcc.base.Obj(obj) # make a copy so I can change obj.site if useGSWavelen . ... tcc.axis.rotFromObs.rotFromObs . ...

Еще в разделе: (Показать все результаты (>1341) - www.apo.nmsu.edu/ )

• lsst.coordConv: coordConv::PVT Class Reference
• lsst.coordConv: coordConv::Coord Class Reference
• lsst.coordConv: coordConv::PVTCoord Class Reference

Stellarium 0.12.3 . ... Classes . ... gSatTEME Class Reference . Sat position and velocity predictions over TEME reference system. ... Set compute epoch for prediction. ... gVector љ . ... Get the TEME satellite position Vector. ... Get the Geographic satellite subpoint Vector calculated by the method compute SubPoint. ... gVector Satellite position vector meassured in Km. x: position[0] y: position[1] z: position[2] . ... gVector Satellite Velocity Vector measured in Km/s x: Vel[0] . ...

Еще в разделе: (Показать все результаты (>1500) - astro.uni-altai.ru/ )

• Stellarium: BigStarCatalogExtension::StarWrapper< Star > Class Template
• Stellarium: Nebula Class Reference
• Stellarium: TelescopeClient Class Reference

... Classes . ... casa::SparseDiffX< T > . ... The function, with fixed parameters a,b: template class T class f { public : T operator ()( const T x) { return a_p*a_p*a_p*b_p*b_p*x; } void set ( const T a, const T b) { a_p = a; b_p = b; } private : T a_p; T b_p; }; // The specialized function template class f SparseDiffX Double { public : T operator ()( const T x) { return a_p*a_p*a_p*b_p*b_p*x; } void set ( ... Referenced by casa::SparseDiffX< T >::operator=() . ...

Еще в разделе: (Показать все результаты (>24343) - www.atnf.csiro.au/ )

• casacore: casa::SparseDiffA< T > Class Template Reference
• casacore: casa::AutoDiffX< T > Class Template Reference
• casacore: casa::AutoDiffA< T > Class Template Reference

The position of the objects on the sky were generally measured to a precision between 1 and 4 arcsec. ... For the stars, the position is always at epoch 2000, whatever J2000 or B1950 coordinates are printed. ... The celestial position is given as coordinates in 4 different systems: . ... B1950 . ... Galactic coordinates in the reference frame called "new" system, adopted by IAU in 1958. Galactic pole at B124900.0+272400, node at ra=282.25,l=33 deg (inclination 62.6 deg). ... 1 arcsec . ...

Еще в разделе: (Показать все результаты (>2068) - www.sao.ru/ )

• HyperLEDA documentation: compilation of morphology (a102)
• Order Definition

... Archives . ... ArXiv] SDSS DR6, July 23, 2007 . Jul 25th, 2007| 03:22 am | ... Statistical Evidence for Three classes of Gamma-ray Bursts by T. Chattopadhyay et. al. In general, gamma-ray bursts (GRBs) are classified into two groups: long (>2 sec) and short (<2 sec) duration bursts. ... The new feature of this article is that Chattopadhyay et. al. applied the k-means and the Dirichlet process model based clustering method to confirm three classes of GRBs. ... Chandra Blog . ...

Еще в разделе: (Показать все результаты (>3980) - hea-www.harvard.edu/ )

• The AstroStat Slog class
• The AstroStat Slog Blog Archive Magnitude [Eqn]
• The AstroStat Slog k-means

... XMM-Newton SOC Home Page Conferences & Meetings . ... Data Analysis SAS News What is SAS? How to use SAS SAS Workshops SAS Version Changes Download and Install SAS Science Simulator (SciSim) . ... EPIC cameras optical loading . ... The PI is invited to cross-check the expected X-ray flux from the target source (and from any other potentially bright source in the target field of view), or to provide the SOC with her/his own estimate, if not originally specified in the proposal. ...

Еще в разделе: (Показать все результаты (>7704) - xmm.vilspa.esa.es/ )

• srcinfov: compute position of SouRCe in Field Of View
• Definitions

Next: CONSTRICTOR Up: Plotting Previous: Adding plot variables Contents . A plot class is basically defined by the list of plot variables displayed in the x,y, and z axis selections of the plot selection widget. ... Furthermore, in the same widget procedure, the name of the new plot class needs to be added to each selection button if required. ... Finally, as far as the plot widgets are concerned, the new class needs to be added for each necessary index selection in ww_indexsel . ...

Еще в разделе: (Показать все результаты (>17164) - www.eso.org/ )

• Astrometry
• API Help
• A More Complete Picture of the Blazar Class

... Content Model: Optional list header (LH), followed by one or more terms (DT) and definitions (DD). A definition list is a list of terms and corresponding definitions. Definition lists are typically formatted with the term on the left with the definition following on the right or on the next line. ... The definition list element can take the COMPACT attribute, which suggests that a compact rendering be used, and is appropriate if the list elements are small and/or the entire list is large. ...

Еще в разделе: (Показать все результаты (>170) - comet.sai.msu.ru/ )

• Divisions
• Captions
• Fill-Out Forms

... These include support for spectral coordinate systems, and compliance with FITS WCS papers I, II and III. ... Supported . ... Supported (all coordinate systems [including helio-ecliptic] and algorithm codes listed in papers I, II and III, with the exception of the ``STOKES'' and ``COMPLEX'' values defined in paper I, the ``CUBEFACE'' value defined in paper II, and the ``-TAB'' algorithm defined in paper III) . ... Supported (all systems, except ecliptic coordinates are currently assumed to be FK5) ....

Еще в разделе: (Показать все результаты (>1756) - www.adass.org/ )

• LINN?, a Software System for Automatic Classification
• Calculating the Position and Velocity Components of HST
• CICADA, CCD and Instrument Control Software

... The exact directions of the offsets are parallel to the rows and columns of the CCD on which the aperture is specified. ... It is often useful to explicitly specify the desired rotation of the WFPC2 field-of-view on the sky. ... Figure 7.8 shows the CCD orientation and aperture locations relative to the U3 axis. ... Obtain the Position Angle (PA) of the source axis on the sky, measured in the standard way, North through East. ... desired source angle in field-of-view measured CW from +U3 axis) . ...

Еще в разделе: (Показать все результаты (>11057) - www.stsci.edu/ )

• Apertures
• Pipeline Code Internal Organization GPI Data Pipeline 1.0 documentation
• Python: module profile

... BIRTHDATE/PLACE: . ... EDUCATION: . ... B.S., Geology, University of California-Santa Barbara, 1990 . M.S., Geology, University of Arizona, 1992 . ... Full Biographical Data . ... M.S., Ocean Engineering, Massachusetts Institute of Technology, 2000 . ... B.S., Electrical Engineering, University of the Pacific, 1984 . ... JAXA Astronaut . ... M.S., Aerospace Engineering, University of Houston Cullen College of Engineering, 1997 . ... Astronaut Candidates | ... Biography Page Curator: Kim Dismukes . ...

Еще в разделе: (Показать все результаты (>1924) - www.jsc.nasa.gov/ )

• Astronaut Class of 1996 (Group 16)
• Astronaut Class of 1998 (Group 17)
• Astronaut Class of 2000

.

Еще в разделе: (Показать все результаты (>240) - zebu.uoregon.edu/ )

• Evolution of Intelligence
• Astronomy 123 Spring 1996
• Physics 162 Winter 1996

It seems that every time I try to correct for a pointing error, I have to figure out the sign of the pointing error as reported by the various routines. The pointing error is computed using the heiles calibration scans and by using the turret scans. ... The center of the pattern is the "computed" position of the source using the ra,dec transformation to az,za and any current pointing model. ... X0, Y0 are reported as the error. ... So for turret scans, Add the az,za error to the pointing model. ...

Еще в разделе: (Показать все результаты (>3721) - www.naic.edu/ )

• http://www.naic.edu/~phil/hardware/byuPhasedAr/rfischercode/userhelp.txt
• http://www.naic.edu/~phil/ter/terfoc.html
• radar calibration via satellites

... Classes . ... Class List . ... Dust :: TMatrix . ... Inheritance diagram for Dust::TMatrix: . ... Collaboration diagram for Dust::TMatrix: . ... TMatrix (unsigned M ) . ... void . Zero (void) . A class to make handling of the dust_tmatrix structure easier . Dust::TMatrix::~TMatrix . The destructor ensures automatic deletion of the data structure . References dust_tmatrix::data . ... unsigned . ... References dust_tmatrix::data , and dust_tmatrix::M . void Dust::TMatrix::Zero . ...

Еще в разделе: (Показать все результаты (>1203) - www.mrao.cam.ac.uk/ )

• DUST: Class Members
• DUST: Class List
• DUST: Dust::MMPUV Class Reference

... public class TiffDecoder . ... static int . ... Field Detail public static final int NEW_SUBFILE_TYPE . ... public static final int IMAGE_WIDTH . ... public static final int IMAGE_LENGTH . ... public static final int BITS_PER_SAMPLE . ... public static final int COMPRESSION . ... public static final int PHOTO_INTERP . ... public static final int IMAGE_DESCRIPTION . ... public static final int STRIP_OFFSETS . ... public static final int ORIENTATION . ... public static final int SAMPLES_PER_PIXEL . ...

Еще в разделе: (Показать все результаты (>897) - www.astro.louisville.edu/ )

• GUI (ImageJ API)
• Uses of Class ij.plugin.filter.PlugInFilterRunner (ImageJ API)
• Measurements (ImageJ API)

... Инициализация процесса (initialization of process) - фаза исполнения процесса , перед началом которой он находился в состоянии " сформированный ". ... Общая схема исполнения предиката включает : 1) Выбор предложения с подходящим заголовком . ... 3) Исполнение соответствующих подцелей доказательства . ... Исполнение программы начинается с доказательства конструктора процесса , заданного в определении проекта , а также формирования процесса , построенного в результате доказательства этого конструктора...

Еще в разделе: (Показать все результаты (>725) - www.cplire.ru/ )

• Actor Prolog User Guide. Residents.

previous contents properties index . ... font-face, 1 , 2 , 3 , 4 , 5 , 6 , 7 . ... media, 1 , 2 , 3 , 4 . ... definition of, 1 . absolutely positioned element, 1 . ... all' media group, 1 . ... anonymous inline boxes, 1 . ... ascent' (descriptor), 1 . ... aural' media group, 1 . ... bitmap' media group, 1 . ... margin, 1 . ... continuous' media group, 1 . ... definition-src' (descriptor), 1 . ... font definition resource, 1 . ... font-family' (descriptor), 1 . ... font-size' (descriptor), 1 . ...

Еще в разделе: (Показать все результаты (>1735) - crydee.sai.msu.ru/ )

• Cascading Style Sheets, Level 2
• Dynamic HTML in Communicator
• Image: When classes are over (or boring :-) we go to the beach

... Planets and Brown Dwarfs . ... Mission Definition . Ask anyone on the street to give an example of a planet, and they'll consider you a bit dim. ... Finally, if you ask "What is the exact scientific definition of 'planet'?", it turns out that nobody can answer it, because there really isn't one. ... The word itself means "wanderer" in Greek, and other cultures generally have words for "planet" with a similar meaning. So why isn't that good enough for us today? ...

Еще в разделе: (Показать все результаты (>823) - www.astrosociety.org/ )

• ASP: Education Newswire
• ASP: The Return of Halley's Comet
• ASP: Black Holes to Blackboards: In the Seventh House of Saturn

... The trgm contrib module provides functions and index classes for determining the similarity of text based on trigram matching. ... The set of trigrams in the word "cat" is " c", " ca", "at " and "cat". *real similarity(text, text) . ... The trgm module comes with an index operator class that allows a developer to create an index over a text column for the purpose of very fast similarity searches. ... CREATE TABLE test_trgm (t text); CREATE INDEX trgm_idx ON test_trgm USING gist(t gist_trgm_ops); . ...

Еще в разделе: (Показать все результаты (>1097) - www.sai.msu.su/ )

• APOD: 2000 June 8 - Active Regions, CMEs, and X Class Flares
• APOD: 2007 November 6 - An X Class Flare Region on the Sun
• APOD: 2013 May 16 - Four X-class Flares

... The width of hydrogen lines is known to depend on the pressure in the photosphere, and then on the luminosity and effective temperature of the star. We have studied this dependence using the spectra of normal B stars from the databases by Jacoby et al., ... The resolution of Jacoby spectra (4.5А) coincides with the resolution of our BTA/UAGS spectra (4.4A). ... Dependence of full width FWZI of hydrogen lines on star spectral type and luminosity class. ...

Еще в разделе: (Показать все результаты (>758) - jet.sao.ru/ )

• LWN: Driver porting: Device classes