... Classes . ... casa . casa::LatticeProgress . ... virtual . ... Tell the number of steps done so far. virtual void . ... Let a derived class initialize itself. uInt . ... A derived class should override the virtual functions from this class. ... virtual void casa::LatticeProgress::done . ... It sets the expected number of steps and calls initDerived, so a derived class can initialize itself. virtual void casa::LatticeProgress::initDerived . ... virtual void casa::LatticeProgress::nstepsDone . ...

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• casacore: casa::CountedPtr< t > Class Template Reference
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Stellarium 0.12.3 . ... Classes . ... FileљStructure . ... Landscape Class Reference abstract . ... More... #include < Landscape.hpp > . ... Landscape (float _radius=2.f) . ... load (const QSettings &landscapeIni, const QString &landscapeId)=0 . ... setBrightness (const float b) . ... floatљ . ... const QStringљ . getTexturePath (const QString &basename, const QString &landscapeId) . ... const floatљ . ... Definition at line 42 of file Landscape.hpp . ... const QString Landscape::getTexturePath . ...

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lsst.coordConv љ unknown . ... Classes . ... coordConv::OtherCoordSys Class Reference . ... OtherCoordSys (std::string const &name, double date=0, DateTypeEnum dateType= DateType_None , bool isMean =false) . ... virtual Coord љ . ... CoordSys (std::string const &name, double date, DateTypeEnum dateType, bool isMean , bool canConvert ) . ... convertFrom ( CoordSys const &fromCoordSys, Coord const &fromCoord, Site const &site, double tai=0) const . ... virtual Coord coordConv::OtherCoordSys::removePM . ...

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• lsst.coordConv: coordConv::FK4CoordSys Class Reference
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• lsst.coordConv: coordConv::FK5CoordSys Class Reference

WFC3 Instrument Handbook for Cycle 24 . ... Wide Field Camera 3 Instrument Handbook for Cycle 24 > Appendix A: WFC3 Filter Throughputs > A.2 Throughputs and S/N Ratio Data . ... Note that the plots show the S/N as a function of source magnitude for exposure times as short as 0.1 s, although the minimum exposure time for the UVIS channel is actually 0.5 s. Wide Field Camera 3 Instrument Handbook for Cycle 24 > Appendix A: WFC3 Filter Throughputs > A.2 Throughputs and S/N Ratio Data . ...

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... XMM-Newton SOC Home Page Conferences & Meetings . ... General User Support XMM-Newton Helpdesk Users Group . ... Data Analysis SAS News What is SAS? ... Data handling units and production of the relevant software, in collaboration with industry . ... AIV support . ... Participation in the development of the electrical ground support equipment . ... Participation in flight operations definition and in the development of data analysis software . ... Development of data analysis software . ...

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• XMM-Newton Trainee Project 2004
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• XMM-Newton Trainee Project 2005

Organisers: Michel Balazard (CNRS, Laboratoire Poncelet) , Michael Tsfasman (CNRS, Laboratoire Poncelet, Institute for Information Transmission Problems) , Alexey Zykin (Laboratoire Poncelet, State University Higher School of Economics) . ... General Information . ... Number theory semester web page . ... Poncelet Laboratory web page . ...

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• Конференция "Дзета функции"
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... As stable VLT work horses during the past 8 years obviously the two FORSes have in many ways also been instrumental to the definition of the VLT queue observing paradigm which includes both systematic collection of calibration data, online and offline reduction pipelines. The original concept for the photometric calibration and the FORS imaging pipelines involved acquisition of simple twilight images which were used for flatfielding, and observation of Landolt photometric standards. ...

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... R2795 Arecibo Observatory Date Received: 2012-Aug-31 15:40:12 William E. Gordon Telescope Observing Time Request COVER SHEET Section I - General Information Submitted for Sep 1 2012. ... These observations continue our six year survey of all the M- and E-class asteroid observable at Arecibo. ... Begin ­ End Interval­Interval 2245 ­ 0200 ­ ­ ­ Days Needed at This Interval 4 Time Constraints (Must Be Justified in the Prop osal Text) Asteroid target is at opposition and SNR is maximized. ...

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• http://www.naic.edu/vscience/schedule/2014Fall/ArchibaldtagP2905.pdf
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... Class . ... java.lang.Object ij.io.ImageReader . public class ImageReader . ... packBitsUncompress (byte[] input, int expected) . ... Reads the image from the InputStream and returns the pixel array (byte, short, int or float). java.lang.Object . ... Skips the specified number of bytes, then reads an image and returns the pixel array (byte, short, int or float). java.lang.Object . ... Skips the specified number of bytes, then reads an image and returns the pixel array (byte, short, int or float). ...

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• SpecifyROI (ImageJ API)
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... Computerised Instrument Control and Data Acquisition (CICADA) is a software system for control of telescope instruments in a distributed computing environment. ... Computerised Instrument Control and Data Acquisition (CICADA) is a software system developed to provide access to, control of, and retrieval of data from, instruments mounted on observatory telescopes. ... Each instrument class generates its own request data structures using its own generate_req method, which is called by the control...

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... The DD tag element specifies a term definition, and follows one or more DT elements. ... CLASS . ... The CLASS attribute is most commonly used to attach a different style to some element, but it is recommended that where practical class names should be picked on the basis of the element's semantics, as this will permit other uses, such as restricting search through documents by matching on element class names. ... CLEAR . ... The CLEAR attribute allows you to move down unconditionally: . ...

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... The CLASS survey is a collaboration between Jodrell Bank, Caltech (USA) and Leiden/Dwingeloo (Netherlands) which aims to find new cases of gravitational lensing. ... Variability is a prerequisite for determining time delays between the components of the lens system and thus estimating the Hubble constant. Good progress towards measurement of the Hubble constant is being made with observations of one JVAS object, 0218+357; a time delay of about 12 days has been determined. ...

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• CMOS tutorial-radiation
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The RHEA spectrograph is an instrument currently under development at Macquarie University in Sydney and is expected to relocate to MSO later this year. ... The new feed is intended to substantially improve the throughput of the telescope-spectrograph system through the use of Phase Induced Amplitude Apodization (PIAA), a beam shaping technique, and a multi-fibre Integral Field Unit (IFU) using a microlens array and single mode fibres (SMF). ...

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• A series of images from Hermann Wehner, showing the telescope in its original
• Software Maintenance Manual
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SETUP : For service mode observations within the SOLARNET Access Program, ROSA and IBIS can be utilized either as stand alone instruments, or combined together. ... PROPOSAL STRUCTURE: Proposals should include up to max 2 pages, including a scientific rationale and technical requests (detailing i.e. spectral filters and wavelength sampling). ... For the case of joint IBIS and ROSA observations, proposals should indicate which instrument is to be considered as the primary one. ... SOLARNET Access . ...

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... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... September Perseid meteors captured by the . ... Its occurrence provides astronomers with interesting new data about the hidden trails of meteoroids тАФ small bodies ranging in size from fine dust particles to objects of marble-size and larger тАФ in the solar system and their supposed sources: comets and asteroids passing through the inner solar system. ... The particular comet that created the September Perseids is unknown...

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... Classes . ... Dust :: MMPUV . The radiation field published by Mezger, Mathis and Panagia. ... Inheritance diagram for Dust::MMPUV: . ... Collaboration diagram for Dust::MMPUV: . ... MMPUV (double chi) . These are the methods for the MMPUV class. virtual double . ... double . ... Returns the radiation field of Mezger, Mathis and Panagia ( 1982A&A... ... 372M ) as ammended in the 1983 paper. chi controls the scaling of the field. double Dust::MMPUV::operator() . ... The Specific Energy density. ...

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• DUST: Dust::RadField Class Reference
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... Exposure Time Calculator (ETC) . Survey processing . ... VISTA is a 4-m class wide field survey telescope for the southern hemisphere, equipped with a near infrared camera (1.65 degree diameter field of view at VISTA's nominal pixel size) containing 67 million pixels of mean size 0.34 arcsec and available broad band filters at Z,Y,J,H,K s and a narrow band filter at 1.18 micron. A wide field visible camera, if constructed, could also be used on VISTA. ... Tile . ... ESO VISTA Public Surveys . ...

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An example of visual expert system. The program is written on Actor Prolog. -- -- (c) Alexei A. Morozov, March 19, 1999. ... Actually I wrote this program to train myself -- -- in carrying out SADT interview. ... A logical description of the blocks of the SADT model. ... The main purpose of these classes is keeping lists of cooking -- -- battery corresponding to various blocks of the SADT model. ...

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• Actor Prolog. Programming language definition.
• Actor Prolog User Guide. Residents.
• Actor Prolog. Example "D:\MOROZOV\Z\DEMO\EXE\EXAMPLES\SADT\JAM\JAM.A"

This is a personal project collecting and documenting early images of Harvard College Observatory, focusing on the site at Observatory Hill (previously Summer House Hill). ... The current focus is through about 1920, and filling out the history of the Cambridge location, and buildings. ... Because I'm also interested in the history of printing and image reproduction, some of the information here will emphasize that viewpoint. ... All images plus additional timeline notes (138) . ... Selina Bond (0) . ...

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... 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. ...

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• LWN: Driver porting: Device model overview
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