... Basic Observables: Zero-differenced phase and code ionosphere-free combinations of global GNSS network stations, corrected by P1-C1 satellite code biases (cc2noncc), daily observations with 30 seconds sampling rate Sites coordinates : IGb08 reference frame coordinates and velocities Displacements: solid tides, ocean loading, pole tide loading (IERS 2010) Geometric model : Receivers antennas eccentricities, absolute receiver and ...

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• Pulkovo NEO Page: Ephemeris Support

... CentralProcessor 0.11 documentation . ... It can be run with the following command, where ?config.in? is a file containing the configuration parameters described in the next section. ... Parset parameters understood by ccontsubtract are given in the following table (all parameters must have CContSubtract prefix, i.e. CContSubtract.dataset ). ... A number of other parameters allowing the user to narrow down the data selection are understood. ... Parameter . ... Data set file name to work with. ...

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• ccalapply (Calibration Applicator) CentralProcessor 0.11 documentation
• Application of a Bayesian Method to Absorption Spectral-Line Finding in
• User Parameters - Preparation of the Science field data CentralProcessor 0.11

polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...

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• ESO - Science Announcements

polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...

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• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)
• TRAXY (V0.4) --- Dec99 --- TRAXY (V0.4)

J/AstL/vol/page SAI Open Clusters Catalog (Glushkova+, 2009) ================================================================================ Automated search for star clusters in large multiband surveys. ... Color excesses E(B-V), distance moduli and ages were determined for 141 new and 27 known, but poorly studied clusters. We present the Sternberg Astronomical Institute Open Clusters Catalog (SAI OCL Catalog) of coordinates, diameters and main physical parameters of these clusters. ...

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• SAI OCL Catalog The Team
• SAI OCL Catalog Description
• SAI OCL Catalog Virtual Observatory

... 13th European VLBI Network Symposium . and Users Meeting . on September 20-23, 2016. ... 13th European VLBI Network Symposium and Users Meeting on September 20-23, 2016. ... Year book "Ephemerides of Minor Planets for 2016" on-line . ...

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• (Untitled)
• Keywords_54
• ENGAMPLE

... We report on the preliminary results of experiments using a Bayesian cluster method to cluster objects present in photographic images of the POSS-II. ... We believe that the application of such algorithms to large-scale astronomical sky surveys can aid in cataloging the detected objects, and may even have the potential to discover new categories of objects. ... We have thus started to explore new clustering analysis and unsupervised classification techniques for this task. ...

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• ADASS 2003 Conference Proceedings
• AIRY: Astronomical Image Restoration in interferometrY
• Building Software from Heterogeneous Environments

... This is done by taking in all input files the extension whose name is specified by the maintable parameter (called 'merged extension' in what follows) and merging the columns into a single output extension of the same name. ... Its contents is taken from the CCDID keyword (and QUADRANT for EPIC PN). ... To propagate other column specific keywords, they must be specified manually via the extensionchecks , mainattributes , maxattributes and minattributes parameters (see above). ...

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• Detailed Description

... Archives . ... Quote of the Week, Aug 31, 2007 . Aug 30th, 2007| 09:36 pm | ... From arxiv/astro-ph:0708.3758v1 . Numerical Color-Magnitude Diagram Analysis of SDSS Data and Application to the New Milky Way Satellites by J. T. A. de Jong et. al. ... A traditional CMD fitting begins with building synthetic CMDs: Completeness of SDSS Data Release 5, Hess diagram (a bivariate histogram from a CMD), and features in MATCH for CMD synthesis were taken into account. ... Chandra Blog . ...

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• The AstroStat Slog Blog Archive [MADS] Semiparametric
• The AstroStat Slog clusters
• *plcreate* -- Defining a Region

... The audience is assumed to have little or no prior exposure to Java and Object-Oriented programming. ... The topics will help you to understand how to use Java to create, access, and support Java applications and applets. ... Introduce object-oriented programming concepts and how they apply to Java programming. ... Java Applications. ... To develop Java applets and applications, one must first understand the fundamental concepts of object-oriented programming (OOP) and application development. ...

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• Internet Programming with Java
• Application to Simulated Data
• Remote Windows

Next: CCD Reductions Up: Analysis of Results Previous: Statistical Tests . ... Multivariate statistical methods can be applied in such a situation to give an objective description of the data. ... Grosb?l, P. : 1979, Image Processing in Astronomy , Eds. G. Sedmark, M. Capaccioli, R.J. Allen, Osservatorio Astronomico di Trieste, p. 371. ... Martin, R., Lutz,R.K. : 1979, Image Processing in Astronomy , Eds. G. Sedmark, M. Capaccioli, R.J. Allen, Osservatorio Astronomico di Trieste, p. 211. ...

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• Maximum Likelihood Application
• A VLA Survey of Rich Clusters of Galaxies II
• Application Commands

Applying Bayesian analysis to polarisation data J. Geisbuesch ( Cambridge ) Bayesian analysis of polarisation data LOFAR MKSP Workshop 1 / 15 Outline 1 2 3 4 Polarisation simulations @ radio wavebands Bayesian analysis Analysis of polarisation data Conclusions J. Geisbuesch ( Cambridge ) Bayesian analysis of polarisation data LOFAR ...

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• http://www.mrao.cam.ac.uk/~krause/Dogliani2003.pdf
• http://www.mrao.cam.ac.uk/~bn204/publications/2010/2010-09-OOFSoftware.pdf
• Description of the OOF software architecture Bojan Nikolic web pages (r. 329)

Next: Initial binary parameters Up: Population synthesis of Previous: Introduction . Monte-Carlo method for statistical simulation of binary evolution was originally proposed by Kornilov & Lipunov (1983a,b) for massive binaries and developed later by Lipunov & Postnov (1987) for low-massive binaries. ... Recently Leitherer & Heckman (1995) have modelled star formation for elliptical and spiral galaxies, taking into consideration only the single stars. ... Initial binary parameters . ...

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• Dependence on the Scenario Parameters and Initial Distributions
• Initial Distributions of Binary Parameters
• Structure of the Galaxy

... Институт прикладной математики им. М.В.Келдыша . БАЛЛИСТИЧЕСКИЙ ЦЕНТР . О Центре . ... Баллистический Центр Института прикладной математики им. М.В.Келдыша РАН . Баллистический центр (БЦ) ИПМ им. М.В. Келдыша создан по предложению С.П. Королева и М.В. Келдыша в 1965 году. На него были возложены работы по баллистико-навигационному обеспечению (БНО) управления полетом пилотируемых кораблей и автоматических космических аппаратов научного и народно-хозяйственного назначения. ...

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The Astronomical Society of Australia has been asked by STANDARDS AUSTRALIA to compile a list of "designated" optical observatories that are valuable resources for (i) research, (ii) education and (iii) community use. The ASA is the final arbiter of whether any particular observatory is so designated. ... Upon receipt of your application form, your observatory will be entered on a list of "Pending Designated Observatories" on the ASA Home Page. ... It will be emailed for you. ... Email . ...

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• Software Maintenance Manual

My main research interests are: . ... The method showed that the star formation in the external disc was quenched about 200 Myr ago, because of the gas removal due to the ram pressure (Pappalardo et al. ... Molecular gas and dust in spiral discs. ... Dust removal in spiral discs. ... Starting from this consideration I am at present analyzing all the spirals discs in the HeVICS sample, to find evidences of dust removed or strongly perturbed by environments, both ram pressure and/or tidal interactions. ...

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• HwB: Apple Digital Video Application (DVA) Connector (Offline)
• mod_proxy_fcgi - Apache HTTP Server
• Determination of the Detector Parameters

Optical characteristics of non-spherical scatterers . ... A list of reviews (under preparation) and links to the databases of Hovenier's and Gustafson's groups on the visible/infrared and microwave light scattering experiments, respectively. ... Light scattering codes . ... Benchmarks in optical properties . Tables of different light scattering characteristics carefully calculated by different codes (methods). Dependence of optical properties on scatterer parameters . ...

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• AI SPbU library of scattering codes
• Database of Optical Properties -- Level: subpage
• Database of Optical Properties -- Level: subsubpage

... FTP access the basic models is here . ... Below, we put short descriptions of the used SED models for the photometric redshifts providing by the current server . ... The uniqueness of this model consists in expanding to the near IR (NIR) of Rocca-Volmerange and Guiderdoni's (1988) atlas of synthetic spectra with a revised stellar library, which includes parameters of cool stars. ... Homepage of the GISSEL model). ... Another model used earlier is the model of synthetic spectra of Poggianti (1997). ...

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... Proposed directory for placement: / pub / os2 /apps/internet/ util Your name: Peter Moylan Email address : peter@pmoylan.org Program contact name: (same) Program contact email : (same) Program URL: http://www.pmoylan.org/ftp/software/ Would you like the contact email address included in listings? no Operating System/Version: OS/2 Warp 3 or later Additional requirements: Replaces : / pub / os2 / ...

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• Notation
• SunSoft
• Def file for LSOF application

... Tombaugh 4 . ... 21.10.2006 . ... But the skilled and careful astronomer also went on to discover star clusters, comets, asteroids, and clusters of galaxies. For example, pictured is galactic or open star cluster Tombaugh 4 in the northern constellation Cassiopeia . ... Publications with keywords: open cluster - star cluster . Publications with words: open cluster - star cluster . ... M45: The Pleiades Star Cluster . ... X Ray Stars of Orion . Starburst Cluster in NGC 3603 . ...

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• Journal "Peremennye Zvezdy"
• Hubble s Messier 5
• Messier 5