User Parameters - Spectral-line Imaging ======================================= There are several steps involved in running the spectral-line imaging, with several optional pre-processing steps: 1. ... Following this pre-processing, the resulting MS is imaged by the simager task, creating a set of spectral cubes. ... channel (:doc:`../calim/mssplit`) | ... The number of channels in the tile size used for the new MS. The | ... imaging individual channels. ... GRIDDER_SPECTRAL_SNAPSHOT_IMAGING`` | ...

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• Apply Your Original Calibration Before Self-Calibrating
• User Parameters - Continuum Self-calibration CentralProcessor 0.11...
• User Parameters - Continuum Source-finding CentralProcessor 0.11 documentation

... 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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Next: Implementation Design of the ASC Data Model . ... The AXAF Science Center (ASC) is using an ``open architecture'' approach to develop its data analysis environment. The system is a loosely coupled environment consisting of several major applications: visualizer, browser, fitter/modeler, as well as the data analysis tool-box. The ASC Data Model and Interprocess Communications (IPC) provide the data interface between applications and tools. ... Figure: Data analysis environment. ...

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• Application of the Minimum Determination Algorithm to the Study of the Fine
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• ADASS 2003 Conference Proceedings

... ASSOCIATE/RANK table col1 col2 [action] . ... BIN/TABLE table col1 col2 [bin] [min] [max] [sigma] . creates a table, bin.tbl with averages of col2 in bins of col1 . COMPARE/2SAM table col1 col2 . ... COMPUTE/FIT image[,error] [= function[(refima)]] . ... COMPUTE/FIT table y[,error] [= function[(ind)]] . ... COMPUTE/FUNCTION image = function[(refima)] . compute function values, result as image . COMPUTE/FUNCTION table y = function[(ind)] . ... define user functions for fitting . ...

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• Maximum Likelihood Application
• Line parameter measurements
• Multivariate Statistical Methods

... 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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... I happened to observe a surge of principle component analysis (PCA) and independent component analysis (ICA) applications in astronomy. ... Category: Algorithms , arXiv , Astro , Cross-Cultural , Data Processing , Jargon | ... Algorithms arXiv Astro Bad AstroStat Bayesian CHASC Cross-Cultural Data Processing Fitting Frequentist Galaxies gamma-ray High-Energy Imaging Jargon Job Languages MC MCMC Meta Methods Misc News Nuggets Objects Optical Physics Quotes Spectral Stars Stat Timing Uncertainty X-ray...

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• *plcreate* -- Defining a Region
• *qplintran* -- Apply linear transformation to a qp file through filter
• The AstroStat Slog Blog Archive [ArXiv] component separation methods

... new LaTeX template, approved version . ... only minor changes for task version 1.4 . ... applies to task version 1.5: . ... applies to task version 1.6: minor updates . ... applies to task version 3.0: new parameter names . ... applies to task version 3.1: parameter gain file removed . ... applies to task version 5.0: new parameter randomization_on . ... applies to task version 5.1: new optional parameter srcposition . ... Null values, high/low accuracy gain/cti correction, new errors and warnings ....

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• Parameters
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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
• Marc White - Astrophysicist - The Australian National University

... Cases of interest include weak absorption lines located in the vicinity of stronger lines, isolated weak lines in relatively noisy spectra, and severely blended, strong saturated lines. ... The top left panel illustrates the input spectrum. The top right panel shows the input spectrum after convolution with the LSF of the 2 0 0 25 slit and the G270H grating. ... The residuals with respect to the original input spectrum are plotted on top of each restored spectrum. ... 1993). ...

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• Application to Simulated Data
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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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• Database of Optical Constants -- Misc: computer codes
• AI SPbU library of scattering codes
• Database of Optical Properties -- Level: subpage

... SPARCompiler(TM) Fortran 90 1.0 . FORTRAN 77 3.0.1 . ... important of these. -ansi: Report non-ANSI extensions. -c: Suppress linking, produce .o files -e: Recognize extended (132 character) source lines -fast: Specify common set of performance options - fixed : Interpret all Fortran source files according to fixed form rules -flags: Print summary of compiler options -fnonstd: Non-standard initialization of floating-point hardware -fnonstop: Execute without trapping on invalid, overflow ...

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• Notation
• Y. Meyer, 1993, Wavelets: Algorithms and Applications, S.I.A.M.
• Gaussian Chirplet

... 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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• http://www.gao.spb.ru/english/as/j2014/presentations/kurdubov.pdf
• http://www.gao.spb.ru/english/as/publ/miller_malkin_ivsgm-2008.pdf
• Pulkovo NEO Page: Ephemeris Support

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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• Cosmology, Extragalactic Astronomy, and Applied Astrophysics 2004
• Change of Binary Parameters: Mass, Semi-major Axis and Eccentricity

MULTISCOPES . MULTISCOPE-EF . ... HOME . ... ABOUT LOMO . PRODUCTS . MICROSCOPES . ... SURGICAL MICROSCOPES . ... Home Products Microscopes Multiscopes Application guide . MULTISCOPE™ APPLICATION GUIDE . Applications . ... Recommended MULTISCOPE™ Configurations . ... Middle School . Life Science . Earth Science . ... Medical School . Veterinary School . ... Biological science . ... LOMO America, Inc. ... 847) 215-8800, Fax: (847) 215-9073 . ...

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• Microscopes
• IQ-702
• IQ-703

CIMA configuration files offer You a conveniant way of saving CIMA set-ups to files. ... Then instead of making this selections interactively when You are observing, You can just load and apply the configuration files. ... Any other set-up will be ignored! ... In that case, You are forced to use the 'Load only' option to load the configuration file, inspect the selected set-up carefully, apply the set-up (with the 'Accept' or 'Apply' buttons) and then save a new version of the configuration file. ...

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• Chapter 5. Listing of Installed Components
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Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...

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... The SDSS 2.5-m primary mirror is supported in a manner similar to the Apache Point Observatory 3.5-m telescope primary. ... The axial support is provided by 48 air pistons. The pistons have the same diameter thereby applying equal forces with the same air pressure. ... Each group supports a 120њ sector of the mirror. ... Figure 1: CAD drawing showing the 2.5-m primary mirror and the locations of actuators (green circles) These actuators apply forces (10*cos2 N) to correct astigmatism. ...

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• Procedure to Collimate the SDSS 2.5m Secondary Mirror
• Astigmatism I
• Instrument Data Fitting

... The general­purpose data reduction package FIGARO is now available to be run from the IRAF CL, and more Starlink applications will follow in due course. ... A system has been developed to enable packages written for the Starlink Software Environment to be run from the IRAF CL so that an IRAF user can mix and match application tasks from the two environments as required to process data, all under the control of the IRAF CL. ... Mixing IRAF and Starlink Applications -- FIGARO under IRAF 179 3. ...

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• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)
• TRAXY (V0.4) --- Dec99 --- TRAXY (V0.4)
• ASNCOMBINE (Nov98) --- nictools --- ASNCOMBINE (Nov98)

... Bojan Nikolic web pages (r. 329) . ... We present a Bayesian approach to calculating the coefficients that convert the outputs of ALMA 183 GHz water-vapour radiometers into estimates of path fluctuations that can be used to correct the observed interferometric visibilities. ... Inference of Coefficients for Use in Phase Correction . ... Simulating Atmospheric Phase Errors, Phase Correction and the Impact on ALMA Science . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

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• Bojan Nikolic -- Nested sampling modelling of Star-Formation History of the
• Inference of Coefficients for Use in Phase Correction
• OptInt PmWiki : PmWiki / Debug Variables

... To achieve a more 3D-like effect on the results of the LIC process, you can apply the following steps: . Duplicate the result of the LIC, call this B. Apply the "Grayify" plug-in to B. Apply the "Relief" plug-in to B. Apply the "Brightness-Contrast-Gamma" (BCG) plug-in to B and adjust the contrast-parameter to your liking. ... Multiply B with the original result of the LIC process, call this C. Use the BCG plug-in again to adjust the brightness and contrast of C. Voila! ...

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