Computer Ephemeris for 2014 from DE200/LE200. Orbital parameters of the Sun. Date Mean Perigee Mean Paral Aberrat Epsilon Nutat longitude longitude anomaly Dec 24 272.6887 283.1787 349.5100 8.941 20.832 2326 6.72 -8.19 Jan 3 282.5451 283.1792 359.3660 8.943 20.837 6.71 -8.18 13 292.4016 283.1796 9.2220 8.942 20.834 6.76 -8.11 23 302.2581 283.1801 19.0780 8.935 20.818 6.87 -7.99 Feb 2 ...

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• Sun orbital parameters for Computer Ephemeris for 2015 (DE200/LE200).
• Sun orbital parameters for Computer Ephemeris for 2016 (DE200/LE200).
• A computer controlled low light photometer for nightglow observations

Operating of the superconducting integrated receiver channel of the TELIS atmospheric sounder. ... The noise temperature of the SIR was measured to be as low as 120 K, with an intermediate frequency band of 4 ­ 8 GHz in double sideband operation; the spectral resolution is well below 1 MHz. The SIR was implemented in the three-channel balloon-borne instrument TELIS (TErahertz and submillimeter LImb Sounder) that detects spectral emission lines of stratospheric trace gases (like ClO and BrO). ...

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• http://www.cplire.ru/html/lab234/pubs/2005-09.pdf
• http://www.cplire.ru/html/lab234/pubs/2004-05.pdf
• Research Activities of InformChaos Lab.

Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents . The parameter file contains information for CONSTRICTOR on the location of the raw data files, start and stop times, integration time, etc. ... The parameter file, YYYY-MM-DD.par , can now be created using the rawlist procedure of . ... Check beginning and tail of the listing for each file. ... Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents Christian Hummel 2015-04-28 ...

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• CONSTRICTOR parameters for astrometric reductions
• Limb darkening
• Parameters

... A technique allowing automatic representation by a relatively small number of independent parameters based on the principal component analysis of data sequences is presented. ... In recent years the spectrum of observed astronomical data can be characterized as greatly varied. ... In this instance, the problem of initial description and classification of newly-observed data becomes most urgent, especially if there is a lack of preliminary observational material and theoretical expectations. ...

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• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
• The SRON-HeaD Data Analysis System
• Indexing and Searching Distributed Astronomical Data Archives

... AMPLE (Adaptable Minor Planet Ephemerides) is integrated software package to deal with a number of problems concerning minor planets with the aid of IBM-type personal computer. ... compiling a list of all numbered minor planets which can be seen at certain moment within specified sky region and visualization of their mutual positions; . ... As AMPLE is able to reproduce virtually any table of "the Ephemerides of Minor Planets" , it may be considered as computer version of the EMP. ...

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• (Untitled)
• Keywords_54

Press the "Reset DSPs" button in kermitui. ... Now try whatever you were doing again and it will probably be better. ... First, make sure the Kermit electronics ("Leach box") are turned on. ... If the LED is on but you're still getting this error message, try turning off the Leach box. ... If this does not fix the problem, let it sit turned off for ten seconds again, turn it on, then press the reset button to the left of the power switch on the Leach box. ... Just type leachd in some xterm. ...

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• Prescription Retrieval
• Fundamental Parameters, Integrated Red Giant Branch Mass Loss, and Dust
• covar2ellipse.pro (JWST Pipeline routines in IDL)

Next: Calling Parameters Up: CAL_rgsgetXRTFigure Previous: CAL_rgsgetXRTFigure Contents . This provides the shape of the XRT along the dispersion direction (integrated in cross-dispersion). ... Numerical integration of the parameterized PSF (see HIGH accuracy level described in section 3.2.1 ) . ... The width of the PSF of the telescope scales as a function of angle of incidence on the gratings and diffration angle of the RGA by the chromatic magnification function . ...

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• Algorithm
• Parameters

... Posts tagged ?parameter estimation? ... Leccardi & Molendi (2007) have a paper in A&A ( astro-ph/0705.4199 ) discussing the biases in parameter estimation when spectral fitting is confronted with low counts data. Not surprisingly, they find that the bias is higher for lower counts, for standard chisq compared to C-stat, for grouped data compared to ungrouped. ... Tags: bias , C-stat , chi-square , chisq , Cstat , Fitting , parameter estimation , Peter Freeman , spectra . ... 1 Comment . ...

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• The AstroStat Slog nuisance parameter
• Thomas A. Fine's Computer and Technical Resources
• The AstroStat Slog Blog Archive On the unreliability of fitting

... G., Filippova A.S. Presented by: Filippova A.S Achievements · Refined model based on the celestial-mechanics methods is presented that is a generalized version of the previously developed basic model · Subtle effects are qualitatively explained based on the amplitude-frequency analysis and the computer numerical modelling of the oscillatory pole motion, where the key feature is the Chandler wobble 2 Basic Model of the Polar Oscillations ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/tsyba.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/suvorkin.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm09b.pdf

... 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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• ASKAPsoft processing of BETA data CentralProcessor 0.11 documentation
• Host Command-Line Interface
• Telescope Parameters and Search Strategy

Next: RECEIVER CHOICE Up: Spectral-Line Observing at AO Previous: Spectral-Line Observing at AO . ... These files are automatically saved into your project area on the observer computer. Note - Your project area is accessible from any Arecibo computer, and is at /share/obs4/usr/aXXXX, where aXXXX is your project number. If you do not have a project area, but still wish to use the gui, you may enter ``a9999" as your project number. ... The ``a9999" project is for testing purposes only. ...

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• pdev_birdies_25jun07
• AGES Database Search
• Arecibo Observatory: S-High Receiver

... 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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• CHIRPLET TRANSFORM SUBSPACES
• Tutorial on Fortran 90, Digital UNIX
• The Chirplet Transform: Physical Considerations

The galactic absorption is computed from Schlegel's maps . Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds", Schlegel et al 1998 . ... For Galactic objects, ag is also provided, although it does not correspond to the real extinction toward a given object (because it integrates the extinction through the whole depth of the Galaxy; for nearby objects it over-estimates the extinction). ... ag(I342)=ag(Schlegel)*3.50 . ... ag(I10)=ag(Schlegel)*3.50 . ...

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• Documentation: LEDA: parameter: vopt
• HyperLEDA documentation: parameter: vrad
• Documentation: LEDA: parameter: m21c

... spectrum . ... sfit . ... define >macro_name< : define a macro . ... meth_range <w1> <w2>: Set wavelength range for fit . data_spectrum <name> : data in "spectrum" format . ... data_sigma <sigma> : define mean standard error in data . ... data_line_set | ... NB: synth uses multiple calls to spectrum , so various Spectrum commands may also be required. synth : find optimum fit by adjusting abundances, v turb , v sin i , and v rad . ... save <fit> : Save the spectrum and best fit from synth . ...

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• Armagh Observatory: Chris Winter [ Bookmarks ]
• SCL Sfit SYN Commands
• sfit help file

Spectrometric complex of RATAN-600. ... There is a system of stable computer driven local oscillators that have accuracy about 10 to degree -8. ... Spectrometer driving system is accomplished with two DVK-4 computers and one IBM PC and make possible to develop radio line observations on the frequency band pass of the input low noise amplifiers ( LNA ): . ... The performance of spectrometric complex is controlled by program driving system ( PDS ) and the data gathering and recording system ( DGS ). ...

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• Spectral energy distribution
• SCORPIO-2 project: description
• Feed cabin 2

... There are a lot of computer codes simulating this scattering and freely available in the Internet (see e.g. links on our JPDOC page ). ... The code and input file are available in the directory . ... A slightly modified code of Barber Hill with a C-shell and input files is available in the directory . ... The code, input and test output files are available in the directory . ... See also readme file. file. ... The code, input file and their description (a TeX file) are available in the directory . ...

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• Database of Optical Constants -- Misc: computer codes
• Textbook on Computer technology for pupils
• Local Access to Electronic Journals (instruction)

... Using the Echelle with TUI . Using the Echelle with Remark . ... Configuring TUI to use the Echelle . Setting up the Echelle exposure parameters . ... Focusing the Echelle . ... Changing the echelle guider filters . ... Configuring Remark to use the Echelle . ... Echelle User's Manual . ... The Echelle home page is http://astro.uchicago.edu/echelle . ... Echelle Description . ... Enclosure . ... schematic CAD files . schematic PDF files . ... enclosure wiring schematic . ...

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• Telescope Parameters
• lsst.coordConv: coordConv::PVTCoord Class Reference

... Meade Instruments Corporation . ... Autostar Computer Controller Instruction Manual . Autostar Computer Controller . ... NOTE: This manual covers both Model #495 Autostar and #497 ETX Autostar Computer Controllers. ... Autostar Primary Menus and Options . ... Chapter 3: Alignment . ... Guided Tour Menu . ... Chapter 5: Autostar Menu Functions . ... Meade Autostar Computer Controller . ... Meade #505 Connector Cable Set Manual . ... Copyright 2006 Meade Instruments Corporation, All Rights Reserved. ...

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• Meade Instruments Corporation - Magellan I Telescope Computer System
• Meade Instruments Corporation - Magellan II Telescope Computer System
• Meade Instruments Corporation - Operating Instructions #505 Connector Cable Set

The technical memorandum: Time and Time Interval Measurement with Application to Computer and Network Performance Evaluation (PostScript) describes a number of techniques for conducting experiments typical of computer network and transmission systems engineering. ... The usual data collected during a performance run of some experiment might include time offsets, time delays, frequency offsets and various error statistics. ...

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• Oleg Bartunov's Home Page
• NIST Modem Time Service

... Obviously, the size of the cavern is of the order of the Schwartzman radius. ... Thus, consideration of the inverse effect of pulsar radiation on the properties of accreting plasma makes the ejection possible even when the Schwartzman radius is smaller than the capture radius. ... If the cavern radius , the condition at its boundary can be written as . ... Apart from magnetic dipole radiation, the cavern may also contain relativistic particles (which are also reflected from the cavern boundary). ...

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• The Model
• Initial Distributions of Binary Parameters
• Dependence on the Scenario Parameters and Initial Distributions