... Dr. Ravil Nazirov is the head of the workshop, and Andrew Ananjev is the secretary of the workshop. ... The workshop is used to be held in the last decade of the month, preferably on Tuesdays. ... The next session will take place October 29, 1996 . ... There is "CONPAS" mailing list which you can join to discuss issues of problem solving and to be automatically notified of important dates and decisions with respect to the coming sessions. ... Secretary of the Workshop: Andrew Ananjev . ...

Еще в разделе: (Показать все результаты (>577) - www.iki.rssi.ru/ )

• Examples of the raw magnetic field information, obtained with the MIF-M
• Short Abstract; Mar. 1995 CONPAS workshop
• Next session; June,18 1996 CONPAS workshop

ON THE IMPACT OF THE GALACTIC ABERRATION ON VLBI-DERIVED PRECESSION MODEL Z.M. MALKIN Pulkovo Observatory Pulkovskoe Ch. ... Corrections to adopted precession rate are usually computed from the linear trends in long-term time series of celestial pole offset (CPO), which are the differences between the measured and the theoretical coordinates of the celestial pole. ... CONCLUSIONS We have estimated the impact of GA on parameters of precession-nutation model derived from VLBI observations. ...

Еще в разделе: (Показать все результаты (>286) - www.gao.spb.ru/ )

• http://www.gao.spb.ru/english/personal/malkin/publ/zm12j.pdf

Next: Multiresolution with scaling Up: Pyramidal Algorithm Previous: The Laplacian Pyramid . To modify the previous algorithm in order to have an isotropic wavelet transform, we compute the difference signal by: . ... The reconstruction method is the same as with the laplacian pyramid, but the reconstruction is not exact. ... If represents the wavelet coefficients pyramid, we look for an image such that the wavelet transform of this image gives . Van Cittert's iterative algorithm gives: . ...

Еще в разделе: (Показать все результаты (>2173) - www.sao.ru/ )

• The Modified Gauss--Newton Method.
• Wavelength calibration
• ASTROMET/COMPUTE

PRE-COSTAR FOS APERTURE THROUGHPUT VARIATIONS DUE TO OTA FOCUS CHANGES D. J. Lindler and R. C. Bohlin FOS Instrument Science Report CAL/FOS-102 93 August ABSTRACT Since the throughput of the FOS entrance apertures depends on the HST focus, estimates of absolute fluxes from observed count rates require a correction for focus effects. ... The 4.3 arcsec aperture throughput observed by a 1.43 arcsec high diode array varies by approximately 10% over this range. ...

Еще в разделе: (Показать все результаты (>15767) - www.stsci.edu/ )

• VAX Computer Account Request: Operations Cluster
• Absolute Photometry
• IR alpha Flats

This document explains values, tables and other matters on solar physics computing pages. ... is040423.ete : SAHA-S tables, interpolation values: T, rho, X. Z is fixed at 0.02. See reference above. opal2005.etf : OPAL EOS, interpolation values: T, rho, X, Z. Downloaded from OPAL site , marked there as "2005", seems to be unpublished. opal2001.etf : OPAL EOS, interpolation values: T, rho, X, Z. Rogers F.J., Nayfonov A. Astrophys. ... The following values can be calculated: . ... dimensionless . ...

Еще в разделе: (Показать все результаты (>2116) - crydee.sai.msu.ru/ )

... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...

Еще в разделе: (Показать все результаты (>920) - jet.sao.ru/ )

• Spectrometric complex LRS
• di_eks

... Archives . ... I asked a couple of astronomers if they heard the term plug-in estimator and none of them gave me a positive answer. ... Whilst clarifying the form of sampling distribution, or on verifying the formulas or estimators of sample mean and sample variance truly match with true mean and true variance, I can drop plug-in part because I know asymptotically such interval (estimator) will cover 68%. ... Category: Bad AstroStat , Cross-Cultural , Data Processing , Jargon , Uncertainty | ...

Еще в разделе: (Показать все результаты (>3799) - hea-www.harvard.edu/ )

• *calc_bary, apply_bary* - Barycentric Time Corrections
• *calc_bary* - Computing Barycentric Corrections
• Bringing up IRAF

... When the source-detection algorithms has run omdetect will compute raw count-rates for each detected source. For point-sources (ie those sources having widths consistent with those of the point-spread function) the count-rates are obtained by aperture photometry. For binned and unbinned images the aperture is 6 and 12 pixels, respectively. ... Extrapolate (if necessary) the source count-rate to the 12 unbinned pixel aperture, using the point-spread function for the filter. ...

Еще в разделе: (Показать все результаты (>6462) - xmm.vilspa.esa.es/ )

• SourceListFile
• Correction of the energy scale in specific pixels
• Photometry

SPECIALIZED COMPUTER SYSTEMS FOR MATHEMATICAL MODELING OF DISCRETE POINT STRUCTURES READOUT PROCESS Aleksandr Reznik, Andrey Torgov, Aleksandr Soloviev Institute of Automation and Electrometry, Siberian Branch, Russian Academy of Sciences The paper describes the specialized software systems that have been used to solve difficult mathematical problems in digital images processing. ... Systems for the first computers based on FORTRAN. ... Systems based on Matlab special environment. ...

Еще в разделе: (Показать все результаты (>528) - www.ssau.ru/ )

• Scientific Computing
• The scientific journal 'Computer Optics' is planned to be issued in English
• Research and Education Center of Computer Science (REC Cs-208)

... 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. ...

Еще в разделе: (Показать все результаты (>2475) - www.meade.com/ )

• Meade Instruments Corporation - The Autostar/LX200 Command Set and Differences
• Meade Instruments Corporation - Magellan II Telescope Computer System
• Meade Instruments Corporation - Magellan I Telescope Computer System

... Tpram - time of the PRAM instrument (aquisition computer) . ... Bx - DC magnetic field with a fixed amplitude calibration; X component . ... The color lines present FFT from the AC magnetic field (Waveform); Bwx, Bwy, Bwz - from the bottom. ...

Еще в разделе: (Показать все результаты (>729) - www.cosmos.ru/ )

• How it all began

... Data archive . Tasks . ... Need to add "wheezy" type debian to pulsar login script . Jenkins . Is Jenkins the long-term solution to building software in Epping? Need to get dspsr building under jenkins . Need to migrate "distribution" tempo2/psrchive to jenkins . Add other software to jenkins . ... Group . Group Members . ... Pulsar Surveys . Pulsar Catalogue . Pulsar Data Archive . PSRFITS pulsar data standard . ... Pulsar Groups . ...

Еще в разделе: (Показать все результаты (>22222) - www.atnf.csiro.au/ )

• WALLABY - the ASKAP HI All-Sky Survey
• Summary
• Time and FITS Files

Results of analysis . ... IAA EOP Service . ... EOP series are regularly submitted to the IERS, and also are available at the IAA EOP Service page. EPN coordinate time series . EUREF Permanent GPS Network (EPN) coordinate time series is computed from analysis of available EUREF weekly solutions. ... Second solution is based on independent combination of individual EPN Analysis Centers' solutions . ... USNO GPS Timing Operations . ... GPS Time Series . ... EPN : European Permanent GPS Network . ...

Еще в разделе: (Показать все результаты (>491) - www.ipa.nw.ru/ )

• (Untitled)
• ENGAMPLE
• Keywords_262

Next: Calibrate data Up: Basic widget procedures Previous: Reduce visibility data Contents . For the reduction of astrometric delays, corrections from atmospheric dispersion and array metrology have to be computed. ... Metrology correction can also be applied to the scan data later, in which case one would initialize these data before averaging. ... Due to the low SNR of the blue channels, R EDUCE D ELAYS P HASE E DIT can be used to flag these. ... I NIT Initialize (zero) metrology corrections . ...

Еще в разделе: (Показать все результаты (>13097) - www.eso.org/ )

• Bias correction
• Dispersion correction
• Astrometry

... commands . ... data_spectrum <name> : data in "spectrum" format . ... Repeat command to add additional mask regions. sigma is the s.d. to apply to the data within the region to be masked. ... Repeat command to add additiona continuum regions. ... cont_reg_clear : Clear current continuum regions . ... The observed spectrum is then multipled by this filter to obtain a new spectrum for use by SFIT. cont_sigma : Computes standard deviation of data in continuum regions and applies it to current data . ...

Еще в разделе: (Показать все результаты (>1818) - star.arm.ac.uk/ )

• High Performance Computing Course
• Computer Systems
• All Ireland Computer Grid

Computer Ephemeris . ... Content of the Computer Ephemeris is the same as content of Soviet Astronomical Almanac (Ezhegodnik), but fully original algorithms and computer methods of calculations were used. Your requests for Computer Ephemeris for years before 2014 and your comments on its contents please direct to the author charlie@mail.univ.kiev.ua . ... Keywords: Computer Ephemerides, Computer Ephemeris, Computer Almanac, Computer Calendar. ...

Еще в разделе: (Показать все результаты (>257) - space.univ.kiev.ua/ )

• Apparent places of fundamental stars for Computer Ephemeris for 2014
• Apparent places of fundamental stars for Computer Ephemeris for 2015
• Apparent places of fundamental stars for Computer Ephemeris for 2016

... 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. ...

Еще в разделе: (Показать все результаты (>1691) - www.adass.org/ )

• Indexing and Searching Distributed Astronomical Data Archives
• The Astrometric Properties of the NOAO Mosaic Imager
• Image Processing of Digitized Spectral Data

Castalia . Asteroid 4769 . Asteroid 4769 Castalia is a near-Earth crossing asteroid that was discovered by Eleanor F. Helin (Caltech) on August 9, 1989. Scientists used radio astronomy and computer modeling to generate this image of Castalia. They obtained the data for the computer model in 1989 using the Arecibo radar/radio telescope in Puerto Rico when the asteroid passed within 5.6 million kilometers (3.5 million miles) of the Earth. ... Topographic Map of Castalia . ...

Еще в разделе: (Показать все результаты (>8832) - www.arcetri.astro.it/ )

• NICMOS3 Detector for Spectroscopy
• Procedures for Data Reduction
• Lunar Orbiter 5

This note outlines how to configure the computers needed to run DIMMWIT. ... dimmwit : ICE (single-board computer in a box) that runs the Starlight Express CCD camera, to which it is connected by a USB interface. dimmwithost : displays the finder application via the X protocol (finder actually runs on dimmwit). Acts as a file server; both the finder software and the DIMM data are stored on dimmwithost. ... mkdir -p /data/oberon/data/finder . chown coast:coast /data/oberon/data/finder . ...

Еще в разделе: (Показать все результаты (>1150) - www.mrao.cam.ac.uk/ )

• Building the OOF package: worked solutions Bojan Nikolic web pages (r. 329)
• Computing atmospheric absorption with AATM Bojan Nikolic web pages (r. 329)
• Galaxy Evolution: Computing

... Avg: the average value of the spectra (maybe throwing out some channels at the edges). <>:average over the spectra (throwing out points at the edges if you want). gCal(f) :- frequency dependence of the tabulated cal values. ... calInK(Avg): Scaler cal value averaged over the band. calOffSpc(Avg): cal off value averaged over the band (in spectrometer counts) . ... cntsToK(avg) = calInK(Avg) / (calDif_cnts(Avg)) . To convert a spectrum b_cnts in spectrometer counts to b_K in Kelvins using cntsToK: . ...

Еще в разделе: (Показать все результаты (>3097) - www.naic.edu/ )

• Gain curve for L narrow
• Spectral-Line Observing
• Computing dates when an LST is at night time