... The SF does not contain all the information required to process the ODF with the SAS. odfingest extends the SF with data extracted from the instrument housekeeping data files and the calibration database. It creates a new summary file: the SAS ODF Summary File (SOSF). ... The user need not have write access to the ODF directory. odfingest uses the parameter outdir to learn where to write the SOSF. ... Alternatively, the name of the SOSF can be passed to odfingest with the parameter summaryfile . ...

Еще в разделе: (Показать все результаты (>38033) - xmm.vilspa.esa.es/ )

• Command line options

... Co-ordinate systems description . Directories structure . The file names' construction . The file set description . ... The orbital information for each month is presented in the separate directory. The INTERBALL orbital data are located on the STDA server, for each month in the separate subdirectory, which name consists from the year (YYYY) and month (MM) numbers. The Parent Directory of the Tail Probe orbital data is http://www.iki.rssi.ru/da/interball/tail/orbit/ . ...

Еще в разделе: (Показать все результаты (>1892) - www.cosmos.ru/ )

• STDA files
• Multipoint correlations of the solar wind parameters observed by several

... The HST-specific Generic Edited Information Set (GEIS) format 1 is the standard format for reducing data from FOC, FOS, FGS, GHRS, HSP, WF/PC-1, and WFPC2. All HST images in GEIS format consist of two components: a header file and a separate binary data file , both of which should reside in the same directory. ... GEIS binary data files, whose suffixes end in "d" (e.g., w0lo0105t.c1d ), contain one or more groups of binary data. ... However, the group parameters are stored in the binary data file. ...

Еще в разделе: (Показать все результаты (>23988) - www.stsci.edu/ )

• http://www.stsci.edu/documents/dhb/web/c03_stsdas.fm2.html
• http://www.stsci.edu/documents/dhb/web/c01_intro.fm4.html
• NICMOS Proposing Example - 1

Next: Software for Geodynamical Researches Used in the LSGER IAA . ... We present DIRT , a Java applet geared toward modeling a variety of processes in envelopes of young and evolved stars. ... A1.00E+00 /I1.00E+13/models.tgz /I3.00E+13/models.tgz A1.00E+01 /I1.00E+13/models.tgz /I3.00E+13/models.tgz . A5.00E+02 /I1.00E+13/models.tgz /I3.00E+13/models.tgz Each models.tgz file is untarred into the temporary area on the server, from which the model data are transferred to the client applet. ...

Еще в разделе: (Показать все результаты (>1995) - www.adass.org/ )

• AIRY: Astronomical Image Restoration in interferometrY
• A Spectroscopy Exposure Time Calculator for IRAF
• TwoFitlines: An Spectrum and Line Analysis Tool

Examples of pipeline processing . ... This page presents examples of "on the fly" processing of FITS astronomical data available on the WEB using the HyperLeda pipeline tools. ... In many cases, raw data are archived and a consisten description of the file (FITS header) allows to process them on the fly. ... This first command makes a "pre-view" display of the image. o=fa:L93111HP1/00147&z=vg . ... The result of a pipeline processing is a FITS file that you can read as a normal disk file. ...

Еще в разделе: (Показать все результаты (>4051) - www.sao.ru/ )

• Edition of the Table Containing the Cloud Model
• Starting up
• Event Handling

... CentralProcessor 0.11 documentation . Utilities . The CASDA upload utility prepares artifacts for submission to the CSIRO ASKAP Science Data Archive (CASDA). ... Evaluation Pipeline Artifacts (any file format) . ... The measurement set is a directory, where CASDA requires a single file per artifact . ... The following example declares four artifacts to be uploaded to CASDA, one for each of the artifact types: image, source catalogue, measurement set and evaluation report. ...

Еще в разделе: (Показать все результаты (>36564) - www.atnf.csiro.au/ )

• Central Processor Manager CentralProcessor 0.11 documentation
• ccontsubtract CentralProcessor 0.11 documentation
• Host Command-Line Interface

In this chapter we will consider two very simple but useful Web agents that I have written on Actor Prolog for my own needs. ... Let us start the Web agent. Fig. ... Start of the Web agent. The Context diagram consists of three blocks: "Logic Programming Sites", "Edit", and "Check". ... Some Web sites that are linked with the logic programming and Prolog are listed in the pulldown list (these addresses are transferred to the "Edit" block from the "Logic Programming Sites" block). ...

Еще в разделе: (Показать все результаты (>681) - www.cplire.ru/ )

• Getting Started in Actor Prolog. Oil Production.
• Actor Prolog User Guide. Residents.
• Getting Started in Actor Prolog. Component-Oriented Programming.

CIMA is more than just the observing tool - in fact, the observing tool is just a part of a bigger package called the CIMA software package. ... There is also a another package called the CIMA WAPP software which contains the WAPP software, the special Tcl/Tk interpreter used by CIMA and support libraries. ... All CIMA software components recognize the following general options that are part of the CIMA version selection system: . ... The select_cima script can be used to set up a default version. ...

Еще в разделе: (Показать все результаты (>7352) - www.naic.edu/ )

• The Arecibo User Manual for Astronomers
• OLD ANALYZ instruction sequences HI in galaxies
• pdev_birdies_25jun07

Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...

Еще в разделе: (Показать все результаты (>715) - xray.sai.msu.ru/ )

• Parameters of binary compact star evolution
• Initial parameters of compact stars
• Structure of the Galaxy

Databases (NSDC) of the Natural Planetary Satellites. ... NSDC: Database of astrometric observations of Natural Planetary Satellites . ... They are thoroughly looking for observations in different sources, creating their owndatabases which are then mostly inaccessible to other researchers. ... In the file "content" with explications, the reference is given to the data source as well as the bibliographic reference. ... Data sources. ... Why a specific bibliographic database for Natural satellites? ...

Еще в разделе: (Показать все результаты (>483) - lnfm1.sai.msu.ru/ )

• IDL programs

... An error involving a missing tasks parameter indicates that the parameter file may have changed between the last time the task was used and the current version. ... If still in trouble, delete the parameter file in `myiraf/uparm' corresponding to the task (the names are somewhat contrived, but with a bit of imagination it is not too difficult to identify the right one). ... The imcnts task and region masks . ... A region descriptor of the kind: . CIRCLE(403, 403, 22.5) . ... See `help regions'.) ...

Еще в разделе: (Показать все результаты (>4362) - hea-www.harvard.edu/ )

• Model Spectra for Spectral-Fitting Program
• QPOE Files
• ChaMPlane data_archive_.html

... Bojan Nikolic web pages (r. 329) . ... Since version 0.12, libAIR comes with a simple command line interface to the routines which retrieve the water vapour and the phase correction coefficient. Currently only the very simplest model is supported, in which the all of pressure, temperature and water vapour column are free parameters, and they are inferred from the four observed water vapour radiometer readings. ... Command line interface to libAIR and water vapour column retrieval . ...

Еще в разделе: (Показать все результаты (>3420) - www.mrao.cam.ac.uk/ )

• Example of an OOF analysis for the GBT
• Example of an OOF analysis for the GBT Bojan Nikolic web pages (r. 329)
• A prototype build system for CASA using SCons Bojan Nikolic web pages (r. 329)

... FileљStructure . ... After downloading all the catalogues, the paths to the various files should look like this: Installation Data Directory / stars / default / stars _0_0v0_1.cat Installation Data Directory / stars / default / stars _1_0v0_1.cat Installation Data Directory / stars / default / stars _2_0v0_1.cat Installation Data Directory / stars / ... In this case, all the files would be in the <Installation Data Directory>/stars/default directory. ...

Еще в разделе: (Показать все результаты (>1746) - astro.uni-altai.ru/ )

• Stellarium: Plugins
• Stellarium: StelModuleMgr Class Reference
• Stellarium: Scripting Engine

... There is an opportunity to perform O-C calculations for objects which are absent in the data base of the package. Such objects can be described by orbital elements or by initial coordinates and velocities. ... On pressing Edit file button user has a possibility to look through the list of object elements or their coordinates and velocities to add or to change it. ... For example, the designations of objects in the list can occupy the last position in each line. ...

Еще в разделе: (Показать все результаты (>834) - www.ipa.nw.ru/ )

• AY2008 (preface)
• AY2009 (preface)

Next: Running CONSTRICTOR Up: How to use CONSTRICTOR Previous: Parameters Contents . ... OutputBeam.BiasMod(07:12) = 1, 7, 10, 8, 3, 5 OutputBeam.StationID(01:04) = 1, 3, 4, 6 OutputBeam.StationID(05:08) = 1, 2, 4, 5 OutputBeam.Wavelength (01:04) = 849.4e-9, 820.9e-9, 793.9e-9, 768.3e-9 OutputBeam.Wavelength (05:08) = 744.2e-9, 722.9e-9, 701.5e-9, 683.1e-9 OutputBeam.Wavelength (09:12) = 664.6e-9, 648.9e-9, 617.7e-9, 603.5e-9 OutputBeam.Wavelength (13:16) = 590.7e-9, 577.9e-9, 566.5e-9, 556.6e-9 ...

Еще в разделе: (Показать все результаты (>21669) - www.eso.org/ )

• ESO - Common Pipeline Library
• DFOS: directory structure
• Preparation of parameter file

... SFIT is a general-purpose code designed to optimize theoretical stellar spectra to an observed spectrum. ... While the programme expects input from "stdio", it is more natural to save commands in a file (eg "sfit_input") and run the code simply by . ... If the spectra to be fitted have a filename "star_spectrum", then the best fit spectrum will be written out, together with the renormalized input spectrum, to a file called "star_spectrum.fit". ... sets up model spectrum grid (and for 2nd star) . ...

Еще в разделе: (Показать все результаты (>3483) - star.arm.ac.uk/ )

• ffit help file
• SCL Sfit Commands
• lte-codes: sterne model atmospheres

... Minute Values of Geomagnetic Field Components . ... AA 1868 - Present (3 hourly and daily) (monthly) (yearly) (Lists and histograms of geomagnetic disturbance and Solar Sunspots) KP_AP 1932 - Present (3 hourly and daily) (Lists and histograms of geomagnetic disturbance and Solar Sunspots) AE_HV 1957-75, 78-88 (hourly) AE_MIN 1978-881-6;198903;1990-94 (minute) DST 1957 - Present (hourly) PC 1975 - Present (15-minute) AMANAS 1959 - Present (3 hourly and daily) KMKNKS 1983 - Present (3 hourly) . ...

Еще в разделе: (Показать все результаты (>9276) - www.wdcb.ru/ )

• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/fo E
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/f min
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/fb Es

System parameters on Digital UNIX . ... Digital and Cray use the number of bytes as the KIND -parameter. ... LOGICAL Default byte word KIND number = 4 1 4 LOGICAL Default double quad KIND number = 4 8 16 INTEGER int15 int31 int63 KIND number = 2 4 8 digits = 15 31 63 radix = 2 2 2 range = 4 9 18 huge = 32767 2147483647 9223372036854775807 bit_size = 16 32 64 REAL single double quad KIND number = 4 8 16 digits = 24 53 113 maxexponent = 128 1024 16384 minexponent = -125 -1021 -16381 ...

Еще в разделе: (Показать все результаты (>6641) - crydee.sai.msu.ru/ )

• NAG's Fortran 90
• The Frequency-Frequency (FF) Plane
• The Chirplet Transform: Physical Considerations

... A file upload element on an HTML form. ... JavaScript 1.1: added type property . ... The HTML INPUT tag, with "file" as the value of the TYPE attribute. For a given form, the JavaScript runtime engine creates appropriate FileUpload objects and puts these objects in the elements array of the corresponding Form object. ... form . ... For all FileUpload objects, the value of the type property is "file" . ... Use the value property to obtain the file name that the user typed into a FileUpload object. ...

Еще в разделе: (Показать все результаты (>11374) - www.arcetri.astro.it/ )

• mod_session_crypto - Apache HTTP Server
• Tirgo Worm Handling
• mod_authn_dbd - Apache HTTP Server

. ___________________________________________________________________ The Electronic Universe Project e-mail: nuts@moo.uoregon.edu

Еще в разделе: (Показать все результаты (>414) - zebu.uoregon.edu/ )