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? ...

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Next: Silicate minerals Up: A Database of Optical Previous: Database of Optical Properties . ... If necessary, data have been determined for the different crystallographic axes. ... In the following we give some examples of the data and their possible applications. Table: Summary of data measured in the Jena laboratory, which are currently available from the JPDOC. compound . ... amorph. ... Next: Silicate minerals Up: A Database of Optical Previous: Database of Optical Properties root 2003-03-06 ...

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• Database of Optical Properties
• Database of Optical Constants -- Level: welcome
• Database of interstellar extinction and polarization curves

... Apache HTTP Server Version 2.2 . ... htdbm is used to manipulate the DBM format files used to store usernames and password for basic authentication of HTTP users via mod_auth_dbm . ... mod_auth_dbm . ... Web password files such as those managed by htdbm should not be within the Web server's URI space -- that is, they should not be fetchable with a browser. ... The MD5 algorithm used by htdbm is specific to the Apache software; passwords encrypted using it will not be usable with other Web servers. ...

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• Determine H0 using a SQL query to LEDA
• LEDA documentation: homogenisation
• HyperLEDA documentation: parameter: objname

... Termcap is a Unix idea, that makes it possible to write software that runs on a wide range of different terminals. ... If SM can't open TERMCAP as a file, it is taken to be the value of the entry for your terminal. ... A TERMCAP variable takes precedence over an entry in your `.sm' file. ... There is a problem with using the last line of the screen as the SM command line, and this is that some terminals use the same screen for graphics as for text, and your graph will merrily scroll away as you type...

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• Why do we need a database protection treaty?
• difx:difxdb [ATNF VLBI Wiki]
• PPTA Wiki | Pipeline / Status

... Apache HTTP Server Version 2.2 . ... htdbm is used to manipulate the DBM format files used to store usernames and password for basic authentication of HTTP users via mod_authn_dbm . ... mod_authn_dbm . ... Web password files such as those managed by htdbm should not be within the Web server's URI space -- that is, they should not be fetchable with a browser. ... The MD5 algorithm used by htdbm is specific to the Apache software; passwords encrypted using it will not be usable with other Web servers....

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• The Arcetri Spectral Code - E.Landi and M.Landini (2001)
• mod_authz_dbd - Apache HTTP Server
• mod_authn_dbd - Apache HTTP Server

System of astrometric databases of Pulkovo observatory. 26-inch refractor . Pulkovo system of astrometric databases consists of three databases, which contain results of processing photographic and CCD observations, obtained with the 26-inch refractor and the Normal astrograph of Pulkovo observatory. Pulkovo photographic catalogs: Pul-2, Pul-3 (Pul-3 SE), Pul ERS . Results of photographic and CCD observations of Solar system objects . ... Normal Astrograph ...

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• Pulkovo Database of Observations of Solar System Bodies
• Pulkovo Database of Observations of Visual Double Stars
• Pulkovo Database of Observations of Solar System Bodies: Help

... In order to compare the number of different evolutionary stages obtained and X-ray luminosity of the chosen X-ray sources with the observed galactic values we use the sum of C/O+O/C , where C and O are the calculated and observed values of a given binary type, respectively. If we make comparison for a number of different binary species (for example, we compare the number of CV, number of X-ray pulsars,   total X-ray luminosity of LMXB, etc.), we write this criterion in the form: . ...

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• E-P transitions for different orbits
• Initial Distributions of Binary Parameters
• Introduction

... Even future mission archives tend to concentrate more on what can be extracted out of a proposal or a Guaranteed Time Observation log than the actual extracted science out of the data itself. ... A year later the data is then publicly available. An archive researcher has then to go through a mass of data to find what may be useful without any indication as to what the actual observer's results were while using the data except the proposal, which in most cases is very general. ...

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• A System for Web-based Access to the HSOS Database
• See Spike Run... Run, Spike, Run
• ADASS 2003 Conference Proceedings

... To select this, type 'use PALFA;' h. To list the tables in the database, type 'show tables;'. ... 2) Tables in the PALFA database : To print the fields contained in each of these tables , follow the steps in 1) for connecting to the database and then type 'describe **tablename**;' where **tablename** is one of the following: atnfshort: This contains the pulsars in the ATNF catalog, with a reduced number of parameters for each pulsar. candidates: This table will contain the candidates ...

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• GOLDMiNe: Virgo cluster optical and HI databases
• Example Observing Projects
• AGES Database Search

FGS Instrument Handbook for Cycle 24 . ... Fine Guidance Sensor Instrument Handbook for Cycle 24 > Chapter 7: FGS AstrometryData Processing > 7.2 Exposure-Level Processing . ... 7.2.2 Observing Mode Dependent Processing . ... After pipeline initialization and data quality assessments, successful observations (i.e., those that acquired the target), are processed according to the FGS observation mode: Position or Transfer. ... The corrections applied to the FGS data are as follows: . ... Transfer mode . ...

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• A New Database of Observed Spectral Energy Distributions of Nearby Starburst
• DrizzlePac: Examples

This page is intended for presentation of astronomical databases maintained at Sternberg Astronomical Institute, Moscow University. These Projects are partially sponsored by INTAS and RFBR foundations. Hypercat mirror , (RFBR #99-07-90067) . ... Catalogue of Spatially Resolved Kinematics of Galaxies , (RFBR #99-07-90067) . ... Online access to SAI catalog of SN Light Curves . ... We have implemented Web gateways to some of our catalogs. ... HTTP access to SAI Catalog of Supernovae Stars . ...

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• FTS Overview
• Full Text Search in databases
• Open Source Convention

... Panchuk V.E. Database "Stellar Spectra" consists of following main units: . ... obtained with various modifications of high resolution echelle-spectrometers at the 6-m telescope. ... Using the spectra obtained at BTA in combination with high resolution echelle-spectrometers LYNX and PFES , Chentsov E.L., Klochkova V.G. and Panchuk V.E. prepare now the next spectral atlas. ... The CATALOGUE of spectral photoplates obtained at the Main Stellar Spectrograph of the 6m telescope. ...

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• LSFVO: Press releases
• Fabry-Perot Interferometer: Data cubes
• Radio sources identfification

The preliminary version of documentation of the format for the interchange of calibrated optical/IR data being developed by Tom Pauls of NRL and John Young of COAST was presented and a number of issues discussed. The proposed format is in the general form of a relational database with different components stored in FITS binary tables. ... Should there be a single data table type that includes all data types, or multiple table types, one per data type? What data types are needed? ...

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• AMI-Planck Follow-up Observation Database
• OptInt PmWiki : PmWiki / Access Keys
• Examples of Dave Green's `cubehelix' colour scheme

GENERAL DESCRIPTION OF DATABASE . It is a matter of common knoledge, that solar magnetic fields and, in particular, magnetic fields of sunspots, play important role in many solar events. In Pulkovo observatory the long-term data set of daily observations of magnetic fields of solar sunspots was accumulated, which contains great potential for further researches in solar physics. ... Second section includes files containing sum data about magnetic fields for every observational day. ...

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• General description of the database
• Combined database of sunspot magnetic fields
• Enslish version of database

Improving the Orbital Parameters of Phobos and Deimos by Using the Universal Programming Complex ERA . ... The ERA system was used for developing the numerical dynamical theory of Phobos and Deimos. ... Very Long Baseline Interferometry (VLBI), Small Solar System Body (SSSB), Phobos, Deimos, improving the orbital parameters, Universal Programming Complex ERA, Martian satellite dynamics, the numerical dynamical theory, the secular acceleration, database of the satellites observations. ...

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• Keywords_79
• Keywords_122
• IAA VLBI Analysis Center

... The information is submitted as the tables and is distributed on given years of the observation, each of that, according to an adopted classification, includes the information about six active basins of the World Ocean: · the Northwest Pacific; · the Northeast Pacific; · the Northern Atlantic; · the Northern Indian ocean; · the Southern Indian ocean; · the Southwest Pacific. ... Lat' is latitude in degrees (up to one tenth) of the geographical place of the disturbance's onset. ...

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• MANAGEMENT PROGRAM FOR 1-MINUTE GEOMAGNETIC DATABASE

... 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 . ...

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... We received the SASS output for the HRI observation of 3C 120 (a highly variable radio galaxy with a prominent jet leaving the core at PA ) and smoothed the data with a Gaussian of FWHM = 3 '' ( Figure 13.1 ). ... The results are shown in Figure 13.2 . ... The FWHM of the original data ( Figure 13.1 ) is 11.8 (PA ); after dewobbling ( Figure 13.2 ) the width of the 50% contour is 7.6 . ... Figure 13.1 : The original data, smoothed with a Gaussian of FWHM = 3 . ...

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• ChaMPlane X-ray catalog walk-through
• ChaMPlane Database Description
• PINTofALE EXAMPLE SESSION: via Dracia

Peremennye Zvezdy ( Variable Stars ) 33 , No. ... The new variable star HD 305629, with a Cepheid-like light curve, is demonstrated, from our optical observations and ASAS-3 data, to actually be an ellipsoidal variable star on a highly eccentric orbit. ... During a systematic search of variable stars in the publicly available ASAS-3 database (Pojmanski 2002), apparent variability was found in the star HD 305629 (10 51 34 35, -60 47 57 4, J2000.0; Fig. ... The light curve and color curves of HD 305629. ...

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• XWare > APOD

. To use a different printer: lpr -Pps9 paper.ps . This sends the file paper.ps to the printer ps9 .

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• UNIXhelp Glossary - "D"
• Examples of using the sort command
• Using a different printer