... Classes . Files . ... File List . File Members . measures . Measures . ... {C, E, 0}, 00098 // {D, C, 0}, 00099 // {C, B, 0}, 00100 // {B, A, 0}, 00101 // {D, B, 0}, 00102 // {E, C, 0} }; 00103 // static uInt state [ntyp][ntyp]; // the resultant transition matrix 00104 // // diagonal == nrout 00105 // // Make the state machine 00106 // MCBase::makeState(made, state [0], ntyp, nrout, routes); 00107 // /srcblock 00108 // /example 00109 // 00110 // motivation 00111 // To ...

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Procedure to be followed by DMD secretary for DFS Group documentation . Initial email comes from author requesting document number. ... An email is then sent by the DMD secretary to the Technical Archive (tecarch@eso.org) with the same information, to request the last 4 digits of the document number (the 'chronological number'). ... Some time will pass and then the author, using the DFS Group tool 'WebCheck', will post a web readable version of the document on the DFS Group website. ...

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• the Technical Archive procedure for issue of documentation
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... Watchouts . ... Any XMM-Newton users, who need to convert OM count rates in the optical and UV filters into fluxes (expressed, e.g. , in erg/cm/cm/s/A), can do it by following any of the methods we outline below. OM count rates can be obtained with SAS. ... UVW1 . ... UVM2 . ... convert from count rate, obtained with SAS (files *SWSRLI*, corrected count rate in CORR_RATE column), to flux, selecting the most appropriate factor for the chosen spectral type and filter from the following Tables: . ...

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lsst.coordConv љ unknown . ... Classes . ... All љ Classes љ Namespaces љ Files љ Functions љ Variables љ Typedefs љ Enumerations љ Enumerator љ Pages . coordConv: Astronomical Coordinate Conversions . The coordConv package provides the following classes and functions. ... Coord : represents a position on the sky, with proper motion and radial velocity; provides easy access to spherical and cartesian position. ... Position conversion functions: . ... Time conversion functions: . ...

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... One Jansky (Jy) is defined as 10 -26 Wm -2 Hz -1 , so it is a unit of measurement of the spectral flux density, F . ... 3x10 -12 . ... erg sec -1 cm -2 ?m -1 . ... where m is the magnitude and F o the zero-point flux for the given photometric band. ... Surface brightnesses are generally measured in Janskys arcsec -2 , MJy steradian -1 or magnitudes arcsec -2 . If you have a surface brightness S in MJy steradian -1 , then you can use: S [Jy arcsec -2 ] = S [MJy ster -1 ] x 0.084616. ...

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• Pipeline Conceptual Overview GPI Data Pipeline 1.0 documentation
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... Data may be optionally rescaled. copyheader copy header keywords from one FITS file to another ( see also FTOOL cphead ). copywcs copy just the World Coordinate System keywords from the header of one FITS image to others. fcolappend append a constant column to a FITS table fitsparsename Prints components of the extended FITS file name. fitspha convert ASCII files to FITS PHA ( See also listhead supplied with FITSIO. modifyheader modifies FITS header. ...

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The HI line magnitude m21 has been corrected for self-absorption effect following Heidmann et al (1972) , with parameter kappa=0.031. The inclination needed to compute this correction is given as parameter incl . If inclination is higher than 89 deg the maximum correction is limited to -0.82 mag. Corrected flux at other wavelengths are given in the parameters: bt , it . The measured HI flux is m21 .

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These are very prominent absorption lines is most all galaxies. ... These pair of absorption lines will appear in all the spectra and they should be your principle source for determining the redshift. ... When this applet opens you will see an iconic representation of galaxies in the left hand side of the applet and a target area in the right side of the applet. ... Note: What you are doing in this excercise is identical to what Hubble did in the 1920's and you are using the same galaxies. ...

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The most recent kpyymm.tab (yymm stands for year and month, each expressed with two digits) files are distributed per e-mail half-monthly by Dr. H.-J. Linthe, mailto:kp_index@gfz-potsdam.de Both recent and past tables are supplied as an archive on the FTP servers . ... Since many observatories are interested mainly in the international quietest and most disturbed days, beginning August 1996 three extra lines have been added to the end of the table containing these values in an easy to read form. ...

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... Apache HTTP Server Version 2.4 . Apache > HTTP Server > Documentation > Version 2.4 > Miscellaneous Documentation . ... This page documents all the relevant standards that the Apache HTTP Server follows, along with brief descriptions. ... http://www.rfc-editor.org/errata.php - RFC Errata . ... This document summarizes the history of HTML development, and defines the "text/html" MIME type by pointing to the relevant W3C recommendations. ... HTML documents are SGML documents. ...

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... SAT Results ./ ... Manuals ./ Manuals/Third Party Documentation ./ Manuals/Third Party Documentation/Heidenhain Documentation ./ Manuals/Third Party Documentation/Emerson CT Documentation ./ Manuals/Third Party Documentation/Phoenix Contact Documentation ./ Manuals/Third Party Documentation/Puls ./ Manuals/Third Party Documentation/Telemecanique Documentation ./ ... Operations & Maintenance Manual Part 1 RevB:12jan15 (.pdf) . ... SAT part 1 Tests in Local Control (.pdf) . ...

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OptInt PmWiki : Pm Wiki / Custom InterMap . ... Custom markup > . ... This page describes PmWiki's default InterMap links, and how a wiki administrator can create additional InterMap links. An intermap entry takes the following format: . ... The default intermap.txt distributed with PmWiki (in the scripts/ directory) includes the following InterMap entries: . PmWiki: http://www.pmwiki.org/wiki/PmWiki/ Cookbook: http://www.pmwiki.org/wiki/Cookbook/ Wiki: http://www.c2.com/cgi/wiki ? ...

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• OptInt PmWiki : Custom InterMap

... We can help students grasp the significance of Hubble's extremely keen eye, and learn a bit about angles and math in the process, with the following in-class activity. ... Looking through binoculars or telescopes allows us to magnify a small section of the sky. To measure sizes or distances in that small section, astronomers divide a degree into 60 smaller pieces called arcminutes, and further subdivide minutes into 60 smaller sections called arcseconds. ... 30 feet = . ... 36 seconds . ...

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XEphem Forum Message . ... Post . ... Re: Catalog Conversion Utility . ... Post Message | ... the old versions and catalogs still exist on the german mirror: . ftp://iphcip1.physik.uni-mainz.de/pub/xephem_3.2/catalogs/ . An other xe to xe2 conversion utility is at: http://www.simg.de/xetoxe2.e.html (HP) . ... www.astronomy.net . About Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• Re: C9.25 Conversion? - an Astronomy Net Celestron Forum Message

Follow-up astrometry and recoveries are made with the ANU 40 inch (1.0-m) f/8 reflector at Siding Spring Observatory (IAU code 413). ... A routine follow-up of 2003 WY153 on 2003 Dec 15 became much more than routine when a faint object with unusual motion vector was found close to the target asteroid. ... During routine astrometry with the 1.0-m to improve the orbit of the Apollo asteroid 2004 CB, the asteroid was found on March 30 to have a short tail! ... Siding Spring Survey Main Page . ...

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• Lesson 1: DC Circuits

Investigation of linear and nonlinear mode conversions in inhomogeneous plasma and finding of new effects of the principal importance including the following: . ... the higher harmonics generation under the electromagnetic wave interactions with the inhomogeneous plasma in the plasma resonance layers presence (together with V.E.Zakharov, N.S.Erokhin); this effect was confirmed experimentally and it is important, in particular, for a plasma diagnostics; . ...

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• About modification of the INTERBALL orbital elements
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The database contains references to the papers, data files and links to the Internet resources related to measurements and calculations of the optical constants in the wavelength interval from X-rays to radio domain. ... References to some useful books and reviews on the subject (e.g. the classical handbooks edited by E.D.Palik) and links to Internet collections of optical constants and personal WWW pages with related software were also placed in the database. You have arrived at our welcome page. ...

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• Database of Optical Properties -- Level: subpage
• Footnotes

. If you wish to get this document direct from the mail based `info-server' please send a message to info-server@uk.ac.nsfnet-relay with a message containing the following body: Request: guestftp Topic: userguide Request: end . Topic userguide.ps will retrieve the PostScript version of the userguide, userguide will retrieve plain ASCII text.

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• Sorting the content of a file
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Astronotes Armagh Planetarium's Stellar Blog! ... Stars . ... Space Flight . ... Some 13.7 billion years ago, a mere millionth of a second after the Big Bang, the first hydrogen and helium nuclei condensed out of a hot, dense soup of quarks and gluons. ... In the very last few kilometres some of the light was scattered by a myriad of water droplets (containing hydrogen nuclei which had existed almost since the Big Bang) slowly descending through the air following a rainshower. ...

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• How To Find Us
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Stellarium 0.12.3 . ... Classes . ... ClassљList . ... Refraction Class Reference . ... virtual voidљ . forward ( Vec3d &altAzPos) const . ... backward ( Vec3d &altAzPos) const . Remove refraction from position ("reduce"). ... forward ( Vec3f &altAzPos) const . ... setupGLSLTransform ( StelGLSLShader *shader) . ... virtual void Refraction::backward . ... virtual void Refraction::disableGLSLTransform . ... virtual void Refraction::forward . ... virtual void Refraction::setGLSLUniforms . ...

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