... HST . ... Data . ... HST Overview . ... The exposure logsheets and RPS2 input files for post-COSTAR programs are available from the PRESTO web page: http://www.stsci.edu/hst/scheduling/program_information . FOS program logsheets and RPS2 (RPSS) input files are available via the FOS WWW page propfind query. ... In summary, since FOS exposures are not interruptible, a single exposure logsheet line or RPS2 exposure line may produce several distinct FOS exposures and hence several sets of data files. ...

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• HST Primer for Cycle 22
• Observation Logs
• ACS Instrument Handbook

Next: Observing the Old-Fashioned Way (Gui-Free Observations) Up: Spectral Line Appendices Previous: OLD Basic Analyz Routines For use with data taken BEFORE March 6, 2000 . This appendix contains example analyz sequences used to look at HI spectra. ... Additionally, if you have not run analyz before, instruction (2) should read: If you have not, instruction (3) should read: . ... 7) redln < rec < n : This first stores the individual ON/OFF - 1 data dumps into registers 100 - 100+ - 1. ...

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• Example Observing Projects
• GOLDMiNe: Virgo cluster optical and HI databases
• The Search for HVCs in Other Galaxies

... Typically, an observation specified by an observer cannot be directly executed by an observatory. Observation specifications need to be configured so that they can be used by other components of the observatory. This paper motivates the need for configuration tools and describes a software architecture which supports configuring astronomical observations. ... This paper describes a system for preparing and configuring individual astronomical observations. ...

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• What Happened to the Results?
• ADASS 2002 Conference Proceedings
• Some Astrophysical and Instrumental Applications of AIPS++

... Here follow some typical calls to epchain : epchain This processes the first IMAGING mode exposure (i.e. PNS010) and is equivalent to one of the calls epchain datamode = IMAGING odfaccess = odf exposure =010 schedule=S epchain datamode = IMAGING odfaccess =oal exposure =1 epchain datamode = IMAGING exposure =1 epchain odfaccess =name ... The call epchain datamode=ALL odfaccess=all will process all exposures of an ODF, independent of observing mode. ...

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... Doug's Home Page . ... In the examples below we show a number of ways that data can be moved back and forth between S-Lang and Perl . ... Source code typeof : "undef"; __END__ __SLang__ variable foo = Any_Type [3]; foo[0] = "a string"; foo[1] = 23; define getfoo(x) { return foo[x]; } message( "In S-Lang:" ); vmessage( "typeof(foo[0]) = %s", string(typeof(foo[0])) ); vmessage( "typeof(foo[1]) = %s", string(typeof(foo[1])) ); vmessage( "typeof(foo[2]) = %s", string(typeof(foo[2])) ); . ...

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• Doug Burke's Perl/S-Lang pages: General examples
• Chandra Images for G054.1+0.3
• Chandra Images for G012.8-00.0

Next: Examples of Setup Files Up: Setup Files Previous: Setup Files Contents . Over 200 standard setup files have been created, covering many of the normal modes of observing. ... These especially include precisely defined, and somewhat complex cases like the Mark III standard modes (although MarkIII went the way of the dinosaur long ago. ... v '' files: . These are setup files for VLBI observations using VLBA recording formats. ... These are setup files for Mark III observations. ...

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• The Schedule File
• Scheduling Mark II Observations
• Using SPC

... Bojan Nikolic web pages (r. 329) . Modelling absorption and emission of radiation by interstellar dust . ... The search results are restrict to these pages only . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

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• Anthony Lasenby: Hompage
• PPEUC Programme - Cosmic Microwave Background Workshop
• OptInt PmWiki : PmWiki / Wiki Trails

Next: NICMOS/HST H-band (F160W) Images Up: NICMOS Science Previous: HST NICMOS Observations of . ... Observations of P . ... The NICMOS team has devised a comprehensive program of observations of the Galactic Center. ... Data in hand give a first look at variability and a detailed look at the search for the tip of the main sequence will be discussed where NICMOS has demonstrated adequate sensitivity and photometric precision to identify likely O8-B1 stars at the Galactic Center. ...

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Peremennye Zvezdy", . ... Star Name: . GSC 3710-00312, USNO-A2.0 1425-04252279 . ... Variability type: . ... USNO-A2.0 1425-04252279 is located at the distance of 15?.7 from the X-ray source 1RXS J031707.9+572942, which is larger than the position error of the source (12?), but its hardness ratio HR1 = 0.03 0.29, typical of chromospherically active stars, and its character of variability allow us to assume that the star is related to the X-ray source. ... Eclipsing variability . Sine wave 1 . ...

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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. ...

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• Examples
• mod_example - Apache HTTP Server
• Echelle Spectra

... Apache HTTP Server Version 2.4 . Apache > HTTP Server > Documentation > Version 2.4 > SSL/TLS . ... Client Authentication and Access Control . ... How can I create an SSL server which accepts strong encryption only? How can I create an SSL server which accepts all types of ciphers in general, but requires a strong cipher for access to a particular URL? ... How can I allow only clients who have certificates to access a particular URL, but allow all clients to access the rest of the server? ...

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• mod_example - Apache HTTP Server
• rotatelogs - Piped logging program to rotate Apache logs - Apache HTTP Server
• mod_proxy_scgi - Apache HTTP Server

Next: Measuring Internet Access Up: Widening Access Previous: First Observation of a Contents . ... The Observatory web-site also increasingly makes available the results of astronomical observations carried out at Armagh, for example images of meteorological or space-weather events such as aurorae (see http://star.arm.ac.uk/images/aurora-2003-Oct/), and transient astronomical events such as occultations, eclipses and transits. ...

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• Armagh Observatory
• Spectrum v1 - Examples
• Asteroid Impact

This module illustrates many of the aspects of the Apache 1.2 API and, when used, demonstrates the manner in which module callbacks are triggered by the server. ... Source File: mod_example.c . ... The files in the src/modules/example directory under the Apache distribution directory tree are provided as an example to those that wish to write modules that use the Apache API. ... Example . ... Uncomment the "AddModule modules/example/mod_example" line near the bottom of the src/Configuration file. ...

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• Apache module mod_vhost_alias
• Apache module mod_setenvif
• Apache module mod_auth_anon.c

Next: Examples of data contained Up: Electronic database Previous: Future plans . In astrophysics, the optical constants mainly are used to calculate the optical properties of scatterers, i.e. cross-sections, scattering matrix, etc. ... Optical properties derived from such models have been discussed in some books (see, e.g., [ 2 , 3 ]) and in principle can be calculated by using various light-scattering tools which are freely available via the internet [ 4 ]. ...

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• Examples of data contained in the JPDOC
• Course of Non-numerical Programming

... 2.3 Establishing the Extragalactic Distance Scale . ... 2.3.2 The Second Rung: Distances to stellar clusters . ... 2.3.4 Distances to Local Group Galaxies . ... The Luminosity Function of Planetary Nebulae . ... 3.2.2 Clusters of Galaxies . ... 4.2 Evidence for Dark Matter as a Function of Scale Size . ... 4.3 Other Dark Matter Indicators for Galaxies . ... What is the nature of the large-scale distribution of matter in the universe as traced by the three-dimensional galaxy distribution? ...

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• Astronomy HyperText Book: Fusion Sequences in Stars
• Digital Stellar Spectra
• Physics 410/510 Observational Cosmology

Magnification (Power) And Using Eyepieces . ... To determine power in a telescope, divide the focal length of the telescope by the focal length of the eyepiece. By exchanging an eyepiece of one focal length for another, you can increase or decrease the power of the telescope. For example, a 25mm eyepiece used on a telescope with a 1000mm focal length would yield a power of 40x (1000 / 25 = 40) and a 10mm eyepiece used on the same telescope would yield a power of 100x (1000 / 10 = 100). ...

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• Astronomy articles, forums, listings, and other resources about Astronomy.
• Human Powered Clock Drive - an Astronomy Net Article
• I Hate To Have You Think I Ignore You. - an Astronomy Net Exploration Forum

To find out if a command name is located in your command path: which ue /usr/local/bin/ue . This returns the information that the MicroEMACS editor (ue) is available on this system as the file /usr/local/bin/ue . ... To find out which (if any) of several commands are available: which delete talk ps No delete in /usr/local/utils/bin:/bin:/usr/bin: /usr/local/ucb/bin:/usr/local/gnu/bin: /usr/local/public/bin:/usr/bin/X11:. /usr/bin/talk /bin/ps . ...

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• Example of changing the login shell with the chsh command
• Understanding host names
• Example of using an if construct

SAI 175 anniversary . ... Moscow University . Search for in SAI Moscow University Search for in Russian astronomical resources . ... SAI Astronomical Databases . ... Browse SAI Software archive(ftp.sai.msu.su) . ASTRONET.RU - Russian Astronomical Network (available in translit also) . ... SAI Supernovae Research Group . ... Department of the Galaxy and Variable Stars (in Russian) . Sternberg Astronomical Institute Seminars . ... All-Russian Astronomical Olympiad (in Russian) . ...

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• GIMP Plug-In Examples
• Lighting plug-in
• Zen: NewExtentsBasedRanking

... Exposure Time Calculator (ETC) . Survey processing . ... VISTA is a 4-m class wide field survey telescope for the southern hemisphere, equipped with a near infrared camera (1.65 degree diameter field of view at VISTA's nominal pixel size) containing 67 million pixels of mean size 0.34 arcsec and available broad band filters at Z,Y,J,H,K s and a narrow band filter at 1.18 micron. A wide field visible camera, if constructed, could also be used on VISTA. ... Tile . ... ESO VISTA Public Surveys . ...

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• VISTA ETC - Exposure Time Calculator

... According to the most popular cosmological paradigm, the greater part of the galaxy mass is accumulated in the dark matter halo. ... The polar ring galaxies (PRGs) reveal external rings or disks of gas, dust and stars rotating in a plane roughly perpendicular to the disk of the central galaxy. ... The shape of the dark halo in the model was chosen so as to achieve the best fit to the observed rotation of both galaxies themselves and their polar rings. ... The SPRC-7 galaxy. ...

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• The GLORIA Project makes available to internet users 13 robotic telescopes in