... The exact directions of the offsets are parallel to the rows and columns of the CCD on which the aperture is specified. ... It is often useful to explicitly specify the desired rotation of the WFPC2 field-of-view on the sky. ... Figure 7.8 shows the CCD orientation and aperture locations relative to the U3 axis. ... Obtain the Position Angle (PA) of the source axis on the sky, measured in the standard way, North through East. ... desired source angle in field-of-view measured CW from +U3 axis) . ...

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• IRCAL Filters, Grisms, and Polarimeter
• Generic Targets List [Generic_Targets]
• Introduction

Astronomy Discussion Forums . Forums: . Atm ћ Astrophotography ћ Blackholes ћ Blackholes2 ћ CCD ћ Celestron ћ Domes ћ Education . ... Discussion Forums . ... Location,location,location! Forum List | ... Post Message | ... www.astronomy.net . ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . 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: Location Of Dome/Observatory - an Astronomy Net Domes Forum Message
• Need Help Locating Power Cord For Early 80's C8 - an Astronomy Net Celestron
• Reference Please - an Astronomy Net Blackholes2 Forum Message

... lcplot (lcplot-1.19.1) [xmmsas_20080701_1801-8.0.0] . ... We note that no RGS Source Time Series FITS file is specified in [ 1 ]. ... Time intervals all have the same length, the first one is TSTART , TSTART + Binsize*TIMEDEL where TIMEDEL is the bin width read from the file [ 1 ]. ... We have assumed it to be given in seconds. ... The mean, variance, Chi Square, etc are provided with six significant digits. ... The output devices are those of the PGPLOT library. ...

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This document explains how Apache uses the URL of a request to determine the filesystem location from which to serve a file. ... User Directories . URL Redirection . ... the URL http://www.example.com/docs/dir/file.html will be served from /var/web/dir/file.html . ... The module mod_userdir extends this idea to the web by allowing files under each user's home directory to be accessed using URLs such as the following. http://www.example.com/~user/file.html . ...

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• How Directory, Location and Files sections work
• Other Programs - Apache HTTP Server
• Apache module mod_auth_digest

... All the parameters provided in this database have been obtained using the the MIRIAD ( Sault et al. 1995 ) task MBSPECT . MBSPECT makes a spectrum of the velocity (or frequency) axis of a cube. The spectrum is beam-weighted, over the width specified, for the other image axes. ... Robust parameters are calculated by using an algorithm which minimises the mean absolute deviation of the flux-weighted velocities. mask= This specifies the x-axis ranges to be excluded from any continuum fit. ...

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• byu phased array feed.
• Your NED Search Results
• software_downloads

... CentralProcessor 0.11 documentation . Platform Documentation . The ASKAP Central Processor platform consists of a Cray XC30 supercomputer and a 1.4PB Cray Sonexion storage system mounted as a Lustre filesystem. 2 x Login Nodes: . ... To login to the ASKAP Central Processor: . ... usr/bin/env bash #SBATCH --time=01:00:00 #SBATCH --ntasks=80 #SBATCH --ntasks-per-node=20 #SBATCH --job-name=myjobname #SBATCH --no-requeue #SBATCH --export=NONE aprun -B ./myprogram . ... Central Processor Platform . ...

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• Set-related user input
• User Parameters - Data Location & Beam Selection CentralProcessor 0.11
• casacore: casa::MeasBase< Mv, Mr > Class Template Reference

TH setINDI 1 .SH NAME setINDI \- set one or more writable INDI property values .SH SYNOPSIS \fBsetINDI [options] device.property.e1[;e2...]=v1[;v2...] ... \fP .SH DESCRIPTION .na .nh .PP setINDI connects to an indiserver and sends commands to set new values for specified properties. ... TP -p <p> connect using alternate port p; the default is 7624. ... SH EXIT STATUS The setINDI program exits with a status of 0 if it suceeded in setting the new value for each specified property. ...

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• Interpreter (ImageJ API)
• ColorThresholder (ImageJ API)
• ImageStack (ImageJ API)

OptInt PmWiki : Pm Wiki / Page List Templates . ... template first:) . ... template last ...:) sections to specify output for the first or last page in the list or a group. ... template]] (:template defaults order=name:) (:template first:) Pages ordered by group (:template first {=$Group}:) Pages in group [[{=$Group}/]] (:template each:) * [[{=$FullName}]] (:template last {=$Group}:) {=$Group} contains {$$GroupPageCount} pages. (:template last:) {$$PageCount} pages total. [[#templateend]] . ...

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• Some notes on the GNU toolchain Bojan Nikolic web pages (r. 329)
• OptInt PmWiki : PmWiki / Links
• OptInt PmWiki : PmWiki / Wiki Style Examples

... Tonight's Sky . ... The Magazine . ... Observing . ... Astronomy for Kids . ... Observing springtime deep-sky objects with a large telescope . ... Follow an urban deep-sky catalog . ... Our т??Holmes Catalogт?? to date, although not definitive, shows how much deep-sky astronomy is possible from city centers. Get instant access to subscriber content on Astronomy.com! ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ... Astronomy Magazine . ...

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• Do the paths of totality during solar eclipses follow a pattern that repeats
• Astronomy Magazine - Interactive Star Charts, Planets, Meteors, Comets,
• Cassini Imaging Central Lab, Boulder, Colorado | Astronomy.com

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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• ELECTRICITY GENERATION

Next: Emission-line galaxies Up: The Hamburg/SAO Survey for Previous: Data reduction . In total 217 candidates were observed during the January - June, 1995, of which 34 objects were observed with the 6m telescope, 183 objects with the Calar Alto 2.2m telescope, and 4 with both instruments. ... For 11 of the known ELGs we measure emission line ratios and make quantitative classification. ... Emission-line galaxies . ... Objects without emission lines . Absorption-line galaxies . ...

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• HTML Tag Reference
• Mapping URLs to Filesystem Locations - Apache HTTP Server
• Properties

Next: A box, to include Up: To produce a region Previous: To produce a region . select cursor and circle . When in the image window, the mouse now has a box shape with an arrow at the upper left corner. The mouse buttons act as follows: . LEFT - to move the center of the circle at the position of the arrow point. ... RIGHT - idle. center the circle at the point source by positioning the arrow point and clicking on the LEFT mouse button. A circle will appear at the arrow position. ...

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• Fixing and Freeing Region Markers
• Array File Specifications
• Getting Common Information About Access Points

Pulkovo NEO Page . ... EPOS Software Package . ... EPOS ( E phemeris P rogram for O bjects of the S olar system) is the Windows PC application for study and ephemeris support of observations of the Solar system objects. ... It controls the part of common data and transfers the control to one of the programs that solve the restricted set of tasks. ... So with the EPOS software package one can calculate the accurate ephemerides for many objects and get the quick illustration of their motion as well. ...

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• Pulkovo Observatory

... FiberGuide Ferrules . V-groove Blocks . ... Ferrule Diameters (+/- .00127 mm) fiber # location 1 location 2 location 3 Average 1 2.14884 2.14884 2.14884 2.14884 2 2.15138 2.15138 2.15138 2.15138 3 2.15138 2.15138 2.15138 2.15138 4 2.15265 2.15265 2.15265 2.15265 5 2.15138 2.15138 2.15138 2.15138 6 2.15138 2.15138 2.15138 2.15138 7 2.14884 2.14884 2.14884 2.14884 8 2.15138 2.15138 ... The angular alignment of the fibers on the V-groove blocks. ...

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• Plug-plate hole tilt
• Mirror baffle measurements
• MCP Menu documentation

... JavaScript 1.1: added current, next, and previous properties. ... To change a window's current URL without generating a history entry, you can use the Location.replace method. ... For example, if the history list contains three named entries, these entries are reflected as history[0] , history[1] , and history[2] . ... back . ... onClick="history.go('home.netscape.com')"> The following button navigates to the URL that is three entries backward in the history list: <P><INPUT TYPE="button" VALUE="Go" ...

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• Mapping URLs to Filesystem Locations - Apache HTTP Server
• mod_auth_digest - Apache HTTP Server
• Embedding JavaScript in HTML

... This function can also be used for particular types of subtypes or kinds: KIND (0) integer KIND (0.0) floating point number KIND (.FALSE.) logical variable KIND ("A") string of characters There is an intrinsic function SELECTED_REAL_KIND , which returns the kind of the type REAL that has a representation with (at least) the precision and the exponential range requested. ... With the choice SELECTED_INT_KIND (5) all integers between (but not including the limits) -100 000 and +100 000 are permitted. ...

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• Announcements of new WWW servers
• About the HTML 4.0 Specification
• Argument association

... Therefore, the menu location # "Blur/Blur" specifies an item name of "Blur" in a submenu entitled # "Blur". ... It is convention to only use the `alt' and `shift' key modifiers for # plug-ins. ... The main application will not use the ` alt ' # or ` shift ' key modifiers. plug-in blur Blur / Blur Alt Key B Alt +B plug-in gauss Blur /Gaussian Blur Shift Alt Key B Shft+ Alt +B plug-in gauss_rle Blur /Gaussian Blur RLE plug-in gauss_recurse Blur /Gaussian ...

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• Configuration Options
• Miscellaneous Options
• Bright Sn in NGC 3877

... The following procedures are specific to the reduction of point astrometry data. dispinit ,[ stars _char ],[ class=class ] Initialize the dispersion corrections. ... Initialize (zero) the dispersion corrections for the specified stars. ... For scan data, initialization means setting the dispersion corrected delays equal to the averaged FDL data. dispflag , channels ,[ beams ] Flag the visibility phase for the specified channels and beams. ... Interpolate to the epochs of the point data. ...

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• Los Cielos de Am , The darkest sky and the two galactic hemispheres
• Command line procedures
• Introduction and command syntax

... At 22:42:27 UT 26/07/09, the Burst Alert Telescope (BAT) on board of the SWIFT multi-wavelength space observatory triggered and located GRB 090726 gamma-ray burst event. ... About half an hour after the BAT trigger, the first images were obtained with the SAO RAS Zeiss-1000 telescope in four BVRI filters (see Fig.1). ... The spectrum of the optical transient was obtained with the SAO RAS 6-m BTA telescope 1.54 hours after the burst, using the SCORPIO instrument in the spectroscopic mode (Fig.2). ...

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• Why Use CEILIDH ?
• Optimization of spectroscopic observations
• String Handling: <string.h>

... Content Model: Optional list header (LH), followed by one or more list items (LI) . An unordered list typically is a bulleted list of items. ... Note: Some legacy documents may include headers or plain text before the first LI element. ... DIR lists are used to present lists of items containing up to 20 characters each. ... CLASS . ... The WRAP attribute is used for multicolumn lists. Use wrap=vert if you want to arrange the list items down the page before wrapping to the next column. ...

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• Character Entity Set(s)
• Figures
• Sorting the content of a file