... Chapter 2: The Basics of Phase II Proposals > 2.4 Examples and General Advice . ... First, you have to acquire an object successfully that is at or near the position at which the science observation will be made. ... The object?s coordinates must be both precise and accurate and any proper motion must be known. ... An offset is explicit when you use a Special Requirement such as POS TARG (see POSition TARGet <X-value>,<Y-value> ) to move the telescope away from the position acquired. ...

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• Fine Guidance Sensor Instrument Handbook
• CCD Position and Orientation on Sky
• WFC3 Instrument Handbook

A typical radio dataset might be a 3-dimensional "cube" named AURORA, with axes RA, DEC and FREQ. ... These can be specified by giving the axis name(s) and grids for each subset. For instance, AURORA specifies the whole 3-dimensional ``cube''; AURORA FREQ 3 specifies the subset FREQ=3 (i.e. the RA-DEC plane at FREQ grid 3) of the set AURORA. ... Specifying only the axis name, and no grids, selects all subsets along that axis: AURORA FREQ selects all RA-DEC planes in AURORA. ... axis centre. ...

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• Number input
• Source Fitting and Positions
• Tape Initialization File

Next: *.imh and *.qp Extensions Up: IRAF/PROS Files Previous: IRAF Image Arrays . The x-ray data are stored in QPOE files (Quick Position-Ordered Events, *.qp ) rather than image arrays. ... Note that, unlike IRAF images, QPOE files have no associated header file, and are always stored in the current directory, unless explicitly specified otherwise. Non-PROS IRAF tasks can also access QPOE data files in place of image arrays. ... rp110590.qp[pi=2:30] . ... The ROSAT PSPC qp file images are . ...

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• Spatial Region Coordinates
• Fixing and Freeing Region Markers
• Doug Burke's Perl/S-Lang pages: Datatype examples

... section 7.4 ) . If the detector map (a grid of positions used to calculate and flux weight the ARF: section 7.3 ) is either psf or flat , the map bounds and pixel size may be specified. ... The user can supply an external detector map instead (section 7.3.2 ), but the bounds must cover the regions. ... The following sub-sections show examples of usage. ... Example 4: Specifying an external detector map for an extended source . Example 5: Using an RMF dataset to specify the energy grid . ...

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• Description
• Example 3: Point source with explicit position

... 295, 2003 H. E. Payne, R. I. Jedrzejewski, and R. N. Hook, eds. The MAST Pointings Tables Pro ject Karen Levay, Paolo Padovani1 , Randall Thompson, Megan Donahue, Michael Corbin Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 Abstract. We have undertaken a pro ject to create a database of all HST imaging observations organized by position on the sky. ... Each sky region was called a "pointing." ... Users select the instrument pointings table they wish to search. ...

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• ADASS 2002 Conference Proceedings
• TransVERSE: An Architecture for Configuring Astronomical Observations
• The SuperCOSMOS Sky Surveys

TUI supports the following offsets: . Object Arc offset by a given amount on the sky (i.e. along the arc of a great circle). ... Arc offsets are useful for moving a different portion of your object or a different nearby object onto the boresight . ... Object Arc XY this is identical to an Object offset except that it has been rotated to align along the instrument x-y axes. ... This is just like the Calibration XY offset, except that it is typically cleared when you slew to a new object. ...

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• TUI:Scripts:Scripting Tutorial:Get Info
• MCP Menu documentation
• TUI:Introduction

NAME ABbuilder - DFO data organization tool SYNOPSIS ABbuilder <options> where <options> are: --raw-dir directory containing raw data --cal-dir directory containing calib data --cal-ldir directory containing symbolic links to calib files --cal-list mcalib list --vcal-dir directory containing virtual products --pro-dir where pipeline products are created --ab-dir where association blocks are created --oca-rul file containing OCA rules --instrume instrument --date YYYY-MM-DD --mode { CALIB | ...

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• http://www.eso.org/paranal/instruments/vlti-visitor/applications.html
• VLTI Calibrator Selection Help Page
• IRAF/STECF imaging linear polarimetry simulation and reduction package

The Spectral Line Handbook (March 2002; includes single pixel and Interim Correlator related aspects). Available Backends for Spectral Line Observations at AO. ... Examples of spectral line projects at Arecibo (From the NAIC/NRAO Single Dish Summer School 06/01). ... For general information on proposing for observing time, telescope schedule, observing software, etc., click on the Observing (general) link on the side menu, or on Observing in the bottom link bar. ...

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• CIMA Auto-Observing
• Chapter 11. Specifying OpenGL Environment Variable Settings
• CIMA Source Catalogs

... 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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• Dynamic HTML in Communicator
• Long description for example illustrating positioning with respect to a
• Long description for example illustrating absolute positioning

... The J, H and K bands are characterized by a bright background, such a background is mainly due to the emission of atmospheric lines and of thermal radiation. ... If the source cover a large fraction of the slit, spectra off-source must be observed to adequately sample the sky background. ... The on chip integration time (time spent in each position of the slit) must not exceed 40 seconds in J and H bands and 60 seconds in K band. ... We suggest a sequence of 10 for each elementary integration time. ...

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• Algorithm
• mod_charset_lite - Apache HTTP Server
• mod_expires - Apache HTTP Server

OptInt PmWiki : Pm Wiki / Wiki Style Examples . Wiki styles | ... PmWiki uses WikiStyles for styling text with color and other attributes. PmWiki 2.0 introduced the ability to control the styling further and to even place styles on blocks. ... In addition, an author can define a style "shortcut" by using the define= property. For example, to define a style of %red% , one can use: . define=mystyle color=red% Here is some %mystyle% red text created using a style shortcut. ...

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

... 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

Contents] [Previous] [Next] [Alphabetical Tag List] [Index] . This section discusses the tags that let you specify positions for HTML content. LAYER . ILAYER . ... Use the LAYER tag to specify an absolute position for a block of content, and use the ILAYER tag to specify a relative position. ... HEIGHT=" height " . ... OnFocus=" JScode " . ... HEIGHT="height" specifies the height of the layer's clipping region and serves as the reference for setting the relative height of children layers. ...

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• HyperLeda: example of online pipeline processing
• What was measured?
• Loading the Telescope and Instrument Specifications

... Several HST instruments both current and decommisioned have provided imaging linear polarimetry capabilities. ... The STECF IRAF layered package impol provides five tasks specifically aimed at reduction of HST imaging polarimetry data. ... Reduction of HST polarimetry data and simulation of raw polarimetry images, together with polarization vector plotting, are covered. ... For reduction of data from imaging linear polarization instruments other than from HST, the instrument name is `SPECIAL'. ...

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• HSTPOLSIM (V1.00) --- April99 --- HSTPOLSIM (V1.00)
• Space Telescope-European Coordinating Facility
• HSTPOLPOINTS (V1.00) --- May99 --- HSTPOLPOINTS (V1.00)

RTT150 . ... This search system is designed for generating the necessary information on series of pointings (observations of each source consist of sets of exposures with different filters and sometimes with different exposure times) for observed sources. Search results appear at the separate page as a table with the following data: . DATE - real (not evening!) observations date (in YYYY-MM-DD format); . ... Bin - minimal CCD binning mode (may vary during the observations); . ...

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• Russian Turkish 1.5-m telescope

The Network Time Protocol (NTP) is used to synchronize the time of a computer client or server to another server or reference time source, such as a radio or satellite receiver or modem. ... Information on the NTP architecture, protocol and algorithms can be found in the following articles and reports, which are available online . Mills, D.L. Internet time synchronization: the Network Time Protocol. ... Mills, D.L. Network Time Protocol (Version 3) specification, implementation and analysis. ...

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• Lighting plug-in
• GIMP Plug-In Examples
• Sternberg Astronomical Institute

Research Technician Radio Meteor Detection A fixed-term Research Technician position is available at the Armagh Observatory funded by the Europlanet Research Infrastructure (RI) under the Seventh Framework Programme of the European Union (EU). ... In addition, the equipment should be capable of operating in the field and at remote sites with a high degree of autonomy. ... For more information about the pro ject, please contact the PI, Dr Apostolos Christou, by email at aac@arm.ac.uk. ...

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• http://star.arm.ac.uk/jobs/2010/aac_research_technician_2010sep14_A4_advert.pdf
• Research Technician Post
• Spectrum v1 - Examples

. To change your login shell to the Korn shell (ksh): chsh Changing login shell for sarah. Old shell name: /bin/csh New shell: ksh . This changes the user's login shell from the C shell (csh) to the Korn shell (ksh). If you mistype the name of the shell or specify a shell that is not available on your system: . you will be given a list of all the shells that are available on your system. or . a message similar to the following will be displayed. name is unacceptable as a new shell .

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• Figures
• Unordered Lists
• Horizontal Tabs

... Meade Instruments Corporation . ... Meade Pictor 616A Color Filter System Instruction Manual . ... Remove the Meade Pictor 616A Color Filter System from the telescope or camera. Use the supplied hex wrench to remove the three screws from the telescope side of the Meade Pictor 616A Color Filter System. Position your Meade Pictor 616A Color Filter System to align with the diagram below. ... Carefully screw each filter into the wheel, and re-assemble the Meade Pictor 616A Color Filter System. ...

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• Meade Instruments - Telescopes, Solar Telescopes, Binoculars, Spotting Scopes
• Meade Instruments Corp. - Meade Customer Support
• Meade Instruments Corporation - Autostar Computer Controller Instruction Manual

... To mark coordinate net in plot, first select Plate in menu bar and then Coordinate net in drop-down menu. ... User has possibility to save plot of sky or to print it using standard means. To save the file select File item in menu bar and then Save As... in drop-down menu. ... To print plot of plate select File item in menu bar and then take advantage of options Print Preview , Print Setup , Print. ... To return to the list of centers click on x button in title bar. ...

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• ENGAMPLE
• NAA 2015-2016 (preface)
• NAA 2013-2014 (preface)