... The current cable tray route specified in the UTE-FTT interface document MRO-ICD-EIE-0032d gives a length of 5.5m from the edge of the optical table to the bottom of Q5, the rack containing the FTT electronics. ... ACTION: - MRO will examine the cable route in detail and estimate the length of cable between the worst case camera position on the optical table and the position of the FTT space in Q5. ... Heat must be extracted from the camera's peltier cooler and also from the camera enclosure. ...

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• http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIFastTipTilt.InterfaceControl/MRO-ICD-CAM-1100-0108%20FTTNAS-FTTA.pdf

Astrophotography Forum Message . Forums: . ... Post . ... What Camera And Adapter? ... Post Message | ... Posted by Chris on January 14, 2007 19:27:11 UTC . ... I need to buy a camera aswell. What adapter will I need and what do I need to ask for in the camera? ... www.astronomy.net . About Astronomy Net | Advertise on 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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• Digital Camera Adapters! - an Astronomy Net CCD Equipment and Techniques Forum
• LXD55 - Through The Lens Camera Adapter - an Astronomy Net Meade Equipment
• Astronomy Image Gallery

... Telescopes . LX850 Series . ... Superb optical performance coupled with time proven computerized pointing and tracking has made the LX200 ACF series a best-seller in the high-performance telescope class. ... Meade's revolutionary LS LightSwitchтДв series of telescopes use advanced technologies to do what no other consumer telescopes have done before: take all the hassle out of using a telescope. ... Meade Variable Projection Camera Adapter (1.25") . ... The Variable Projection Camera Adapter. ...

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• Meade Basic Camera Adapter (1.25")
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• Meade Basic Camera Adapter (1.25") - Photography Accessories - Accessories -

Main Sections LabIR main page . Instrument page . ... Special Sections Software Page . ... LabIR staff . Companion Pages Skysoft Home . Tirgo Page . ... LabIR Hotlist . ... Arcetri Infrared Instrumentation Group . Largo E.Fermi 5 I-50125 Firenze . Phone (Italy) 055 2752 289 . Fax (Italy) 055 2752 292 . ... Firenze, August 1997 ...

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• Per-user web directories - Apache HTTP Server
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• Chapter 11. Specifying OpenGL Environment Variable Settings
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... Near Infrared Camera and Multi-Object Spectrometer Instrument Handbook for Cycle 17 > Chapter 6: NICMOS Apertures and Orientation > 6.3 Orients . ... NICMOS orientations are specified relative to the +y axis shown in Figure 6.1 . ... The NICMOS coordinate system is rotated by approximately 225 degrees from U3 axis. ... Due to the linear arrangement of the three NICMOS cameras on the sky, it may be advantageous to consider the specification of a unique telescope orientation. ...

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• IRCAL: an IR Camera for Adaptive optics at Lick
• WFC3 Instrument Handbook
• Mode = ACCUMConfig = NIC1 or NIC2 or NIC3

... Drag data has the following properties: . Drag action type (ie GDK_ACTION_COPY, GDK_ACTION_MOVE). ... A GDK_ACTION_COPY would be a typical drag-and-drop without the source data being deleted while GDK_ACTION_MOVE would be just like GDK_ACTION_COPY but the source data will be 'suggested' to be deleted after the received signal handler is called. ... Sent and received data format types ( selection target ) come into play only in your request and received data handler functions. ...

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Next: Power Law fit to Up: Spectral Analysis Previous: Error Determination . With PROS2.3 all fitting is performed using Poisson statistics , rather than Gaussian, so that results will be correct even for small counts ( ) in some channels. Power Law fit to a Point Source . Raymond Model . Two-Temperature Raymond Model . Limiting Energy Channels Input to the Fit . Multiple Data Sets . ... Fit a source with a small number of net counts . Inspection of results . ...

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• Autoconfigure of Frame #1
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... The initial descriptions of the FITS format provided a simplified method for describing the physical coordinate values of the image pixels, but deliberately did not specify any of the detailed conventions required to convey the complexities of actual image projections. ... They were CRPIX n for the reference pixel location on pixel axis n , CRVAL n for the coordinate value at that pixel, CDELT n for the increment at that pixel in the coordinate value, and CTYPE n for the type of coordinate. ...

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• Restoration of HST WFPC2 Images in Gyro-Hold Mode
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. Go Here for Hubble Ultra Deep Field . ___________________________________________________________________ The Electronic Universe Project e-mail: nuts@moo.uoregon.edu

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... This is done by taking in all input files the extension whose name is specified by the maintable parameter (called 'merged extension' in what follows) and merging the columns into a single output extension of the same name. ... Its contents is taken from the CCDID keyword (and QUADRANT for EPIC PN). ... To propagate other column specific keywords, they must be specified manually via the extensionchecks , mainattributes , maxattributes and minattributes parameters (see above). ...

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• Data-set
• dataset

adjustable array . The array in a subprogram has a variable dimension just as in Fortran 77 through that both the array name and the dimension (all dimensions) are dummy arguments. ... Array sections can be used here instead of arrays. array function . ... An array in a subprogram which is not local and has a certain data type and a certain rank. ... Each Fortran program has to consist of exactly one main program and and any number of subroutines, functions, modules and BLOCK DATA program units. ...

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Stellarium 0.12.3 . ... Classes . ... ClassљList . ... TuiNodeActivate Class Reference . ... voidљ . ... TuiNodeActivate (const QString &text, QObject *receiver, const char *method, TuiNode *parent=NULL, TuiNode *prev=NULL) . Create a TuiNodeActivate node. ... virtual TuiNodeResponse љ . handleKey (int key) . ... TuiNode (const QString &text, TuiNode *parent=NULL, TuiNode *prev=NULL) . ... virtual TuiNode *љ . ... virtual voidљ . ... Contains the numbers of the parent nodes in the hierarchy. ...

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Symbolic circuit-matrix processor and evaluator . ... This software is reliable over the range of benchmark circuit complexity (both *.CIR and *.MAT file). ... SYMBOL is a symbolic-algebra package which in contrast to REDUCE, MACSYMA, MAPLE, MATHEMATICA, MathLAB, MathCAD and other known multi-purpose systems is especially intended for analysis of any lumped, linear, time-invariant circuit. ... pure ASCII text . ... CIRSYM - SYMbolic CIRcuit processor used to format ASCII text file *.out for CALCSYM. ...

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... public class WindowManager . ... This class consists of static methods used to manage ImageJ's windows. ... static void . ... Adds the specified window to the Window menu. static boolean . ... Returns a reference to the active image or null if there isn't one. static ImageWindow . ... Makes the image contained in the specified window the active image. static void . ... Returns the first image that has the specified title or null if it is not found. public static void addWindow (java.awt.Frame win) ....

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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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• impos
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The Status window shows the status of the telescope and (on unix and Windows) contains TUI's menus. ... The top panel shows user-specified information about the current target and also the progress of slews: . Name : object name . Obj Pos1/2 (e.g. RA/Dec): net object position. including object and arc offsets. ... Object Arc Off: the current object arc offset . Object Arc Off X,Y: the current object arc offset rotated to instrument xy coordinates (this may vary if the field rotates). ...

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• DIS Commands
• TUI:Telescope:Slew Window:Options:Drift Scan
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... Imaging spectrometer for atmosphere and ionosphere spectral investigation consist the static Michelson interferometer and CCD camera. The prototype of the onboard CCD camera for the spectrometer used the Toshiba 2048 pixels CCD linear array (TCD 1201D) with FPGA-based controller. The controller is building on ACTEL A1020A field programmable gates array with maximum data rate 40 MHz and can be used with linear and area array CCD. ... Toshiba CCD Linear Image Sensor Data Book, 1997. ...

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• Optical static Fourier spectrometer

... Site Map . ... Science Users Information > Science Publications > Science Announcements > Data Format Specification for APEX Sub-millimetre Sky Maps and LESS Phase 3 Data Release . ... Observing with ESO Telescopes . ... The Phase 3 data format specifications and Phase 3 validator have now been extended to astrometrically registered and flux calibrated sky maps in the submillimetre domain. This format is relevant to the Phase 3 data release for the LESS extra-galactic submillimetre survey. ...

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• OmegaCAM, the monster camera of the VLT Survey Telescope | ESO
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... The predictive power of current models (the so-called meteor forecasting) has given us the exact timing of the Leonid storms of 2001 and 2002 to the nearest hour and are now used to predict the arrival times of major annual showers such as the Perseids . ... Towards this goal, the Observatory has installed a sky-monitoring system, consisting of one medium angle (MA) and two wide-angle (WA) video cameras linked to software designed to detect motion. ... Bright Taurid Meteor . ... Meteors on Mars . ...

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