Next: Pulsar bin-mode observations Up: ATCA Bin Mode Observations Previous: ATCA Correlator Bin Modes . Miriad 's atlod task has an option, options=hires which converts a RPFITS file observed in high time resolution bin-mode into an apparently normal dataset with fine time resolution. ... In high resolution time mode, the time difference between consecutive integrations might be smaller than this tolerance. ... Miriad manager . ...

... There are number of features that can be set by the user in the Sparkle Dialog box. ... The Sparkle plug-in computes the luminosity (level of whiteness) of each pixel in the image (the user can see this when the progress window labeled Generating luminosity array... is displayed). ... The threshold value is currently a slider/text field pair which have a precision of .0001. ... Like the Threshold value, the Flare Intensity has both a slider and a text input field for specifying its value. ...

Allows you to specify a desired wrap for the azimuth axis and the instrument rotator. ... If the axis is being driven in mount coordinates then your wrap preference will be recorded, but ignored (for mount coordinates you specify exactly the position you want; a different wrap is never chosen). The wrap preferences are: . Nearest pick the position nearest the current position . ... Positive pick the larger angle . Middle pick the position nearest the center of the allowed range of motion . ...

... CYLINDRICAL PROJECTIONS: -Jc lon0 / lat0 / scale (Cassini) -Jj lon0 / scale (Miller) -Jm scale ( Mercator - Greenwich and Equator as origin) -Jm lon0 / lat0 / scale ( Mercator - Give meridian and standard parallel) -Joa lon0 / lat0 / azimuth / scale (Oblique Mercator - point and azimuth) -Job lon0 / lat0 / lon1 / lat1 / scale (Oblique Mercator - two points) -Joc lon0 / Je lon0 / lat0 / scale (Equidistant). Jf lon0 / lat0 / horizon / scale (Gnomonic). ...

Next: Quadrant DC Offset Removal in NICMOS Images Using an Eye-pleasing Criterion . ... This paper describes a simple imaging model which allows the limits of dithered imaging to be readily appreciated and briefly reviews available software. ... Dithered imaging can improve this sampling. ... ACOADD was originally developed for combining images with different PSFs but can also be used, with shifted PSFs and sub-sampled output images, for combining dithered under-sampled images. ...

... Meta Index / Home Page / Description By default, an ARF will be created which has been corrected for the area lost by the gaps between CCDs and by bad pixels. ... The extendedsource option tells arfgen to produce the ARF relevant for an extended source. ... In practice, for an extended source the ARF has no correction for encircled energy, the mirror vignetting is averaged over the whole source area and area lost due to bad pixels and chip gaps is not convolved with the Point Spread Function (PSF). ...

. To make a lasting change, create a file named .exrc , containing the set commands, in your home directory. The next time you use vi these options will take effect and will remain in force until you edit the .exrc file to change them. You can, of course, temporarily change the value of any option. List of options . Examples . Did You Know? .

... HST . ... Data . ... News and . ... HST Peer Review Process . ... HST Overview . Overview . ... DD Time . ... Retrieving HST Data . ... Data Analysis . ... Target Acquisition . ... COS Data Handbook . ... The new algorithm works with all of the COS FUV gratings, and observers are invited to use them all in Cycle 19 Phase II proposals. The new algorithm considers only data from segment A of the FUV detector and requires a signal-to-noise ratio of 25 to compute an accurate centroid. ...

The XImtool control panel is the main interface for the XImtool display program, on which SAOtng is based. The SAOtng GUI duplicates the most of the functionality of the control panel in its menu and accel buttons, but the control panel is offered as a window-based alternative to run-of-the-mill menus. ... Tile Frames . ... The text display window gives the field X,Y center, X,Y scale factors, and the X,Y zoom factors. ... Fit Frame makes the display window the same size as the frame buffer. ...

Appendix E. Dots Per Inch . ... DPI (Dots Per Inch), also known as PPI (Pixels Per Inch), is a property of an X screen that describes the physical size of pixels. Some X applications, such as xterm, can use the DPI of an X screen to determine how large (in pixels) to draw an object in order for that object to be displayed at the desired physical size on the display device. ... The NVIDIA X driver reports the size of the X screen in pixels and in millimeters. ... grep -B1 dot . ...

... Дни открытых дверей к юбилею САО РАН (12-14 апреля 2016 г.) . Международная конференция "Dark Ages and White Nights (Spectroscopy of the CMB)" (20-24 июня 2016 г.) . ... Международная конференция MULTI-SPIN GALAXIES - 2016 (26-30 сентября 2016 г.) . Международная астрономическая конференция "Физика звезд: от коллапса до коллапса" (3-7 октября 2016 г.) Архив . ... Подробнее.. ... 10.02.16 . ... БТА в реальном времени . ... Цейсс-1000 в реальном времени . ... Последнее обновление: 22/03/2016 ...

The form on this Web page allows specifying a celestial position for which the full 4x4 degree NVSS FITS image is desired. ... Other services of the NVSS survey include: . ... NVSS Postage stamp (small FITS or jpeg file) server . direct ftp to NVSS 4x4 deg. FITS image and documentation server . NVSS source catalog and software ftp server - but please note that you will need to schedule an overnight job for a quiet time slot to download the 150Mb CATALOG.FIT file to avoid timeouts etc. ...

... Class . ... FRAMES NO FRAMES All Classes . ... FIELD | CONSTR | METHOD . DETAIL: FIELD | ... java.lang.Object ij.plugin.Options . ... PlugIn . public class Options . ... This plugin implements most of the commands in the Edit/Options sub-menu. ... This method is called when the plugin is loaded. Methods inherited from class java.lang.Object . ... This method is called when the plugin is loaded. 'arg', which may be blank, is the argument specified for this plugin in IJ_Props.txt. ...

Next: C Standard Library Functions Up: Common C Compiler Options Previous: Common C Compiler Options . c Suppress linking with ld(1) and produce a .o file for each source file. A single object file can be named explicitly using the -o option. ... Sends the output to the standard output, or to a file named with the -o option. Includes the cpp line numbering information. ... When this option is given, the -O and -R options are suppressed. -help Display helpful information about compiler. ...

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 | ...

Silicon/Tungsten ECal for SiD ­ Status and Progress Ray Frey University of Oregon ICLC Paris , April 22, 2004 · Overview (brief) · Current R D detectors electronics timing · Hybrid Status from K.U. · Summary ICLC Paris R. Frey 1 SD Si/W M. Breidenbach, D. Freytag, N. Graf, G. Haller, O. Milgrome Stanford Linear Accelerator Center R. Frey , D. Strom U. Oregon V. Radeka Brookhaven National Lab ICLC Paris R. Frey 2 Concept ...

To main of Laboratory . The research work and design of optical and optical-electronic devices are carries out by laboratory staff: . ... Lens: . ... In the layout 1 prism systems perform functions of dispersive element, corrector of aberrations, optical reducer. ... Spectral range 200 - 400 nm; . ... Back Forward . ... The main corrector's function are compensation of field aberrations of the main spherical mirror of a telescope (diameter of 600 mm, f'=1200 mm) and increase aperture ratio. ...

Next: Acknowledgements Up: Echelle Reduction Previous: Instrument Description: CASPEC . The two following diagrams summarise the successive steps performed by high-level procedures RESPONSE/ECHELLE and REDUCE/ECHELLE depending on the main options: . Flat-field correction can be performed or not . Instrumental response correction can be skipped, or performed using either a standard-star or IUE-like methods. Figure: Response/Echelle . Figure: Reduce/Echelle (1) . ...

Armagh Planetarium Mars HiRISE Wallpapers . High Resolution Imaging Science Experiment (HiRISE) is flying onboard the Mars Reconnaissance Orbiter (MRO) mission. Mouse over the thumbnails for a larger view of the image. ... When the image has entirely loaded, right click on it and choose option 'Set as background' or 'Set as wallpaper' depending of your Windows version. ... Historical Images . ... Mars Wallpapers . 1024 x 768 px . 1600 x 1200 px . Image Info . ... 1600 x 1200 pix . ...

... Apache HTTP Server Version 2.4 . Apache > HTTP Server > Documentation > Version 2.4 > Programs . ... htcacheclean is used to keep the size of mod_cache_disk 's storage within a given size limit, or limit on inodes in use. ... If one or more URLs are specified, each URL will be deleted from the cache, if present. ... Specify limit as the total disk cache size limit. ... By passing the -a or -A options to htcacheclean , the URLs within the cache will be listed as they are found, one URL per line. ...