... All images on this page are copyright Robert H. McNaught. ... There have been so many requests for high resolution copies of these images that I ask that all enquiries for these to go directly to Science Photo Library. C/2006 P1 on Jan 18, 10:22 UT. Photo: R. H. McNaught, Siding Spring Observatory. Canon 5D, 135mm, f/2.0, 2 sec exp., ISO 1600 . ... ISO 200 . ... Canon 5D, 50mm, f/2.0, 30 sec exp., ... Canon 5D, 135mm, f/2.0, 120 sec exp., ... Canon 5D, 50mm, f/2.0, 110 sec exp., ...

M1 image More About M1 Nice Color Picture . ... M16 image More About M16 HST image . ... M31 image More About M31 Nice Color Picture . ... M42 image ; M43 image More About M42/43 Nice Color CCD Picture . M51 image More About M51 Color Image of M51 M51 Supernova . M57 image More About M57 Nice Color CCD Picture Very Deep M57 Image . ... M81 image More About M81 M81 Supernova Ultraviolet Image of M81 More about Ultraviolet Imaging . M82 image More About M82 M82 False Color M82 True Color . ...

You can also see this page in Russian with using KOI8 (X Windows) or CP1251 (MS Windows) Cyrillic coding. The Laboratory supports the space TV experiments, mainly in the planetary exploration missions. ... Image Co-registration . ... PHOBOS mission - Martian satellites investigations. Phobos on the Martian limb, the image from Phobos-2 probe from 02/28/89. ... Russian Space Bulletin. ... Last modified at June,26 1997 Alexey Kuzmin: akuzmin@mx.iki.rssi.ru . Back to IKI home page ...

... 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. ...

... omdetect (omdetect-5.14.2) [?? Meta Index / Home Page / Source Flagging Algorithms Since the object producing a read-out streak may lie outside the image, another algorithm is also used by omdetect. ... nMin = int( 0.6 (ny + 1)) where ny is the number of rows in the image (image height) . ... Loop through all the columns of the image . ... n4 = count(image(i0, :) image(i0 + 1, :) ) Count the number of pixels along column i0 that have a greater value than their neighbour in column i0 + 1 . ...

This describes the exposure window used by each instrument (the graphical interface for the hub's expose command). ... To open the expose window for a given instrument, bring up that instrument's main window, then press the Expose... button along the bottom. ... The top panel shows the status of the current exposure sequence (regardless of who started it). ... File: the file name for the current exposure, or the most recent exposure if not exposing. ... Download: exposure download preferences. ...

... A2010 is doing 600 second drift scans with alfa (each 600 second drift is refered to as a strip). ... For each strip the total power was computed for each beam/pol after removing frequency channels with rfi. ... Images were made of this value with strip number vs sample. ... The images below show the total power for a strip versus strip number. ... At strip number 150 (the dashed line in the image) the amplifier was installed in pixel2a,b. Pixel 0 a,b (.gif) image. Pixel 1 a,b (.gif) image. ...

Astronotes Armagh Planetarium's Stellar Blog! ... Monthly Sky Notes . ... Image credit: Julie Thompson / Armagh Planetarium) . ... These seven entrants and their class have won a free trip to the Planetarium.€а All entries are on display in our Exhibition Area.€а A number have been included in a special Christmas trailer running before all shows in our Digital Theatre throughout December so why not check out the works by the countryтАЩs budding new artists this Christmas break at Armagh Planetarium? ...

... A number of the above steps require the combination of a number of IR images. ... The command COMBINE/CCD is used to combine several images. The command itself has a number of options to use DO tables or catalogues, but the simplest version takes the form: COMBINE/CCD type images output . ... will combine the images kflat1 , kflat2 and kflat3 into an output image kflat using the combination options specified for the FF image type. ...

The following options are available via the file menu: . Display File Browser . ... XDir then can be used to send image file names to SAOtng for display. ... Regardless of the original image file format, SAOtng maintains a FITS image of the displayed image section in its memory. ... Pressing carriage return in the text window or clicking the OK button will cause SAOtng to store the current display frame in GIF format. ... Re-extract an image section from the current image file and re-display it. ...

Kermit output files are named ker number_object_filter_time .fits. number is a four-digit integer that increments for each subsequent exposure. object is the object name (with spaced removed) as entered by the observer. filter is the name of the currently selected filter wheel position. time is the current UTC time as a six-digit integer, HHMMSS. ... Kermit has three selectable pixel timing modes: fast readout, slow readout, and slow readout with reset. ... Kermit has three readout modes: . ...

Next: Image Coordinate Systems Up: Image Data Concepts Previous: Image Data Concepts . Most of the items which are used to build up an image follow a FITS-like convention. ... The image item contains the pixel data, stored as floating point numbers. ... Finally the history item contains a text file describing the history of the dataset. A complete list of the items that are potentially contained within an image dataset is given in Appendix B . ...

... The Einstein On-Line Service (EOLS) is a simple menu-driven system which provides an intuitive method of querying over one hundred database catalogs. In addition, the EOLS contains over 30 CD-ROMs of images from the Einstein X-ray Observatory which are available for downloading. The EOLS provides all of our databases to the NASA Astrophysics Data System (ADS) and our documents which describe each table are written in the ADS format. ... The EOLS provides three options for data retrieval. ...

... The function is accessible, if the file with the image is open, and Ю identification of a star field is made. ... a) Load a first image by the command " Open ", and others by the command " Open +". b) Make an identification of the field. c) Open the menu " File ", select " Next " or press . ... It is necessary tree or more images. a) Load the first image by the command " Open" , and others by the command " Open + ". b) Open the menu " Marking ", select "Detect moving objects" or press - . ...

Canadian Paper Money] . This page will attempt to answer questions pertaining to Canadian Paper Money.љ ... 4) What does the "*" beside the serial number represent? ... Following the creation Canada's central bank, the Bank of Canada introduced its first paper money issue.љ ... Starting with the 1954 Bank of Canada issue, defective notes produced during the printing process were replaced by these 'replacement notes' which carried the asterisk before the serial number.љ ...

... The TRACE images may be used without restrictions in publications of any kind. ... These two images, taken on 18 November 2000 at 15:54UT and 16:11UT, respectively, show such an event: the red circle in the image to the left shows a region where many loops are cooling, with bright loop tops (the intensity scales with the square root of the image to reduce the dynamic range). ... See also a collection of images related to the Sun, other cool stars, and solar-terrestrial effects . ... Images | ...

... These images were provided to Winer Observatory by Mike Shade of Sonoita Hills Observatory as an example of the outstanding work done by local Sonoita amateur astronomers. ... All images on this page were taken with a 6-inch Astro-Physics aprochromatic refractor at Sonoita Hills Observatory using an SBIG ST-7 camera. ... Object: Galaxy Messier 100 . ... Date: March 2001 . ... All images on this page were taken with an f/5 Newtonian reflector at Sonoita Hills Observatory using an SBIG ST-7 camera. ...

Home About Meade Product Information Dealer Locator Customer Support Investor Relations Dealer Support Employment Opportunities Site Map . Meade Instruments Corporation . ... Meade Pictor XT-Series CCD Autoguider/Imagers . Section 13: Viewing and Processing Images . ... The software can read most images in these formats, and convert between them using the File, Save As command. ... This is done by placing the information in a .txt file with the same name as the image file). ... Merge Images: . ...

In this section we demonstrate how to use PEARL (formerly called IMAGR), OYSTER's own imager, to make an image of the triple star Eta Virginis. ... get_data,'2002-02-15.cha' HDS-file opened; mode=READ. ... We also will plot visibilities from a previously made model, even though a model is normally created after the image has shown which components to include in a model. ... Then use the command uvimage,/uv to display the model visibility amplitudes as an image underlying the uv-tracks. ...

... This program was created for correlating chosen regions in the series of fts images. ... Chosen regions' . ... In this section the program counts the integral for each region of the grid for each image. ... As a matter of fact, the integral is total brightness of the region and it is counted by 'int_tabulated' IDL function. ... In addition, the program will show the count of the regions which correlate with the corresponding region (the brighter region means the bigger count) and its contour. ...