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 ...

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• The Face on Mars
• Sensors

... 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., ...

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• Siding Spring Survey Follow-up Obs
• Siding Spring Survey Telescope Images
• Mike Bessell, MSSSO - Images

. Go Here for Hubble Ultra Deep Field . ___________________________________________________________________ The Electronic Universe Project e-mail: nuts@moo.uoregon.edu

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• The Galaxy Gallery: Messier Objects
• Fabry-Perot Images of Spiral Galaxies
• Galaxy Gallery Page II

... CentralProcessor 0.11 documentation . Calibration and Imaging Documentation . The cmodel pipeline task is responsible for extracting a local sky model (LSM) from the global sky model (GSM) and building an image from the components and/or images resulting from the request. ... MPI wrapper> cmodel -c config.in . ... None . ... If Cmodel.gsm.database is set to asciitable then a row/column (space separated) file is used as the global sky model source. ... cmodel (Model Image Generator) . ...

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• ccontsubtract CentralProcessor 0.11 documentation
• PmWiki | PmWiki / Images
• Workshop 2001 - exercise 1

... This section describes three functions which have been created to cleanup defects in images. The first two functions for cleaning rows and columns are particularly useful for CCD--images. ... These can often be removed with the commands: MODIFY/COLUMN INPUT OUTPUT [C or V] [columns] . ... This is particularly useful for removing the permanent defects which may exist in the CCD--frames and which cannot be removed by the MODIFY/COLUMN or MODIFY/ROW commands. ...

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• CCD Image Quality - PixelVision
• Product Folder: TC237, 680- X 500-PIXEL CCD IMAGE SENSOR DATA SHEET
• Product Folder(Obsolete): TC236P, 680- X 500-PIXEL CCD IMAGE SENSOR

... Главная страница / Кометы и астероиды / "Нас не догонишь". Комета 217P/LINEAR, M42, M43, Бегущий Человек и пролетающие спутники. ... M42 , M43 , БегущийЧеловек , 217P/LINEAR . ... Комета C/2009 R1 (McNaught) . ... Все права на размещенные в галерее фотографии принадлежат их авторам. ... Киевский клуб любителей астрономии "Астрополис" . Движок галереи: 4images 1.7 ...

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This is an interim program to convert Arecibo data into `regular' fits format files. ... Offset 5400.000000 (5399.719945) Object:U4131 Number of scans in an image:4 Number of dumps in a scan:300 Commands are (all caps required): QUIT to stop converting, DRIVE to finish entire file with same object name, UNTIL <scan> to continue for num or until reaching scan, SKIP <num> to skip to scan <num>, ASKFREQ to prompt for frequencies each time, ASKMAP to prompt for map pos. ...

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• M42 Color Images
• xband rfi measurements
• Planetary Radar: Arecibo Radar Images of Asteroids

... Finding Stars . ... Handling Bad Pixels . ... The guide camera image controller can control one or more guide cameras. ... Each time the camera is read, the image is automatically saved to a fits file on a shared disk. ... Cameras that have bad pixels require "bad pixel maps" in order to find stars, centroid or even compute statistics for the image. ... View this image (for instance in NIH Image) and determine an upper and lower cutoff; pixels whose values are outside of this range are considered...

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• Astrophysical Research Consortium - Apache Point Observatory
• PVCam Gotchas
• Agile Procedures

... Reprocessing WFC3/UVIS and ACS/WFC images requires DrizzlePac v1.1.10 . ... HST Peer Review Process . ... DrizzlePac . ... As of September 10, 2013, MAST calibrated data products for WFC3/UVIS contain additional header extensions describing the image distortion. ... However, in order to be compatible with the updated DrizzlePac software (which expects a separate solution for each chip, as required by the new WFC3/UVIS correction), the format of the ACS D2IMFILE has changed, as shown below. ...

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• Hcompress Image Compression Software
• HDF-S Flanking Fields Data Reduction / Technical Issues
• Overhead Times

... This is a personal project collecting and documenting early images of Harvard College Observatory, focusing on the site at Observatory Hill (previously Summer House Hill). ... Earliest source: "[Observatory women computers], 1891." ... A group photo of computers at Harvard together with Mary Anna Palmer Draper, aka Mrs. Henry Draper. ... 1891 . General: The women depicted in this photograph analyized stellar photographs and computed data at the Harvard College Observatory. [link] 1891 . ...

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• The AstroStat Slog Blog Archive [tutorial] multispectral imaging, a case study
• Printing an Image
• The AstroStat Slog Blog Archive [ArXiv] NGC 6397 Deep ACS Imaging, Aug. 29,...

Next: Ionospheric Corrections in AIPS++ . ... Previous: AIRY: Astronomical Image Restoration in interferometrY . ... Calculate residual images for all facets (using 2-D transforms). Partially deconvolve individual facets and update the image model for each facet. ... The image in Figure 1 was made using the AIPS++ widefield algorithm with 225 facets. ... In calculating the residual image the residual visibility re-projection for the different facets can be estimated independently. ...

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• Imaging by an Optimizing Method
• Astronomical Image Compression Using the Pyramidal Median Transform
• Automated Photometric Calibration Software For IRAF

... SDSSmosaic allows you to create science image mosaics of SDSS frames in 3 easy steps, described below (see Usage). ... SDSSmosaic requires a standard IRAF installation (including STSDAS and tables packages); python (including urllib); SExtractor and Swarp by E. Bertin (can be obtained at http://astromatic.iap.fr/software/ ). ... The package is developed by Stefano Zibetti (2009-.. ... If you received this package from a third party, please notify the author ( zibetti at arcetri.astro.it ). ...

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• The Face on Mars
• The ARNICA Imaging Camera
• Using mod_rewrite to control access - Apache HTTP Server

You must have a Java-enabled browser to run ImageJ. For Firefox, use these settings to allow Java: . ... Enable Java . If you accept the certificate you will be able to view images that are stored on your computer. ... You may need to install the Java Runtime Environment for your computer if it is not already installed. If you are unsure, tryout the browser test at SUN's Java website: . Java Browser Test and follow the instructions. ... kielkopf at louisville dot edu . ...

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• ImageJ Applet with Images of the Tarantula Nebula for Astronomy at the
• Alsvid - Python Programs for Processing FITS Astronomical Image Data
• ImageJ for Astronomy at the University of Louisville

Dr. Phil Plait , aka "The Bad Astronomer" . ... Images . ... Bad Astronomy site . The following are high-resolution images suitable for promos, newspapers, brochures, and the like. Clicking on the thumbnail image will bring up the high resolution image. High resolution (1.3 Mb) . Medium resolution (550 kb) . ... Dr. Plait giving a TV interview at NASA's Goddard Space Flight Center about the transit of Venus in 2004. ... Dr. Plait posing with a model of the Apollo 11 landing site. ...

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• Phil Plait's Bad Astronomy: Misconceptions: Hoagland's Bizarre Image
• Phil Plait's Bad Astronomy: Misconceptions: The Not-Always-Red Planet

... Asteroid 23593 images obtained using the Faulkes Telescope North at Haleakala, operated by Las Cumbres Observatory. ... My main project was to search through archive images of the Subaru telescope looking for and identifying asteroids. ... Two of the known asteroids were asteroid 23593 and asteroid 71250. ... The pictures below were taken with the Faulkes telescope and show the asteroid 23593 in its state at 11/08/2015 ten years after I identified it in the Subaru telescope's image archive. ...

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• Gary, Callum and Peter: `Stars' of the Future
• Doppler Imaging and Flare Activity on HR1099
• Terry Mosely's Bulletins

... I first saw this referred to as a KPT effect called Canvas or something like that. ... You can create some very nice paper/stone textures using a noisy bump-map. ... Let's start with a blank image and Add Noise to it at 70 (Note: this blank image should be the same size as the image you want to canvas-ify, in this case 200x200): . ... 5) Our image has been canvas-ified! As you can see, the final image looks very much like it's printed/painted on a canvas, or a canvas-textured substance. ...

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• APOD: Asteroid 433 Eros Stereo Images
• Hands On; Texture Wrapping
• Supernova 2003gd in M74

Supernova 2009H in NGC 1084 . This page is devoted to information on Supernova 2009H in NGC 1084 . Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . Information on the original web pages for many of these images can be found on the updates and links web pages. Yet another discovery by Lick Observatory Supernova Search (USA). ... Web pages dedicated to this SN. SNWeb has a 2009H page . ... 2009/01/02 . ...

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• Supernova 2009js in NGC 918
• Supernova 2009I in NGC 1080
• Supernova 2011iy in NGC 4984

... Meta Index / Home Page / Algorithm . The following summarizes the way the program works for IMAGING mode data. ... FAST mode data is processed in a simpler fashion- the extended-source algorithms are not used. ... Look for largish extended sources . Look for smaller extended sources . Look for faint sources . ... If any largish extended sources have been found re-compute the background image . ... Check for faint extended-sources near much brighter sources, and delete if necessary. ...

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• OPERATION
• Usage
• regionmask: convert FITS REGION to image MASK

... The STECF IRAF layered package impol provides five tasks specifically aimed at reduction of HST imaging polarimetry data for ACS, FOC, NICMOS and WFPC2. ... Reduction of HST polarimetry data and simulation of raw polarimetry images, together with polarization vector plotting, are covered. ... hstpolsim -- Produce simulated polarization input data frames for HST instruments from images of the total signal, the linear polarization and the position angle of the polarization vectors. ...

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• FORS Sec Std and Abs Phot Project
• Frequently Asked Questions
• Los Cielos de Am , The darkest sky and the two galactic hemispheres

This WWW form allows the user simplified access to images produced by the NRAO/VLA Sky Survey (NVSS). This service determines which NVSS image is desired based on a celestial position and returns either the image directly or a Web page with a link to the file. ... The NVSS Postage stamp (small FITS file) server can be used to obtain images with other geometries.) ... Web browsers use external viewers to display files like FITS images which they do not understand. ...

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• NVSS Image ftp service (5 August 1998)
• Lucky Imaging Publications
• OptInt PmWiki : PmWiki / Markup Master Index