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 ...

... 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., ...

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

... 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) . ...

... 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. ...

... 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 ...

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. ...

... 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...

... 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. ...

... 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 . ...

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. ...

... 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 ). ...

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 . ...

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. ...

... 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. ...

... 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. ...

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 . ...

... 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. ...

... 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. ...

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. ...