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

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• Fabry-Perot Images of Spiral Galaxies
• CCD Astronomy Magazine Article Page 5
• HST Deep Field Data

WFPC2 . Images: version1 , version2 . Catalogs: Version 1 HDF-S , HDF-N ;Version 2 HDF-S . STIS . ... NICMOS . Images: Camera 3 , V2 of psf-convolved STIS 50CCD on NICMOS . ... Images: WFPC2 FF , STIS FF ; Version2: WFPC2 FF , STIS FF , NICMOS FF . Catalogs: Version2 WFPC2 FF , STIS FF , NICMOS FF . ... Check the instrument specific technical pages for a description of the data products and the implemented data reduction steps: STIS , WFPC2 , NICMOS , Flanking Fields . ...

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• Frontier Fields HST Data
• The Multiband Imaging Photometer for Spitzer (MIPS)
• Ghost Images

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
• Auroral Images

NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...

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... The improvement will be more pronounced in our crowded Wide Field Camera (WFC) images, and may be increased further through use of a more sophisticated method of combining the individual dithered images. Our analysis allows us to check for point spread function shape variations in the HST Planetary Camera (PC) field. ... In crowded field images, we are deriving information about the faint end of the luminosity function (LF) from the texture of the image background. ...

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• Starfinder: a Code for Crowded Stellar Fields Analysis
• Parallelization of Widefield Imaging in AIPS++
• ADASS 2003 Conference Proceedings

... Fields Observed . ... Data Archive . ... Complete Optical and X-ray data for all ChaMPlane fields are available through the DS9 VO interface . ... functionality of DS9 is available to manipulate the results in addition to those provided by the "Champlane tools" You can select images, compare . ... our region of interest has been selected by drawing a red square region on the image. at bottom left the high res optical image of that selected region, and on the right is the X-ray image. ...

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• *imcnts* - Radial Profile of an extended source at the field center
• Chandra Images for SNR J0500.0-7007
• ChaMPlane

. Album : asv-album :: Travels to distant places and countries :: 1997/08 Kyoto, Nara (Japan) :: 24/08 Nara . Up . << Prev . Countryside. You can see rice fields in the foreground (this is the road from Nara to Kyoto). Next >> . Photo album generated by album script from MarginalHacks by Dave Madison on Tue Jun 23 14:46:24 2015 .

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• Image: Rose alley; you can see fountain in the background.
• Image: Trees in the Vatican. San Pietro is on the background.
• Image: We're getting closer; Mt. Athos is at the background. It is about 2000

... 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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• Wide Field Survey Images
• Miscellaneous Wide Field Images
• Siding Spring Survey Follow-up Obs

We present H I imaging of the galaxy group IC 1459 carried out with six antennas of the Australian Square Kilometre Array Pathfinder equipped with phased-array feeds. ... We present H I images, velocity fields and integrated spectra of all detections, and highlight the discovery of three H I clouds - two in the proximity of the galaxy IC 5270 and one close to NGC 7418. Each cloud has an H I mass of ~109 Msun and accounts for ~15 per cent of the H I associated with its host galaxy. ...

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• Peculiar Gas Dynamics in the Starburst Galaxy NGC 253
• News Results
• The Circinus Galaxy

... 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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• ESO - HUGS HAWK-I imaging data release
• Basic CCD image processing
• GOODS

... 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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... OM grism data are obtained as image mode data. However the different nature of this type of data, spectra of the objects in the field of view instead of their "sky" image, makes that a special processing must be applied to the grism images. ... They are concatenated in a perl script, omgchain , which works in a similar way to the image and fast mode chains. ... All necessary corrections are applied to the grism data files. ... As we have pointed out OM grism data are image mode data. ...

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• Creating reconstruction image and background image from an input source list
• Correcting the image
• How to extract MOS background spectra from blank fields event lists

... 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 | ...

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• research field
• THE ISOGAL +45 FIELD
• NASA's Observatorium--Image Gallery: Stars

... SN Refsdal: The First Predicted Supernova Image . ... Most bright spots in the featured image are galaxies in this cluster. ... Gravity caused the cluster to act as a massive gravitational lens , splitting the image of Supernova Refsdal into multiple bright images . ... Four more bright images peaked in April in the lowest red circle, spread around a massive galaxy in the cluster as the first Einstein Cross supernova. ... A Supernova through Galaxy Dust . ... Giant Cluster Bends Breaks Images . ...

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• A Wide Field Image of the Galactic Center
• Астронет > A Wide Field Image of the Galactic Center
• Galaxy and Cluster Create Four Images of Distant Supernova

CATS home ] [ Back to CATS list ] [ ftp ] . ... 117.1578Bock+ The Molonglo Observatory Synthesis Telescope, operating at 843 MHz with a 5 deg^2 field of view, is carrying out a radio imaging survey of the sky south of declination -30 deg. This survey (the Sydney University Molonglo Sky Survey, or SUMSS) produces images with a resolution of 43"x43" csc|delta| and an rms noise level of ~1 mJy beam^-1. ... See also MGPS2 Galactic plane survey. ...

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• Direct electron imaging-model
• Combining Images
• CCD Image Quality - PixelVision

Next: The Evolution of Stars Up: NICMOS Science Previous: A Coronagraphic Search for . ... The NICMOS Parallel program . ... The Stellar Population . ... NICMOS Camera 3 is being used in parallel mode to observe galactic fields at both high and low galactic latitudes. ... Most of the fields are at high galactic latitude; as Figure 1 shows, only 8 pointings are within |b| = 10 o , i.e. the galactic disk. Figure 1: NICMOS parallel fields distribution in galactic latitude. ... Figure 6 ). ...

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• ST-ECF IRAF package
• STScI NICMOS Software
• SLITLESS (Oct97) --- ST_ECF --- SLITLESS (Oct97)

... In typical nightly use, the wide field and planetary telescope and cameras record images of favorably placed objects in the sky, including constellations, bright variable stars, nebulae through narrow-band filters, comets, the Moon, and planets. ... Shared Skies telescopes are available for use by students at the University of Louisville and the University of Southern Queensland, and by teachers and students in middle and high schools mentored by faculty at the universities. ...

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• Wide Field Spectral Imager
• MaximumFinder (ImageJ API)
• TiffDecoder (ImageJ API)

... 2015 December 21 . SN Refsdal: The First Predicted Supernova Image . ... Most bright spots in the featured image are galaxies in this cluster. ... Gravity caused the cluster to act as a massive gravitational lens , splitting the image of Supernova Refsdal into multiple bright images . ... Four more bright images peaked in April in the lowest red circle, spread around a massive galaxy in the cluster as the first Einstein Cross supernova. ... Follow APOD on: Facebook , Google Plus , or Twitter . ...

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• APOD: 2012 January 6 - A Wide Field Image of the Galactic Center
• APOD: 2015 March 9 - Galaxy and Cluster Create Four Images of Distant Supernova
• APOD: June 28, 1996 - A Distant Galaxy in the Deep Field

... Three day radio-astronomical forecast of the proton activity of the Sun: The figure shows multiwave radio emission scans - graphs of the distribution of intensity I and circular polarization V across the solar disk, obtained at RATAN-600. ... According to this criterion, for a proton flare to arise, the flux of radio emission must be sufficiently high at short wavelengths (blue color scans) and should increase with time compared to the general intensity. ... More about the solar activity . ...

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• Measurement of the dark halo shape in polar ring galaxies
• important11-15_en
• Image directory

. I-GALFA Image Gallery . Interesting survey images will be posted here as they become available. 2009 December . I-GALFA View of a Galactic Tangent Region . 2009 September . I-GALFA Survey Coverage Complete . 2009 May . I-GALFA Reveals Dynamic Events in Our Galaxy . 2008 October . Making Maps: Example + Animation . 2008 June . Infrared Emission in I-GALFA . 2008 January . Planned I-GALFA Survey Fields . I-GALFA main page

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• NRAO Image Gallery
• M42 Color Images
• First Galfa H I Map