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1. Impact Hazard
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Risks Comparable to NEOs . ... The Increasing Rate of Discovery of Asteroids . ... Comet and Asteroid Collision Probabilities . ... Extreme albedo comets and the impact hazard (PDF Format) . ... Asteroid Impact Animations . ... Workshop on Scientific Requirements for Mitigation of Hazardous Comets and Asteroids - 2002 . ... The Spaceguard Survey Report, 1992 (PDF) . Tsunami from Asteroid/Comet Impacts . ...
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Ссылки http://star.arm.ac.uk/impact-hazard/ -- 11.3 Кб -- 29.06.2012
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2. Laboratory of spectroscopy and photometry of extragalactic objects : Devices
. Go to RUSSIAN (KOI-8) . The spectrum of giant HII region in galaxy NGC 1084: . Grating : R1302(17) . Halpha region . Exposure time: 780s . Processing: 2 exposures sum with cosmic hits cleaning . The spectrum of bright HII region M17: . Grating : R1302(17) . Halpha region . Exposure time: 600s . Processing: 2 exposures sum with cosmic hits cleaning . Back to LSS main page. Back to Laboratory Home Page .
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Ссылки http://mavr.sao.ru/hq/lsfvo/devices/lss/lse_sobj.html -- 3.2 Кб -- 28.12.2007
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/lsfvo/devices/lss/lse_sobj.html -- 3.2 Кб -- 02.10.2012
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[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/lsfvo/devices/lss/lse_sobj.html -- 3.2 Кб -- 02.10.2012
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3. The Galaxy Gallery: Messier Objects
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 . ...
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Ссылки http://zebu.uoregon.edu/messier.html -- 7.0 Кб -- 23.07.2004
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4. Near Infrared Camera and Multi-Object Spectrometer Instrument Handbook for
... Near Infrared Camera and Multi-Object Spectrometer Instrument Handbook for Cycle 17 > Chapter 4: Imaging > 4.6 Photon and Cosmic Ray Persistence . ... HgCdTe detector arrays like those in NICMOS are subject to image persistence. ... Experiments using Cycle 7 NICMOS data have shown that it is possible to scale and subtract such ?post-SAA darks? from subsequent science exposures taken later in the same orbit, and thus to remove a significant fraction of the CR persistence signal. ...
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Ссылки http://www.stsci.edu/hst/nicmos/documents/handbooks/current_NEW/c04_imaging.6.7.html -- 122.3 Кб -- 05.02.2013
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5. IKI IPL home page
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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6. A Search for Bright Kuiper Belt Objects
... Search . ATNF Home . About ATNF . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Parkes radio telescope . ... Parkes | ... A Search for Bright Kuiper Belt Objects . ... Since 1992, 60 large Kuiper belt objects have been detected by ground-based telescopes. ... The detection of brighter objects would improve our ability to determine the Kuiper belt objects' surface composition and provide constraints on the population statistics of different formation mechanisms. ...
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Ссылки http://www.atnf.csiro.au/pasa/15_2/brown/paper/index.html -- 51.7 Кб -- 08.04.2016
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7. ESO - How can I run the pipeline when there are no bright objects in the
... Science . ... Science Users Information > Data Handling and Products > Data Reduction FAQ > How can I run the pipeline when there are no bright objects in the individual image? ... Observing with ESO Telescopes . ... The default use of the visir_img_combine recipe of the VISIR pipeline is with the "ref" option set to false. ... The VISIR pipeline will create the combination of the nodded images using the ESO SEQ CUMOFFSETX and ESO SEQ CUMOFFSETY offset information in the fits file headers. ...
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Ссылки http://www.eso.org/sci/data-processing/faq/how-can-i-run-the-pipeline-when-there-are-no-bright-objects-in-the-individual-image.html -- 24.8 Кб -- 10.04.2016
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8. XID: Cross-Association of ROSAT/Bright Source Catalog
[ CATS home ] [ Back to CATS list ] [ ftp ] . 2000ApJS..131..335Rutledge+ . Division of Physics, Mathematics and Astronomy MS 220-47, California Institute of Technology, Pasadena, CA 91107 rutledge@srl.caltech.edu, rb@astro.caltech.edu, prince@srl.caltech.edu
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Ссылки http://www.sao.ru/cats/doc/RBSC-USNO.html -- 8.2 Кб -- 18.03.2015
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9. Shared Object Cache in Apache HTTP Server - Apache HTTP Server
... Apache HTTP Server Version 2.4 . Apache > HTTP Server > Documentation > Version 2.4 . ... The Shared Object Cache provides a means to share simple data across all a server's workers, regardless of thread and process models . ... Initialize the cache. ... Destroy a given cache instance object. apr_status_t store(ap_socache_instance_t *instance, server_rec *s, const unsigned char *id, unsigned int idlen, apr_time_t expiry, unsigned char *data, unsigned int datalen, apr_pool_t *pool) . ...
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Ссылки http://www.arcetri.astro.it/manual/fr/socache.html -- 10.2 Кб -- 19.11.2015
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10. ASP: More About Deep Space Objects and Cosmic Terms
... SEARCH ASP SITE: Match ALL words Match ANY word . ... Astronomy . ... Hubble Space Telescope Images: http://hubblesite.org/newscenter/newsdesk/archive/releases/image_category/ . ... The Chandra x-ray telescope (in orbit around Earth) has been sending back a wide range of images of what deep space objects would look like if seen with "x-ray sensitive" eyes. ... Web Sites for Asking Astronomy Questions . ... Ask an Astronomer for Kids: http://coolcosmos.ipac.caltech.edu/cosmic_kids/AskKids/index.shtml...
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Ссылки http://www.astrosociety.org/edu/family/resources/deepspace2.html -- 25.7 Кб -- 02.10.2012
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11. APM 08279+5255: The Brightest Object Yet Known
... The recently discovered quasar labeled APM 08279+5255 has set a new record as being the brightest continuously emitting object yet known. APM 08279+5255 's great distance, though, makes it only appear as bright as magnitude 15.2, an object which can be seen with a moderate sized telescope. ... One possible explanation of APM 08279+5255's record luminosity is that it is partly a mirage: its light is highly magnified by an intervening galaxy that acts as a gravitational lens . ...
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Ссылки http://www.astronet.ru/db/xware/msg/1165178 -- 15.4 Кб -- 09.08.2004
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12. ADASS 2003 Conference Proceedings
... Low resolution, slitless spectral images were obtained at the Loiano Observatory in the wavelength window 3300-6420 ?, in order to identify in extragalactic objects targets displaying the most prominent features that characterise the spectrum of bright hot stars, WR and Luminous Blue Variables (LBV), and of nebular regions as well. We present the results with the well studied galaxy M 101, where the previously known H II regions with WR star signatures are easily identified. ...
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Ссылки http://www.adass.org/adass/proceedings/adass03/P10-2/ -- 13.2 Кб -- 13.08.2004
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13. APOD: August 18, 1998 - APM 08279+5255: The Brightest Object Yet Known
... August 18, 1998 . APM 08279+5255: The Brightest Object Yet Known . ... Explanation: It shines with the brightness of 100 billion Suns. ... The recently discovered quasar labeled APM 08279+5255 has set a new record as being the brightest continuously emitting object yet known. APM 08279+5255 's great distance, though, makes it only appear as bright as magnitude 15.2, an object which can be seen with a moderate sized telescope. ... About APOD > . ...
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Ссылки http://www.sai.msu.su/apod/ap980818.html -- 4.7 Кб -- 02.10.2012
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14. http://www.astro.spbu.ru/staff/ilin2/INTAS2/DOCS/summary.txt
PROJECT SUMMARY (max 3000 characters) The principal goals of the project are the observational and theoretical investigation of complex cosmic objects where the processes of dust scattering, absorption and emission play significant roles. ... Development of light scattering theory and computer codes to calculate the optical properties of non-spherical inhomogeneous particles and laboratory measurements of light scattering characteristics of irregularly shaped particles. ...
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Ссылки http://www.astro.spbu.ru/staff/ilin2/INTAS2/DOCS/summary.txt -- 4.6 Кб -- 19.11.2010
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15. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B8A3C8865-5C69-4E65-9A69-DFEA0A4D24D8%7D
This New Horizons LOng Range Reconnaissance Imager (LORRI) composite image shows the detection of PlutoтАЩs largest moon, Charon, cleanly separated from Pluto itself. Pluto is the brighter object near the center, and Charon is the fainter object near its 11 oтАЩclock position. The circles denote the predicted locations of the objects, showing that Charon is where the team expects it to be relative to Pluto. No other Pluto system objects are seen in these images. ...
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B8A3C8865-5C69-4E65-9A69-DFEA0A4D24D8%7D -- 3.9 Кб -- 10.04.2016
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16. Detection of unique bright radio flare of X-ray binary
... The Galactic low-mass X-ray binary GS 2023+338 was discovered during the burst on May 22, 1989 with the Japanise satellite Ginga (aka Galaxy). The flux reached 17 crabs (this unit of flux measurement is an bright X-ray source, Crab Nebula) at 10-35 keV. ... No other radio telescope worldwide carried out multi-frequency measurements. ... Upon 14 days the radio flux fell below the detection level at the RATAN-600 in relation to the decrease of the X-ray flux. ...
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Ссылки http://www.sao.ru/Doc-en/SciNews/2016/Trushkin/ -- 8.4 Кб -- 10.04.2016
[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/2016/Trushkin/ -- 8.4 Кб -- 10.04.2016
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[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/2016/Trushkin/ -- 8.4 Кб -- 10.04.2016
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17. Bright Supernova pages - Statistics for 1996
... Sorted by Name For the year 1996 , 96 supernovae and 0 extragalactic novae were reported. 96 of these supernovae were named by CBAT, 0 were given possible supernova designations, and 0 were not reported to CBAT. 24 supernovae were found in NGC/IC galaxies, 36 were found in named galaxies 24 objects were discovered by amateurs 0 were brighter than 13th Magnitude 8 were brighter than 16th Magnitude 27 were brighter than 18th Magnitude 54 Type I supernovae were ...
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Ссылки http://www.rochesterastronomy.org/SNIMAGES/snstats1996.html -- 5.2 Кб -- 10.04.2016
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18. S.P. Korolev RSC Energia - International Space Station
... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . Brief History of Rocket and Space Technology . ... Flights Chronology . ... Project History . ISS Russian Segment . Steps of ISS Assembly . Spaceflights Chronology . Chronology of Extravehicular Activity . ISS 45/46 . ... An additional objective is to detect micro-particles in the vicinity of the space station. ... 2015 JSC "S.P. Korolev RSC "Energia" . ...
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Ссылки http://www.energia.ru/en/iss/researches/ray/01.html -- 23.8 Кб -- 10.04.2016
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19. Siding Spring Survey
T he Siding Spring Survey (SSS) is a Near-Earth Object search program that utilises the 0.5-m Uppsala Schmidt Telescope at Siding Spring Observatory, N.S.W., Australia. ... The mission of the Siding Spring Survey is to contribute to the inventory of near-earth objects (NEOs), or more specifically, the potentially hazardous asteroids (PHAs) and comets (PHOs) that may pose a threat of impact and thus harm to civilization. ... Based on the CSS Mission page . ... Siding Spring Survey Main Page . ...
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Ссылки http://www.mso.anu.edu.au/~rmn/ -- 11.4 Кб -- 23.12.2011
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20. ImageConverter (ImageJ API)
... This class converts an ImagePlus object to a different type. ... Converts a 3-slice (hue, saturation, brightness) 8-bit stack to RGB. void . ... Converts this ImagePlus to RGB. public void convertToRGBStack () . Converts an RGB image to an RGB (red, green and blue) stack. public void convertToHSB () . Converts an RGB image to a HSB (hue, saturation and brightness) stack. public void convertRGBStackToRGB () . Converts a 2 or 3 slice 8-bit stack to RGB. public void convertHSBToRGB () . ...
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Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/ij/process/ImageConverter.html -- 16.8 Кб -- 02.12.2010
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Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
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