AND HERE IS YET ANOTHER EPISODE FOR HOURS OF DOOM FUN. ... Additional Credits to : ID Software: DOOM, Geoff Allan: DoomEd, Brendon Wyber & Rapha‰l Quinet: DEU. Play Information * Episode and Level # : E1M1 Single Player : Yes Cooperative 2-4 Player : Yes Deathmatch 2-4 Player : Yes Difficulty Settings : Yes New Sounds : No New Graphics : No * Construction * Base : New level from scratch Build Time : 1 hour Editor(s) used : Windows DoomEd v2.60 & DEU v5.1 for grouping. ...

Astronomy Picture of the Day . Starbirth in the Lagoon Nebula . ... 24.10.1996 . ... Big Throughput Camera , . 4-m Blanco Telescope , CTIO , Chile Explanation: Stars are forming even today in the Lagoon Nebula. ... Many of the stars appear red because of the high amount of dust in the Lagoon Nebula . Red light penetrates dust clouds best, although enough dust will block all visible light and leave a dark nebula. ... October 1996 . ... NASA Web Site Statements, Warnings, and Disclaimers . ...

Supernova 2009ip in NGC 7259 . This page is devoted to information on Supernova 2009ip in NGC 7259 . ... In July 2012, CRTS noticed that this object had started to brighten again. ... Then in September of 2012 it got brigher again. ... Cornell University The Unprecedented Third Outburst of SN 2009ip: A Luminous Blue Variable Becomes a Supernova . ... UIS Henry Barber Research Observatory 2009ip page . ... 2009/08/26.11 . ... Joseph Brimacombe . ... Stan Howerton . ... Stan Howerton Light curve . ...

In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...

... While the three NICMOS cameras are no longer at a common focus, under many circumstances it is desirable to obtain data simultaneously in multiple cameras. ... From the ground, the infrared background is affected by telluric absorption and emission which limits the depth of astronomical imaging. ... Now, the dominant sources of background radiation will be the zodiacal light at short wavelengths and the thermal background emission from the telescope at long wavelengths. ...

LBV 2009ip in NGC 7259 . This page is devoted to information on LBV 2009ip in NGC 7259 . 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. ... Discovery page . SNWeb has a 2009ip page . ... Click on the name in the "Image Credit" column to see the image. ... 2009/08/26.11 . ... Joseph Brimacombe . ...

... Classes . ... casa::MSValidIds . ... MSValidIds (const MeasurementSet &ms) . ... antenna1 ( uInt rownr) const . ... antenna2 ( uInt rownr) const . ... dataDescId ( uInt rownr) const . ... fieldId ( uInt rownr) const . ... observationId ( uInt rownr) const . ... processorId ( uInt rownr) const . ... stateId ( uInt rownr) const . ... polarizationId ( uInt rownr) const . The polarizationId comes from the DATA_DESCRIPTION subtable, so dataDescId must first be valid in order for this to also be valid. ...

You Can Make Stellar Images Brighter . Articles | ... A few months ago I wrote an article titled "You Can’t Make Them Brighter". So why am I now writing that you can make them brighter. ... The image of a focused star is actually a small disk called the Airy disk, named after the 19 th century scientist Sir George Airy. ... For a given aperture, a smaller Airy disk means that the light is focused to a smaller disk and is therefore brighter. ... www.astronomy.net . About Astronomy Net | ...

... Stars . ... Straight away the three stars in his belt will grab your attention, followed by the glittering white star Rigel in his left foot and the bright orangish star Betelgeuse in his right shoulder (assuming Orion is standing facing us and not with his back to us). ... Orion Belt?s with the stars Alnitak, Alnilam and Mintaka. ... In short, Orion was a big, loud giant of a man and indeed a mighty hunter, he also inherited some aquatic superpowers from his father who was the sea god Neptune. ...

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... Since moonshine is really reflected sunlight, the full Moon is on the average slightly brighter in mid-winter, when Earth is closest to the Sun. In addition, the distance of the full Moon also varies, due to the ellipticity ("eccentricity") of the Moon's orbit. On 22 December, 1999, the two effects combined to produce the brightest full Moon of the century. ... This year will be the first full moon to occur on the winter solstice, Dec. 22nd, commonly called the first day of winter. ...

ATMoB "Open Cluster Observing Award " Guidelines Purpose: To promote observing among the membership of the Amateur Telescope Makers of Boston through participation in the Open Clusters Observing Awards program. Introduction: This awards program is oriented towards visually observing open clusters above magnitude 9.9. ... It turns out that a very unprejudiced and convenient method to dermine the limiting magnitude is to count the number of visible stars in certain areas on the sky. ...

From: TerryMosel aol.com Date: Sun, 3 Jul 2005 18:53:52 EDT Subject: More on Deep Impact Hi all, Some of you won't have got my last email because your firewall or server or ISP rejected it since it had a starmap attached as a JPEG file. ... The map showed the position of Comet 9P / Tempel 1 from Monday night to Saturday night, so you could have a look to see what effect the NASA Deep Impact probe would have on the comet (it's expected to make it brighten from 10th to about 6th magnitude). ...

... I write two Whitelist files, since the >> spamassassin systems on cfa0 and on head are different. ... DEBUG print found addr $t\n ; $addrs{ whitelist_from $t } = 1 ; } } } open( FILE , $ spam_filter ) || die Cannot open spam filter $ spam_filter ; while ( FILE ) { chop ; tr/[ A-Z ]/ a-z ]/; $addrs{$_} = 1 ; } close ( FILE ) ; open( FILE , $ spam_filter ) || die Cannot open spam filter $ spam_filter ; $ DEBUG ...

. At 7:15 p.m. MST on the evening of March 16, longtime Astronomy magazine contributor Chris Schur obtained a more close-up image of Comet PANSTARRS than we've been receiving. He attached his Canon XTi DSLR to a 3.2-inch Zeiss apochromatic refractor at f/4.6. He set the ISO to 200 and took a 5-minute exposure from his home in Payson, Arizona. The comet still had a total integrated magnitude of 1.5. As a comparison, the two brightest stars in the image (to the upper right) shine at magnitude 6.3. Chris Schur

MINUTES of the RadioAstron Teleconference on December 09, 2009 N. Kardashev chaired the teleconference. ... V. Andreyanov presented information about tests at LA. Integration tests of the flight SRT are being continued. ... SRT was tested together with the Flight model of the high data rate radio communication system (VIRK). ... S.Likhachev provided information on activities in development and tests of Russian data recorder and correlator. ... ASC software correlator was used for the corealtion. ...

Have you ever heard the name of a star or constellation and wondered what it meant? ... I've compiled a table of commonly known star names and their definitions in the Western tradition, grouped by constellation. ... Following each constellation entry are any named stars found therein (in order from brightest to faintest), listing the Bayer (Greek letter) or other common designation, the star name, and English translation. ... Some other sites with star name information: . ...

... 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. ...

In autumn 1994, two groups of astronomers announced that they had discovered Cepheid variable stars in a distant cluster of galaxies. ... As the term suggests, variable stars change in brightness over time. ... Variable stars are an ideal way to get high-school students doing real science, with real data, from the real sky. ... a sky chart to find the stars . ... Students can use the nearby stars to estimate the magnitude of Delta. ... Locate the star Delta in Cepheus and estimate its brightness . ...

Организаторы: Michel Balazard (CNRS, Лаборатория Понселе) , Михаил Цфасман (CNRS, Лаборатория Понселе, ИППИ РАН) , Алексей Зыкин (Лаборатория Понселе, ГУ ВШЭ) . О конференции . Общая информация . ... Практическая информация . ... Using Miyawaki-Ikeda lifting and Rankin-Selberg method I explicitly compute critical values for spinor and standard L-functions attached to Siegel cusp form of genus three and weight twelve. Страница Лаборатории Понселе . ...