... ESO is building what will be the World's largest optical telescope array, The Very Large Telescope (VLT). The VLT Project organisation is responsible for the design and construction of the Unit Telescopes, including enclosures, optics, adapter-rotators and coating unit. ... Unit Telescopes Overview - This page is outdated, an update is in process. ... Secondary mirror (M2 Unit) - This page is outdated, an update is in process. ... Coating Unit - This page is outdated, an update is in process. ...

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• Los Cielos de Am , The darkest sky and the two galactic hemispheres

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Astronomy Discussion Forums . ... God and Science ћ SETI ћ Software ћ UFO ћ XEphem . ... OSETI On Steroids (Venus Lights Up In Spots) . ... Post Message | ... OSETI might want to monitor the "Venus Transit" and record those "Unnatural Ashen Lights". ... Topic: Venus 'Ashen Light' seen! by; Dave Lillis . ... www.astronomy.net . About Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• Does Sound Or Light Stop At Some Point? - an Astronomy Net Blackholes2 Forum
• Light Pulses - an Astronomy Net Blackholes2 Forum Message
• If Light Cannot Escape, How Can Gravity? - an Astronomy Net Blackholes Forum

... This is done by taking in all input files the extension whose name is specified by the maintable parameter (called 'merged extension' in what follows) and merging the columns into a single output extension of the same name. ... Its contents is taken from the CCDID keyword (and QUADRANT for EPIC PN). ... To propagate other column specific keywords, they must be specified manually via the extensionchecks , mainattributes , maxattributes and minattributes parameters (see above). ...

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• Extraction of a X-ray light curve for a point-like source
• Extraction and correction of an X-ray light curve for a point-like source
• Comments

... Classes . ... Class List . ... casa . casa::StreamIO . Public Member Functions | ... StreamIO (const String &hostname, uShort portNumber) . ... This function always returns True. virtual Bool . ... This function always returns False. virtual Int64 . ... Name lookup is not currently done so that the dotted quad notation must be used. virtual casa::StreamIO::~StreamIO . ... virtual Bool casa::StreamIO::isReadable . ... Not a meaningful function for this class and this function always returns -1. ...

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• Set-related user input
• Number input
• IFCHAN

OptInt PmWiki : MROI Delay Line SW / Requirements Review . The requirements review took place on 21 May 2009. ... Requirement specifications for the MROI production delay line software . Delay Line Production Software Development Statement of Work (not attached as it contains confidential salary costs) . ... Requirements Specification for the MROI Delay Line System . ... Printable View of http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/pmwiki.php/MROIDelayLineSW/RequirementsReview) ...

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• OptInt PmWiki : MROIFastTipTilt / Doc Man
• OptInt PmWiki : Requirements Review | History
• OptInt PmWiki : PmWiki / Wiki Style Examples

Stellarium 0.12.3 . ... Classes . ... ClassљList . ... Refraction Class Reference . ... virtual voidљ . forward ( Vec3d &altAzPos) const . ... backward ( Vec3d &altAzPos) const . Remove refraction from position ("reduce"). ... forward ( Vec3f &altAzPos) const . ... setupGLSLTransform ( StelGLSLShader *shader) . ... virtual void Refraction::backward . ... virtual void Refraction::disableGLSLTransform . ... virtual void Refraction::forward . ... virtual void Refraction::setGLSLUniforms . ...

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• Stellarium: StelProjector::ModelViewTranform Class Reference
• Stellarium: StelProjector::Mat4dTransform Class Reference
• Stellarium: SphericalRegion::DrawParams Struct Reference

... GHRS IMAGEs and MAPs are obtained with the focus diodes (see Section on page 80 ) at the ends of the array of main science diodes. ... An IMAGE can only record the light in the 1.74 1.74 arcsec region of the LSA. ... A standard IMAGE will have a pixel spacing of 0.109 arcsec and will cover the entire LSA aperture of 1.74 1.74 arcsec. You may also select pixel spacings of 0.055 or 0.027 arcsec, with proportionately smaller regions of the sky covered in a 16 16 (the default) IMAGE. ...

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• The Hubble Deep Field - scattered light subtraction
• The Hubble Deep Field - version 1 scattered light subtraction
• CSPICE Routines: EKUCEI_C

Region markers can be moved, resized, rotated, zoomed, deleted, and can change geometric type. ... For example, markers placed on astronomical catalog positions should be fixed so that one cannot accidentally move them off the specified position. ... Parameters can be fixed using the fix option of the regions public access point (for fixing classes of markers) or by means of a fix keyword in the definition of an externally loaded marker. ... In the command: echo "regions fix all -position -size" | ...

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• *ltcplot* - Plot the light curve
• Spatial Region Coordinates
• Array File Specifications

... Following the Observatory's initiative in 2002, drawing attention locally to the issue of light pollution and the problems it produces both for astronomy and awareness of the night sky, and for saving energy and improving the natural environment, Mark Bailey made a presentation on light pollution, on 7 May 2003, to the Armagh City and District Council Environment, Health and Recreation Committee. This focused specifically on the growing problem of light pollution in the City of Armagh. ...

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• Abstract
• Terry Mosely's Bulletins
• ULTRACAM Observations of Subdwarf B Stars

... Imagine that for every pixel in the color image, you take its luminance value (that's how bright it appears). ... In the end, you will have a histogram which counts how many times each luminance value appears in the image (that histogram can be used to analyze the distribution of the luminance values in the image). ... For the watermark effect, we want to use the same value that we used in the Stretch Contrast step, so that the lightest color will be in fact white (255), and nothing will get clamped...

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• Lighting plug-in
• Light Curve Templete/Observing Form For Visual SNe Observers.
• APOD: 2012 April 5 - Zodiacal Light Panorama

Astronotes Armagh Planetarium's Stellar Blog! ... Stars . ... Space Flight . ... Some 13.7 billion years ago, a mere millionth of a second after the Big Bang, the first hydrogen and helium nuclei condensed out of a hot, dense soup of quarks and gluons. ... In the very last few kilometres some of the light was scattered by a myriad of water droplets (containing hydrogen nuclei which had existed almost since the Big Bang) slowly descending through the air following a rainshower. ...

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• Our Galaxy | Astronotes - Part 5
• Universe | Astronotes - Part 5
• Astronotes | Armagh Planetarium's astronomy news from across the Universe -

... NASA's Stratospheric Observatory For Infrared Astronomy, or SOFIA, reached its "First Light" flight milestone during the early morning hours of May 26, when the aircraft's telescope and attached infrared camera collected light from celestial . targets for the first time at altitude. ... the Faint Object infraRed Camera for the SOFIA Telescope (FORCAST). ... For comparison, the human eye sees light with wavelengths between 0.4 and 0.7 microns.) ...

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• ASP: Black Holes to Blackboards: Seeing the Light
• ASP: Making a Rainbow
• ASP: Making Your Own Astronomical Camera

... Bad Astronomy . Misconceptions . ... Bad Astronomy : "We're light years more advanced than our competition!" ... Even the closest astronomical object, the Moon, is 400,000 kilometers away! ... A beam of light will travel 9,500,000,000,000 kilometers in one year. This distance is defined as a light year ; the distance light travels in a year. ... This is another example of Bad Astronomy; like a light year, a parsec is a unit of distance, not time (to be specific, it equals 3.26 light years) . ...

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• Phil Plait's Bad Astronomy: Bitesize Astronomy
• Phil Plait's Bad Astronomy: Bad TV

... Credit Copyright: Miloslav Druckm ller (UM FSI, Brno Univ. of Technology ), Shadia Habbal ( IfA, Univ. of Hawaii ) Explanation: Sweeping from the eastern to western horizon, this 360 degree panorama follows the band of zodiacal light along the solar system's ecliptic plane . ... In the mosaic projection, the plane of our Milky Way Galaxy runs at an angle , crossing the horizontal band of zodiacal light above the two horizons. ... Publications with keywords: zodiacal light . ... A Zodiacal Skyscape ....

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• XWare > APOD
• Startling Star V838 Mon

. elstream.ru: онлайн видеотрансляции с Эльбруса . GAMIT . Tags: видео . This entry was posted on Saturday, January 28th, 2012 at 10:12 am and is filed under Uncategorized . You can follow any responses to this entry through the RSS 2.0 feed. Responses are currently closed, but you can trackback from your own site. Comments are closed. Лаборатория лазерной интерферометрии is proudly powered by WordPress . Entries (RSS) and Comments (RSS) .

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• elstream.ru: онлайн видеотрансляции с Эльбруса Лаборатория лазерной
• GAMIT Лаборатория лазерной интерферометрии

... Procedure . ... Wind Baffle Pendant Control, located in the 2.5m enclosure. Spreader Bar for wind baffle counterweights, located behind the Machine shop. ... Wind baffle frame tied to eyebolt in floor. ... Move the inner white wind baffle counterweight from the temporary mounting blocks at the front of the wind baffle frame to the standard location at the back. ... Rig the secondary truss to the overhead crane using a large shackle and 4 long nylon straps (load capacity of 1000 Lb. each). ...

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• Procedure to Remove 2.5m Secondary Mirror
• Procedure to Install 2.5m Secondary Mirror
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... Team . ... GRB mini-workshop 2006 . ... Our study of GRB fields in optical range efforts to shed light on the progenitor problem and it is naturally splitting into two directions. The first one is study of GRB OT via follow-up observations, while the second way is investigation of GRB host galaxies. ... The first stage consists in observational data acquision, the second one yields estimates of GRB OT characteristics and its host galaxy parameters. ... Do GRB hosts differ from field galaxies? ...

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• Глава 5. Ethernet/IEEE 802.3
• Why Use CEILIDH ?
• IPC:Shared Memory

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 . ...

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• THE BRIGHT SUPERNOVA 1991T IN NGC 4527; AN AMATEURS PRESPECTIVE
• Supernova 2004gt in NGC 4038
• Supernova 2006el and 2006dn in UGC 12188

... Image Quality of the VLT . Total Optical Control . First light for the ESO VLT unit telescope 1 occurred during the workshop. ... The image shown (Figure 1 ) here was obtained with the VLT on May 16, 1998, in red light (R band), i.e. while the mirror was still uncoated. ... In this diagram (FIgure 2), the measured image quality of the VLT UT1 astronomical images is plotted versus the ``seeing", as measured by the Seeing Monitor, a small telescope also located on top of the Paranal Mountain. ...

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