ARTI, 1999 , ARTI, 2000 , ARTI, 2001 , ARTI, 2002 , . LVOV, 1993 , LVOV, 1994 , LVOV, 1995 , LVOV, 1996 , LVOV, 1997 , LVOV, 1998 , LVOV, 1999 , LVOV, 2000 , LVOV, 2001 . MOSCOW, 1992 , MOSCOW, 1993 , MOSCOW, 1994 , MOSCOW, 1995 , MOSCOW, 1996 , MOSCOW, 1997 , MOSCOW, 1998 , MOSCOW, 1999 , MOSCOW, 2000 , MOSCOW, 2001 , MOSCOW, 2002 , MOSCOW, 2003 , MOSCOW, 2004 , MOSCOW, 2005 , MOSCOW, 2006 , MOSCOW, 2007 , . ...

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. Contact Webmaster for web page errors, corrections, ommisions, and/or additions. This page last updated: March 5, 2008 - JMD . This page last checked: February 23, 2007 - JMD . Click for forcast Click for IR Loop . NWS HAFB Topo Loop . NWS El Paso Topo Loop .

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• Astrophysical Research Consortium Small Aperture Telescope
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Демонстраторы лунного посадочного модуля (лэндера) Pixel и Texel были созданы для участия в проводимом фондом X-Prize (при участии NASA) конкурсе в категории Lunar Lander Challenge . ... На соревнования в в 2008 году аппарат компании выиграл Northrop Grumman Lunar Lander Challenge, но это уже другая история, так как разработка пилотируемого корабля к этому моменту практически прекратилась. ...

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Input file: lector.dvi % +first-page:* +last-page:* +double-sided:- +skip-sides:0 +number-of-sides:65535 +backward:off +left-margin: 0in +top-margin: 0in +height:11in +width:8.5in +transformation:0 +page-width:8.5in +page-height:11in +page-left-margin:1in +page-top-margin:1in +backside-offset-x: 0in +backside-offset-y: 0in +columns:1 +rows:1 +section-count:0 +section-size:0 +full-last-section:off +fold-other:off +page-shift: ...

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The first near-infrared IFU spectrograph was the 3D instrument , constructed by the Max Planck Institut f r Extraterrestrische Physik. ... An effective slit width of 0.1" was chosen in order to probe to spatial scales approaching the 0.07" diffraction-limited image core size expected from the Gemini adaptive optics system at 2.2 microns while maintaining an acceptable field-of-view. ... The field mirror array then feeds the spectrograph collimator mirror (seen at left in the above figure). ...

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Fermi arxiv: 1007.4556 : Ilias Cholis Jo Bovy CCPP, NYU HEA, , 2010 Spherical harmonics of gamma-rays and DM annihilation Dmitry Malyshev, NYU Motivation DM annihilation at high latitudes is a large scale small amplitude signal: ``Fourier transform'' is a tool of choice for such signals Advantages of spherical harmonics decomposition for large scale structure searches: 1. ... Spherical harmonics are a natural choice for fitting the large scale structures in gamma-rays. ...

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Astrophotography Forum Message . ... The resolution of a CCD camera does not depend on the number of pixels in the camera, rather it depends on the size of the pixels making up the chip and the focal length of the lens forming the image. ... A larger chip made from the same substrate will have identical pixel sizes, just more of them. ... With a fixed focal length telescope we don't have that luxury, in which case smaller pixel size rather than larger chip size is the only way to increase resolution. ...

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... Recognition of Anomalous Events S. Monai 1,2 and F.Pasian 2 1 Osservatorio Astronomico di Brera Merate, Italy 2 Osservatorio Astronomico di Trieste, Italy Abstract. We present an original algorithm for the recognition of anomalous events in a CCD frame (i.e., cosmic hits, bad pixels etc.) ... Raw images, as read from a CCD, are often a#ected by some events which are revealed by anomalous pixel values, i.e., single saturated pixels or pixels at zero intensity (also named hot or bad pixels). ...

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• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)
• TRAXY (V0.4) --- Dec99 --- TRAXY (V0.4)
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... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

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SLAC Jan 2004 CCD Radiation Damage Studies J. Brau, O. Igonkina , N. Sinev, C. Potter (University of Oregon) January 9, 2004 Outline: Ї Introduction Ї Neutron and Electron irradiation Ї Study of SLD VXD3 Ї Measurement of the trap filling time Ї Conclusions O. Igonkina for U.Oregon CCD Radiation Damage Studies 1 SLAC Jan 2004 CCD The ... But is it radiation tolerant? ... The study is to be continued O. Igonkina for U.Oregon CCD Radiation Damage Studies 12 ...

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... Exit Sub End If ' First argument is the FITS file to read filename = WScript.Arguments.Item(0) ' Create the ASCOM FITS driver object Set image = CreateObject( FITS. Image ) ' Read the file from disk WScript.Echo Reading filename ... image .ReadFromFile filename WScript.Echo ...done ' Read image dimensions WScript.Echo WScript.Echo ...

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... were entered in the atlas. ... In so doing lines were selected which yielded radial velocities close to the symbiotic velocity of MWC 560 (+35 km/s). ... The visible spectrum of MWC 560 is poor in absorption lines especially near the brightness maximum. In our atlas are visible only the blue-shifted components of , , NaI and FeII(42), interstellar lines NaI, a few diffuse interstellar bands (DIB) and telluric lines of and and, at length, traces of the spectra of the M giant. ...

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MESSENGER s First Day . ... Credit Copyright: NASA / JHU APL / CIW Explanation: One solar day on a planet is the length of time from noon to noon. ... On Mercury a solar day is about 176 Earth days long. And during its first Mercury solar day in orbit the MESSENGER spacecraft has imaged nearly the entire surface of the innermost planet to generate a global monochrome map at 250 meters per pixel resolution and a 1 kilometer per pixel resolution color map. ... NASA Official: Jay Norris. ...

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... Earth is the tiny spot between Jupiter and the Sun). ... Distance Radius Mass Name Orbits (000 km) (km) (kg) --------- ------- -------- ------- ------- Sun 697000 1.99e30 Jupiter Sun 778000 71492 1.90e27 Saturn Sun 1429000 60268 5.69e26 Uranus Sun 2870990 25559 8.69e25 * Neptune Sun 4504300 24764 1.02e26 * Earth Sun 149600 6378 5.98e24 Venus Sun 108200 6052 4.87e24 Mars Sun 227940 3398 6.42e23 Ganymede Jupiter 1070 2631 1.48e23 + Titan ... Extrema .. ...

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APRIL, 2005 . ... MAY, 2005 . ... JUNE, 2005 . ... AUGUST, 2005 . ... SEPTEMBER, 2005 . ... OCTOBER, 2005 . ... NOVEMBER, 2005 . ... Head of homepage . Data archive . ...

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... The described algorithm is suitable for measurements of complex images of stars. ... a) the zero-based number of stars in the complex (multicentric) image, . b) set of preliminary coordinates - x i , y i , for all stars, index i is number of a star, . ... i - index of a star in the complex image; . ... These parameters are calculated by a nonlinear method of a least squares.The main output parameters of this algorithm are x i , y i ; where the index i is number of a star in the multicentric image. ...

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... Цифровая астрономическая камера DSI II (цветная) . ... 1.25" окулярная посадка . ... Камера Meade DSI II претерпела принципиальное изменение - новая CCD матрица высокой чувствительности с пониженным уровнем шума, что чрезвычайно важно для астрофотографии объектов предельной яркости. ... Цифровая камера DSI II . ... Вентилятор для цифровой астрономической камеры DSI . ... Зеркальные цифровые фотоаппараты PENTAX . ... Copyright PENTAR ©2004-2016. (бинокли, цифровые фотоаппараты, телескопы) . ...

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MSU-E data examples. ... MSU-E . ... 16/03/1995 10:40 Msk . Pseudo-colour image. Red - channel 3, Green - channel 2, Blue -channel 1 . scale of projection 40 m/pixel . ... True-color image (786486K) . ... Channel 4 . ...

39. Equipment - Page 4

40. http://www.puldb.ru/nikolaev_2011/PUB_NIKOLAEV_2011/mu.pdf