... Eric Torrence 2/12 February 2004 Phase 0 (Now) DchDigis EmcDigis EmtSim trgDC L1Accept This IS the current SP6 (14.3.X) Base simulation code unchanged, only the interface elements (Digis, TsfLUT) Eric Torrence 3/12 February 2004 Phase I DchDigis TsfSim BltSim PtdSim EmcDigis EmtSim Glt Interface GltSim Deployed Validated Written Not written L1Accept Significant upgrade to L1 Simulation Could be deployed in SP6 to improve ... Eric Torrence 12/12 February 2004 ...

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... 2011 February 22 . Star Size Comparisons . ... Explanation: How big is our Sun compared to other stars? In a dramatic and popular video featured on YouTube , the relative sizes of planets and stars are shown from smallest to largest. ... Note that the true sizes of most stars outside of the Sun and Betelgeuse are not known by direct observation, but rather inferred by measurements of their perceived brightness , temperature , and distance. ... About APOD | ...

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Armagh Observatory, 1 March 1999 . According to Armagh Observatory, the total rainfall during February amounted to 2.00 inches, slightly less than the average February figure of 2.31 inches. ... Overall the month was quite mild with an average temperature of 5.8 degrees Celsius (42.4 degrees Fahrenheit) compared with the mean February value of 4.2 degrees C (39.5 degrees F). ... FOR FURTHER INFORMATION CONTACT: John McFarland at the Armagh Observatory. ... Last Revised: 15th June 1999 . ...

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... Mass . 17a. Measuring Mass . ... A medium-size (1.25 inch wide) binder clip, as is used in offices to hold papers together--the type made of flat blue steel, with two wire handles. ... The theory predicts that the oscillation period should be proportional to the square root of the oscillating mass, including the mass of the clip. Note that gravity plays no part here: the oscillation period would be the same on the Moon or in zero-g. Denoting square root by SQRT, we have . ...

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... International workshop “The Europa Lander: science goals and experiments” is organized by the Space Research Institute (IKI) of Russian Academy of Sciences, on February 9-13, 2009, in Moscow, Russia. The workshop will last 5 days including the days of arrival/departure and some sightseeing events, and focus on the scientific goals and technical aspects of the project, key issues of Europa science with the special emphasis on astrobiology and requirements to scientific instruments. ...

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... The 7 and 15 um observations of selected fields in the Galactic Plane obtained with ISOCAM during the ISOGAL program offer an unique possibility to search for previously unknown YSOs, undetected by IRAS because of lower sensitivity or confusion problems. ... The main indications of the previous analysis are confirmed, but the criteria for selecting YSO candidates had to be revised to select only bright objects, in order to limit the contamination of the sample by Post-MS stars. ...

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... This thread uses PINTofALE to generate a simulated Chandra spectrum. ... define a DEM . ... pset marx .par ExposureTime=50000 OutputDir='sim_ marx ' \ ; GratingType='NONE' DetectorType=' ACIS-I ' SourceFlux=-1 \ ; SpectrumType='FILE' SpectrumFile='spec_ marx .dat' \ ; SourceType='POINT' DitherModel='INTERNAL' ; marx TSTART=2006.46 ; marx2fits sim_ marx / spec_ marx .evt ; dmextract infile= spec_ marx .evt[EVENTS][(x,y)=circle(4018,4141,10)] ; [bin pi=1:1024:1] outfile= spec_ ...

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... We measured these galaxies individually, and they are distinguished in our list by the suffixes a, b, c,... in order of increasing J2000 right ascension. ... The first column contains the UGC catalog number, to which we have added lower-case suffixes a, b, c,\dots in order of increasing J2000 right ascension to distinguish individual galaxies in groups. ... The third column lists the degrees, arcminutes, and arcseconds of J2000 declination plus the rms uncertainty in arcseconds. ...

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... December 21, 1997 . ... Advantages are briefly discussed of gaining in spectral resolution, which is accompanied by losses in signal level, as compared with the attempts to improve the accuracy of measurement of line parameters by means of rising the S/N ratio alone with increasing the exposure time. To partially solve the problem of observations of faint objects at the BTA a new design echelle spectrometer is proposed. high resolution spectroscopy . ...

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... This distinctive spiral-shaped sunspot caught the attention of National Solar Observatory astronomers and was photographed on February 19, 1982 with the Vacuum Solar Telescope on Kitt Peak. Sunspots appear dark only because they are relatively cool - about 4,000 degrees compared to the 6,000 degrees Celsius of the surrounding solar surface. ... A maximum in sunspot numbers occurs every 11 years with the next maximum expected around the year 2001. ... Publications with keywords: Sun - sunspot . ...

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. NATIONAL ASTRONOMY AND IONOSPHERE CENTER . NSF . UMET . SRI . USRA . Trip Advisor . Home . Science . Astronomy . Planetary . Atmospheric . Information . Visitor Center . Contact . Donate! . Description . Facilities . Exhibits . Visiting Hours . Galaxy Shop . Space Academy . 2012 . February . January . 2011 . December . November . October . тАЛScientific CommunityтАЛ тАЛ . HOME . Science . Information . Visitor Center . Contact . Disclaimer

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... Electronic Raman scattering in Tl 2 Ba 2 CuO 6+ d : Symmetry of the order parameter, oxygen doping effects, and normal-state scattering. Abstract: . Single crystals of the optimally doped, moderately and strongly overdoped high-temperature superconductor Tl 2 Ba 2 CuO 6+ d (Tl-2201) with T c = 80, 56, and 30 K, respectively, have been investigated by polarized Raman scattering. ...

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Astronotes Armagh Planetarium's Stellar Blog! ... Moon . Planets . ... Monthly Sky Notes . ... February . ... The ringed planet will be quite bright, but unlike Jupiter it will not be the brightest point of light in the sky, this accolade will return to Sirius which is the brightest star in our night sky in the constellation of Canis Major. ... Seven days later on February 18, the Moon will be in its full Moon phase. ... Tweets that mention Wonders of the February Night Sky | ... Astronotes . ...

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Successful ESO proposals an overview Bruno Leibundgut (ESO) ESO Proposals, Prague - 27 February 2009 European Southern Observatory This is the right time to start .. Call for proposal is open since yesterday (26 February ) ESO Proposals , Prague - 27 February 2009 European Southern Observatory Structure of the ESO OPC Observing Programmes Committee 4 scientific categories · Cosmology (A) · Galaxies and Active Galactic Nuclei (B) · Interstellar ...

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Proceedings of the Particle Physics and Early Universe Conference (PPEUC). For this paper: postscript PPEUC CMB index 1 Introduction.. ... Madingley Road, Cambridge CB3 0HE, U.K. CMB experiments using amplifiers cover the full range of angular scales of interest, from to , and provide constraints on the CMB power spectrum with similar sensitivity to bolometric measurements. ... 1 Introduction . ... 3 Beam-switching experiments . ... PPEUC Proceedings . ...

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... Students Life . ... Schools . University history . ... V.љN. Karazin . ... February 17, 2014 . International Winter School of High Energy Physics: Wrap-Up . An International Winter School of High Energy Physics was held at Karazin University on February 12-14, 2014. ... One of the lectures was delivered to senior pupils of Kharkiv Lyceum of Physics and Mathematics No. 27 that the University actively cooperates with. ... Scientists of the University Present the Red Book of Kharkiv Region . ...

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... Meta Index / Home Page / Some functions for testing/debugging . This function returns .true. if the given pair of values agree with each other in the given precision (order), or .false. otherwise. LOGICAL(bool) FUNCTION isNearlyEqual(cmp, compared, precision) REAL, intent(in) :: cmp, compared ! or INTEGER INTEGER, intent(in) :: precision END FUNCTION isNearlyEqual . For the pair of the first two arguments, any combination of int8 , int16 , int32 , single and double is allowed. ...

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Next: Methods for Structuring and Searching Very Large Catalogs . ... We have explored two automated classification methods: supervised classification using Artificial Neural Networks (ANN) and unsupervised classification using Self Organized Maps (SOM). These methods are used to classify IUE low-dispersion spectra of normal stars with spectral types ranging from O3 to G5. This paper describes the application of automated methods to the problem of the classification of stellar spectra. ...

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