Download Izmccd (~2.7 MB). Solution of problems at identification of star field. ... 2) Scale is not correct. ... In this case algorithm of identification will revise all values of scale from twice smaller up to twice greater. ... There should be more than value of the field "Number of stars in frame". ... The star field is considered identified if number of the identified stars more or equally to this value. It is necessary to set value from 4 up to value of field "Number of stars in frame". ...

... NASA's Hubble Space Telescope has detected a long-sought population of comets dwelling at the icy fringe of the solar system . The observation, which is the astronomical equivalent to finding the proverbial needle-in-a-haystack, bolsters proof for a primordial comet reservoir just beyond Neptune , currently the farthest planet from the Sun . ... The comet-disk lies just beyond Neptune and might stretch 500 times farther from the Sun than Earth . ... Comet Introduction Kuiper Belt Objects . ...

Large-scale wave processes in space plasma. ... G.V.Lizunov, O.P. Verkhoglyadova, and K.I. Churyumov, Plasma- beam instabilities in comatary ionospheres, Russian Astronomical Journ. ... Verkhoglyadova, O.P., V.V. Grimalsky, Propagation of ion- sound solitons in unhomogeneous plasma, Ukrainian Phys. Journ., ... Verkhoglyadova, O.P., Ivchenko, V.N., Plasma regime identification technique using magnetospheric satellite measurements, Space Sci. and Technology, 4 (5/6), 18-27 (1998) (in Ukrainian). ...

... Aug 16, 2006 LSC DetChar R. Frey 1 Aug 16, 2006 LSC DetChar R. Frey 2 a CR event A B Slow falloff (80 kHz sampling) Fast rise GPS time stamp (10 ns resolution) C D Aug 16, 2006 LSC DetChar R. Frey 3 Pulse height distributions Aug 16, 2006 LSC DetChar R ... The S5 events will be put in the LIGO data base soon (ligo light weight) · LHO considering frames insertion · LLO ?? ... Aug 16, 2006 LSC DetChar R. Frey 11 the biggest CR shower (contd) 12 ...

... indices rather than retrieve abundances: 1.2, 1.5, 2.0 µm · Work with calibrated radiances rather than relative spectra · Ad hoc atmospheric corrections Spectral index : S( ABCD) - S1 Index = S( ABCD) Correction on atmospheric absorption ·MOLA topography ·CO2: p,T ­ from European Mars Climate Database ·H2O column (Ls, ) - from TES observations ·H2O (, l, z) ­ from GFDL MGCM model ·HITRAN(2004) OMEGA DETECTOR C Wavelength,µm Errors and uncertainities ...

... Flux density at 1 GHz (/Jy): 2.9 . ... X-ray: X-ray pulsar, and extended emission from remnant. Point sources: X-ray pulsar associated with soft gamma repeater. ... Molonglo at 408 MHz (3') and Parkes 64-m at 5 GHz (4'). ... Effelsberg 100-m at 4.9 GHz (2'.6). ADS . Kulkarni & Frail 1993, Natur, 365, 33. ... 1994, ApJ, 436, L23. X-ray observations. ... VLA at 1.4 GHz (31") and 8.4 GHz (5".5) ADS . ... X-ray pulsar detection. ... 2001, ApJS, 134, 77. ... 2001, ApJ, 559, 963. ...

SINGULAR POINTS IN THE SOLAR CHROMOSPHERE . ... In the structure of the solar chromosphere, containing information on the configuration of the magnetic field, we have found and identified all the main types of the singular points ( see Fig. 1 ), which are known as inherent features of the 2-D vector field. ... The main types of the singular points are the node, the focus, the center, and the saddle. ... Singular point of the focus type in the solar chromosphere. ...

... The <HR> element is used for horizontal rules that act as dividers between sections. The SRC attribute can be used to designate a custom graphic, otherwise subclass HR with the CLASS attribute and specify the appropriate rendering with an associated style sheet. ... An SGML identifier used as the target for hypertext links or for naming particular elements in associated style sheets. ... CLASS . ... CLEAR . ... The CLEAR attribute allows you to move down unconditionally: . clear=left . ...

USING THE CORRELATION BETWEEN ISGRI SURVEY RESULTS AND OTHER CATALOGUES TO AID SOURCE IDENTIFICATION John B. Stephen, A. Malizia and L. Bassani IASF-INAF, Via P. Gobetti 101, 40129 Bologna, ITALY, E-mail: stephen@iasfbo.inaf.it ABSTRACT In order to help in the identification of INTEGRAL/ISGRI sources, we have developed a software package which allows a rapid and detailed cross-correlation to be performed between various source catalogues. ... We show below some preliminary results from this analysis. ...

... This image shows clearly the 3-D structure of this star formation region: a large cavity, created by the radiation pressure from new-born stars located in the brightest area of the image, lies within a huge cloud of dust and gas. Identified as a truly indepedent star cluster, NGC 1980 is associated with this well-studied star formation region, around the brightest star seen at the bottom of this image, Iota Ori. ...

Optical and UV Spectrophotometric Standard Stars . ... The HST project has identified six types of calibration targets essential to the good calibration of HST data: . UV spectrophotometric calibrations stars . Optical photometric and spectrophotometric calibration stars . ... ApJS, 73, 413, 1990) discuss the UV calibration of HST standards from IUE data. ... There are spectra available for 23 stars in this white dwarf flux system and the data are held in the CALSPEC data base at STScI. ...

... l - the mean galactic longitude; . ... mul - the median proper motion along galactic longitude of the stars of the OB-association, in units of 0.001 arcsec year -1 ; . dml - the estimation of mul dispersion in the OB-association, in 0.001 arcsec year -1 ; . mub - the median proper motion along galactic latitude of the stars of the OB-association, in units of 0.001 arcsec year -1 ; . dmb - the estimation of mub dispersion in the OB-association, in 0.001 arcsec year -1 ; . ...

... For massive binaries,   we assumed an initial mass ratio exponent , and obtained the total amount of both types of binary PSR with BH per Galaxy of 2 , which is in agreement with independent estimates of Narayan et al. ... The above estimate of number of bright BH+II binaries (similar to Cyg X-1), about 10 per Galaxy, yields a lower limit for the expected N(PSR+BH) 0.3 per 700 single pulsars (Figure 34 ). ... These estimates mean that PSR+BH systems may be discovered in the near future. ...

... The Solar TErrestrial RElations Observatory (STEREO) provides high cadence and high resolution images of the structure and morphology of coronal mass ejections (CMEs) in the inner heliosphere. ... MAGIC observations of MWC 656, the only known Be/BH system . ... The system has been associated with a gamma-ray flaring event detected by the AGILE satellite in July 2010. Aims: Our aim is to evaluate if the MWC 656 gamma-ray emission extends to very high energy (VHE > 100 GeV) gamma rays. ...

Astronotes Armagh Planetarium's Stellar Blog! ... Stars . ... Telescopes and Observatories . ... The majestic star-forming region in the Lagoon Nebula. The pale ring to the right is an internal reflection in the telescope.€а (Image credit: ESO/ VPHAS+/ V. Kalari and J. Vink (Armagh Observatory) . ... The 18 component images were further processed twice. ... Venu and his colleagues use images like this to identify individual young forming stars in the Lagoon Nebula and determine their ages. ...

Cost Estimating Web Site . ... 2005 NASA Cost Analysis Symposium Databases . ... World , European Communities , Other European Countries , Americas , Asia , Africa , General US , US Federal Government , US Department of Defense , Aerospace Industry , NASA , Science & Engineering Handbooks . NASA Cost Estimating Handbook 2004 , Parametric Estimating Handbook .. ... Consumer Price Index , Employment Cost Index , GDP Deflator , Import Price Index , NASA New Start Index , Producer Price Index . ...

... The algebra U (g) bears a natural filtration by the degree with respect to the generators. ... Let Z S (g) = S (g)g be the center of S (g) with respect to the Poisson bracket, and let µ g = g be a regular semisimple element. ... If µ is a regular element contained in the Cartan subalgebra h g, then h Aµ , and if µ = f is the principal nilpotent element then the subalgebra Af contains the principal nilpotent subalgebra zg (f ). ...

Microsymposium 38, MS067, 2003 (A4 format) SURVEY OF MARS CRATER TOPOGRAPHY FROM MOLA DATA. Michael G. G., European Space Agency, Research and Scientific Support Department, ESA/ESTEC, Noordwijk, The Netherlands, greg.michael@esa.int An algorithm for autonomous identification of crater centres from topography data has been improved in accuracy since [1,2] by taking account of the slope direction on the interior of the crater rim. ... References: [1] Michael G. G. (2002) Vernadsky-Brown 36, abs. ...

The AstroGuide . ... AstroGuide | ... AstroGuide Listing . Login . See many more Astronomy Listings by: Category or Alphabet . Here you can find freeware programs that help you calculate lunar occultations. Their main program is called "Lunar Occultation Workbench." ... Web Site . ... Web . ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . are trademarks of John Huggins ...