Results of calculation of O – C can be saved and printed with the help of usual means of Windows. ... Saving and printing results . It should be taken in mind that the type of extension that is actual in default of specifications is “.ocr” ( O – C results ). ... NOTE : Paper size different from A4 is not recommended: in this case the part of data can be out of print area. If printer resolution is lower then 300 dpi then problems can occur when printintig text in Portrait mode. ...

A completely new possibility of Fortran 90 is recursion. Note that it requires that you give a new property RESULT for the output variable in the function declaration. ... Here follows two examples, first recursive calculation of the factorial, then recursive calculations of the Fibonacci-numbers. ... The listings of the routines follow, the output variables are called FAC_RESULT and FIBO_RESULT , respectively. ... Not only functions but also subroutines can be recursive. ...

Next: Discussion Up: Old neutron star distribution Previous: Galactic potential . It proves to be teachful to have a look at the calculated distribution (Fig. ... The galactic z -distribution of stars and peculiar velocities slightly smear out this narrow boundary. ... The final picture (Fig. ) of the old neutron star density distribution is obviously the sum of filled equipotential lobes with different weighted with the probability shown in the Fig. ...

... 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 . ...

... These are: X14H0203T, X14H0204T, X14H0302T, X14H0303T, and X14H0304T. GEOMETRY OF THE PROBLEM In the five cases of interest, the observed GS motions are confined to the sub-dominant FGS resulting in a roll of the HST focal plane about the dominant Guide Star. ... Again, this is compatible with the explanation provided for X14H0203T. X14H0302T, X14H0303T, and X14H0304T At roughly 220 seconds into the observation X14H0302T, a disturbance resulted in a ~1.65" shift of the sub-dominant GS (see Fig. ...

... Even future mission archives tend to concentrate more on what can be extracted out of a proposal or a Guaranteed Time Observation log than the actual extracted science out of the data itself. ... A year later the data is then publicly available. An archive researcher has then to go through a mass of data to find what may be useful without any indication as to what the actual observer's results were while using the data except the proposal, which in most cases is very general. ...

Next: Bibliography Up: On the metallicities of Previous: Observations and data reduction . The results of chemical abundance determination for the studied galaxies are presented in Table 2 . The comparison of the respective data for UM 133 and UM 382 with the abundance ratios from Izotov & Thuan ([ 1999 ]) shows that they well agree with the derived average values for the sample of low metallicity BCGs. ... The full range of the velocity curve is about 100 km s -1 . ... UM 133 . ... UM 283 . ...

... The perceptron structure, on the basis of which the database is built, is defined by a number of the input and output parameters and a required accuracy. ... The output perceptron data are the expansion coefficients of the scattering matrix elements in series of the generalized spherical functions. ... As the cluster structure depends on the generation conditions the expansion coefficients were averaged over 5--7 realizations of the clusters (for N . ... is the coefficient number. ...

... OOF holography home Quick Links: . ... Scans 2002+: Aperture, Residuals, Residuals (log plot) , FITS file of the calculated phase map, ASCII file of the calculated phase map, . Scans 3001+: Aperture, Residuals, Residuals (log plot) , FITS file of the calculated phase map, ASCII file of the calculated phase map, . Scans 4001+: Aperture, Residuals, Residuals (log plot) , FITS file of the calculated phase map, ASCII file of the calculated phase map, . ... Scans 3001+: Aperture . ...

The AstroGuide . ... AstroGuide | ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . Page of Krono Branch of the Polish Amateur Astronomers Society. Info about our activity, results of latest observation and links to other Polish sities are included . ... Listed Since October 26, 2004 . ... Web Site . http://ptma-krosno.teleskopy.pl/ . ... Web . www.astronomy.net . About Astronomy Net | ... dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

. English . Russian KOI8 . Current server sed.sao.ru . Dissertation of Doctor of Sciences degree ( close to German Habilitation ) . A time to cast away stones, . and a time to gather stones together . Ecclesiastes, Ch. 3 ; 5 . Full gzipped PostScript version (in Russian) is here (2005), autoreferat (short thesis in Russian) is here . Main results of dissertation work . Continue...

. Next: *xflux, hxflux* - Calculation Up: Spectral Analysis Previous: *search_grid* - Customized grid . input file: rp90_a_grd.tab . sp> grid_plot rp90_a . Plot will appear in graphics window. With cursor in window, type = for hard copy, type q to exit from graphics mode. Fig. 7.1b. shows a sample result. rsdc@cfa.harvard.edu . 1998-06-10

APAO is a relatively new Olympiad which was founded in the spring 2005 as an international regional programme in line with the International Astronomy Olympiad. The 11 th Asian-Pacific Astronomy Olympiad (XI APAO) took place in November 2015 in Ashulia , Savar, North-West suburban area in Dhaka province , Central part of Bangladesh ). ... Theoretical and Practical rounds were held in Daffodil International University auditoriums. ... For the best result in all the rounds . ...

This source is hiding behind our Galaxy at a distance of ~18 Mpc, located at a galactic latitide of 0 degrees. ... As we look towards longer wavelengths, 60 micron, to try and penetrate the Galactic Plane, we still see confusion from galactic sources. ... If the image seems some what confusing that is because the MOST is a continuum radio telescope and when it looks in the direction of our Galaxy it detects radiation from sources within our Galaxy and from sources that may lie behind our Galaxy. ...

... Type: planetary nebula . This is one of the most complex of the planetary nebulae. The HST images seem to indicate that the central star is actually a binary system and that the nebula we see today is actually the result of at least two separate events. See the NASA press release for more info. HST 112k gif . HST 26k jpg . HST 1000k tiff . ... HST 142k gif . HST 40k jpg . HST 555k tiff . BB 5k jpg . ...

Next: References Up: On the problem of Previous: The spectrograph design and . Figure: Fragment of the echelle spectrum of protoplanetary nebula RAFGL 618 in H . In Fig. 3 are shown fragments of the echelle spectra of the quasar S5 0014+81 ( ) obtained with the PF echelle spectrograph within the frames of the programme of study of absorption spectra of bright quasars (authors of the programme are D.A.Varshalovich and A.V.Ivanchik). ...

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . Brief History of Rocket and Space Technology . ... Project History . ISS Russian Segment . Steps of ISS Assembly . ... ISS 45/46 . ... The crew training without the actual science hardware before the first session of operation with this science hardware (for which there is a virtual manual) with a log file generated; . ... HISTORY . ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

Arecibo Galaxy Environment Survey (AGES) The M74 group is a gas-rich galaxy group located at roughly 10 Mpc and is similar in makeup to the Local Group. M74 dominates the surrounding region and is accompanied by several dwarf galaxies, some of which are star-forming. ... We have decided upon a drift mapping approach to scan the entire region. We have defined 5 constant declination scans 5 in length, separated by approximately one full ALFA footprint. ... START TIME (AST) . END TIME (AST) . ...

THE PHOTOMETRIC RESEARCHS OF THE MERCURY'S SURFACE BY MEANS OF DIGITAL MODELS. ... The surface brightness of Mercury was measured Danjon (1933, 1949, 1953) and Harris (1961) in phase angle 3o-123o. The analysis of the various data of the integral photometric gives the results of determination of the main photometric constants for Mercury. ... THE PHOTOMETRIC RESEARCHS OF THE MERCURY'S SURFACE: S.G. Pugacheva The surface brightness of the Mercurian images was established on the geologic map Mercury. ...

Full-Text Search . ... astro-ph . ... SAI VO . Search sort results by Date Relevance . ... Whitespace-separated words are treated as AND ed. Show 10 50 100 articles per page in Full Compact mode . Normalized to: Branch, M. 1 article(s) in total . ... Bessoff, Aaron. Corley, Richard. ... Elston, Richard. Eriksen, John-David. ... Gonzalez, Anthony H.. ... Hon, David. Julian, Jeff. Julian, Roger. ... Rashkin, David. ... SAI MSU . ...