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1. Ultraviolet through Far-Infrared Spatially Resolved Analysis of the Recent Star
... We derive several relationships to obtain total IR luminosities from IR monochromatic fluxes, and we compare five different star formation rate (SFR) estimators for H II regions in M81 and M51: the UV, HЮБ, and three estimators based on Spitzer data. ... For the entire M81 galaxy, about 50% of the total SF is obscured by dust. ...
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Ссылки http://www.stsci.edu/~kgordon/papers/2006ApJ...648..987P.html -- 5.2 Кб -- 21.01.2016
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2. High Resolution HST Images of Pluto and Charon (ESO Press Release 09/94)
... The remote planet Pluto and its moon Charon orbit the Sun at a mean distance of almost 6,000 million kilometres, or nearly fourty times farther out than the Earth. During a recent investigation by an international group of astronomers [1], the best picture ever of Pluto and Charon [2] was secured with the European Space Agency's Faint Object Camera at the Hubble Space Telescope (HST). ... The new HST image was taken when Charon was near its maximum elongation from Pluto (0.9 arcseconds). ...
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Ссылки http://www.eso.org/~ohainaut/nice/pluto.html -- 8.5 Кб -- 18.08.2004
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3. The ISOPHOT Interactive Analysis PIA, a Calibration and Scientific Analysis...
Next: Calibration with the ISOPHOT Interactive Analysis (PIA) . ... ISO P HOT I nteractive A nalysis, PIA , is a scientific and calibration data analysis tool for ISOPHOT data reduction. The PIA software was designed both as a tool for use by the instrument team for calibration of the PHT instrument during and after the ISO mission, and as an interactive tool for ISOPHOT data analysis by general observers. ... PIA is entirely based on the Interactive Data Language IDL (IDL92). ...
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Ссылки http://www.adass.org/adass/proceedings/adass96/gabrielc1.html -- 12.8 Кб -- 23.06.1998
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4. East Siberian Center for the Earth's Ionosphere Research. Modelling, secondary
Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Although their determination is based on the scattering process model, independent check-ups by rocket experiments have shown their correctness in experimental applications. ... Ionospheric data analysis, especially during strong disturbances, cannot be without some other kinds of diagnostic tools. ... The lack of data has always been a challange in this case. ...
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Ссылки http://rp.iszf.irk.ru/esceir/isr/ismodelen.htm -- 5.9 Кб -- 04.06.2001
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5. Project Tanagra
... Kashyap, V., Drake, J., Smith, R., & Wargelin, B., 2014, 15 Years of Science with Chandra Symposium, Spectrum Ultimum Capellae: XV Years of Chandra Observations of Capella . ... Kashyap, V.L., Connors, A., Drake, J., Lee, T., Posson-Brown, J., Saar, S., Scargle, J., van Dyk, D., & Wong, R., 2014, AAS/HEAD 14, 119.05 TANAGRA: Timing Analysis of Grating Data . ... Audard, M., G del, M., Drake, J.J., & Kashyap, V.L., 2000, ApJ, 541, 396 . Audard, M., G del, M., & Guinan, E.F., 1999, ApJ, 513, L53 . ...
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Ссылки http://hea-www.harvard.edu/tanagra/ -- 15.3 Кб -- 09.04.2016
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6. http://www.gao.spb.ru/english/personal/malkin/publ/zm03d.pdf
On Systematic Differences in Individual Solutions and IERS Products Zinovy Malkin Institute of Applied Astronomy RAS, St. Petersburg, Russia 1 Present status Proper determination, modelling, and accounting for systematic differences between contributed series is of the great importance in compilation of the IERS products. ... Possible sources of systematic differences are: · Different reference systems (e.g. TRF, CRF, geopotential, time scale). ... 87 IERS Technical Note No. ...
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Ссылки http://www.gao.spb.ru/english/personal/malkin/publ/zm03d.pdf -- 27.7 Кб -- 21.05.2007
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7. Deforming Plug-plates
... The plug-plates of SDSS project are responsible for locating the optical-fiber plugs spatially and for defining the plug tilt with respect to the surface of best focus. ... Previous attempts to match the SDSS plug-plates to the surface of best focus were conducted using only the bending fixture. The analyses performed indicated that by adding a central constraint to the plug-plate deformation process, the plates could be made to match the surface of best focus within an acceptable range of error. ...
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Ссылки http://www.apo.nmsu.edu/Telescopes/SDSS/eng.papers/19961230_PlateBending/19961230.html -- 8.7 Кб -- 19.05.1998
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8. http://lnfm1.sai.msu.ru/~tempus/english/science/articles/ZotovPoster_APSG2013.pdf
... Gravity data reflect changes, related to the groundwater redistribution, ice melting, and precipitation accumulation. ... We apply Multichannel Singular Spectrum Analysis (MSSA, or extended EOF) technique to filter GRACE data and separate the principal components (PCs) of different periods. We performed data averaging over the large river basins of Russia. ... Fig 1. ... MSSA is a promising method for GRACE data processing, de-striping, filtering, and Principal Components (PCs) separation. ...
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Ссылки http://lnfm1.sai.msu.ru/~tempus/english/science/articles/ZotovPoster_APSG2013.pdf -- 1294.1 Кб -- 07.11.2013
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9. The Spectrophotometrical complex in Nasmyth-1 focus
The spectrophotometrical complex of the 6-m telescope in Nasmyth-1 focus . ... A new sample of 360 blue compact galaxies with a strong star formation was build on the base of the Second Byurakan Survey. ... More that 20 galaxies with the extremely low-abundances of heavy elements in the range of 1/30-1/10 of the Sun's one, were found. ... During the 15-years observation term near 500 spectra of the unique source SS~433, from which the relativistic jets were found for the first time, were obtained. ...
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Ссылки http://www.sao.ru/precise/Laboratory/Highlights/SFC_eng.html -- 9.0 Кб -- 09.11.2004
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10. A homogeneous chemical analysis of the inner Galactic disk from the first data
... A homogeneous chemical analysis of the inner Galactic disk from the first data release of Gaia-ESO . ... Gaia-ESO is a public spectroscopic survey designed with this goal in mind. ... These first results highlight the potential of the Gaia-ESO survey to explore areas of the Milky Way still poorly studied, such as the inner disk, and to give new constraints on Galactic chemical evolution models. ... Map of observed targets of the first data release of the Gaia-ESO Survey. ...
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Ссылки http://www.arcetri.astro.it/en/home-english/204-scientific-news/698-gaia-eso -- 27.0 Кб -- 10.04.2016
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11. Description
... flspec computes the spectrum of the background fluctuations in EPIC Imaging data in different offaxis annular regions. ... Once the 'flatfielded' image is free from detected sources, its pixels are binned according to the input parameter binsize and classified as 'positive' (if they have more counts than the median in the image) and 'negative' pixels (less counts than the median). ... The positive and negative spectra are extracted with an spectral binning of 15 eV (MOS) and 5 eV (PN). ...
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Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/flspec/node3.html -- 7.3 Кб -- 02.07.2008
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12. University of Oregon Center for High Energy Physics - ATLAS
... This precise description is called the standard model of electroweak physics. ... What brings about this important difference in the mass of these "field" particles? ... The Oregon group participates in the ATLAS experiment to investigate this question. ... Since Oregon joined ATLAS early in 2006, the group has devoted its effort to the process of selection of interesting events generated by the collisions of high energy particles within the ATLAS detector. ...
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Ссылки http://zebu.uoregon.edu/~uochep/atlas.html -- 3.5 Кб -- 20.12.2007
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13. Database of Optical Constants -- Level: welcome
The database contains references to the papers, data files and links to the Internet resources related to measurements and calculations of the optical constants in the wavelength interval from X-rays to radio domain. ... References to some useful books and reviews on the subject (e.g. the classical handbooks edited by E.D.Palik) and links to Internet collections of optical constants and personal WWW pages with related software were also placed in the database. You have arrived at our welcome page. ...
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Ссылки http://www.astro.spbu.ru/JPDOC/ -- 10.8 Кб -- 19.11.2010
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14. http://www.issp.ac.ru/journal/composites/2014/content_04_eng.pdf
... 3 2014 Композиты и наноструктуры COMPOSITES and NANOSTRUCTURES CONTENS S.T.Mileiko, N.I.Novokhatskaya, A.M.Stolin, P.M.Bazhin PRODUCING SILICIDE/MOLYBDENUM COMPOSITES BY USING INTERNAL CRYSTALLIZATION METHOD .. 185 There is shown a possibility to use the internal crystallysation method, which was developed earlier as a base for crystallisat ion of oxide fibres in a molybdenum matrix, to produce silicide/molybdenum composites. ...
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Ссылки http://www.issp.ac.ru/journal/composites/2014/content_04_eng.pdf -- 119.5 Кб -- 16.01.2015
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15. Analysis of a multiperiodic signal
Next: Transform of modulated Up: No Title Previous: Frequency/duration relation. Let us now turn to gradually more complicated signals, for which we soon lose the support of analytical expressions of the transforms. First, examine the sum of 3 cosine waves at different frequencies and phases. The Mexican hat wavelet analysis is carried out as above, yielding the wavelet map (Fig. ... Figure 11: g2 transform of a multiperiodic signal. ... Mon Nov 13 10:51:25 EST 1995 ...
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Ссылки http://crydee.sai.msu.ru/~vab/Wavelet.rsc/Tutor.dir/node11.html -- 3.1 Кб -- 12.04.1998
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16. Data and Analysis
AO Home AO Astronomy Schedule Receivers CIMA AO IDL . IDL is the recommended data-reduction package for Arecibo spectral-line data. The different back-ends produce different data format. ... Mock spectrometer standard FITS format headers . Mock spectrometer PSRFITS format headers . WAPP CIMAFITS format headers . Interim Correlator IDL headers . ... Search WAPP data . ... How to fix WAPP FITS files taken with doppler tracking in order to read them with standard FITS readers . ...
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Ссылки http://www.naic.edu/~astro/Data.shtml -- 5.1 Кб -- 09.04.2016
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17. http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/proceedings/sydney2003.pdf
... 217, 2004 Pierre-Alain Duc, Jonathan Braine and Elias Brinks, eds. On the nature of dwarf galaxies in the interacting group HCG 31 ґ Angel R. Lґpez-Sґnchez & Cґsar Esteban o a e Instituto de Astrofґ ica de Canarias, E38200, Tenerife, Spain is Mґnica Rodrґ uez o ig INAOE, Apdo. ... We show the positionvelocity diagrams in Figure 1. ... B shows a solid-body rotation pattern (Figure 1a ) that could be affected by a possible tidal streaming motion along the direction towards the A+C complex. ...
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Ссылки http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/proceedings/sydney2003.pdf -- 74.8 Кб -- 03.02.2008
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18. Atmospheric influence on the different radioengineering systems functioning.
. ATMOSPHERIC INFLUENCE ON THE DIFFERENT RADIO-ENGINEERING . SYSTEM FUNCTIONING . The calculations of the atmospheric impact on terrestrial and satellite communication links with frequencies above 10 GHz using the ITU-R data bank. The correction of the Earth cover optical images obtained from the satellite/ . The Earth atmospheric influence on the radiowave propagation parameters in wide frequency range (from SLF to UV). Contact e-mail: . Pozhidayev Victor, Ph.D - vic@cplire.ru . © IRE RAS 1996-20 11
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Ссылки http://www.cplire.ru/html/atm/index.html -- 10.3 Кб -- 18.10.2011
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19. Work Scan Program + Data Viewer (IDL widget)
For the calibration of RATAN-600 data you will need to Download Nobeyama Fluxes (1, 2, 3.75, 9.4, 17 GHz): year 1999 2000 2001 2002 2003 . Brief description of Work Scan . Main functions of processing, realized in the program are: . ... Correction of various (not fatal) defects of data; . ... Calculating of the lower enveloping curve or an average scan from observations data for a few days; . ... COMMENT This table contains the set (TFIELDS) of 1-dimensional (TFORM# . ... AZIMUTH = 'float' / . ...
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Ссылки http://mavr.sao.ru/hq/sun/software.htm -- 8.5 Кб -- 24.02.2010
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[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/sun/software.htm -- 8.5 Кб -- 24.02.2010
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[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/sun/software.htm -- 8.5 Кб -- 24.02.2010
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/sun/software.htm -- 8.5 Кб -- 24.02.2010
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20. Abstract 200
The total radiative power output from the hot outer layers of six late-type stars (of different spectral types and luminosity class) is derived via an emission measure technique. This analysis was based on observational data from the spectral range 100A to 3000A obtained as a result of three separate satellite missions, i.e. Hubble Space Telescope, International Ultraviolet Explorer and the Extreme Ultraviolet Explorer. ...
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Ссылки http://star.arm.ac.uk/~ambn/abstract200.html -- 2.3 Кб -- 15.08.1996
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Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
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