Next: Column COOLING Up: Detectors Previous: Column DET . The spectral responsivity of a photomultiplier depends on the photocathode composition, the window composition, and the mode of illumination (i.e., from the vacuum side or the substrate side). ... The estimated value of the dead-time parameter itself, in seconds, goes in a Real*4 column called DEADTIME, and the uncertainty of the dead-time parameter, again in seconds, goes in a Real*4 column called DEADTIMEERROR. ...

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The efficiency of interaction of radiation with a particle and hence its optical properties depend on the particle chemical composition, size, shape, structure, etc. ... Particle size expressed in units of the wavelength of incident radiation, together with chemical composition, most strongly affects the optical properties of a scatterer. ... There are many methods to solve the light-scattering problem for a homogeneous spheroid (our survey of the light-scattering methods see here ). ...

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We model the spectral chanages of late oxygen-rich Miras observed in different pulsation phases. From a combination of variable near-IR spectra and UKIRT spectrophotometry of the 9.7 \mu m silicate dust emission feature in different phases we study the influence of the changing atmospherical circumstances on the conditions in the circumstellar dust shell. ... A comparision with the modelling results for another long period Mira U Ori is also provided. ...

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• http://star.arm.ac.uk/~csj/papers/abstracts/sdbb.abstract
• Influence of Climate Variables on Tree-Ring Widths of Different Species
• Armagh Observatory

... In spite of the good potential possibilities, some of the station "Dnepr" design characteristics did not allow us to apply the usual special IS radar measurement methods. ... Thus for IS signal measurements at the "Dnepr" station, we have developed special methods for recording and processing IS signals in order to determine plasma ionospheric parameters. ... Equations (4-5) from the basis for data post processing to obtain ionosphere parameters. ...

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• East Siberian Center for the Earth's Ionosphere Research. Modelling, secondary

Name: PGSCF Purpose: set character font Category: GRAPHICS File: pgplot.src Author: T.J. Pearson Use: see description below. Description: SUBROUTINE PGSCF (FONT) INTEGER FONT Set the Character Font for subsequent text plotting. Four different fonts are available: 1: (default) a simple single-stroke font ("normal" font) 2: roman font 3: italic font 4: script font This call determines which font is in effect at the beginning of each text string. ...

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• http://www.atnf.csiro.au/vlbi/dokuwiki/lib/exe/fetch.php/difx/socorro2010/20101109_complex_sampling.pdf
• Selection effects
• Keyin Free-format Input

Detection technique . We are using ISIS , the optimal image subtraction method developed by C. Alard & R.H. Lupton, to search for SNe in our images. ... The second image shows the same subtraction, but after the convolution of the best image with ISIS: . ... For this reason, we are suggested to search for nuclear SNe with NICMOS on HST, to exploit its stable PSF, sensitivity and angular resolution to detect from space nuclear obscured SNe which might have been missed by ground-based surveys. ...

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• IBIS - Flat Fielding

... Product details: . ... 2 Composition/Data on components: . ... Information pertaining to particular dangers for man and environment . ... 4 First aid measures . ... Use fire fighting measures that suit the surrounding fire. ... Measures for environmental protection: . ... This information is furnished without warranty, and any use of the product not in conformance with this Material Safety Data Sheet, or in combination with any other product or process, is the responsibility of the user. ...

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• Laboratory for Spectroscopy of Molecular Structures
• SPECIALITY 01.04.07 - CONDENSED MATTER PHYSICS SUPPLEMENTARY PROGRAM

... The variability of the spectrum of the optical component of the IR-source IRAS01005+7910 was discovered for the first time in the BTA spectra [1]. ... The spectral features include absorptions that form in near-photospheric layers, narrow envelope emissions, and emission-absorption profiles that form in photosphere-to-envelope transition layers (the wind). ... Discovery of spectral variation in the optical counterpart of IRAS01005+7910. ... Dashed line - envelope curve of all the SiII 5979 profiles ...

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• important11-15_en

To main of Laboratory . The research work and design of optical and optical-electronic devices are carries out by laboratory staff: . ... Lens: . ... In the layout 1 prism systems perform functions of dispersive element, corrector of aberrations, optical reducer. ... Spectral range 200 - 400 nm; . ... Back Forward . ... The main corrector's function are compensation of field aberrations of the main spherical mirror of a telescope (diameter of 600 mm, f'=1200 mm) and increase aperture ratio. ...

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The beam pattern and the polarization characteristics . of the radio telescope RATAN-600 . The Mueller matrix elements was computed via formulas [1]: . ... The BP were computed by the aperture method, proceeding from the fild distribution in the aperture of the primary mirror. The components of the main and cross-polarization components of the electric field in the vertical aperture of the primary mirror was computed in Frenel diffraction approximation. ...

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• Determination of atmospheric parameters and calculation of chemical composition
• Laboratory for the Stellar Magnetism Study of SAO of the RAS - Home
• Spectral energy distribution

Next: Other People's Software . ... Quality system management of computer workstations for astronomy can be achieved with relatively small manpower requirements, if the right cost-effective administrative design decisions are made. ... This is all done with essentially one system manager. ... The system is designed so that one doesn't depend on four or more hosts, (such as a software server, cpu server, data file server, font server, etc.) to get work done. ...

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• Simulation of HST PSFs using Tiny Tim
• Towards Optimal Analysis of HST Crowded Stellar Fields
• Using Massively Parallel Processing of a NLTE Spectrum Synthetic Code and an

Atmospheric influence on the different radio-engineering system functioning . ESTIMATION OF ATMOSPHERIC OPTICAL CHARACTERISTICS AND REMOTELY SANSED IMAGE CORRECTION . ... Direct transmittance estimation results for 12 channels of the spectrometer CHRIS. ... We have managed to develop a direct method of estimating the discrete Normalized Atmospheric Point Spread Function (NAPSF) from available images alone, not using any external sources of information about the atmosphere. ... IRE RAS 1996-20 11 ...

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• Project 8 - RFBR - Dynamical and non-equilibrium electron transport and

Star Formation in HI-Selected Galaxies Jessica Rosenber George Mason University AKARI Arecibo Today s Technology Spitzer The Next Generation SKA ALMA JWST Herschel Questions to address by studying SF in HIselected galaxies · What is the best way to measure SF in galaxies that, in some cases, may be metal poor · What is the SF rate density in the local universe? ... How does SF efficiency vary with galaxy mass? ... ADBS Not a star an ultra compact star forming dwarf galaxy! ...

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• http://www.naic.edu/~astro/frontiers/vlbi.pdf
• http://www.naic.edu/~phil/rfi/fm/fcc_73.317_fmstations.pdf
• http://www.naic.edu/~astro/aotms/performance/Antenna-loss.pdf

... Early studies of PMS stars focused on T associations, especially Taurus-Auriga. However, one might expect low mass star formation to be different in OB associations. ... He identified Orion OB1a as the stars northwest of the belt. Orion OB1b is composed of the stars near the belt, including the belt stars and Orionis. ... He finds no perceptible distance change within the Orion OB1b association and finds the distance modulus to be 7.8 and 7.9 for Orion OB1a and OB1b respectively. ...

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• Rapidly Rotating Stars
• The AstroStat Slog effective area
• Quantum Efficiency Correction (a.k.a. `flat-fielding')

These observations are aimed at fully charactering FORS1 photometric system (UBVRI zero-points, color-terms and extinction coefficients) for the Tektronix 2048x2048 pixel CCD (24µm px) . To this aim, the two Landolt/Stetson photometric fields SA95 and SA101 will be observed on a number of epochs and at different airmasses during February and March 2007. ... SA101 . ... OBs for SA101 have to be observed during evenigh twilight (exceptions are expected for the second half of March) . ...

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• Effective temperatures
• Colours and magnitudes
• The Effect of Continuum Variability on Spectral Indices

... As with all tutorials, this document describes detailed steps to just one particular effect. ... Create a new Greyscale image, and put some text in it. ... Duplicate U1, then run Gaussian blur 5.00. ... Then, invert the image so it is white on black. ... Multiply U2 and U3. ... Invert U1, so it is white text on black background. ... Then run Gaussian Blur 4.00. ... If you like you can multiply this by a texture, for a textured background, but for this tutorial the background is white. ...

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• APOD: 2004 November 30 - Lake Effect Snow on Earth
• APOD: 2011 April 18 - Visual Effects: Wonders of the Universe
• APOD: 2015 December 6 - A Force from Empty Space: The Casimir Effect

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. ...

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• http://selena.sai.msu.ru/San/Publications/m44_56_leikin_sanovich.pdf
• http://selena.sai.msu.ru/Pug/Publications/ms42/m42_60.pdf
• http://selena.sai.msu.ru/Bus/Publications/m44_14_busarev_etal.pdf

... Tsupko Gravitational Lensing in Plasmic Medium Plasma Physics Reports, 2015, Vol. ... 562­581 The influence of plasma on different effects of gravitational lensing is reviewed. Using the Hamiltonian approach for geometrical optics in a medium in the presence of gravity, an exact formula for the photon deflection angle by a black hole (or another body with a Schwarzschild metric) embedded in plasma with a spherically symmetric density distribution is derived. ...

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• Cosmic rays [Oulu]
• DIGITAL WDC EXCHANGE FORMAT FOR OBSERVATORY 1.0 MINUTE VALUES
• The Triad Spacecraft

Astronomy Picture of the Day . ... The different colors of this planetary nebula are determined by small differences in its composition. This bipolar nebula will continue to shine brightly for only a few thousand more years, after which its central star will fade and become a white dwarf star. ... Publications with keywords: bipolar - planetary nebula - butterfly nebula . Publications with words: bipolar - planetary nebula - butterfly nebula . ... NGC 3132: The Eight Burst Nebula . ...

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• Journal "Peremennye Zvezdy"
• A Colorful Lunar Corona
• PG 1115+080: A Gravitational Cloverleaf

... I normally begin by asking the class what they think would be different if the Moon didn't exist, or if the Sun were closer to Earth, or if a star exploded nearby. ... The winds would be much stronger. ... In using what-if questions in the classroom, it is worth bearing in mind that students extrapolating the effects of new scenarios will encounter two different situations: direct changes to the new version of Earth and indirect changes resulting from the direct changes. ...

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• ASP: Using Multicultural Dimensions to Teach Astronomy
• ASP: A Taste of Real Astronomy ? The ESA/ESO Astronomy Exercises
• ASP's 2012 Annual Meeting