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• ESPAC

OptInt PmWiki . MROI Fast Tip Tilt / . ... MROI Delay Line Design Contract . ... Document Management . ... Requirements . ... Design Documents . ... MROI . ... Derived Requirements Document Outline . ... Do any derived requirements depend on others? ... Conceptual Design Assumptions . ... Note that there is a top-level requirement on the pixel scale for the FLC. ... May refer to high-level features of assumed design described above in "Conceptual Design Assumptions" . Derived requirements . ...

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• OptInt PmWiki : Derived Requirements Document Outline | History
• OptInt PmWiki : MROIFastTipTilt / Derived Requirements Document Outline
• OptInt PmWiki : Derived Requirements Document Outline | Attach

. Next: Pulsar ages Up: The galactic population of Previous: The observed distribution . љ . Account for selection effects of surveys . , peak of distribution not seen . Derive Observable population . Account for beaming fraction . Total population around 500,000 . љ љ . Figure 19: The observed and derived luminosity functions. From Lyne & Graham-Smith 1990 [ 23 ]. Jon Bell . Thu Dec 19 15:15:11 GMT 1996

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• Australia Telescope National Facility
• HIPASS Bright Galaxy Catalog
• casacore: derivedmscal/DerivedMC/DerivedColumn.h File Reference

. Next: Absolute magnitudes Up: Command line procedures Previous: Limb darkening Contents . Subsections . Absolute magnitudes . Distances . Diameters . Orbital inclinations, semi-major axes, and secondary masses . Christian Hummel 2015-04-28

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• ESO - I derived quantities related to the performance of an instrument. How do
• Effective temperatures
• Absolute visual magnitudes

. [к родительской папке] . 11 марта 2006 г. 19:39 <папка> _vti_cnf . 11 марта 2006 г. 19:39 856 nortbots.htm .

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• www.schools.keldysh.ru - /sch877/_derived/
• www.schools.keldysh.ru - /sch725/_derived/_vti_cnf/
• www.schools.keldysh.ru - /sch877/_derived/_vti_cnf/

True Color Image Gallery: Galactic SNR | ... nH was derived by fitting the trail of central source which is believed not to be piled-up. nH was derived from the trail of the central source . ... Statistic value = 53.6161 . ... spectrum was refitted with nH fixed at the value derived from the trail of central source. source=(xswabs * powlaw1d) . ... shell was fitted by 3 thermal plasma model with nH fixed. source=(xswabs * ((xsraymond + xsraymond) + xsraymond)) . ... Back to SNRJ 0540.1-6919 Index . ...

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• Chandra Images for SNR J0519.5-6902
• Chandra Images for SNR J0526.0-6604
• PINTofALE EXAMPLE SESSION: via Dracia

... Determine the net instrument response desired. ... Use a numerical algorithm, the convolution network (discussed in detail below), to search for the solution that provides the desired mapping of the observed data to the desired form. ... We first made preliminary studies investigating recovery of images that have been broadened by the HST's mirror by modeling its PSF as shown in Fig. ... Our recovery procedure was applied also to spectral data, in this case to a tunable diode laser (TDL) spectrum. ...

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• L and M dwarf spectral standards
• Untitled Page
• Small Polycyclic Aromatic Hydrocarbons in the Red Rectangle

A determination of the surface gravity and an abundance analysis of helium in a sample of 17 He-rich and 5 normal, reference stars is presented. ... The helium abundances derived from the models used are very close to 0.1 for normal, reference stars are larger for the others, clearly indicating the He-rich phenomenon in them. NLTE effects, errors on the microturbulence value or on the surface gravity do not influence the estimated helium abundances. ...

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• Armagh Observatory

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 . ...

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• Optical spectroscopy
• Results and discussion
• Documentation: LEDA: parameter:

Programs to generate color spectra ================================== These programs were developed to produce realistic color spectra from digital data. ... The distribution here contains the original source code for colorspec and solar in C, and a version of solar written in Fortran. ... It will produce a color spectrum of any digital spectrum. ... The 800x50 image solarflux.ppm was generated by colorspec and the file fluxatlas.dat, a reformatted NSO Solar Flux Atlas in the data directory. ...

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• Moore Observatory's Colorspec

This service contributes to the International Service of Geomagnetic Indices (ISGI) of the IAGA . ... The Kp numbers of the previous month are available in tabular format . ... There are available also historical and current Kp and derived indices per anonoymos FTP (see below). ... U.S.A. FTP server: ftp://ftp.ngdc.noaa.gov/STP/GEOMAGNETIC_DATA/INDICES/KP_AP/ . monthly update) . ... contains the monthly Kp / ap tables in a simple text format readable for both humans and computers (*.tab). ...

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• Space Weather Dials Interpretation Guide
• Identities

... The zero point was derived in the following way: ffl Matching the OM repsonse using the measurements of BPM16274 and LBB227. ffl the zeropoints in U, B, V are set in a way that the simulations with the Vega spectrum (from ESO ftp server) matches the average brightness found in the literature which is (0.025, 0.03, 0.03) mag respectively. ffl In the UV filters the ESO Vega brightness is arbitrarily set to the U value, i.e. 0.025 mag ... The analysis comprised of the following steps: 1. ...

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• http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200102/MOS_badpix-B_Altieri.pdf
• http://xmm.vilspa.esa.es/sas/7.0.0/watchout/5.2/rgsproc.par
• http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200904/haberl-epic-cal-200904-Mallorca.pdf

Astronomy Picture of the Day . ... 20.05.1996 . ... Credit Copyright: EIT Consortium , SOHO project , ESA , NASA Explanation: Above is an image of the relatively quiet Sun made on May 18 in light emitted by ionized Helium atoms in the Solar chromosphere . ... Lockyer relied on a recently developed technique of spectroscopy , dissecting sunlight into a spectrum, and the idea that each element produces a characteristic spectral pattern of bright lines. ... May 1996 . ... The Solar Spectrum . ...

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• Journal "Peremennye Zvezdy"
• Астронет > Helios Helium

... Публикации: (1) Derived categories of quadric brations and intersections of quadrics, Advances in Mathematics, V. 218 (2008), N. 5, 1340-1369. ... 4) Derived categories of cubic fourfolds, принята к публикации в сборнике \Rationality problems" (editors F.Bogomolov and Yu.Tschinkel), Progress in Mathematics. ... 12] Derived categories of cubic fourfolds, preprint math.AG/0808.3351; to appear in \Rationality problems" (editors F.Bogomolov and Yu.Tschinkel), Progress in Mathematics. ...

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• IUM (Fall 2015)
• Labo J.-V.Poncelet: A.Kuznetsov
• Dubna-2015: M. Simon

... Helios Helium . ... Explanation: This image of the relatively quiet Sun was made using ultraviolet light emitted by ionized Helium atoms in the Solar chromosphere . Helium was first discovered in the Sun in 1868, its name fittingly derived from from the Greek word Helios, meaning Sun. ... Lockyer relied on a then recently developed technique of spectroscopy , dissecting sunlight into a spectrum, and the idea that each element produces a characteristic spectral pattern of bright lines. ...

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• APOD: May 20, 1996 - Helios Helium
• APOD: 2001 January 20 - Helios Helium
• Astronomical Names

TWO IMPORTANT ISSUES FOR FFT SPECTROMETERS June 28, 2003 Carl Heiles ABSTRACT We discuss two important issues for power spectra derived from FFTing a time series. These are weighting, which eliminates spectral leakage, and \overlapping the chunks", which eliminates the nonessential increased variance that results from dividing the time series into chunks. ... We have M consecutive chunks of N-point time series, so that we have a continuous time series of length NM with no gaps. ...

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• ALFA Performance at 1665 MHz
• ALFA performance at 1.665 GHz AO Technical Memo 2004-01
• HI Mass Function

... the radiative transfer equation (RTE) for the randomly-irregular magnetized plasma has been derived on the base of general grounds of the multiple scattering theory . ... Solutions of several absolute tasks of the scattering theory have been obtained (on the optical depth of the ionospheric plasma layer, on the value of radio wave anomalous attenuation, on anomalous refraction, on the backscattered signal intensity for the source being placed within a plasma layer). ...

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• Vladimir Marsakov Abstracts
• F-stars in galactic disk, figures

... The MIDAS Data Organizer, a customizable utility to analyze and identify associations in a database of astronomical observations, is described. ... On-line Data Reduction: . ... The main characteristics of the on-line implementation of the DO at the ESO New Technology Telescope (NTT) are described below. The database for all operations is a MIDAS (ESO-IPG 1993) table, the so-called Observation Summary Table (OST) which contains all relevant parameters extracted from the FITS keywords. ...

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• ADASS 2002 Conference Proceedings
• SVDFIT: An IRAF Task for Eigenvector Sky Subtraction
• ASC Data Structures and Model

.

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• Lecture XVI.

... Constraints on cosmic silicates. ... Optical constants: . O-deficient circumstellar silicate . ... The optical constants of the O-deficient silicate were derived from [C abs (lambda)/V] (C abs and V are the cross-section and volume of grains) derived from observational data using Kramers-Kronig relation and some assumptions on the size and shape distributions of grains. ... The optical constants of the O-rich silicate were obtained in a similar but more complex way. Back to silicate page . ...

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• Amorphous magnesium silicate
• Cylinders
• Database of Optical Properties