... We have simulated the observations of a very distant cluster of galaxies at high redshift. ... The simulations are made for the HST instruments FOC, WFPC II, and the Advanced Camera, and for an 8-m telescope on the ground equipped with adaptive optics. ... A comparison of the fields of view of post-COSTAR HST imaging instruments with the Advanced Camera (AC) and the ground-based adaptive optics camera (AO) is shown in Fig. 1 superimposed on the noise-free cluster simulation. ...

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• FUV-MAMA Repeller Off as an Available Mode for High Resolution Spectroscopy
• Roelof's Citation Statistics
• GHRS Data Handbook

... Day-by-day lines contain complete set and intended for those who have been there (I mean, in Kyoto :) . ... Large format is mainly for 1600x1200 screens and fast link (pictures are up to 150K in size). Normal is for typical 1024x768 screen (i.e. 15" monitors). ... Photos look incredible on it. ... Large . ... Normal . ... Thumbnails . ... Contents with thumbnails: Large | ... Nara, one of the historical cities of Japan . ... August 17, Sunday. ... Nara. ... return to photo album contents | ...

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• Photo album: Italy: Florence and Rome, September 1999

... Archives . ... One realization of mine during the meeting was related to a cultural difference; therefore, there is no relation to any presentations during the 212th AAS in this post. ... I cannot cover all perspectives from both disciplines but I think there are two distinct fashions in practicing normalization. $$\frac{1}{N(\theta)}\int_{\Omega} f(x;\theta)dx=1$$ . ... This is my last posting on my first AAS . Tags: AAS , measure , measure theory , normalization , PDF , pmf . ... Chandra Blog . ...

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• The AstroStat Slog Blog Archive a century ago
• The AstroStat Slog normalization
• The AstroStat Slog normal

... Observation pre-processing consists of standard bias, dark and flat-field corrections. The package provides different commands to average images, extract sub-images or normalize flat-fields. General information related to preprocessing commands is available in the section Dark, Bias and Flat-Field of SHOW/LONG and can be obtained by: . ... The command PREPARE/LONG extracts sub-images. ... The command processes a catalog by default or an image if the name is provided with the extension .bdf . ...

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• Artifacts
• File naming
• Power of test statistics

Hide Zen home . ... Extent is a shortest and non-nested sequence of words, which satisfy a query . ... We don't consider normalization of document weight to 1, since we have no global information about document collection. w{i}, len{i} - weight and length of i-th extent . ... Next - the number of unique extents. freq{i} - frequency of i-th extent . We could consider strict and soft uniqueness of an extent, depending on how do we consider the order of words in extent. ... 2 - document length . ...

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• APOD: 2005 August 8 - Mars to Appear Normal this August
• APOD: 2001 May 1 - Antarctica Hears Little Normal Matter in the Big Bang
• APOD: 2000 December 10 - Too Close to a Black Hole

... Meta Index / Home Page This section documents warnings and errors generated by this task (if any). ... error . ... No variance image was supplied, so the task has tried to use the inset as its own variance image. ... The user has set smoothstyle =`adaptive' and withuserwidths =`yes', but hasn't supplied any convolvers in userwidths . ... The user probably ought to check the output to make sure that it looks ok. corrective action: Such pixels are set to zero. negativeValuesInVarianceOutput . ...

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• How to reprocess ODFs to generate calibrated and concatenated EPIC event lists
• Generation from Ground Calibration Data
• Generation from In-Orbit Data

... They normally have 1 hz resolution. hp1: this is the LO for the rf to if1 mixing (1st lo) . hp2: this is used to generate the 2130 Mhz signal for the sband. 250 Mhz from downstairs gets added to this to generate 2380 Mhz which then drives the sband exciter. We own 3 of the hp32712 synths . ... To check our setup, we generated a birdie at 8446.231359 Mhz (with the hp83712 synth downstairs). ... hp83712 hp2 as sband synth . ... hp83712: downstairs, agc works, but only has KHz resolution . ...

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• high resolution decimation test
• CIMA Auto-Observing
• The Mock Spectrometer

... We consider stars with a constant (solar) initial chemical composition. Before the Roche lobe overflow, the components evolve as single stars (see for details LPP96). ... If the mass transfer onto a normal star occurs on a time-scale ten time shorter than the thermal Kelvin-Helmholz time for this star or a compact star is engulfed by a giant companion (e.g. as a result of the kick), the common envelope (CE) stage of the binary evolution is set in (Paczynski 1976). ...

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• Star Formation Rate and Normalization of Stellar Populations
• Why do Radiopulsars not Usually Form Pairs with Normal Stars?
• Contents

... SFIT is a general-purpose code designed to optimize theoretical stellar spectra to an observed spectrum. ... While the programme expects input from "stdio", it is more natural to save commands in a file (eg "sfit_input") and run the code simply by . ... If the spectra to be fitted have a filename "star_spectrum", then the best fit spectrum will be written out, together with the renormalized input spectrum, to a file called "star_spectrum.fit". ... sets up model spectrum grid (and for 2nd star) . ...

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• Spectrum v1 - Examples
• Armagh Observatory

... In combining the data, it is assumed that the low resolution image better represents the short spacing data, whereas the high resolution best represents the fine structure. ... Key: out The output image. ... Key: factor The flux calibration factor. ... In practise, the calibration may not be perfect, and an extra calibration factor will be required to align the flux scales. "factor" gives the factor to scale the low resolution image to put it on the same flux scale as the high resolution image. ...

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• Tools - Random numbers
• Parkes Clock Corrections for TEMPO (Outdated procedure)
• casacore: casa::Normal Class Reference

Magnetic stars, 2004, 210-211 ° Searching for the depression at 5200 A in some HgMn stars Chountonov G.A. Special Astrophysical Observatory of the Russian AS, Nizhnij Arkhyz 369167, Russia Abstract. Tens of sp ectrograms of HgMn, normal and Si stars have taned at the 1 m telescop e with a resolution of ab out 3 ° in the A ° Maitzen depressions were calculated by integration in the g 5200 A. y bands. ... It is very likely that the depression is caused by Si or rare earth elements. ...

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• Description of algorithm
• Determination of atmospheric parameters and calculation of chemical composition

... astro-ph . ... We present the goals and preliminary results of an unbiased, near-infrared, narrow-band imaging survey of the First Galactic Quadrant (10deg<l<65deg ; -1.3deg<b<+1.3deg). ... We publish 16 Doppler imaging temperature maps for the years 1994-2002 of the active RS CVn star II Peg. ... Through Doppler imaging we want to study the spot evolution of the star and in particular compare this with previous results showing a cyclic spot behaviour and persistent active longitudes. ...

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... This paper describes the main algorithms used by the Einstein Level One processing to create the exposure masks and the background maps for Einstein IPC images, and how these algorithms were recreated in the IRAF environment. Our goal was to recreate the algorithms used by the Level One Processing to create exposure masks and background maps for Einstein Image Proportional Counter (IPC) data (cf. sections 2.5 and 2.7 of Harnden et al. ...

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• Fitting and Modeling of AXAF Data with the ASC Fitting Application
• ADASS 2003 Conference Proceedings
• Wavelength Calibration at Moderately High Resolution

... MIPT Solid State Physics Department . ... Interacting Electrons in Normal Metals . ... The course is an introduction to interacting Fermi-particle physics and intended for future experimentalists. ... Hartree-Fock approximation. ... Linear reaction function. Calculation of density-density reaction function. Relation of density-density reaction function to compressibility of Fermi liquid and thermodynamic state density. ... Density-density reaction function of free Fermi gas in long-wave limit. ...

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• Department of Solid State Physics MIPT
• Laboratory of spectroscopy of defect structures ISSP RAS

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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• Usage Statistics for mail.cplire.ru - Summary by Month

... ESO Science Newsletter April 2016 . ... Follow the links or visit ESO Science Announcements to read more. ... Read more . ... The ALMA Director, on behalf of the Joint ALMA Observatory (JAO) and the partner organizations in East Asia, Europe, and North America, is pleased to announce the ALMA Cycle 4 Call for Proposals (CfP) for scientific observations to be scheduled from October 2016 to September 2017. ... Upcoming ESO or ESO-Related Workshops . ... Joint ESO, ALMA, NAOJ, NRAO Workshop. ...

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• ESO - Science Announcements
• Visiting with an Old and Active Friend (ESO PR Photos 07a-b/01)
• Different X-ray Spectra

Photon Scattering: Basic Principle of Photon Scattering . Audio Narration is available . No Scattering: Photon Source and Detector . ... For optical photons, scattering goes as wavelength to the -4 power. In the case of blue photons compared to red photons, this means that blue photons are about 10 times more likely to get scattered than red photons. ... Watch the blue photons scatter away from the detector . ... Interstellar dust make stars appear redder than they really are . ...

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• Astronomy HyperText Book: Stellar Evolution
• Summary of Friction
• Cosmological Issues for Theorists

... For the past years I have been working on the problem of synthesis of light curves of close binary systems, consisting of a normal star and a compact object (point object with fixed X-ray luminosity). ... Possible existence of a bright spot on the disk's lateral surface is taken into account. ... The last of then will be published in Gordon and Breach Publishers ( Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ... Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ...

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Modules | ... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Modules . ... Description: . User authentication using MD5 Digest Authentication. Status: . Extension . ... This module implements HTTP Digest Authentication ( RFC2617 ), and provides a more secure alternative to mod_auth_basic . ... Questions on how to manage the Apache HTTP Server should be directed at either our IRC channel, #httpd, on Freenode, or sent to our mailing lists . ...

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• VLT Unit Telescopes Named at Paranal Inauguration (ESO Press Release 06/99)
• mod_cern_meta - Apache HTTP Server
• mod_expires - Apache HTTP Server

... Satellite data ] . SMIS ] . The program is designed to process the specific AVHRR instrument data for calculation and analysis of temperature fields on the sea surface and upper level of clouds. It performs brightness correction for visible channels with regards to clouds altitude. ... The program features a wide variety of classification algorithms (including two-dimensional histogram analysis) and enables to construct personal procedures for classification. ... Back to SMIS Home Page . ...

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• XV-IMAGE