... This effect is visible in Figure 4.3 which shows a logarithmic stretch of the image resulting from a 100s exposure on a star of V magnitude 2.6 through filter F502N in the PC. Extreme overexposure of the Loral CCDs is not believed to cause any permanent effects, and therefore the WFPC2 does not have a bright object limit. ... Several other artifacts that are common in saturated stellar images are also obvious in Figure 4.3 . ... Figure 4.3: Saturated Stellar Image Showing Horizontal Smearing. ...

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... Following a micrometeoritic impact in Rev.#961 (March 2005), a new hot column appeared, whose effects leak across the whole column RAWX=318 . While a correction for this hot column is possible and implemented for MOS1 exposures taken in Imaging Mode, the offset value in MOS1 exposures taken in Timing Mode is too high for any meaningful correction to be possible. ... mos1.evt is the name of the MOS1 event list . ... RAWX in [320:329])" . ... Calculate the effective area due to the excised columns . ...

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• Effects to be Considered
• Files and columns
• Intrinsic dispersion

... This section describes three functions which have been created to cleanup defects in images. The first two functions for cleaning rows and columns are particularly useful for CCD--images. ... These can often be removed with the commands: MODIFY/COLUMN INPUT OUTPUT [C or V] [columns] . ... This is particularly useful for removing the permanent defects which may exist in the CCD--frames and which cannot be removed by the MODIFY/COLUMN or MODIFY/ROW commands. ...

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• Column NDVALUE
• Column label: TUBELEN
• Permanent telescope parameters

... SiD workshop, Fermilab, April 9-11 2007 April 9, 2007 Nick Sinev, SiD design Workshop, Fermilab 1 Topics 1. ... What and how was simulated What and was One column clusters effects Accepted background density Hit reconstruction efficiency Hit efficiency How to improve efficiency Conclusions April 9, 2007 Nick Sinev, SiD design Workshop, Fermilab 2 What is this April 9, 2007 Nick Sinev, SiD design Workshop, Fermilab 3 Marty's idea Shift charge in neighboring columns in opposite directions. ...

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• The Greenhouse Effect.

... Bojan Nikolic web pages (r. 329) . ... Since version 0.12, libAIR comes with a simple command line interface to the routines which retrieve the water vapour and the phase correction coefficient. Currently only the very simplest model is supported, in which the all of pressure, temperature and water vapour column are free parameters, and they are inferred from the four observed water vapour radiometer readings. ... Command line interface to libAIR and water vapour column retrieval . ...

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• Introduction to phase correction for ALMA Bojan Nikolic web pages (r. 329)
• Bojan Nikolic -- Turbulent 3d fields and bnlib-1.3
• ALMA Phase Calibration Techniques at the Cavendish Astrophysics Group

... Imagine that for every pixel in the color image, you take its luminance value (that's how bright it appears). ... In the end, you will have a histogram which counts how many times each luminance value appears in the image (that histogram can be used to analyze the distribution of the luminance values in the image). ... For the watermark effect, we want to use the same value that we used in the Stretch Contrast step, so that the lightest color will be in fact white (255), and nothing will get clamped...

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• APOD: 2004 November 30 - Lake Effect Snow on Earth
• APOD: 2011 April 18 - Visual Effects: Wonders of the Universe
• GIMP Effect: Tiles

... Posts tagged ?Sunyaev-Zel?dovich effect? ... A fast Bayesian approach to discrete object detection in astronomical datasets ? ... ArXiv] A fast Bayesian object detection? ... Comment . ... Entries RSS . Comments RSS . ... Algorithms arXiv Astro Bad AstroStat Bayesian CHASC Cross-Cultural Data Processing Fitting Frequentist Galaxies gamma-ray High-Energy Imaging Jargon Job Languages MC MCMC Meta Methods Misc News Nuggets Objects Optical Physics Quotes Spectral Stars Stat Timing Uncertainty X-ray . ...

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• The AstroStat Slog positional citation effect
• The AstroStat Slog effective area
• Evolutionary Effects

Next: The Browne & March? Up: THE DEEP X-RAY RADIO Previous: BL Lacs . Several effects may bias samples of blazars, causing them to miss objects which fall within their survey area and flux limits. ... It is safe to say that there is probably no survey which is completely immune from selection effects. The impact of selection effects upon most previous surveys is not known, but must be understood to make progress towards better understanding the AGN phenomenon. ... The Browne & March? ...

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• The Browne & March? Effect
• The Effect of Continuum Variability on Spectral Indices
• Effective temperatures

... Obviously, the size of the cavern is of the order of the Schwartzman radius. ... Thus, consideration of the inverse effect of pulsar radiation on the properties of accreting plasma makes the ejection possible even when the Schwartzman radius is smaller than the capture radius. ... If the cavern radius , the condition at its boundary can be written as . ... Apart from magnetic dipole radiation, the cavern may also contain relativistic particles (which are also reflected from the cavern boundary). ...

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• The ``Reflection'' Effect
• Effect of sources evolution on
• The Effect of Kick Velocity on Binary Pulsar Populations

... In this talk, I will discuss a study of the effect of ionization on the low end of HI mass function. The existence of a large population of low mass galaxies follows from CDM theory. ... HIDEEP found no low HI column density galaxies. One possible explanation is that the disks are "frozen". ... We assume that galaxies are exposed to an ionizing background radiation, from a uniform quasar distribution. ... We find a gap in the average column densities around N H which drops to 10 17 cm -2 . ...

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• The Analysis

... The improvement will be more pronounced in our crowded Wide Field Camera (WFC) images, and may be increased further through use of a more sophisticated method of combining the individual dithered images. Our analysis allows us to check for point spread function shape variations in the HST Planetary Camera (PC) field. ... In crowded field images, we are deriving information about the faint end of the luminosity function (LF) from the texture of the image background. ...

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• Simulation of HST PSFs using Tiny Tim
• ADASS 2002 Conference Proceedings
• A New PROS Task for Calculating HRI Source Intensities or Upper Limits

. The Doppler Effect . Spectroscopy . Wavelengths . The Electromagnetic Spectrum . Spectrographs . PPT Slide . What’s this got to do with velocities? . The Doppler Effect: . How does this affect the spectra? . The Maths . Example. Author: Paul Francis . Email: pfrancis@mso.anu.edu.au . Home Page: http://msowww.anu.edu.au/~pfrancis/astr1001/ . Other information: . Course Notes for ASTR1001 Astronomy

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• The Doppler Effect:
• Filter Throughput Curves
• Gemini Near-Infrared Integral-Field Spectrograph (NIFS) Diffraction.

previous next contents properties index . Contents . 11.1 Overflow and clipping . 11.1.1 Overflow: the 'overflow' property . ... Generally, the content of a block box is confined to the content edges of the box. ... This may happen when an element's 'width' property has a value that causes the generated block box to spill over sides of the containing block. ... Specifying a small clipping region may cause clipping of otherwise visible contents. 'overflow' . Value: . ... visual . ...

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• Long description of example illustrating hidden internal borders
• Long description of example illustrating the separated borders model
• Long description of example illustrating rows separated by a border

... Doppler effect . Apply to both rotational and orbital periods . Any line-of-sight acceleration contributes to . ... Important for many msp ages and B fields . Differential Galactic rotation . Vertical acceleration in Galactic potential . Accelerations in Globular cluster potentials . Changes in apparent semi-major axis . Gravitational lensing in binaries . Gravitational redshift . ... Thu Dec 19 15:15:11 GMT 1996 ...

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• casacore: casa::MSSpectralWindowEnums Class Reference
• Selection effects
• Orientation and Evolutionary Effects in Active Galactic Nuclei

... A Force from Empty Space: The Casimir Effect . ... Measuring slightly over one tenth of a millimeter, the ball moves toward a smooth plate in response to energy fluctuations in the vacuum of empty space. ... The form and genesis of dark energy is almost completely unknown, but postulated as related to vacuum fluctuations similar to the Casimir Effect but generated somehow by space itself . ... Publications with keywords: Casimir effect - dark energy . ... Distant Supernova Dark Energy ...

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... Terraforming . Terraforming Information Pages http://www.users.globalnet.co.uk/~mfogg/index.htm . A superb source of information on terraforming by Martyn J. Fogg . ... Mars Colonization . Mars Millennium Project http://www.mars2030.net . ... Mars Project Phase One http://marsproject.com/ . ... The Mars Society http://www.marssociety.org/ . An information source to be sure, but the direct aim of the Society is to further the work to colonize Mars. << previous page | ...

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• ASP: Simple Effective Education and Dissemination (SEED) Grants For Astronomy
• ASP: AstroCappella - A Musical Exploration of the Universe
• ASP: Sharing the Universe

... Tonight's Sky . ... The Magazine . ... Observing . ... Magazine . ... Gravitational wave search provides insights into galaxy evolution and mergers . ... galaxies . ... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... Astronomy for Kids . ... The doppelgУ?nger effect . ... Get instant access to subscriber content on Astronomy.com! ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ... Astronomy Magazine . ...

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• Effects of the eclipse | Astronomy.com
• Is it possible that the gravitational effects attributed to dark matter could
• What effect, if any, do the objects in the Kuiper Belt and Oort Cloud have on

... The behaviour of the polarization efficiency (see Eq. ( 14 )) for non-absorbing and absorbing spheroids is shown in Fig. 11 for the case when a maximum polarization is expected (PF alignment, ). ... Figure 11: Polarization efficiency against for prolate and oblate spheroids with and , picket fence orientation, . The size/shape effects are illustrated. ... Figure: Polarization efficiency as a function of particle equivolume radius for prolate core-mantle spheroids with and , PF orientation, . ...

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• Polarization properties (transmitted radiation)
• Database of Optical Properties -- Level: subsubpage
• Linear polarization: wavelength dependence

... SCIENCE AND BUSINESS . Such a trifle as a starry night sky of largest observatories turned out to be a small change coin in commercial bargains for exclusive communal services in Russia, and for a few elite flats in penthouses in Ukraine. SCIENCE AND BUREAUCRATISM . ... Till in Russian) . ... Clericalization of science and education (Till in Russian). ... Researcher of the Sternberg Astronomical Institute, The Moscow University. ... SAI home page . ... October, 2008) . ... November, 2007) . ...

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• harak_e
• Description of algorithm
• Observational data

... Abstract: We present Monte Carlo radiative transfer simulations for spiral galaxies modelled as a stellar disk and a two-phase clumpy dust distribution. ... As a general result, clumpy models are less opaque than the corresponding homogeneous models. ... 0.00 0.15 0.50 0.1 0.5 1.0 2.0 5.0 10.0 0.25 X . ... We have also produced several homogeneous models, to compare to the clumpy models. ... Homogeneous and clumpy models with the same tauV have the same dust mass. ...

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• CHIANTI atomic database
• Educator's Guide to Convection
• IBIS - Flat Fielding