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w' (wiggles) Use scale of power spectrum wiggles as standard candle ... The challenges II. Lensing measurements with shapelets ...
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Effects of shear, PSF &c analytic. Model sources as PSF elliptical galaxy: ... Size determined by Gauss fit to each source (quantized harmonically) ...
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More baryons. Potential. Density photons plasma ... baryon/photon ratio enhances peaks 1,3,5,... Strong measurement of baryon density ...
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Scientific Detectors Workshop 2005 - SDW2005AD - Taormina (Sicily) June 20-24 A summary: A) ESO Presentations B) Sicily C) Optical Detectors D) IR Detectors
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... ontwikkelingen in de astronomie, informatie technologie en instrumentele techniek samenkomen om te begrijpen hoe ons Heelal in elkaar steekt.
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OmegaCAM: The 16k x 16k Survey Camera for the VST. Calibration, Data Analysis ... Universit ts-Sternwarte M nchen: R. Bender, L. Greggio, R. H fner, U. Hopp, H. ...
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ELT Design Study Contract No 011863 ... line of sight kinematics: convolve with observational effects (errors, binaries, sampling...
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Ludovic Van Waerbeke
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Weak Gravitational Lensing by LargeScale Structure
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VO-user's desire: 'going backstage' Data quality assessment by user (talk Gilmore) ... Upper-limits, swamping by false positives, homogenizing psf-dependent ...
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Ph D. thesis Radio Investigations of Cluster of Galaxies 1976 - 1979. Notion: ... Miley. R ttgering. Venemans. Leiden 29 Nov 2001. Harry van der Laan Symposium ...
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Lecture 5. Population synthesis of NSs Sergei Popov (SAI MSU) Population synthesis in astrophysics Why PS is necessary? Tasks Two variants Examples Magnetorotational ...
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Title: OmegaCAM: The 16k x 16k Survey Camera for the VST Last modified by: Edwin A. Valentijn Document presentation format: On-screen Show Other titles
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1937 Zwicky suggested that galaxy clusters may produce observable lensing. ... 1954 Shane and Wirtanen's galaxy maps showed 'a strong tendency for clusters ...
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Universit ts-Sternwarte G ttingen: R. Harke, H. Nicklas, W. Wellem ... Proper motions (asteroids, nearby stars) Flux variations. Monitor instrument (calibration files) ...
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Inertial Effects from Companion Galaxies Driving Warps in Disk Galaxies N. F. Comins1, N. Palestini1, E. F. Borra2, R. Hohlfeld3,4,5, L. Wholly1
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Observations de la Mati re Noire Fran oise Combes Observatoire de Paris (Luminy Septembre 02) Quelques points abord s Courbes de rotation Forme g n rale de tous ...
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Some observed properties of Dark Matter: Gerry Gilmore. Institute ... dispersion profile, with assumed isotropy, and smooth functional fit to the light profile ...
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Shear Measurement Review
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The Bulge/Bar. A very complex system where a LOT is happening. ... and absolute proper motions of globular clusters in the bulge (Dinescu et al. 2003) ...
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... PI (Quinn) STECF(Benvenuti), CDS (Genova), TERAPIX (Mellier), ASTROGRID ... AVO approved with EU funds ~2 Million (total budget ~4 M ...
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Lance Miller, Catherine Heymans, Alan Heavens, Ludo Van Waerbeke. Miller et ... Measure PSF create a model convolve with PSF determine the likelihood of the fit ...
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... type & cluster age (OB ass)] b) 49 OB associations: birth ... Kick velocity. ISM distribution. Spin initial distribution, evolution and critical periods ...
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LEIDEN GRONINGEN MUNCHEN PARIS NAPLES BONN EDINBURGH CAMBRIDGE IMPERIAL. 60 b=45 30 ... Magnification. Reasonable approximations to PSF & galaxies ...
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Dynamics, abundances with Mark Wilkinson, Rosie Wyse, ... dispersion profile, with assumed isotropy, and smooth functional fit to the light profile ...
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Gradient of deflection coherent distortions of galaxy shapes ... Pixellation (=boxcar smoothing subsampling) Noise. Some of the information loss irretrievable ...
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The D_z Project or is it the Dark Energy Survey perhaps HIDEOUS TOUCAN '
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( left) Bar radius from isophote having maximum ellipticity. ( right) Bar radius derived from faintest distinct isophote. Here, r(CR)/r(bar) =1.29 /- 0.12. ...
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Reveal positions to within 1 pixel. Well-separated sources. Input catalogues rigorously with ei(e) =0. Brute-force PSF convolution, pixellation: ...
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