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<meta http-equiv="Content-Type" content="text/html; charset=iso-8859-1"> <body> program for <a href="http://www.iap.fr/col2004">http://www.iap.fr/col2004</a> as of 27 May 2004:<br><br> <table border="1" align="center" id=" "> <tr> <td height="20"><p align="center">9h</p> </td> <td width="150" rowspan="6" align="center" valign="middle" bgcolor="#99CCCC"><p align="center"><em>Registration</em></p></td> <td width="150" rowspan="8" bgcolor="#E9DBD8"><p align="center">R. Bond</p> <p align="center">Cosmological parameters </p></td> <td width="150" rowspan="8" bgcolor="#E9DBD8"><div align="center"> <p>F. Bernardeau</p> <p>Weak lensing in CMB / Correlation with other catalogs </p> </div></td> <td width="150" rowspan="8" bgcolor="#E9DBD8"><div align="center"> <p>B. Barreiro</p> <p>Source Extraction</p> </div></td> <td width="150" rowspan="8" bgcolor="#E9DBD8"><div align="center">P. Natoli</div> <div align="center"> <p>Map-Making </p> </div></td> </tr> <tr> <td height="20"><p align="center">9h05</p> </td> </tr> <tr> <td height="20"><p align="center">9h10</p> </td> </tr> <tr> <td height="20"><div align="center">9h15</div></td> </tr> <tr> <td height="20"><div align="center">9h20</div></td> </tr> <tr> <td height="20"><div align="center">9h25</div></td> </tr> <tr> <td height="20"><div align="center">9h30</div></td> <td width="150" rowspan="8" align="center" valign="middle" bgcolor="#E9DBD8"><p align="center">A. Liddle </p> <p align="center">Review of the theoretical bases: Inflation perturbations anisotropies polarisation Cl</p> </td> </tr> <tr> <td height="20"><div align="center">9h35</div></td> </tr> <tr> <td height="20"><div align="center">9h40</div></td> <td width="150" rowspan="5" align="center"><p>B. Lew</p> <p>An alternative way of using high redshift AGNs to constrainlocal cosmological parameters</p> <p align="center"> </p> <p align="center"> </p></td> <td width="150" rowspan="5"><div align="center"> <p>C. Baccigalupi</p> <p>Weak lensing on CMB and impact on cosmological parameters</p> </div></td> <td width="150" rowspan="5"><div align="center"> <p>M . Lopez-Caniego</p> <p>Bayesian Approach for the Detection of Compact Sources</p> </div></td> <td width="150" rowspan="5" align="center"><p>T. Souradeep</p> <p>Statistical isotropy of CMB maps : A Bipolar Spherical harmonic analysis. </p></td> </tr> <tr> <td height="20"><div align="center">9h45</div></td> </tr> <tr> <td height="20"><div align="center">9h50</div></td> </tr> <tr> <td height="20"><div align="center">9h55</div></td> </tr> <tr> <td height="20"><div align="center">10h</div></td> </tr> <tr> <td height="20"><div align="center">10h05</div></td> <td width="150" rowspan="5"><div align="center"> <p>J. Muecket</p> <p>Measuring the Mach Number of the Universe via the Sunyaev-Zeldovich Effect</p> </div></td> <td width="150" rowspan="5"><p align="center">N. Padmanabhan</p> <p align="center">Cross correlating SDSS Luminous Red Galaxies and WMAP : ISW and Lensing</p></td> <td width="150" rowspan="5"><div align="center"> <p>S. Majumdar</p> <p>Self Calibration in Upcoming SZ Cluster Surveys</p> <p> </p> </div></td> <td width="150" rowspan="8" bgcolor="#E9DBD8"><div align="center"> <p>A. Jaffe</p> <p>Cl extraction </p> </div></td> </tr> <tr> <td height="20"><div align="center">10h10</div></td> <td width="150" rowspan="5" align="center" valign="middle"><div align="center"> J-P. Uzan </div></td> </tr> <tr> <td height="20"><div align="center">10h15</div></td> </tr> <tr> <td height="20"><div align="center">10h20</div></td> </tr> <tr> <td height="20"><div align="center">10h25</div></td> </tr> <tr> <td height="20"><div align="center">10h30</div></td> <td colspan="3" rowspan="6" bgcolor="#8DAFCA"><div align="center"><em>Pause</em></div></td> </tr> <tr> <td height="20"><div align="center">10h35</div></td> <td width="150" rowspan="5" align="center" valign="middle" bgcolor="#8DAFCA"><div align="center"><em>Pause</em></div></td> </tr> <tr> <td height="20"><div align="center">10h40</div></td> </tr> <tr> <td height="20"><div align="center">10h45</div></td> <td width="150" rowspan="6" bgcolor="#8DAFCA"><div align="center"> <p><em>Pause</em></p> </div></td> </tr> <tr> <td height="20"><div align="center">10h50</div></td> </tr> <tr> <td height="20"><div align="center">10h55</div></td> </tr> <tr> <td height="20"><div align="center">11h</div></td> <td width="150" rowspan="8" align="center" valign="middle" bgcolor="#E9DBD8"><p align="center">A. Riazuelo </p> <p align="center">"Exotic" models : dark energy, cosmic defects, branes, cosmic topology</p></td> <td width="150" rowspan="5"><div align="center"> <p>D. Pogosian</p> </div></td> <td width="150" rowspan="8" bgcolor="#E9DBD8"><div align="center"> <p>R. Crittenden</p> <p>ISW Correlation with galaxy surveys</p> </div></td> <td width="150" rowspan="8" bgcolor="#E9DBD8"><div align="center"> <p>B. Guiderdoni </p> <p>IR and Radio foregrounds</p> </div></td> </tr> <tr> <td height="20"><div align="center">11h05</div></td> </tr> <tr> <td height="20"><div align="center">11h10</div></td> </tr> <tr> <td height="20"><div align="center">11h15</div></td> <td width="150" rowspan="5" align="center"><p>M. Douspis</p> <p>Initial Power Spectrum and CMB</p></td> </tr> <tr> <td height="20"><div align="center">11h20</div></td> </tr> <tr> <td height="20"><div align="center">11h25</div></td> <td width="150" rowspan="5"><div align="center"> <p> M. Kunz</p> <p>Constraints on dark energy evolution</p> <p> </p> </div></td> </tr> <tr> <td height="20"><div align="center">11h30</div></td> </tr> <tr> <td height="20"><div align="center">11h35</div></td> </tr> <tr> <td height="20"><div align="center">11h40</div></td> <td width="150" rowspan="5" align="center" valign="middle"><div align="center"> <p>M. Sakellariadou</p> <p>Constraints on Supersymmetric Grand Unified Models of Inflation from the CMB data</p> </div></td> <td width="150" rowspan="5"><div align="center"> <p>P. Fosalba</p> <p>Detection of the ISW effect</p> </div></td> <td width="150" rowspan="5"><div align="center"> <p>M. Tucci</p> <p>Limits on the detectabililty of the CMB B-mode polarization imposed by foregrounds</p> </div></td> <td width="150" rowspan="5"><div align="center"> <p>A. Slosar</p> <p>Probability distribution for quadrupole and octupole realisations from WMAP data</p> </div></td> </tr> <tr> <td height="20"><div align="center">11h45</div></td> </tr> <tr> <td height="20"><div align="center">11h50</div></td> <td width="150" rowspan="5"><div align="center"> <p>A. Aliaga</p> <p>Non-Gaussianity analysis of CMB interferometric data</p> </div></td> </tr> <tr> <td height="20"><div align="center">11h55</div></td> </tr> <tr> <td height="20"><div align="center">12h</div></td> </tr> <tr> <td height="20"><div align="center">12h05</div></td> <td width="150" rowspan="5" align="center" valign="middle"><div align="center"> <p>F. Vernizzi </p> <p>Mixed inflaton and curvaton perturbations </p> </div></td> <td width="150" rowspan="5"><div align="center"> <p>C. Hernandez-Monteagudo</p> <p>On the Hot Gas Induced Signal in WMAP's First Year Data</p> </div></td> <td width="150" rowspan="5"><div align="center"> <p>G-C. Liu </p> <p>CMB polarisation from clusters and filaments</p> <p> </p> <p> </p> </div></td> <td width="150" rowspan="5"><div align="center"> <p>B. Roukema</p> <p>A Hint of Poincaré Dodecahedral Topology in the WMAP First Year Sky Map</p> </div></td> </tr> <tr> <td height="20"><div align="center">12h10</div></td> </tr> <tr> <td height="20"><div align="center">12h15</div></td> <td width="150" rowspan="8" bgcolor="#E9DBD8"><div align="center"> <p>J. Ruhl</p> <p>SouthPole</p> </div></td> </tr> <tr> <td height="20"><div align="center">12h20</div></td> </tr> <tr> <td height="20"><div align="center">12h25</div></td> </tr> <tr> <td height="20"><div align="center">12h30</div></td> <td width="150" rowspan="8" align="center" valign="middle" bgcolor="#E9DBD8"><div align="center"> <p>S. Matarrese </p> <p>Primordial non-gaussianity </p> </div></td> <td width="150" rowspan="8" bgcolor="#E9DBD8"><div align="center"> <p>M. Strauss</p> <p>SDSS</p> </div></td> <td width="150" rowspan="8" bgcolor="#E9DBD8"><div align="center"> <p>A. Lewis</p> <p>E/B separation </p> </div></td> <td width="150" rowspan="5"><div align="center"> <p>P. Koch</p> <p>Merger influence on the thermal SZ effect: model, simulation and observation</p> </div></td> </tr> <tr> <td height="20"><div align="center">12h35</div></td> </tr> <tr> <td height="20"><div align="center">12h40</div></td> </tr> <tr> <td height="20"><div align="center">12h45</div></td> </tr> <tr> <td height="20"><div align="center">12h50</div></td> </tr> <tr> <td height="20"><div align="center">12h55</div></td> <td width="150" rowspan="3" bgcolor="#8DAFCA"><div align="center"><em>Pause</em></div></td> <td width="150" rowspan="5" align="center"><p> A. Da-Silva</p> <p>he CLEF-SSH simulation project: Modeling the SZ cluster population with radiative gas cooling and energy feedback.</p> </td> </tr> <tr> <td height="20"><div align="center">13h05</div></td> </tr> <tr> <td height="20"><div align="center">13h10</div></td> </tr> <tr> <td height="20"><div align="center">13h15</div></td> <td colspan="4" rowspan="15" align="center" valign="middle" bgcolor="#8DAFCA"><div align="center"><em>Pause</em></div></td> </tr> <tr> <td height="20"><div align="center">13h20</div></td> </tr> <tr> <td height="20"><div align="center">13h25</div></td> <td rowspan="13" align="center" valign="middle" bgcolor="#8DAFCA"><em>Pause</em></td> </tr> <tr> <td height="20"><div align="center">13h30</div></td> </tr> <tr> <td height="20"><div align="center">13h35</div></td> </tr> <tr> <td height="20"><div align="center">13h40</div></td> </tr> <tr> <td height="20"><div align="center">13h45</div></td> </tr> <tr> <td height="20"><div align="center">13h50</div></td> </tr> <tr> <td height="20"><div align="center">13h55</div></td> </tr> <tr> <td height="20"><div align="center">14h</div></td> </tr> <tr> <td height="20"><div align="center">14h05</div></td> </tr> <tr> <td height="20"><div align="center">14h10</div></td> </tr> <tr> <td height="20"><div align="center">14h15</div></td> </tr> <tr> <td height="20"><div align="center">14h20</div></td> </tr> <tr> <td height="20"><div align="center">14h25</div></td> </tr> <tr> <td height="20"><div align="center">14h30</div></td> <td width="150" rowspan="8" align="center" valign="middle" bgcolor="#E9DBD8"><div align="center"> <p>A. Kogut</p> <p>WMAP 1 </p> </div></td> <td width="150" rowspan="8" bgcolor="#E9DBD8"><div align="center"> <p>I. Tauber</p> <p>Planck </p> </div></td> <td width="150" rowspan="8" bgcolor="#E9DBD8"><div align="center"> <p>N. Sugiyama</p> <p>Reionisation: state of the art</p> </div></td> <td width="150" rowspan="8" bgcolor="#E9DBD8"><div align="center"> <p>J.-F. Cardoso</p> <p>Component separation</p> <p> </p> </div></td> <td width="150" rowspan="18" bgcolor="#E9DBD8"><div align="center"> <p>Pannel talk</p> </div></td> </tr> <tr> <td height="20"><div align="center">14h35</div></td> </tr> <tr> <td height="20"><div align="center">14h40</div></td> </tr> <tr> <td height="20"><div align="center">14h45</div></td> </tr> <tr> <td height="20"><div align="center">14h50</div></td> </tr> <tr> <td height="20"><div align="center">14h55</div></td> </tr> <tr> <td height="20"><div align="center">15h</div></td> </tr> <tr> <td height="20"><div align="center">15h05</div></td> </tr> <tr> <td height="20"><div align="center">15h10</div></td> <td width="150" rowspan="5" align="center" valign="middle"><div align="center"> <p>H. Peiris </p> <p>Can We Observe Planck/String Scale Physics via the CMB? </p> </div></td> <td width="150" rowspan="5"><div align="center"> <p>M. Tristram</p> <p>Archeops improved results on angular power spectrum</p> </div></td> <td width="150" rowspan="5"><div align="center"> <p>F. Daigne</p> <p>Pop. III star formation : reionization vs cosmic chemical evolution <br> constraints.</p> </div></td> <td width="150" rowspan="5"><div align="center"> <p>J. McEwen</p> <p>A Fast Directional Spherical Wavelet Transform with Application to CMB non-Gaussianity Detection</p> <p> </p> </div></td> </tr> <tr> <td height="20"><div align="center">15h15</div></td> </tr> <tr> <td height="20"><div align="center">15h20</div></td> </tr> <tr> <td height="20"><div align="center">15h25</div></td> </tr> <tr> <td height="20"><div align="center">15h30</div></td> </tr> <tr> <td height="20"><div align="center">15h35</div></td> <td width="150" rowspan="5" align="center" valign="middle"><div align="center"> <p>L. Pogosian </p> <p>String Renaissance?</p> </div></td> <td width="150" rowspan="5"><div align="center"> <p>A. Miller</p> <p>QUIET CMB Experiment</p> </div></td> <td width="150" rowspan="5"><div align="center"> <p>I. Iliev</p> <p>Reionization, CMB and small-scale structure</p> </div></td> <td width="150" rowspan="5"><div align="center"> <p>M. Cruz</p> <p>Is the cold spot found in the WMAP 1-year data compatible with Gaussianity?</p> <p> </p> </div></td> </tr> <tr> <td height="20"><div align="center">15h40</div></td> </tr> <tr> <td height="20"><div align="center">15h45</div></td> </tr> <tr> <td height="20"><div align="center">15h50</div></td> </tr> <tr> <td height="20"><div align="center">15h55</div></td> </tr> <tr> <td height="20"><div align="center">16h</div></td> <td colspan="5" rowspan="6" align="center" valign="middle" bgcolor="#8DAFCA"><div align="center"><em>Pause</em></div></td> </tr> <tr> <td height="20"><div align="center">16h05</div></td> </tr> <tr> <td height="20"><div align="center">16h10</div></td> </tr> <tr> <td height="20"><div align="center">16h15</div></td> </tr> <tr> <td height="20"><div align="center">16h20</div></td> </tr> <tr> <td height="20"><div align="center">16h25</div></td> </tr> <tr> <td height="20"><div align="center">16h30</div></td> <td width="150" rowspan="8" align="center" valign="middle" bgcolor="#E9DBD8"><div align="center"> <p>O. Doré </p> <p>WMAP results </p> </div></td> <td width="150" rowspan="8" bgcolor="#E9DBD8"><div align="center">K. Ganga</div></td> <td width="150" rowspan="8" bgcolor="#E9DBD8"><div align="center"> <p> </p> <p>F. Boulanger</p> <p>galactic emission</p> </div></td> <td width="150" rowspan="8" bgcolor="#E9DBD8"><div align="center"> <p> </p> </div> <div align="center"></div> <div align="center"> <p>U. Seljak</p> <p>Lyman alpha forest: state of the art</p> <p> </p> </div> <div align="center"> <p> </p> </div></td> <td width="150" rowspan="8" bgcolor="#E9DBD8"><div align="center"> <p>J. Peebles</p> <p>Conclusion and wrap-up </p> </div></td> </tr> <tr> <td height="20"><div align="center">16h35</div></td> </tr> <tr> <td height="20"><div align="center">16h40</div></td> </tr> <tr> <td height="20"><div align="center">16h45</div></td> </tr> <tr> <td height="20"><div align="center">16h50</div></td> </tr> <tr> <td height="20"><div align="center">16h55</div></td> </tr> <tr> <td height="20"><div align="center">17h</div></td> </tr> <tr> <td height="20"><div align="center">17h05</div></td> </tr> <tr> <td height="20"><div align="center">17h10</div></td> <td width="150" rowspan="5" align="center" valign="middle"><div align="center"> <p>L. Mersini-Houghton</p> <p>Observational Evidence for String Theory from CMB</p> </div></td> <td width="150" rowspan="5"><div align="center"> <p>E. Battistelli</p> <p>CMB observations from MITO</p> </div></td> <td width="150" rowspan="5"><div align="center"> <p>S. Hildebrandt</p> <p>New results on galactic anomalous microwave emission</p> <p> </p> </div></td> <td width="150" rowspan="5"><p align="center">K. Basu</p> <p align="center">CMB as a tool to probe metal enrichment and reionization</p> </td> <td width="150" rowspan="10" bgcolor="#8DAFCA"><div align="center"></div> <div align="center"></div></td> </tr> <tr> <td height="20"><div align="center">17h15</div></td> </tr> <tr> <td height="20"><div align="center">17h20</div></td> </tr> <tr> <td height="20"><div align="center">17h25</div></td> </tr> <tr> <td height="20"><div align="center">17h30</div></td> </tr> <tr> <td height="20"><div align="center">17h35</div></td> <td width="150" rowspan="5" align="center" valign="middle"><div align="center"> <p align="center">Y. Wiaux </p> <p align="center">Strong equivalence principle and CMB spectrum</p> <p> </p> </div></td> <td width="150" rowspan="5"><div align="center"> <p>R. Kneissl</p> <p>SZ cluster survey with AMI</p> </div></td> <td width="150" rowspan="5"><div align="center"> <p>H. Asareh</p> <p>Foreground contamination of the CMB anistropies </p> <p> </p> </div></td> <td width="150" rowspan="5" bgcolor="#8DAFCA"><div align="center"> <p>Visit to the Invalides </p> <p> </p> </div></td> </tr> <tr> <td height="20"><div align="center">17h40</div></td> </tr> <tr> <td height="20"><div align="center">17h45</div></td> </tr> <tr> <td height="20"><div align="center">17h50</div></td> </tr> <tr> <td height="20"><div align="center">17h55</div></td> </tr> <tr> <td height="20"><div align="center">18h</div></td> <td colspan="3" align="center" valign="middle" bgcolor="#8DAFCA"><div align="center"></div></td> <td align="center" valign="middle" bgcolor="#8DAFCA">Dinner at the Invalides </td> <td align="center" valign="middle" bgcolor="#8DAFCA"> </td> </tr> </table> </body> </html>
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Topic revision: r1 - 27 May 2004,
BoudRoukema
Cosmo
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