ROE - JSPS Workshop 2007 Programme
ROE - JSPS Workshop 2007 Abstract booklet
| Time | Title | Speaker | Talk |
|---|---|---|---|
| Wednesday 24th October |
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| 09.30--11.00 | START OF MEETING, COFFEE, REGISTRATION | ||
| 11.00--12.30 | 1: The state of the Universe | ||
| 11.00--11.10 | Welcome | ||
| 11.10--11.55 | The State of the Universe | Spergel | ppt |
| 11.55--12.30 | The direct detection of Dark Matter | Murphy | |
| 12.30--14.00 | LUNCH | ||
| 14.00--15.35 | 2: Dark Energy | ||
| 14.00--14.35 | Dark Energy Theory | Copeland | |
| 14.35--14.55 | Anisotropic Clustering of Galaxies in High-z Universe as a Probe of Dark Energy | Matsubara | pptx |
| 14.55--15.15 | Optimisation of large surveys to probe the dark energy | Parkinson | ppt |
| 15.15--15.35 | DUNE: the Dark UNiverse Explorer | Refregier | |
| 15.35--16.00 | TEA | ||
| 16.00--17.30 | 3: Science with Subaru | ||
| 16.00--16.35 | Wide-field surveys with the Subaru telescope | Yamada | ppt |
| 16.35--17.10 | Hyper Suprime-Cam | Miyazaki | |
| 17.10--17.30 | Constraining Galaxy Formation and Reionization by Deep and Wide-Field Surveys | Ouchi | |
| 19.30--20.30 | Public Lecture by David Spergel | ||
| Thursday 25th October |
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| 09.00--10.30 | 4: Large scale structure with photo-z surveys | ||
| 09.00--09.35 | Review of weak lensing and large-scale structure | Mellier | |
| 09.35--10.10 | Photometric redshifts for LRGs, DES and DUNE and the cross talk with Dark Energy | Lahav | ppt |
| 10.10--10.30 | Pan-STARRS | Phleps | ppt |
| 10.30--11.00 | COFFEE | ||
| 11.00--12.40 | 5: Baryonic Acoustic Oscillations | ||
| 11.00--11.20 | BAOs in the 2dFGRS and SDSS | Percival | ppt |
| 11.20--11.40 | Photo-z versus Spectroscopic Routes to BAOs | Shanks | ppt |
| 11.40--12.00 | The PAU BAO Experiment | Jimenez | |
| 12.00--12.20 | BOSS: The Baryon Oscillation Spectroscopic Survey | Padmanabhan | |
| 12.20--12.40 | FastSound: a near-infrared BAO survey by Subaru/FMOS | Totani | ppt |
| 12.40--13.50 | LUNCH | ||
| 13.50--15.25 | 6: Galaxy formation and clustering | ||
| 13.50--14.25 | Galaxy formation theory and modelling | Cole | ppt |
| 14.25--14.45 | Galaxy clustering in UKIDSS Large Area Survey | Loveday | ppt |
| 14.45--15.05 | Statistics of high redshift galaxies from MUSYC | Padilla | |
| 15.05--15.25 | Photoionization Impact of Galaxies and QSOs on the IGM | Meiksin | |
| 15.25--15.45 | TEA | ||
| 15.45--17.20 | 7: Nearby cosmology | ||
| 15.45--16.20 | Nearby cosmology review | Helmi | |
| 16.20--16.40 | The dSph satellites of the Milky way as Dark Matter tests | Gilmore | ppt |
| 16.40--17.00 | Near-field cosmology: structure and dynamics of the old galactic components | Chiba | |
| 17.00--17.20 | Reconstructing the Formation Histories of the Milky Way and Andromeda Galaxies | Font | ppt |
| 17.30 | Departure of buses to Mary King's Close tours | ||
| 18.00--19.40 | Mary King's Close tours | ||
| From 19.45 | Conference Dinner at the George Hotel | ||
| Friday 26th October |
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| 09.00--10.35 | 8: Supernovae | ||
| 09.00--09.35 | Type Ia Supernova and Dust Extinction | Doi | |
| 09.35--09.55 | Verifying the Utility of Distant Supernovae as Precision Cosmology Probes | Ellis | |
| 09.55-10.15 | The Supernova Legacy Survey | Sullivan | ppt |
| 10.15-10.35 | Cosmology with the European ELT | Hook | |
| 10.35--11.00 | COFFEE | ||
| 11.00--13.00 | 9: Modified gravity and more BAOs | ||
| 11.00--11.35 | Modified gravity models | Maartens | ppt |
| 11.35--11.55 | Observational tests of modified gravity models with future imaging survey of galaxies | Yamamoto | ppt |
| 11.55--12.10 | A closure theory for non-linear evolution of power spectrum | Taruya | ppt |
| 12.10--12.25 | The impact of non-linear evolution of cosmological matter power-spectrum on the measurement of neutrino masses | Saito | ppt |
| 12.25--12.40 | The detectability of baryonic acoustic oscillations in future galaxy surveys | Angulo | |
| 12.40--13.00 | The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) | Hill | |
| 13.00--14.15 | LUNCH | ||
| 14.15--15.35 | 10: Surveys at other wavelengths | ||
| 14.15--14.35 | Evidence for a Population of High-Redshift Submillimeter Galaxies from Interferometric Imaging | Younger | ppt |
| 14.35--14.55 | Surveys of high-z galaxies and galaxy clusters with Herschel and SCUBA-2 | Van Kampen | ppt |
| 14.55--15.15 | Decrypting the Universe with LOFAR | Best | ppt |
| 15.15--15.35 | The Square Kilometre Array (SKA) | Rawlings | ppt |
| 15.35--16.00 | TEA | ||
| 16.00--17.30 | 11: Synergy of methods | ||
| 16.00--16.35 | The non-Gaussian signatures in cosmic shear fields | Takada | ppt |
| 16.35--16.55 | Complementarity of Future Dark Energy Probes | Weller | ppt |
| 16.55--17.30 | Summary remarks | Suto & Ellis | Suto.pdf Ellis.pdf |
Note: Talk schedule is inclusive of question time.
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