October 30, Tuesday
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8:30 - 9:10
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Registration / Coffee & Snacks
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9:10 - 9:20 |
Welcome Remarks - Changbom Park (KIAS)
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Morning Session I - LSS (Velocity fields)
Chair: Shude Mao
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9:20 - 9:50 |
Matthew
Colless (AAO) - The local density and velocity fields from the 6dF Galaxy Survey
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9:50 ~ 10:10 |
Teppei Okumura (IEU) - Distribution function approach to redshift space distortion
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10:10 ~ 10:30 |
Jaiyul Yoo
(Zürich) -
Going beyond the Kaiser Redshift-Space Distortion Formula
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10:30 ~ 10:50 |
Yong-Seon Song
(KASI) - Unplugged determination of expansion history of the universe using redshift distortions
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10:50 - 11:20 |
Coffee Break
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Morning Session II - LSS (Survey Sciences - I)
Chair: Shude Mao
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11:20 - 11:50 |
David J.
Schlegel (LBNL) - BOSS, BigBOSS and Beyond
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11:50 ~ 12:10 |
Juhan Kim (KIAS) - The Horizon Run Simulations
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12:10 ~ 12:30 |
Melody Wolk (IAP) - Hierarchical amplitudes in the CFHTLS Wide survey: evolution since z~1
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12:30 - 14:00 |
Lunch
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Afternoon Session I - LSS (Survey Sciences - II)
Chair: Ilian T. Iliev
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14:00 - 14:30 |
István Szapudi (Hawaii) Cross-correlation of WMAP7 and the WISE Full Data Release
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14:30 ~ 14:50 |
Xiaohu Yang
(SHAO) - Mapping the star formation histories of the Universe
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14:50 ~ 15:10 |
Graziano Rossi (Saclay) - Cosmic web statistics and halo triaxiality: new insights
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15:10 ~ 15:30 |
Cheng Li
(SHAO) - Linking galaxies to dark matter halos with stellar mass or with stellar velocity dispersion?
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15:30 - 16:00 |
Coffee Break
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Afternoon Session II - LSS (Cosmology test); Poster Introductions
Chair: Ken Ganga
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16:00 - 16:30 |
Changbom Park (KIAS) - The Challenge of the Largest Structures in the Universe to Cosmology
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16:30 ~ 16:50 |
Yun-Young
Choi (Kyung Hee) - Topology of SDSS Luminous Red Galaxies: genus statistics and non-Gaussianity
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16:50 ~ 17:10 |
Young-Rae Kim (KIAS) - Modelling the non-linear systematic effects on genus statistics for large scale structure topology
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17:10 ~ 17:30 |
Jinn-Ouk
Gong (APCTP) - Non-linear and non-Gaussian contributions to galaxy
bias
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17:30 - 18:10 |
Poster Introductions
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