Slide 1Late gas accretion onto primordial mini-halos a model for pre-reionization dwarfs and extragalactic compact High-Velocity Clouds Massimo Ricotti (U of Maryland) Slide…

Slide 1FIGGS: The Faint Irregular Galaxy GMRT Survey Jayaram N Chengalur NCRA/TIFR Ayesha Begum I. D. Karachentsev Sambit Roychowdhury S. Kaisin, M. Sharina Slide 2 Near…

Slide 1Stellar-mass Metallicity Relation at High Redshifts Stellar-mass Metallicity Relation at ｚ～１． 4 Kouji OHTA （ Kyoto University ） K. Yabe, F. Iwamuro, S.…

Slide 1 The LAMOST 1d Spectroscopic Pipeline A-Li LUO LAMOST team, NAOC 2008/12/3 The KIAA-Cambridge Joint Workshop on Near-Field Cosmology and Galactic Archeology Slide…

The Local Group 35 - 40 members M31, and its satellites (red) Milky Way, and its satellites (blue) Isolated dwarfs (blue) THE LOCAL GROUP Mass Length Time Stellar Archaeology…

… to millimetron instrument WG 12 m telescope Cooling: Y Single-dish & interferometry Wide freq range (FTS) Polarization mode Sensitivity: NEP \sim 10^{-19} ToO: 1hr-time…

Near-field Cosmology from the Andromeda galaxy and subgroup Scott C. Chapman IoA, University of Cambridge With: R.Ibata, M.Irwin, G.Lewis, A.Ferguson, N.Tanvir, N.Martin,…

The LAMOST 1d Spectroscopic Pipeline A-Li LUO LAMOST team, NAOC 2008/12/3 The KIAA-Cambridge Joint Workshop on Near-Field Cosmology and Galactic Archeology Lessons from SDSS…

Slide 1 Precision Stellar astrophysics with song Marc Pinsonneault (OSU) Precision Stellar Astrophysics New Era in Astronomy Seismology Large Surveys We can now measure things…

… to millimetron instrument WG 12 m telescope Cooling: Y Single-dish & interferometry Wide freq range (FTS) Polarization mode Sensitivity: NEP \sim 10^{-19} ToO: 1hr-time…