Slide 1L. Perivolaropoulos http://leandros.physics.uoi.gr Department of Physics University of Ioannina Open page S. Nesseris, LP, astro-ph/0610092, astro-ph/0611238 Slide…
… 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…
First Stars, Quasars, and the Epoch of Reionization Jordi Miralda Escudé Institut de Ciències de l’Espai (IEEC-CSIC, ICREA), Barcelona. Instituto de Astrofísica de Canarias,…
… 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…