11. … 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 scale repointing Camera size: 10^4 simultaneous pixels

12. Emission line galaxies (deep-field) cosmology: BAO + LSS blind search for SZE in clusters astrophysics: SFR, metallicity, UVB Global geometrical probes UCO + SLS pec.V + cosmological proper motion mod. G in extreme G environments (close to BH event horizon) probes of accretion flows and B-field effect & topology & feedback (BHs, microQSO, AGNs,QPO’s) accretion flows and warping effects (CO masers, AGNs, micro-QSOs) Acceleration mechanisms around BH and in jets (imaging and spectral evolution, polarization) double QSOs and X-shaped objects interferomety,. Spectra, polariz.) Search for WarmHoles and observational probes (B-field, intensity variations, interferometry, polariz.) Dwarf stars Rydberg atoms and B-field effects (single-dish, spectra, polariz.) Spectral and spatial microsctructure of CM; B fluctuations (molecules at high-z) (Dark Ages of the Universe) probing SMBH (primordial BHs) at z>10 SZE spectro-polarimetry and imaging clusters: cosmoogy, Dark Matter, dark Energy, mod-G,… RG lobes: evolution and acceleration processes B_field effect: polarization ToO: GRBs, SNRs, transients,.. (1hr re-pointing)