… 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

• 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)