The Large Sky Area Multi-Object Fiber Spectroscopic Telescope Project (The LAMOST Project) National Astronomical Observatories Chinese Academy of Sciences Web page: http://www.lamost.org The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) project as one of the National Major Scientific Projects is a quasi-meridian reflecting Schmidt telescope laid down on the ground with its optical axis fixed in meridian plane. ...

Bright sources . with CATS-identifications) . Galactic plane sources . ... 3CR sources . ... Trushkin, 1999) . 1Jy-sources . ... COLD"-sources, DEC=5d . Bursov, 1996) . 9C sources . Waldram+,2003) . ... VSOP sources . ... Taylor, 2001) +CATSidn . PMN-sources . Mingaliev+ 1999) +CATSidn . CLASS sources . ... WMAP sources . Trushkin, 2003) . NCP-sources . Mingaliev+ 2001)+CATS idn . ... Konnikova+,1989) +CATS idn . ... 1996 Nizhnij Arkhyz . ...

... Divisions . ... Astrospectroscopy laboratory . Laboratory of Extragalactic Astrophysics and Cosmology . Laboratory for the Stellar Magnetism Study . Laboratory of spectroscopy and photometry of extragalactic objects . ... Observations Support Laboratory . Group of extragalactic systems investigation . ... Group of relativistic astrophysics . ... RADIO ASTRONOMICAL DIVISIONS . Radio astrophysics laboratory . ... Group of the Sun study . ... Laboratory for the Radio Astronomy Study . ...

The project of the informational system creation on the problem of evolution of radio galaxies, as a part of the "Big Trio" project aimed on studing of distant radio galaxies, is designed. This system allows a user to operate with simulated curves of spectral energy distributions (SED) to estimate ages and redshifts by photometry data. Authors use SEDs of several models for different types of galaxies. ... The HTTP and e-mail access is organized to this system. ...

... Corresponding gates in each row are connected in parallel at both edges of the array. ... Other gates. ... otherwise indicated, 45 kpixels/sec and standard voltages using a dual slope CDS circuit (8 µs integration time) Minimum Format Pixel Size Imaging Area Dark current (MPP), 20° C equivalent Readout noise Front Back Full Well signal Output gain CTE per pixel Typical 512 x 512 pixels 24 µm x 24 µm 12.3 mm x 12.3 mm 50 pa/cm2 5 electrons 7 electrons 350,000 electrons 1.5 µV/ electron 0 ...