... Project Team" CMBA experiments, 1968-1998 .. Project parameters errors: RATAN-600 versus other best projects .. ... Related: * Experiment "Cold" * "Dark Ages" of the Universe * Spectral-Spatial Fluctuations (SSF) of CMBR . ... The most intensive one - "Experiment Cold" (Parijskij, Korolkov,1986). For the list of "Project Team" CMBA experiments, 1968-1998, look here . ... RATAN-600 . ... Cosmological Gene" project belongs to this class of CMBA experiments. ... COSMOLOGICAL GENE . ...

... ADS doc The Westerbork Northern Sky Survey (WENSS) is a radio survey made with the WSRT at wavelengths 92 and 49 cm. At 92 cm the entire sky above declination 30 degrees is covered. ... To move grating rings of the map 6 different baseline settings are used, so 1 mosaic data block involves 72 hours of observational data. ... As a result the final catalogue will consist of 300,000 sources at 92 cm and 60,000 at 49 cm. ... With the WSRT high quality wide field polarization maps can be made. ...

... The variability of the spectrum of the optical component of the IR-source IRAS01005+7910 was discovered for the first time in the BTA spectra [1]. ... The spectral features include absorptions that form in near-photospheric layers, narrow envelope emissions, and emission-absorption profiles that form in photosphere-to-envelope transition layers (the wind). ... Discovery of spectral variation in the optical counterpart of IRAS01005+7910. ... Dashed line - envelope curve of all the SiII 5979 profiles ...

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 ...