Astron.Astrophys.Suppl.Ser. 139 (1999) 545-554 We present observational results for extragalactic radio sources with
milliarcsecond components, obtained with the 600 meter ring radio telescope
...RATAN-600 from 1st to 22nd December, 1997. For each source, a six frequency
broad band radio spectrum was obtained by observing simultaneously with an
accuracy up to a minute at 1.4, 2.7, 3.9, 7.7, 13 and 31 cm. The observed list
is selected from Preston et al. (1985) VLBI survey and contains all the sources
in the declinations between -30deg and +43deg with a correlated flux density
exceeding 0.1 Jy at 13 cm. The sample includes the majority of sources to be
studied in the current VSOP survey and the future RadioAstron Space VLBI
mission.
Grav.Cosmol. 10 (2004) 1-10 We present new RATAN-600 data on the synchrotron Galaxy radiation at the
PLANCK Mission and WMAP frequencies at high Galactic latitudes upto l=3000. The
difference between ...the standard synchrotron template (l<50) of the WMAP group
and RATAN-600 data was detected with the strong synchrotron ``longitude
quadrant asymmetry''. It may change the WMAP estimates of z_{reheating} from
low l polarization data. The polarized synchrotron noise for very deep
observations (<< 1 microK) at the PLANCK HFI was not detected at l>200 scales.
``Sakharov Oscillations'' in the E-mode (500<l<2000) should be well visible
even at ~10 GHz. The polarized noise from relic gravitational waves (l~80) may
be confused with B-mode of synchrotron Galaxy polarized noise at the
frequencies below 100 GHz, but there are no problems at HFI-band.
A survey of the North Celestial Pole region using the RATAN-600 radio
telescope at five frequencies in the range 2.3 to 21.7 GHz is described.
Sources were chosen from the NVSS catalogue. The flux ...densities of 171 sources
in the Declination range +75 to +88 are presented; typical flux density errors
are 5-10 percent including calibration errors. About 20 percent of the sources
have flat spectra or a flat component.
We present observational results for extragalactic radio sources with milliarcsecond components, obtained with the 600 meter ring radio telescope RATAN-600 from 1st to 22nd December, 1997. For each ...source, a six frequency broad band radio spectrum was obtained by observing simultaneously with an accuracy up to a minute at 1.4, 2.7, 3.9, 7.7, 13 and 31 cm. The observed list is selected from Preston et al. (1985) VLBI survey and contains all the sources in the declinations between -30deg and +43deg with a correlated flux density exceeding 0.1 Jy at 13 cm. The sample includes the majority of sources to be studied in the current VSOP survey and the future RadioAstron Space VLBI mission.
We present new RATAN-600 data on the synchrotron Galaxy radiation at the PLANCK Mission and WMAP frequencies at high Galactic latitudes upto l=3000. The difference between the standard synchrotron ...template (l<50) of the WMAP group and RATAN-600 data was detected with the strong synchrotron ``longitude quadrant asymmetry''. It may change the WMAP estimates of z_{reheating} from low l polarization data. The polarized synchrotron noise for very deep observations (<< 1 microK) at the PLANCK HFI was not detected at l>200 scales. ``Sakharov Oscillations'' in the E-mode (500<l<2000) should be well visible even at ~10 GHz. The polarized noise from relic gravitational waves (l~80) may be confused with B-mode of synchrotron Galaxy polarized noise at the frequencies below 100 GHz, but there are no problems at HFI-band.
A survey of the North Celestial Pole region using the RATAN-600 radio telescope at five frequencies in the range 2.3 to 21.7 GHz is described. Sources were chosen from the NVSS catalogue. The flux ...densities of 171 sources in the Declination range +75 to +88 are presented; typical flux density errors are 5-10 percent including calibration errors. About 20 percent of the sources have flat spectra or a flat component.
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