... See also MRC 1Jy sample I. and MRC 1Jy sample II. 20deg but excluding the R.A. range 14h03m--20h20m. Quasar classifications are based on high-resolution radio images, deep optical identifications, and follow-up spectroscopy of sources in the strip. The relatively low radio frequency of the finding survey and the complete optical identification of quasars to faint magnitudes ensure that the MQS is relatively free from orientation biases that affect most other samples of radio-loud quasars. ...

... 1969 1.049 - 3 CR, KPW 10 178 Veron 1977 1.19 - - 11 318 Condon and Jauncey 1974a 1.05 1.5 Jy - 12 318 Condon and Jauncey 1974b 1.05 1.5 Jy - 13 318 Veron and Veron 1978 1.06 - - 14 408 Grueff and Vigotti 1968 1.13 - BOL 15 408 Ekers 1969 - - Pks 16a 408 Colla et al. ... 1971 - - Pks 45 2700 Shimmins and Bolton 1972 - - Pks 46 2700 Bolton and Shimmins 1973 - - Pks 47 2700 Wall and Cannon 1973 - - 48 2700 Shimmins and Bolton 1974 - - Pks 49 2700 Bolton et al. ... 1975 - - Pks 52 2700 Shimmins et al. ...

... We present new progress in our extensive pro ject mCPod (On­line database of photometric observations of magnetic CP stars), which was initiated five and a half years ago (Mikulґ et. al, 2007). ... The database consists of two parts, the Data and the References. In the References one finds the sources of data, the bibcodes including links to the corresponding papers, names of comparison and check stars (if available), the number of observations in individual filters (see Fig. ...

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 ...