Titlebook: Radio Astronomy and Cosmology; David L. Jauncey Book 1977 International Astronomical Union 1977 Cosmology.Gravity.STR.Universe.astronomy

雕鏤

The Parkes 2700 Mhz Survey: Counts of the Sources and their Distribution on the Sky; part 11 and subsequent parts consist of re-surveys of some areas to fainter flux density limits. The current version of the composite catalogue for the 7.36 sr covered (Fig. 1) contains about 7500 sources, together with the results of identification programmes and flux density measurements at other frequencies.

詞匯記憶方法

Decrepit

jettison

The Molonglo Radio Source Surveys at 408 MHzeing undertaken; this involves multiple observations within narrow strips at selected declinations. The signal-to-noise ratio is some three to five times better than in normal surveying and the confusion limit is approached.

Deduct

reception

Parameter

The 6C Surveyincluding Warner, Kenderdine, Waggett, Masson and Mayer. The results of the first observations are at present in a preliminary state but we hope that in time they will form the first part of the 6C survey. The purpose of the survey is not to reach the faintest sources detected so far in aperture syn

pericardium

COKE

Interim Report on the Texas Surveyin the range 335–380 MHz. Primary goals are (i) determination of accurate ~l“) positions for about 50,000 sources, followed by (ii) optical identification of the sources on the basis of exact radio-optical position coincidence; (iii) provision of rough structure models for all listed sources; and (i

conflate

The Molonglo Radio Source Surveys at 408 MHzsky south of +18° declination. Commencing in late 1967, the survey has been continuing at a low priority until it is now complete to a declination of ?85°, except for some small areas affected by interference or instrumental problems which are being re-observed. A program of ‘deep surveys’ is also b