The Parkes 2700 MHz Survey (Eighth Part). Catalogue for the Declination Zone ?65° to ?75°

Abstract

Abstract. A catalogue of 515 radio sources is presented for the region between declinations -65° and -75° (0·374sr). The survey is believed to be complete to 0·22Jy at 2700 MHz (-'900 sources per steradian). Flux densities at 5009 MHz have been measured for most of the sources stronger than o· 35 Jy at 2700 MHz.

A radio continuum study of the Magellanic Clouds

“…Later, McGee et al (1976) presented a list of sources towards the Small Magellanic Cloud (SMC) at 5.00 GHz (See Table 2 for a summary of the radio-source surveys of the SMC). McGee et al (1972b) and Bolton & Butler (1975) observed the MCs at 2.70 GHz which became part of the PKSCAT-90 catalogue (Otrupcek & Wright 1991). After Mills & Aller 1971 detected a few sources at 0.408 GHz, as a part of a whole sky survey, Clarke et al (1976) observed the MCs with the Molonglo radio telescope and produced the MC4 catalogue of 227 sources towards the LMC and 75 towards the SMC.…”

A radio continuum study of the Magellanic Clouds

“…The median of the ratio between our estimates and PKSCAT-90 is 1.01 (our flux densities are higher) with a standard deviation of 0.30. Figure 1b presents a comparison of the integrated flux density from our survey at 2.45 GHz versus the flux density at 2.70 GHz (McGee et al 1976;Bolton & Butler 1975;Broten 1972) for 18 sources in common (excluding four very extended sources). The resulting median is 1.14 with a standard deviation of 0.16.…”

“…To establish the relative flux density scales of our catalogues at 1.42, 2.45, 4.75 and 8.55 GHz we have compared our flux density with those from the PKSCAT-90 catalogue (Otrupcek & Wright 1991) which includes sources from surveys at 1.40 GHz (Mathewson & Healey 1964;McGee et al 1976), 2.70 GHz (McGee et al 1976Bolton & Butler 1975;Broten 1972), 5.00 GHz and 8.80 GHz (McGee et al 1976). Few sources in the SMC are contained in the PKSCAT-90 catalogue at 1.40 GHz.…”

A radio continuum study of the Magellanic Clouds. IVa. Catalogue of radio sources in the Large Magellanic Cloud at 2.30 GHz$^{\bf (\lambda=13 cm)}$

“…3a we show a comparison of the integrated flux density from our survey at 2.30 GHz with the flux density at 2.70 GHz (McGee et al 1972a;Bolton & Butler 1975) for 58 sources (excluding 30 Dor as it is very extended). The resulting mean ratio is 1.06±0.02 (our flux densities are higher) with a scatter of 13.4%.…”

“…To establish the relative flux density scales of our catalogue at 2.30 GHz we have compared our flux densities with those from the PKSCAT-90 catalogue (Otrupcek & Wright 1991) which includes sources from surveys at 2.70 GHz (McGee et al 1972a;Bolton & Butler 1975).…”