The radio-source population at 100 GHz

Details The radio-source population at 100 GHz The radio-source population at 100 GHz

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atnf.prop..317s&link_type=abstract

ATNF proposal C1392, Semester: April, 2006

Computer Science

Extragalactic, Atca

Scientific paper

Improving our knowledge of the radio-source population at 100 GHz is important (i) to interpret the data from future CMB missions, (ii) to identify 'extreme GPS' sources believed to represent the earliest (t<1000 yr) stages of radio-galaxy evolution, and (iii) to identify new mm calibrators for the ATCA and ALMA. Our C1392 observations in 2005 showed that robust 3mm fluxes can be measured for continuum sources detected at 20 GHz in the AT20G survey, and we now request time to observe a complete sub-sample of AT20G sources at 95-100 GHz.

Affiliated with

Also associated with

No associations

Rating

The radio-source population at 100 GHz does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The radio-source population at 100 GHz, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The radio-source population at 100 GHz will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1161709