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Millimeter Continuum Monitoring of Extragalactic Radio Sources with the IRAM 30M Telescope

Published online by Cambridge University Press:  12 April 2016

H. Ungerechts ,
C. Kramer ,
B. Lefloch ,
S. Leon ,
F. Masset ,
R. Moreno ,
G. Paubert ,
D. Reynaud ,
A. Sievers  and
W. Wild
H. Ungerechts
Affiliation:
IRAM, Avenida Divina Pastora 7-NC, E-18012 Granada, Spain
C. Kramer
Affiliation:
IRAM, Avenida Divina Pastora 7-NC, E-18012 Granada, Spain
B. Lefloch
Affiliation:
IRAM, Avenida Divina Pastora 7-NC, E-18012 Granada, Spain
S. Leon
Affiliation:
IRAM, Avenida Divina Pastora 7-NC, E-18012 Granada, Spain
F. Masset
Affiliation:
IRAM, Avenida Divina Pastora 7-NC, E-18012 Granada, Spain
R. Moreno
Affiliation:
IRAM, Avenida Divina Pastora 7-NC, E-18012 Granada, Spain
G. Paubert
Affiliation:
IRAM, Avenida Divina Pastora 7-NC, E-18012 Granada, Spain
D. Reynaud
Affiliation:
IRAM, Avenida Divina Pastora 7-NC, E-18012 Granada, Spain
A. Sievers
Affiliation:
IRAM, Avenida Divina Pastora 7-NC, E-18012 Granada, Spain
W. Wild
Affiliation:
IRAM, Avenida Divina Pastora 7-NC, E-18012 Granada, Spain

Abstract

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We continue to determine flux densities at 3mm, 2mm, and 1.3mm wavelength for selected extragalactic sources. Light-curves for some sources now cover nearly 12 years.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 149 - 150
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

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