| Issue |
A&A
Volume 376, Number 3, September IV 2001
|
|
|---|---|---|
| Page(s) | 1123 - 1125 | |
| Section | Numerical methods and codes | |
| DOI | https://doi.org/10.1051/0004-6361:20010975 | |
| Published online | 15 September 2001 | |
Pointing sources for southern submm telescopes *,**
1
Astronomisches Institut der Ruhr-Universität Bochum, Universitätsstrasse 159/NA 7, 44780 Bochum, Germany
2
European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching bei München, Germany
3
Swedish-ESO Submillimetre Telescope, European Southern Observatory, Casilla 16001, Santiago 19, Chile
4
Onsala Space Observatory, 439 92 Onsala, Sweden
Corresponding author: A. Adraou, adraou@astro.ruhr-uni-bochum.de
Received:
23
April
2001
Accepted:
13
June
2001
We present the results of a 230 GHz survey of
quasars and BL Lacertae objects performed with the SEST. The sample
consists of objects with flat radio spectra and is taken from various
radio surveys. Repeated observations for individual sources indicates
variability by factors of 2-5 within a single night. Comparing
measurements over longer periods, even changes by factors of 10-25 at
230 GHz have been observed. The present catalog contains the 130
brightest objects whose 230 GHz flux densities are above 500 mJy
most of the time. This, and their declination below 
, makes
them useful candidates for future pointing sources at
southern submillimeter telescopes. First measurements of
flux densities at 345 GHz are given for six objects.
Key words: galaxies: active / BL Lacertae objects: general / quasars: general / radio continuum: general
© ESO, 2001
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