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Home All issues Volume 503 / No 3 (September I 2009) A&A, 503 3 (2009) 747-754 Full HTML
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Table 3:

Integrated flux densities on the observed sources.
Source Frequency Flux density Reference
  MHz Jy  
NGC 0628 57.5 $2\pm1$ 1
  324.4 $0.49 \pm0.03$ This work
  1400 $0.15 \pm0.01$ 2
  1515 $0.16 \pm 0.01$ This work
  4850 $0.060 \pm 0.005$ 3
NGC 3627 57.5 $2.3\pm 0.7$ 1
  160 $1.6 \pm 0.3^a$ 4
  325.5 $0.97 \pm 0.03$ This work
  408 $0.93 \pm 0.05$a 5
  611 $0.87 \pm 0.1^a$ 4
  1370 $0.5 \pm 0.01$ 6
  1425 $0.38 \pm 0.01$ This work
  2695 $0.2 \pm 0.04$ 4
  4850 $0.14\pm 0.02$ 7
NGC 7331 74 $1.12\pm 0.18$ 8
  325 $0.935\pm 0.004$ 9
  325.9 $0.94\pm 0.02$ This work
  1489 $0.32\pm0.01$ This work
  1400 $0.33 \pm 0.01$ 2
  1369 $0.35 \pm 0.01$ 6
  2380 $ 0.18\pm 0.01$ 10
  4850 $ 0.096\pm 0.013$ 7
a Flux density scale from Wyllie (1969).
References and telescopes: 1. Israel & Mahoney (1990): Clark Lake radio Telescope; 2. Condon et al. (1998b): NVSS - NRAO VLA D array; 3. Gregory et al. (1996): NRAO Green Bank Telescope; 4. Haynes et al. (1975): CSIRO telescope; 5. Large et al. (1981): Molonglo Radio Telescope; 6. Braun et al. (2007): Westerbork Telescope WSRT; 7. Gregory & Condon (1991): NRAO Green Bank; 8. Cohen et al. (2007): NRAO VLA B array; 9. Rengelink et al. (1997): WENSS - WSRT; 10. Dressel & Condon (1978): Arecibo Telescope.

Source LaTeX | All tables | In the text

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