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Table 1:

Integrated fluxes for M 87 in the infrared-submm wavelength region between 15 and 1000 $\mu $m.
Instrument $\lambda$ ($\mu $m) $F_\lambda$ (Jy) Source
ISOCAM 15 $0.106 \pm 0.021$ Xilouris et al. (2004)
MIPS 24 $0.171 \pm 0.013$ Shi et al. (2007)
IRAS 25 $0.187 \pm 0.028$ Golombek et al. (1988)
IRAS 60 $0.546 \pm 0.082$ Golombek et al. (1988)
MIPS 70 $0.455 \pm 0.009$ Shi et al. (2007)
IRAS 100 $0.559 \pm 0.084$ Golombek et al. (1988)
PACS 100 $0.517 \pm 0.129$a this paper
MIPS 160 $0.582 \pm 0.010$ Shi et al. (2007)
PACS 160 $0.673 \pm 0.168$a this paper
SPIRE 250 $0.860 \pm 0.215$a this paper
SPIRE 350 $1.070 \pm 0.267$a this paper
SCUBA 450 $1.320 \pm 0.396$ Haas et al. (2004)
SPIRE 500 $1.430 \pm 0.375$a this paper
SCUBA 850 $2.480 \pm 0.496$ Haas et al. (2004)

Notes. (a) We assume a conservative uncertainty in the PACS and SPIRE flux densities of 25%, which includes the 15% uncertainty in the absolute flux calibration (Swinyard et al. 2010; Poglitsch et al. 2010), uncertainties introduced by the map-making techniques, and the possible contamination of background objects. Colour corrections were applied, but they turned out to be very small (1.8% for the PACS 100 band and smaller than 1% for the remaining bands).


Source LaTeX | All tables | In the text

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