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Table 3:

Multiwavelength nucleus data for NGC 4278.

$\nu$ 		$\nu L_{\nu}$ Aperture Satellite/filter Date Reference
(Hz) (erg s-1) (arcsec)      

$1.93\times10^{18}$ 		$7.83\times10^{39}$ 3.34 Chandra/ACIS-S February 2007 This work
$1.93\times10^{18}$ $5.56\times10^{40}$ 10 XMM-Newton/EPIC-pn May 2004 This work
$1.21\times10^{17}$ $1.32\times10^{40}$ 3.34 Chandra/ACIS-S February 2007 This work
$1.21\times10^{17}$ $5.96\times10^{40}$ 10 XMM-Newton/EPIC-pn May 2004 This work
$1.42\times10^{15}$ $1.05\times10^{41}$ 0.28 HST/F218W January 1995 Cardullo et al. (2009)
$1.42\times10^{15}$ $6.75\times10^{40}$ 0.28 HST/F218W June 1994 Cardullo et al. (2009)
$1.30\times10^{15}$ $1.21\times10^{41}$ 3 XMM-Newton/UVM2 May 2004 This work
$6.32\times10^{14}$ $3.03\times10^{40}$ 0.15 HST/F475W January 2007 This work
$6.32\times10^{14}$ $2.51\times10^{40}$ 0.15 HST/F475W December 2006 This work
$5.76\times10^{14}$ $1.13\times10^{40}$ 1.26 HST/F555W May 1994 Lauer et al. (2005)
$3.65\times10^{14}$ $6.95\times10^{39}$ <6 HST/F814W May 1994 Capetti et al. (2002)
$3.32\times10^{14}$ $2.83\times10^{40}$ 0.15 HST/F850LP January 2007 This work
$3.32\times10^{14}$ $2.61\times10^{40}$ 0.15 HST/F850LP December 2006 This work
$2.40\times10^{14}$ $4.56\times10^{42}$ 8.00 1.54 m Mount Lemmon/J   Heckman et al. (1983)
$1.82\times10^{14}$ $7.77\times10^{42}$ 7.20 3.8 m UKRIT/H   Longmore & Sharples (1982)
$1.36\times10^{14}$ $4.50\times10^{42}$ 7.20 3.8 m UKRIT/K   Longmore & Sharples (1982)
$8.69\times10^{13}$ $9.57\times10^{41}$ 8.00 1.54 m Mount Lemmon/L   Heckman et al. (1983)
$2.97\times10^{13}$ $1.15\times10^{41}$ 5.60 1.54 m Mount Lemmon/N   Heckman et al. (1983)
$2.20\times10^{10}$ $5.36\times10^{38}$ <1 VLA August 2003 Giroletti et al. (2005)
$1.50\times10^{10}$ $4.00\times10^{38}$ 0.15 VLA September 1999 Nagar et al. (2001)
$8.40\times10^{9}$ $2.66\times10^{38}$ $(3.2\times1.9)\times10^{-3}$ VLBA/VLA August 2000 Giroletti et al. (2005)
$5.00\times10^{9}$ $2.00\times10^{38}$ $(3.2\times1.9)\times10^{-3}$ VLBA July 1995 Giroletti et al. (2005)
$5.00\times10^{9}$ $2.25\times10^{38}$ $2.5\times10^{-3}$ VLBA/VLA August 2000 Giroletti et al. (2005)
$1.67\times10^{9}$ $1.00\times10^{38}$ $5.0\times10^{-3}$ VLBI May 1979 Jones et al. (1984)

Notes. Infrared, optical and UV luminosities are corrected for galactic extinction.


Source LaTeX | All tables | In the text

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