The conversion between magnitudes and flux density
is given
explicitly in equation A.1. All we need is to
specify the zero-point flux,
.
The zero-point flux,
, is determined for a number of
photometric systems. In Table A.2 we tabulate
the zeropoints,
and
, for IRAC.
In Table A.3, we display the zeropoints in the 2MASS passbands (see: http://www.ipac.caltech.edu/2mass/releases/second/doc/sec4_5.html).
In Table A.4 we tabulate
the zeropoints,
and
, adopted for NICMOS, based on the CIT system (Beckwith et
al., 1976, ApJ, 208, 390).
In Table A.5, we display the zeropoints in the Johnson UBVRI+ system (see: Allen's Astrophysical Quantities, Fourth Edition, 2001, Arthur N. Cox (ed.), Springer-Verlag; Campins, Rieke, & Lebofsky 1985, AJ, 90, 896; Rieke, Lebofsky & Low 1985, AJ, 90, 900).
We have developed an online
magnitude
flux density converter. Check the SSC
tools website:
Gillian Wilson 2006-11-09