A.2 Converting Between Flux Density and Magnitudes

The conversion between magnitudes and flux density $ F_\nu $ is given explicitly in equation A.1. All we need is to specify the zero-point flux, $ F_{\nu_0}$.

The zero-point flux, $ F_{\nu_0}$, is determined for a number of photometric systems. In Table A.2 we tabulate the zeropoints, $ F_{\nu_0}$ and $ F_{\lambda_0} = a_\lambda F_{\nu_0} /
\lambda^2$, for IRAC.


Table A.2: The photometric zeropoints for the Spitzer/IRAC instrument.
$ \lambda \; [\mu {\rm m}]$ $ F_{\nu_0}$ [Jy] $ F_{\lambda_0}$ $ [{\rm erg}\; {\rm cm}^{-2}\; {\rm s}^{-1} \;\mu {\rm m}^{-1}]$
3.6 277.5 $ 6.42\times 10^{-8}$
4.5 179.5 $ 2.66\times 10^{-8}$
5.8 116.6 $ 1.04\times 10^{-8}$
8.0 63.1 $ 2.96\times 10^{-9}$


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).


Table A.3: The photometric zeropoints in the 2MASS filters.
Band $ \lambda [\mu m]$ $ F_{\nu_0}$ [Jy]
J 1.235 1594
H 1.662 1024
Ks 2.159 666.7


In Table A.4 we tabulate the zeropoints, $ F_{\nu_0}$ and $ F_{\lambda_0} = a_\lambda F_{\nu_0} /
\lambda^2$, adopted for NICMOS, based on the CIT system (Beckwith et al., 1976, ApJ, 208, 390).


Table A.4: The photometric zeropoints in the CIT system.
Band $ \lambda [\mu {\rm m}]$ $ F_{\nu_0}$ [Jy] $ F_{\lambda_0}$ $ [{\rm erg}\; {\rm cm}^{-2}\; {\rm s}^{-1} \;\mu {\rm m}^{-1}]$
V 0.56 3540 $ 3.39\times 10^{-5}$
R 0.70 2870 $ 1.76\times 10^{-5}$
I 0.90 2250 $ 8.83\times 10^{-6}$
J 1.25 1670 $ 3.20\times 10^{-6}$
H 1.65 980 $ 1.08\times 10^{-6}$
K 2.2 620 $ 3.84\times 10^{-7}$
L 3.4 280 $ 7.26\times 10^{-8}$
M 4.8 150 $ 1.95\times 10^{-8}$
N 10.1 37 $ 1.09\times 10^{-9}$
Q 20.0 10 $ 7.5 \times 10^{-11}$


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).


Table A.5: The photometric zeropoints in the Johnson UBVRI+ system.
Band $ \lambda [\mu m]$ $ F_{\nu_0}$ [Jy]
U 0.36 1823
B 0.44 4130
V 0.55 3781
R 0.71 2941
I 0.97 2635
J 1.25 1603
H 1.60 1075
K 2.22 667
L 3.54 288
M 4.80 170
N 10.6 36
O 21.0 9.4


We have developed an online magnitude $ \leftrightarrow$ flux density converter. Check the SSC tools website:

http://ssc.spitzer.caltech.edu/tools/

Gillian Wilson 2006-11-09