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conversions

Fluxes from a Zero mag Source and
Conversion of Magnitudes to Janskys and F-Lambda

The tables below give bandpass, effective or isophotal wavelength or frequency for the bandpass (see this discussion for important notes on definitions), flux in Wm-2 µm-1 and Jansky, and AB mags, for a zero magnitude source. One Jansky represents an incident energy flux density of 10-26 W m-2 Hz-1. The two datasets below were calculated in slightly different ways but the results agree within 2%.


WFCAM ZY and Mauna Kea Filter Bandpasses


3.071E+14
 
Tokunaga & Vacca 2005 PASP and priv. comm.
P. Hewett priv. comm.
Band   
Isophotal
Wavelength
(µm)
Flux
(Wm-2 µm-1)
Isophotal
Frequency
Hz
  S (Jy)
  AB
mag
Effective
Wavelength
(µm)
Flux
(Wm-2 µm-1)
  S (Jy)
  AB
mag
                   
V
0.5450
3.58E-08
5.490E+14
3630
0.026
       
Z
0.9206
8.74e-09
2270
0.535
0.8817
8.59E-09
2232
0.528
Y
1.036
5.81e-09
2.870E+14
2060
0.640
1.0305
5.71E-09
2026
0.634
J
1.250
3.01e-09
2.394E+14
1560
0.941
1.2483
2.94E-09
1530
0.938
H
1.644
1.18e-09
1.802E+14
1040
1.38
1.6313
1.14E-09
1019
1.379
K'
2.121
4.57e-10
1.413E+14
686
1.84
 
 
 
 
Ks
2.149
4.35e-10
1.395E+14
670
1.86
 
 
 
 
K
2.198
4.00e-10
1.364E+14
645
1.90
2.2010
3.89E-10
630
1.900
L'
3.754
5.31e-11
7.982E+13
249
2.93
 
 
 
 
M'
4.702
2.22e-11
6.350E+13
163
3.40
 
 
 
 

Older Filter Bandpasses
Beckwith et al. (1976, ApJ, 208, 390), with modifications at
10 and 20 microns to be consistent with Tokunaga (1984, AJ, 89, 172)

Band (µm)
S (Jy)
Flux (Wm-2 µm-1)
     
V (0.5556)
3540
3.44e-08
I (0.9)
2250
8.25e-09
J (1.25)
1600
3.07e-09
H (1.65)
1020
1.12e-09
K (2.20)
657
4.07e-10
L (3.45)
290
7.30e-11
L'(3.80)
252
5.24e-11
M (4.80)
163
2.12e-11
(7.8)
65.3
3.22e-12
(8.7)
53.0
2.10e-12
(9.8)
42.3
1.32e-12
N (10.1)
39.8
1.17e-12
(10.3)
38.5
1.09e-12
(11.6)
30.5
6.81e-13
(12.5)
26.4
5.07e-13
Q (20.0)
10.4
7.80e-14
Contact: Andy Adamson. Updated: Sat Jun 4 13:51:43 HST 2005

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