FOREGROUND GALACTIC EXTINCTION for NVSS J042407+132331 (Back to INDEX)
Galactic Extinction from the Schlafly & Finkbeiner 2011, Appendix; 2011ApJ...737..103S (SF11) recalibration of the Schlegel, Finkbeiner & Davis 1998, Appendix B; 1998ApJ...500..525S (SFD98) infrared-based dust map. The map is based on dust emission from COBE/DIRBE and IRAS/ISSA; the recalibration assumes a Fitzpatrick (1999PASP..111...63F) reddening law with Rv = 3.1 and different source spectrum than SFD98.
| L a n d o l t | S D S S | U K I R T |
Filter [µm] | U (0.35) | B (0.43) | V (0.54) | R (0.64) | I (0.80) | u (0.36) | g (0.47) | r (0.62) | i (0.75) | z (0.89) | J (1.25) | H (1.66) | K (2.19) | L' (3.78) |
Aλ [mag] | 2.608 | 2.182 | 1.650 | 1.305 | 0.906 | 2.551 | 1.988 | 1.375 | 1.022 | 0.760 | 0.427 | 0.270 | 0.182 | 0.092 |
Show/Hide Aλ magnitudes in all 88 photometric bands based on SF11
Bandpass [µm] | Aλ [mag] |
Landolt | U | (0.35) | 2.608 |
Landolt | B | (0.43) | 2.182 |
Landolt | V | (0.54) | 1.650 |
Landolt | R | (0.64) | 1.305 |
Landolt | I | (0.80) | 0.906 |
CTIO | U | (0.37) | 2.471 |
CTIO | B | (0.43) | 2.191 |
CTIO | V | (0.55) | 1.614 |
CTIO | R | (0.65) | 1.275 |
CTIO | I | (0.80) | 0.912 |
UKIRT | J | (1.25) | 0.427 |
UKIRT | H | (1.66) | 0.270 |
UKIRT | K | (2.19) | 0.182 |
UKIRT | L' | (3.78) | 0.092 |
Gunn | g | (0.52) | 1.754 |
Gunn | r | (0.66) | 1.237 |
Gunn | i | (0.79) | 0.936 |
Gunn | z | (0.91) | 0.743 |
Spinrad | R_S | (0.69) | 1.156 |
Stromgren | u | (0.35) | 2.591 |
Stromgren | b | (0.47) | 2.016 |
Stromgren | v | (0.41) | 2.282 |
Stromgren | beta | (0.49) | 1.915 |
Stromgren | y | (0.55) | 1.616 |
SDSS | u | (0.36) | 2.551 |
SDSS | g | (0.47) | 1.988 |
SDSS | r | (0.62) | 1.375 |
SDSS | i | (0.75) | 1.022 |
SDSS | z | (0.89) | 0.760 |
DSS-II | g | (0.46) | 2.035 |
DSS-II | r | (0.65) | 1.256 |
DSS-II | i | (0.81) | 0.895 |
PS1 | g | (0.49) | 1.909 |
PS1 | r | (0.62) | 1.367 |
PS1 | i | (0.75) | 1.012 |
PS1 | z | (0.87) | 0.796 |
PS1 | y | (0.97) | 0.654 |
PS1 | w | (0.62) | 1.409 |
LSST | u | (0.37) | 2.494 |
LSST | g | (0.48) | 1.948 |
LSST | r | (0.62) | 1.368 |
LSST | i | (0.75) | 1.013 |
LSST | z | (0.87) | 0.796 |
LSST | y | (0.97) | 0.655 |
WFPC2 | F300W | (0.31) | 2.950 |
WFPC2 | F450W | (0.46) | 2.052 |
WFPC2 | F555W | (0.54) | 1.658 |
WFPC2 | F606W | (0.60) | 1.453 |
WFPC2 | F702W | (0.69) | 1.172 |
WFPC2 | F814W | (0.79) | 0.932 |
WFC3 | F105W | (1.04) | 0.583 |
WFC3 | F110W | (1.12) | 0.530 |
WFC3 | F125W | (1.23) | 0.437 |
WFC3 | F140W | (1.37) | 0.369 |
WFC3 | F160W | (1.53) | 0.308 |
WFC3 | F200LP | (0.55) | 1.780 |
WFC3 | F218W | (0.22) | 4.670 |
WFC3 | F225W | (0.24) | 4.206 |
WFC3 | F275W | (0.27) | 3.302 |
WFC3 | F300X | (0.29) | 3.146 |
WFC3 | F336W | (0.34) | 2.680 |
WFC3 | F350LP | (0.59) | 1.579 |
WFC3 | F390W | (0.40) | 2.344 |
WFC3 | F438W | (0.43) | 2.180 |
WFC3 | F475W | (0.48) | 1.955 |
WFC3 | F475X | (0.50) | 1.875 |
WFC3 | F555W | (0.53) | 1.718 |
WFC3 | F600LP | (0.74) | 1.072 |
WFC3 | F606W | (0.59) | 1.497 |
WFC3 | F625W | (0.62) | 1.359 |
WFC3 | F775W | (0.76) | 0.989 |
WFC3 | F814W | (0.80) | 0.924 |
WFC3 | F850LP | (0.91) | 0.727 |
ACS | clear | (0.62) | 1.466 |
ACS | F435W | (0.43) | 2.172 |
ACS | F475W | (0.48) | 1.967 |
ACS | F550M | (0.56) | 1.577 |
ACS | F555W | (0.54) | 1.680 |
ACS | F606W | (0.59) | 1.487 |
ACS | F625W | (0.63) | 1.335 |
ACS | F775W | (0.77) | 0.980 |
ACS | F814W | (0.80) | 0.918 |
ACS | F850LP | (0.90) | 0.748 |
DES | g | (0.48) | 1.948 |
DES | r | (0.64) | 1.309 |
DES | i | (0.78) | 0.960 |
DES | z | (0.91) | 0.732 |
DES | Y | (0.99) | 0.637 |
For completeness, we include the original SFD98 values:
| L a n d o l t | S D S S | U K I R T |
Filter [µm] | U (0.34) | B (0.44) | V (0.54) | R (0.65) | I (0.81) | u (0.35) | g (0.49) | r (0.63) | i (0.78) | z (0.93) | J (1.27) | H (1.67) | K (2.22) | L' (3.81) |
Aλ [mag] | 3.226 | 2.562 | 1.968 | 1.587 | 1.152 | 3.060 | 2.252 | 1.633 | 1.238 | 0.878 | 0.535 | 0.342 | 0.218 | 0.091 |
Galactic Extinction based on H I Column Densities and Galaxy Counts (Burstein & Heiles; 1982AJ.....87.1165B) assuming Rv = 3.1: AB = 0.960 mag
See Notes on Galactic Extinction for important caveats.
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