FOREGROUND GALACTIC EXTINCTION for SSTSL2 J163809.97-101250.0 (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] | 2.043 | 1.709 | 1.293 | 1.022 | 0.709 | 1.998 | 1.557 | 1.077 | 0.800 | 0.595 | 0.334 | 0.212 | 0.142 | 0.072 |
Show/Hide Aλ magnitudes in all 88 photometric bands based on SF11
Bandpass [µm] | Aλ [mag] |
Landolt | U | (0.35) | 2.043 |
Landolt | B | (0.43) | 1.709 |
Landolt | V | (0.54) | 1.293 |
Landolt | R | (0.64) | 1.022 |
Landolt | I | (0.80) | 0.709 |
CTIO | U | (0.37) | 1.936 |
CTIO | B | (0.43) | 1.716 |
CTIO | V | (0.55) | 1.264 |
CTIO | R | (0.65) | 0.999 |
CTIO | I | (0.80) | 0.715 |
UKIRT | J | (1.25) | 0.334 |
UKIRT | H | (1.66) | 0.212 |
UKIRT | K | (2.19) | 0.142 |
UKIRT | L' | (3.78) | 0.072 |
Gunn | g | (0.52) | 1.374 |
Gunn | r | (0.66) | 0.969 |
Gunn | i | (0.79) | 0.733 |
Gunn | z | (0.91) | 0.582 |
Spinrad | R_S | (0.69) | 0.906 |
Stromgren | u | (0.35) | 2.029 |
Stromgren | b | (0.47) | 1.579 |
Stromgren | v | (0.41) | 1.788 |
Stromgren | beta | (0.49) | 1.500 |
Stromgren | y | (0.55) | 1.266 |
SDSS | u | (0.36) | 1.998 |
SDSS | g | (0.47) | 1.557 |
SDSS | r | (0.62) | 1.077 |
SDSS | i | (0.75) | 0.800 |
SDSS | z | (0.89) | 0.595 |
DSS-II | g | (0.46) | 1.594 |
DSS-II | r | (0.65) | 0.984 |
DSS-II | i | (0.81) | 0.701 |
PS1 | g | (0.49) | 1.495 |
PS1 | r | (0.62) | 1.071 |
PS1 | i | (0.75) | 0.793 |
PS1 | z | (0.87) | 0.623 |
PS1 | y | (0.97) | 0.512 |
PS1 | w | (0.62) | 1.104 |
LSST | u | (0.37) | 1.954 |
LSST | g | (0.48) | 1.526 |
LSST | r | (0.62) | 1.071 |
LSST | i | (0.75) | 0.794 |
LSST | z | (0.87) | 0.624 |
LSST | y | (0.97) | 0.513 |
WFPC2 | F300W | (0.31) | 2.311 |
WFPC2 | F450W | (0.46) | 1.607 |
WFPC2 | F555W | (0.54) | 1.299 |
WFPC2 | F606W | (0.60) | 1.138 |
WFPC2 | F702W | (0.69) | 0.918 |
WFPC2 | F814W | (0.79) | 0.730 |
WFC3 | F105W | (1.04) | 0.457 |
WFC3 | F110W | (1.12) | 0.415 |
WFC3 | F125W | (1.23) | 0.342 |
WFC3 | F140W | (1.37) | 0.289 |
WFC3 | F160W | (1.53) | 0.241 |
WFC3 | F200LP | (0.55) | 1.394 |
WFC3 | F218W | (0.22) | 3.658 |
WFC3 | F225W | (0.24) | 3.295 |
WFC3 | F275W | (0.27) | 2.586 |
WFC3 | F300X | (0.29) | 2.464 |
WFC3 | F336W | (0.34) | 2.099 |
WFC3 | F350LP | (0.59) | 1.237 |
WFC3 | F390W | (0.40) | 1.837 |
WFC3 | F438W | (0.43) | 1.708 |
WFC3 | F475W | (0.48) | 1.531 |
WFC3 | F475X | (0.50) | 1.469 |
WFC3 | F555W | (0.53) | 1.346 |
WFC3 | F600LP | (0.74) | 0.840 |
WFC3 | F606W | (0.59) | 1.173 |
WFC3 | F625W | (0.62) | 1.065 |
WFC3 | F775W | (0.76) | 0.774 |
WFC3 | F814W | (0.80) | 0.724 |
WFC3 | F850LP | (0.91) | 0.569 |
ACS | clear | (0.62) | 1.148 |
ACS | F435W | (0.43) | 1.702 |
ACS | F475W | (0.48) | 1.540 |
ACS | F550M | (0.56) | 1.235 |
ACS | F555W | (0.54) | 1.316 |
ACS | F606W | (0.59) | 1.165 |
ACS | F625W | (0.63) | 1.046 |
ACS | F775W | (0.77) | 0.768 |
ACS | F814W | (0.80) | 0.719 |
ACS | F850LP | (0.90) | 0.586 |
DES | g | (0.48) | 1.526 |
DES | r | (0.64) | 1.026 |
DES | i | (0.78) | 0.752 |
DES | z | (0.91) | 0.574 |
DES | Y | (0.99) | 0.499 |
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] | 2.484 | 1.973 | 1.516 | 1.222 | 0.887 | 2.357 | 1.734 | 1.258 | 0.954 | 0.676 | 0.412 | 0.263 | 0.168 | 0.070 |
Galactic Extinction based on H I Column Densities and Galaxy Counts (Burstein & Heiles; 1982AJ.....87.1165B) assuming Rv = 3.1: AB = 0.790 mag
See Notes on Galactic Extinction for important caveats.
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