FOREGROUND GALACTIC EXTINCTION for SSTSL2 J163809.14-101242.3 (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] | 2.046 | 1.712 | 1.295 | 1.024 | 0.711 | 2.002 | 1.560 | 1.079 | 0.802 | 0.596 | 0.335 | 0.212 | 0.143 | 0.072 |
Show/Hide Aλ magnitudes in all 88 photometric bands based on SF11
Bandpass [µm] | Aλ [mag] |
Landolt | U | (0.35) | 2.046 |
Landolt | B | (0.43) | 1.712 |
Landolt | V | (0.54) | 1.295 |
Landolt | R | (0.64) | 1.024 |
Landolt | I | (0.80) | 0.711 |
CTIO | U | (0.37) | 1.939 |
CTIO | B | (0.43) | 1.719 |
CTIO | V | (0.55) | 1.266 |
CTIO | R | (0.65) | 1.001 |
CTIO | I | (0.80) | 0.716 |
UKIRT | J | (1.25) | 0.335 |
UKIRT | H | (1.66) | 0.212 |
UKIRT | K | (2.19) | 0.143 |
UKIRT | L' | (3.78) | 0.072 |
Gunn | g | (0.52) | 1.376 |
Gunn | r | (0.66) | 0.970 |
Gunn | i | (0.79) | 0.734 |
Gunn | z | (0.91) | 0.583 |
Spinrad | R_S | (0.69) | 0.907 |
Stromgren | u | (0.35) | 2.033 |
Stromgren | b | (0.47) | 1.582 |
Stromgren | v | (0.41) | 1.791 |
Stromgren | beta | (0.49) | 1.503 |
Stromgren | y | (0.55) | 1.268 |
SDSS | u | (0.36) | 2.002 |
SDSS | g | (0.47) | 1.560 |
SDSS | r | (0.62) | 1.079 |
SDSS | i | (0.75) | 0.802 |
SDSS | z | (0.89) | 0.596 |
DSS-II | g | (0.46) | 1.596 |
DSS-II | r | (0.65) | 0.986 |
DSS-II | i | (0.81) | 0.702 |
PS1 | g | (0.49) | 1.498 |
PS1 | r | (0.62) | 1.072 |
PS1 | i | (0.75) | 0.794 |
PS1 | z | (0.87) | 0.624 |
PS1 | y | (0.97) | 0.513 |
PS1 | w | (0.62) | 1.105 |
LSST | u | (0.37) | 1.957 |
LSST | g | (0.48) | 1.528 |
LSST | r | (0.62) | 1.073 |
LSST | i | (0.75) | 0.795 |
LSST | z | (0.87) | 0.625 |
LSST | y | (0.97) | 0.514 |
WFPC2 | F300W | (0.31) | 2.315 |
WFPC2 | F450W | (0.46) | 1.610 |
WFPC2 | F555W | (0.54) | 1.301 |
WFPC2 | F606W | (0.60) | 1.140 |
WFPC2 | F702W | (0.69) | 0.920 |
WFPC2 | F814W | (0.79) | 0.731 |
WFC3 | F105W | (1.04) | 0.458 |
WFC3 | F110W | (1.12) | 0.416 |
WFC3 | F125W | (1.23) | 0.343 |
WFC3 | F140W | (1.37) | 0.289 |
WFC3 | F160W | (1.53) | 0.242 |
WFC3 | F200LP | (0.55) | 1.397 |
WFC3 | F218W | (0.22) | 3.664 |
WFC3 | F225W | (0.24) | 3.300 |
WFC3 | F275W | (0.27) | 2.591 |
WFC3 | F300X | (0.29) | 2.469 |
WFC3 | F336W | (0.34) | 2.103 |
WFC3 | F350LP | (0.59) | 1.239 |
WFC3 | F390W | (0.40) | 1.840 |
WFC3 | F438W | (0.43) | 1.711 |
WFC3 | F475W | (0.48) | 1.534 |
WFC3 | F475X | (0.50) | 1.471 |
WFC3 | F555W | (0.53) | 1.348 |
WFC3 | F600LP | (0.74) | 0.841 |
WFC3 | F606W | (0.59) | 1.175 |
WFC3 | F625W | (0.62) | 1.067 |
WFC3 | F775W | (0.76) | 0.776 |
WFC3 | F814W | (0.80) | 0.725 |
WFC3 | F850LP | (0.91) | 0.570 |
ACS | clear | (0.62) | 1.150 |
ACS | F435W | (0.43) | 1.705 |
ACS | F475W | (0.48) | 1.543 |
ACS | F550M | (0.56) | 1.237 |
ACS | F555W | (0.54) | 1.318 |
ACS | F606W | (0.59) | 1.167 |
ACS | F625W | (0.63) | 1.048 |
ACS | F775W | (0.77) | 0.769 |
ACS | F814W | (0.80) | 0.721 |
ACS | F850LP | (0.90) | 0.587 |
DES | g | (0.48) | 1.528 |
DES | r | (0.64) | 1.027 |
DES | i | (0.78) | 0.753 |
DES | z | (0.91) | 0.575 |
DES | Y | (0.99) | 0.500 |
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] | 2.486 | 1.974 | 1.517 | 1.223 | 0.888 | 2.359 | 1.736 | 1.259 | 0.955 | 0.677 | 0.413 | 0.264 | 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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