FOREGROUND GALACTIC EXTINCTION for SSTSL2 J174232.10-263739.3 (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.
WARNING: This position with |Galactic latitude| < 5 deg has unreliable extinction estimates.
| 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] | 9.341 | 7.815 | 5.910 | 4.675 | 3.244 | 9.136 | 7.119 | 4.925 | 3.660 | 2.722 | 1.528 | 0.968 | 0.651 | 0.330 |
Show/Hide Aλ magnitudes in all 88 photometric bands based on SF11
Bandpass [µm] | Aλ [mag] |
Landolt | U | (0.35) | 9.341 |
Landolt | B | (0.43) | 7.815 |
Landolt | V | (0.54) | 5.910 |
Landolt | R | (0.64) | 4.675 |
Landolt | I | (0.80) | 3.244 |
CTIO | U | (0.37) | 8.852 |
CTIO | B | (0.43) | 7.847 |
CTIO | V | (0.55) | 5.781 |
CTIO | R | (0.65) | 4.567 |
CTIO | I | (0.80) | 3.267 |
UKIRT | J | (1.25) | 1.528 |
UKIRT | H | (1.66) | 0.968 |
UKIRT | K | (2.19) | 0.651 |
UKIRT | L' | (3.78) | 0.330 |
Gunn | g | (0.52) | 6.281 |
Gunn | r | (0.66) | 4.429 |
Gunn | i | (0.79) | 3.352 |
Gunn | z | (0.91) | 2.660 |
Spinrad | R_S | (0.69) | 4.140 |
Stromgren | u | (0.35) | 9.279 |
Stromgren | b | (0.47) | 7.220 |
Stromgren | v | (0.41) | 8.175 |
Stromgren | beta | (0.49) | 6.860 |
Stromgren | y | (0.55) | 5.789 |
SDSS | u | (0.36) | 9.136 |
SDSS | g | (0.47) | 7.119 |
SDSS | r | (0.62) | 4.925 |
SDSS | i | (0.75) | 3.660 |
SDSS | z | (0.89) | 2.722 |
DSS-II | g | (0.46) | 7.287 |
DSS-II | r | (0.65) | 4.500 |
DSS-II | i | (0.81) | 3.205 |
PS1 | g | (0.49) | 6.837 |
PS1 | r | (0.62) | 4.895 |
PS1 | i | (0.75) | 3.625 |
PS1 | z | (0.87) | 2.849 |
PS1 | y | (0.97) | 2.343 |
PS1 | w | (0.62) | 5.046 |
LSST | u | (0.37) | 8.934 |
LSST | g | (0.48) | 6.977 |
LSST | r | (0.62) | 4.899 |
LSST | i | (0.75) | 3.630 |
LSST | z | (0.87) | 2.851 |
LSST | y | (0.97) | 2.345 |
WFPC2 | F300W | (0.31) | 10.565 |
WFPC2 | F450W | (0.46) | 7.350 |
WFPC2 | F555W | (0.54) | 5.938 |
WFPC2 | F606W | (0.60) | 5.205 |
WFPC2 | F702W | (0.69) | 4.199 |
WFPC2 | F814W | (0.79) | 3.339 |
WFC3 | F105W | (1.04) | 2.088 |
WFC3 | F110W | (1.12) | 1.899 |
WFC3 | F125W | (1.23) | 1.565 |
WFC3 | F140W | (1.37) | 1.321 |
WFC3 | F160W | (1.53) | 1.104 |
WFC3 | F200LP | (0.55) | 6.375 |
WFC3 | F218W | (0.22) | 16.725 |
WFC3 | F225W | (0.24) | 15.063 |
WFC3 | F275W | (0.27) | 11.826 |
WFC3 | F300X | (0.29) | 11.268 |
WFC3 | F336W | (0.34) | 9.598 |
WFC3 | F350LP | (0.59) | 5.656 |
WFC3 | F390W | (0.40) | 8.397 |
WFC3 | F438W | (0.43) | 7.809 |
WFC3 | F475W | (0.48) | 7.000 |
WFC3 | F475X | (0.50) | 6.716 |
WFC3 | F555W | (0.53) | 6.153 |
WFC3 | F600LP | (0.74) | 3.839 |
WFC3 | F606W | (0.59) | 5.362 |
WFC3 | F625W | (0.62) | 4.869 |
WFC3 | F775W | (0.76) | 3.541 |
WFC3 | F814W | (0.80) | 3.311 |
WFC3 | F850LP | (0.91) | 2.604 |
ACS | clear | (0.62) | 5.250 |
ACS | F435W | (0.43) | 7.781 |
ACS | F475W | (0.48) | 7.044 |
ACS | F550M | (0.56) | 5.647 |
ACS | F555W | (0.54) | 6.018 |
ACS | F606W | (0.59) | 5.326 |
ACS | F625W | (0.63) | 4.783 |
ACS | F775W | (0.77) | 3.511 |
ACS | F814W | (0.80) | 3.289 |
ACS | F850LP | (0.90) | 2.679 |
DES | g | (0.48) | 6.977 |
DES | r | (0.64) | 4.690 |
DES | i | (0.78) | 3.438 |
DES | z | (0.91) | 2.623 |
DES | Y | (0.99) | 2.280 |
For completeness, we include the original SFD98 values:
WARNING: This position with |Galactic latitude| < 5 deg has unreliable extinction estimates.
| 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] | 11.311 | 8.982 | 6.900 | 5.564 | 4.038 | 10.730 | 7.895 | 5.726 | 4.342 | 3.079 | 1.878 | 1.199 | 0.764 | 0.318 |
See Notes on Galactic Extinction for important caveats.
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