FOREGROUND GALACTIC EXTINCTION for GRB 100206A (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] | 1.645 | 1.376 | 1.041 | 0.823 | 0.571 | 1.609 | 1.254 | 0.867 | 0.645 | 0.479 | 0.269 | 0.170 | 0.115 | 0.058 |
Show/Hide Aλ magnitudes in all 88 photometric bands based on SF11
Bandpass [µm] | Aλ [mag] |
Landolt | U | (0.35) | 1.645 |
Landolt | B | (0.43) | 1.376 |
Landolt | V | (0.54) | 1.041 |
Landolt | R | (0.64) | 0.823 |
Landolt | I | (0.80) | 0.571 |
CTIO | U | (0.37) | 1.559 |
CTIO | B | (0.43) | 1.382 |
CTIO | V | (0.55) | 1.018 |
CTIO | R | (0.65) | 0.804 |
CTIO | I | (0.80) | 0.575 |
UKIRT | J | (1.25) | 0.269 |
UKIRT | H | (1.66) | 0.170 |
UKIRT | K | (2.19) | 0.115 |
UKIRT | L' | (3.78) | 0.058 |
Gunn | g | (0.52) | 1.106 |
Gunn | r | (0.66) | 0.780 |
Gunn | i | (0.79) | 0.590 |
Gunn | z | (0.91) | 0.468 |
Spinrad | R_S | (0.69) | 0.729 |
Stromgren | u | (0.35) | 1.634 |
Stromgren | b | (0.47) | 1.272 |
Stromgren | v | (0.41) | 1.440 |
Stromgren | beta | (0.49) | 1.208 |
Stromgren | y | (0.55) | 1.020 |
SDSS | u | (0.36) | 1.609 |
SDSS | g | (0.47) | 1.254 |
SDSS | r | (0.62) | 0.867 |
SDSS | i | (0.75) | 0.645 |
SDSS | z | (0.89) | 0.479 |
DSS-II | g | (0.46) | 1.283 |
DSS-II | r | (0.65) | 0.793 |
DSS-II | i | (0.81) | 0.564 |
PS1 | g | (0.49) | 1.204 |
PS1 | r | (0.62) | 0.862 |
PS1 | i | (0.75) | 0.639 |
PS1 | z | (0.87) | 0.502 |
PS1 | y | (0.97) | 0.413 |
PS1 | w | (0.62) | 0.889 |
LSST | u | (0.37) | 1.573 |
LSST | g | (0.48) | 1.229 |
LSST | r | (0.62) | 0.863 |
LSST | i | (0.75) | 0.639 |
LSST | z | (0.87) | 0.502 |
LSST | y | (0.97) | 0.413 |
WFPC2 | F300W | (0.31) | 1.861 |
WFPC2 | F450W | (0.46) | 1.294 |
WFPC2 | F555W | (0.54) | 1.046 |
WFPC2 | F606W | (0.60) | 0.917 |
WFPC2 | F702W | (0.69) | 0.739 |
WFPC2 | F814W | (0.79) | 0.588 |
WFC3 | F105W | (1.04) | 0.368 |
WFC3 | F110W | (1.12) | 0.334 |
WFC3 | F125W | (1.23) | 0.276 |
WFC3 | F140W | (1.37) | 0.233 |
WFC3 | F160W | (1.53) | 0.194 |
WFC3 | F200LP | (0.55) | 1.123 |
WFC3 | F218W | (0.22) | 2.946 |
WFC3 | F225W | (0.24) | 2.653 |
WFC3 | F275W | (0.27) | 2.083 |
WFC3 | F300X | (0.29) | 1.985 |
WFC3 | F336W | (0.34) | 1.690 |
WFC3 | F350LP | (0.59) | 0.996 |
WFC3 | F390W | (0.40) | 1.479 |
WFC3 | F438W | (0.43) | 1.375 |
WFC3 | F475W | (0.48) | 1.233 |
WFC3 | F475X | (0.50) | 1.183 |
WFC3 | F555W | (0.53) | 1.084 |
WFC3 | F600LP | (0.74) | 0.676 |
WFC3 | F606W | (0.59) | 0.944 |
WFC3 | F625W | (0.62) | 0.858 |
WFC3 | F775W | (0.76) | 0.624 |
WFC3 | F814W | (0.80) | 0.583 |
WFC3 | F850LP | (0.91) | 0.459 |
ACS | clear | (0.62) | 0.925 |
ACS | F435W | (0.43) | 1.370 |
ACS | F475W | (0.48) | 1.241 |
ACS | F550M | (0.56) | 0.995 |
ACS | F555W | (0.54) | 1.060 |
ACS | F606W | (0.59) | 0.938 |
ACS | F625W | (0.63) | 0.842 |
ACS | F775W | (0.77) | 0.618 |
ACS | F814W | (0.80) | 0.579 |
ACS | F850LP | (0.90) | 0.472 |
DES | g | (0.48) | 1.229 |
DES | r | (0.64) | 0.826 |
DES | i | (0.78) | 0.605 |
DES | z | (0.91) | 0.462 |
DES | Y | (0.99) | 0.402 |
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] | 2.078 | 1.650 | 1.268 | 1.022 | 0.742 | 1.972 | 1.451 | 1.052 | 0.798 | 0.566 | 0.345 | 0.220 | 0.140 | 0.059 |
Galactic Extinction based on H I Column Densities and Galaxy Counts (Burstein & Heiles; 1982AJ.....87.1165B) assuming Rv = 3.1: AB = 0.670 mag
See Notes on Galactic Extinction for important caveats.
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