FOREGROUND GALACTIC EXTINCTION for GRB 090712 (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] | 1.443 | 1.207 | 0.913 | 0.722 | 0.501 | 1.411 | 1.100 | 0.761 | 0.565 | 0.421 | 0.236 | 0.149 | 0.101 | 0.051 |
Show/Hide Aλ magnitudes in all 88 photometric bands based on SF11
Bandpass [µm] | Aλ [mag] |
Landolt | U | (0.35) | 1.443 |
Landolt | B | (0.43) | 1.207 |
Landolt | V | (0.54) | 0.913 |
Landolt | R | (0.64) | 0.722 |
Landolt | I | (0.80) | 0.501 |
CTIO | U | (0.37) | 1.367 |
CTIO | B | (0.43) | 1.212 |
CTIO | V | (0.55) | 0.893 |
CTIO | R | (0.65) | 0.706 |
CTIO | I | (0.80) | 0.505 |
UKIRT | J | (1.25) | 0.236 |
UKIRT | H | (1.66) | 0.149 |
UKIRT | K | (2.19) | 0.101 |
UKIRT | L' | (3.78) | 0.051 |
Gunn | g | (0.52) | 0.970 |
Gunn | r | (0.66) | 0.684 |
Gunn | i | (0.79) | 0.518 |
Gunn | z | (0.91) | 0.411 |
Spinrad | R_S | (0.69) | 0.640 |
Stromgren | u | (0.35) | 1.433 |
Stromgren | b | (0.47) | 1.115 |
Stromgren | v | (0.41) | 1.263 |
Stromgren | beta | (0.49) | 1.060 |
Stromgren | y | (0.55) | 0.894 |
SDSS | u | (0.36) | 1.411 |
SDSS | g | (0.47) | 1.100 |
SDSS | r | (0.62) | 0.761 |
SDSS | i | (0.75) | 0.565 |
SDSS | z | (0.89) | 0.421 |
DSS-II | g | (0.46) | 1.126 |
DSS-II | r | (0.65) | 0.695 |
DSS-II | i | (0.81) | 0.495 |
PS1 | g | (0.49) | 1.056 |
PS1 | r | (0.62) | 0.756 |
PS1 | i | (0.75) | 0.560 |
PS1 | z | (0.87) | 0.440 |
PS1 | y | (0.97) | 0.362 |
PS1 | w | (0.62) | 0.779 |
LSST | u | (0.37) | 1.380 |
LSST | g | (0.48) | 1.078 |
LSST | r | (0.62) | 0.757 |
LSST | i | (0.75) | 0.561 |
LSST | z | (0.87) | 0.441 |
LSST | y | (0.97) | 0.362 |
WFPC2 | F300W | (0.31) | 1.632 |
WFPC2 | F450W | (0.46) | 1.135 |
WFPC2 | F555W | (0.54) | 0.917 |
WFPC2 | F606W | (0.60) | 0.804 |
WFPC2 | F702W | (0.69) | 0.649 |
WFPC2 | F814W | (0.79) | 0.516 |
WFC3 | F105W | (1.04) | 0.323 |
WFC3 | F110W | (1.12) | 0.293 |
WFC3 | F125W | (1.23) | 0.242 |
WFC3 | F140W | (1.37) | 0.204 |
WFC3 | F160W | (1.53) | 0.170 |
WFC3 | F200LP | (0.55) | 0.985 |
WFC3 | F218W | (0.22) | 2.584 |
WFC3 | F225W | (0.24) | 2.327 |
WFC3 | F275W | (0.27) | 1.827 |
WFC3 | F300X | (0.29) | 1.741 |
WFC3 | F336W | (0.34) | 1.483 |
WFC3 | F350LP | (0.59) | 0.874 |
WFC3 | F390W | (0.40) | 1.297 |
WFC3 | F438W | (0.43) | 1.206 |
WFC3 | F475W | (0.48) | 1.081 |
WFC3 | F475X | (0.50) | 1.038 |
WFC3 | F555W | (0.53) | 0.951 |
WFC3 | F600LP | (0.74) | 0.593 |
WFC3 | F606W | (0.59) | 0.828 |
WFC3 | F625W | (0.62) | 0.752 |
WFC3 | F775W | (0.76) | 0.547 |
WFC3 | F814W | (0.80) | 0.511 |
WFC3 | F850LP | (0.91) | 0.402 |
ACS | clear | (0.62) | 0.811 |
ACS | F435W | (0.43) | 1.202 |
ACS | F475W | (0.48) | 1.088 |
ACS | F550M | (0.56) | 0.872 |
ACS | F555W | (0.54) | 0.930 |
ACS | F606W | (0.59) | 0.823 |
ACS | F625W | (0.63) | 0.739 |
ACS | F775W | (0.77) | 0.542 |
ACS | F814W | (0.80) | 0.508 |
ACS | F850LP | (0.90) | 0.414 |
DES | g | (0.48) | 1.078 |
DES | r | (0.64) | 0.725 |
DES | i | (0.78) | 0.531 |
DES | z | (0.91) | 0.405 |
DES | Y | (0.99) | 0.352 |
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] | 1.808 | 1.435 | 1.103 | 0.889 | 0.645 | 1.715 | 1.262 | 0.915 | 0.694 | 0.492 | 0.300 | 0.192 | 0.122 | 0.051 |
Galactic Extinction based on H I Column Densities and Galaxy Counts (Burstein & Heiles; 1982AJ.....87.1165B) assuming Rv = 3.1: AB = 1.710 mag
See Notes on Galactic Extinction for important caveats.
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