FOREGROUND GALACTIC EXTINCTION for GRB 080702A (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] | 2.880 | 2.409 | 1.822 | 1.441 | 1.000 | 2.817 | 2.195 | 1.518 | 1.128 | 0.839 | 0.471 | 0.298 | 0.201 | 0.102 |
Show/Hide Aλ magnitudes in all 88 photometric bands based on SF11
Bandpass [µm] | Aλ [mag] |
Landolt | U | (0.35) | 2.880 |
Landolt | B | (0.43) | 2.409 |
Landolt | V | (0.54) | 1.822 |
Landolt | R | (0.64) | 1.441 |
Landolt | I | (0.80) | 1.000 |
CTIO | U | (0.37) | 2.729 |
CTIO | B | (0.43) | 2.419 |
CTIO | V | (0.55) | 1.782 |
CTIO | R | (0.65) | 1.408 |
CTIO | I | (0.80) | 1.007 |
UKIRT | J | (1.25) | 0.471 |
UKIRT | H | (1.66) | 0.298 |
UKIRT | K | (2.19) | 0.201 |
UKIRT | L' | (3.78) | 0.102 |
Gunn | g | (0.52) | 1.936 |
Gunn | r | (0.66) | 1.365 |
Gunn | i | (0.79) | 1.033 |
Gunn | z | (0.91) | 0.820 |
Spinrad | R_S | (0.69) | 1.276 |
Stromgren | u | (0.35) | 2.860 |
Stromgren | b | (0.47) | 2.226 |
Stromgren | v | (0.41) | 2.520 |
Stromgren | beta | (0.49) | 2.115 |
Stromgren | y | (0.55) | 1.785 |
SDSS | u | (0.36) | 2.817 |
SDSS | g | (0.47) | 2.195 |
SDSS | r | (0.62) | 1.518 |
SDSS | i | (0.75) | 1.128 |
SDSS | z | (0.89) | 0.839 |
DSS-II | g | (0.46) | 2.246 |
DSS-II | r | (0.65) | 1.387 |
DSS-II | i | (0.81) | 0.988 |
PS1 | g | (0.49) | 2.108 |
PS1 | r | (0.62) | 1.509 |
PS1 | i | (0.75) | 1.118 |
PS1 | z | (0.87) | 0.878 |
PS1 | y | (0.97) | 0.722 |
PS1 | w | (0.62) | 1.555 |
LSST | u | (0.37) | 2.754 |
LSST | g | (0.48) | 2.151 |
LSST | r | (0.62) | 1.510 |
LSST | i | (0.75) | 1.119 |
LSST | z | (0.87) | 0.879 |
LSST | y | (0.97) | 0.723 |
WFPC2 | F300W | (0.31) | 3.257 |
WFPC2 | F450W | (0.46) | 2.266 |
WFPC2 | F555W | (0.54) | 1.831 |
WFPC2 | F606W | (0.60) | 1.605 |
WFPC2 | F702W | (0.69) | 1.294 |
WFPC2 | F814W | (0.79) | 1.029 |
WFC3 | F105W | (1.04) | 0.644 |
WFC3 | F110W | (1.12) | 0.585 |
WFC3 | F125W | (1.23) | 0.482 |
WFC3 | F140W | (1.37) | 0.407 |
WFC3 | F160W | (1.53) | 0.340 |
WFC3 | F200LP | (0.55) | 1.965 |
WFC3 | F218W | (0.22) | 5.156 |
WFC3 | F225W | (0.24) | 4.644 |
WFC3 | F275W | (0.27) | 3.646 |
WFC3 | F300X | (0.29) | 3.474 |
WFC3 | F336W | (0.34) | 2.959 |
WFC3 | F350LP | (0.59) | 1.743 |
WFC3 | F390W | (0.40) | 2.589 |
WFC3 | F438W | (0.43) | 2.407 |
WFC3 | F475W | (0.48) | 2.158 |
WFC3 | F475X | (0.50) | 2.070 |
WFC3 | F555W | (0.53) | 1.897 |
WFC3 | F600LP | (0.74) | 1.183 |
WFC3 | F606W | (0.59) | 1.653 |
WFC3 | F625W | (0.62) | 1.501 |
WFC3 | F775W | (0.76) | 1.092 |
WFC3 | F814W | (0.80) | 1.021 |
WFC3 | F850LP | (0.91) | 0.803 |
ACS | clear | (0.62) | 1.619 |
ACS | F435W | (0.43) | 2.399 |
ACS | F475W | (0.48) | 2.171 |
ACS | F550M | (0.56) | 1.741 |
ACS | F555W | (0.54) | 1.855 |
ACS | F606W | (0.59) | 1.642 |
ACS | F625W | (0.63) | 1.474 |
ACS | F775W | (0.77) | 1.082 |
ACS | F814W | (0.80) | 1.014 |
ACS | F850LP | (0.90) | 0.826 |
DES | g | (0.48) | 2.151 |
DES | r | (0.64) | 1.446 |
DES | i | (0.78) | 1.060 |
DES | z | (0.91) | 0.809 |
DES | Y | (0.99) | 0.703 |
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] | 3.537 | 2.808 | 2.158 | 1.740 | 1.263 | 3.355 | 2.469 | 1.790 | 1.358 | 0.963 | 0.587 | 0.375 | 0.239 | 0.100 |
Galactic Extinction based on H I Column Densities and Galaxy Counts (Burstein & Heiles; 1982AJ.....87.1165B) assuming Rv = 3.1: AB = 1.160 mag
See Notes on Galactic Extinction for important caveats.
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