FOREGROUND GALACTIC EXTINCTION for GRB 110212A (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] | 3.499 | 2.927 | 2.214 | 1.751 | 1.215 | 3.422 | 2.666 | 1.845 | 1.371 | 1.020 | 0.572 | 0.362 | 0.244 | 0.124 |
Show/Hide Aλ magnitudes in all 88 photometric bands based on SF11
Bandpass [µm] | Aλ [mag] |
Landolt | U | (0.35) | 3.499 |
Landolt | B | (0.43) | 2.927 |
Landolt | V | (0.54) | 2.214 |
Landolt | R | (0.64) | 1.751 |
Landolt | I | (0.80) | 1.215 |
CTIO | U | (0.37) | 3.316 |
CTIO | B | (0.43) | 2.939 |
CTIO | V | (0.55) | 2.165 |
CTIO | R | (0.65) | 1.711 |
CTIO | I | (0.80) | 1.224 |
UKIRT | J | (1.25) | 0.572 |
UKIRT | H | (1.66) | 0.362 |
UKIRT | K | (2.19) | 0.244 |
UKIRT | L' | (3.78) | 0.124 |
Gunn | g | (0.52) | 2.352 |
Gunn | r | (0.66) | 1.659 |
Gunn | i | (0.79) | 1.255 |
Gunn | z | (0.91) | 0.996 |
Spinrad | R_S | (0.69) | 1.551 |
Stromgren | u | (0.35) | 3.475 |
Stromgren | b | (0.47) | 2.704 |
Stromgren | v | (0.41) | 3.062 |
Stromgren | beta | (0.49) | 2.570 |
Stromgren | y | (0.55) | 2.168 |
SDSS | u | (0.36) | 3.422 |
SDSS | g | (0.47) | 2.666 |
SDSS | r | (0.62) | 1.845 |
SDSS | i | (0.75) | 1.371 |
SDSS | z | (0.89) | 1.020 |
DSS-II | g | (0.46) | 2.729 |
DSS-II | r | (0.65) | 1.686 |
DSS-II | i | (0.81) | 1.200 |
PS1 | g | (0.49) | 2.561 |
PS1 | r | (0.62) | 1.833 |
PS1 | i | (0.75) | 1.358 |
PS1 | z | (0.87) | 1.067 |
PS1 | y | (0.97) | 0.878 |
PS1 | w | (0.62) | 1.890 |
LSST | u | (0.37) | 3.346 |
LSST | g | (0.48) | 2.613 |
LSST | r | (0.62) | 1.835 |
LSST | i | (0.75) | 1.359 |
LSST | z | (0.87) | 1.068 |
LSST | y | (0.97) | 0.878 |
WFPC2 | F300W | (0.31) | 3.957 |
WFPC2 | F450W | (0.46) | 2.753 |
WFPC2 | F555W | (0.54) | 2.224 |
WFPC2 | F606W | (0.60) | 1.950 |
WFPC2 | F702W | (0.69) | 1.573 |
WFPC2 | F814W | (0.79) | 1.250 |
WFC3 | F105W | (1.04) | 0.782 |
WFC3 | F110W | (1.12) | 0.711 |
WFC3 | F125W | (1.23) | 0.586 |
WFC3 | F140W | (1.37) | 0.495 |
WFC3 | F160W | (1.53) | 0.413 |
WFC3 | F200LP | (0.55) | 2.388 |
WFC3 | F218W | (0.22) | 6.265 |
WFC3 | F225W | (0.24) | 5.642 |
WFC3 | F275W | (0.27) | 4.430 |
WFC3 | F300X | (0.29) | 4.221 |
WFC3 | F336W | (0.34) | 3.595 |
WFC3 | F350LP | (0.59) | 2.118 |
WFC3 | F390W | (0.40) | 3.145 |
WFC3 | F438W | (0.43) | 2.925 |
WFC3 | F475W | (0.48) | 2.622 |
WFC3 | F475X | (0.50) | 2.516 |
WFC3 | F555W | (0.53) | 2.305 |
WFC3 | F600LP | (0.74) | 1.438 |
WFC3 | F606W | (0.59) | 2.009 |
WFC3 | F625W | (0.62) | 1.824 |
WFC3 | F775W | (0.76) | 1.326 |
WFC3 | F814W | (0.80) | 1.240 |
WFC3 | F850LP | (0.91) | 0.975 |
ACS | clear | (0.62) | 1.967 |
ACS | F435W | (0.43) | 2.914 |
ACS | F475W | (0.48) | 2.638 |
ACS | F550M | (0.56) | 2.115 |
ACS | F555W | (0.54) | 2.254 |
ACS | F606W | (0.59) | 1.995 |
ACS | F625W | (0.63) | 1.791 |
ACS | F775W | (0.77) | 1.315 |
ACS | F814W | (0.80) | 1.232 |
ACS | F850LP | (0.90) | 1.003 |
DES | g | (0.48) | 2.613 |
DES | r | (0.64) | 1.757 |
DES | i | (0.78) | 1.288 |
DES | z | (0.91) | 0.982 |
DES | Y | (0.99) | 0.854 |
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] | 4.430 | 3.518 | 2.702 | 2.179 | 1.581 | 4.202 | 3.092 | 2.243 | 1.700 | 1.206 | 0.735 | 0.470 | 0.299 | 0.125 |
See Notes on Galactic Extinction for important caveats.
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