FOREGROUND GALACTIC EXTINCTION for GRB 070419B (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] | 0.391 | 0.327 | 0.248 | 0.196 | 0.136 | 0.383 | 0.298 | 0.206 | 0.153 | 0.114 | 0.064 | 0.041 | 0.027 | 0.014 |
Show/Hide Aλ magnitudes in all 88 photometric bands based on SF11
Bandpass [µm] | Aλ [mag] |
Landolt | U | (0.35) | 0.391 |
Landolt | B | (0.43) | 0.327 |
Landolt | V | (0.54) | 0.248 |
Landolt | R | (0.64) | 0.196 |
Landolt | I | (0.80) | 0.136 |
CTIO | U | (0.37) | 0.371 |
CTIO | B | (0.43) | 0.329 |
CTIO | V | (0.55) | 0.242 |
CTIO | R | (0.65) | 0.191 |
CTIO | I | (0.80) | 0.137 |
UKIRT | J | (1.25) | 0.064 |
UKIRT | H | (1.66) | 0.041 |
UKIRT | K | (2.19) | 0.027 |
UKIRT | L' | (3.78) | 0.014 |
Gunn | g | (0.52) | 0.263 |
Gunn | r | (0.66) | 0.186 |
Gunn | i | (0.79) | 0.140 |
Gunn | z | (0.91) | 0.111 |
Spinrad | R_S | (0.69) | 0.173 |
Stromgren | u | (0.35) | 0.389 |
Stromgren | b | (0.47) | 0.303 |
Stromgren | v | (0.41) | 0.343 |
Stromgren | beta | (0.49) | 0.287 |
Stromgren | y | (0.55) | 0.243 |
SDSS | u | (0.36) | 0.383 |
SDSS | g | (0.47) | 0.298 |
SDSS | r | (0.62) | 0.206 |
SDSS | i | (0.75) | 0.153 |
SDSS | z | (0.89) | 0.114 |
DSS-II | g | (0.46) | 0.305 |
DSS-II | r | (0.65) | 0.189 |
DSS-II | i | (0.81) | 0.134 |
PS1 | g | (0.49) | 0.286 |
PS1 | r | (0.62) | 0.205 |
PS1 | i | (0.75) | 0.152 |
PS1 | z | (0.87) | 0.119 |
PS1 | y | (0.97) | 0.098 |
PS1 | w | (0.62) | 0.211 |
LSST | u | (0.37) | 0.374 |
LSST | g | (0.48) | 0.292 |
LSST | r | (0.62) | 0.205 |
LSST | i | (0.75) | 0.152 |
LSST | z | (0.87) | 0.119 |
LSST | y | (0.97) | 0.098 |
WFPC2 | F300W | (0.31) | 0.443 |
WFPC2 | F450W | (0.46) | 0.308 |
WFPC2 | F555W | (0.54) | 0.249 |
WFPC2 | F606W | (0.60) | 0.218 |
WFPC2 | F702W | (0.69) | 0.176 |
WFPC2 | F814W | (0.79) | 0.140 |
WFC3 | F105W | (1.04) | 0.088 |
WFC3 | F110W | (1.12) | 0.080 |
WFC3 | F125W | (1.23) | 0.066 |
WFC3 | F140W | (1.37) | 0.055 |
WFC3 | F160W | (1.53) | 0.046 |
WFC3 | F200LP | (0.55) | 0.267 |
WFC3 | F218W | (0.22) | 0.701 |
WFC3 | F225W | (0.24) | 0.631 |
WFC3 | F275W | (0.27) | 0.496 |
WFC3 | F300X | (0.29) | 0.472 |
WFC3 | F336W | (0.34) | 0.402 |
WFC3 | F350LP | (0.59) | 0.237 |
WFC3 | F390W | (0.40) | 0.352 |
WFC3 | F438W | (0.43) | 0.327 |
WFC3 | F475W | (0.48) | 0.293 |
WFC3 | F475X | (0.50) | 0.281 |
WFC3 | F555W | (0.53) | 0.258 |
WFC3 | F600LP | (0.74) | 0.161 |
WFC3 | F606W | (0.59) | 0.225 |
WFC3 | F625W | (0.62) | 0.204 |
WFC3 | F775W | (0.76) | 0.148 |
WFC3 | F814W | (0.80) | 0.139 |
WFC3 | F850LP | (0.91) | 0.109 |
ACS | clear | (0.62) | 0.220 |
ACS | F435W | (0.43) | 0.326 |
ACS | F475W | (0.48) | 0.295 |
ACS | F550M | (0.56) | 0.237 |
ACS | F555W | (0.54) | 0.252 |
ACS | F606W | (0.59) | 0.223 |
ACS | F625W | (0.63) | 0.200 |
ACS | F775W | (0.77) | 0.147 |
ACS | F814W | (0.80) | 0.138 |
ACS | F850LP | (0.90) | 0.112 |
DES | g | (0.48) | 0.292 |
DES | r | (0.64) | 0.197 |
DES | i | (0.78) | 0.144 |
DES | z | (0.91) | 0.110 |
DES | Y | (0.99) | 0.096 |
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] | 0.495 | 0.393 | 0.302 | 0.243 | 0.177 | 0.470 | 0.345 | 0.251 | 0.190 | 0.135 | 0.082 | 0.052 | 0.033 | 0.014 |
Galactic Extinction based on H I Column Densities and Galaxy Counts (Burstein & Heiles; 1982AJ.....87.1165B) assuming Rv = 3.1: AB = 0.340 mag
See Notes on Galactic Extinction for important caveats.
|