FOREGROUND GALACTIC EXTINCTION for 2MASX J03142892+3058239 (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] | 1.397 | 1.169 | 0.884 | 0.699 | 0.485 | 1.366 | 1.065 | 0.736 | 0.547 | 0.407 | 0.229 | 0.145 | 0.097 | 0.049 |
Show/Hide Aλ magnitudes in all 88 photometric bands based on SF11
Bandpass [µm] | Aλ [mag] |
Landolt | U | (0.35) | 1.397 |
Landolt | B | (0.43) | 1.169 |
Landolt | V | (0.54) | 0.884 |
Landolt | R | (0.64) | 0.699 |
Landolt | I | (0.80) | 0.485 |
CTIO | U | (0.37) | 1.324 |
CTIO | B | (0.43) | 1.173 |
CTIO | V | (0.55) | 0.864 |
CTIO | R | (0.65) | 0.683 |
CTIO | I | (0.80) | 0.489 |
UKIRT | J | (1.25) | 0.229 |
UKIRT | H | (1.66) | 0.145 |
UKIRT | K | (2.19) | 0.097 |
UKIRT | L' | (3.78) | 0.049 |
Gunn | g | (0.52) | 0.939 |
Gunn | r | (0.66) | 0.662 |
Gunn | i | (0.79) | 0.501 |
Gunn | z | (0.91) | 0.398 |
Spinrad | R_S | (0.69) | 0.619 |
Stromgren | u | (0.35) | 1.387 |
Stromgren | b | (0.47) | 1.080 |
Stromgren | v | (0.41) | 1.222 |
Stromgren | beta | (0.49) | 1.026 |
Stromgren | y | (0.55) | 0.866 |
SDSS | u | (0.36) | 1.366 |
SDSS | g | (0.47) | 1.065 |
SDSS | r | (0.62) | 0.736 |
SDSS | i | (0.75) | 0.547 |
SDSS | z | (0.89) | 0.407 |
DSS-II | g | (0.46) | 1.090 |
DSS-II | r | (0.65) | 0.673 |
DSS-II | i | (0.81) | 0.479 |
PS1 | g | (0.49) | 1.022 |
PS1 | r | (0.62) | 0.732 |
PS1 | i | (0.75) | 0.542 |
PS1 | z | (0.87) | 0.426 |
PS1 | y | (0.97) | 0.350 |
PS1 | w | (0.62) | 0.754 |
LSST | u | (0.37) | 1.336 |
LSST | g | (0.48) | 1.043 |
LSST | r | (0.62) | 0.733 |
LSST | i | (0.75) | 0.543 |
LSST | z | (0.87) | 0.426 |
LSST | y | (0.97) | 0.351 |
WFPC2 | F300W | (0.31) | 1.580 |
WFPC2 | F450W | (0.46) | 1.099 |
WFPC2 | F555W | (0.54) | 0.888 |
WFPC2 | F606W | (0.60) | 0.778 |
WFPC2 | F702W | (0.69) | 0.628 |
WFPC2 | F814W | (0.79) | 0.499 |
WFC3 | F105W | (1.04) | 0.312 |
WFC3 | F110W | (1.12) | 0.284 |
WFC3 | F125W | (1.23) | 0.234 |
WFC3 | F140W | (1.37) | 0.198 |
WFC3 | F160W | (1.53) | 0.165 |
WFC3 | F200LP | (0.55) | 0.953 |
WFC3 | F218W | (0.22) | 2.501 |
WFC3 | F225W | (0.24) | 2.253 |
WFC3 | F275W | (0.27) | 1.768 |
WFC3 | F300X | (0.29) | 1.685 |
WFC3 | F336W | (0.34) | 1.435 |
WFC3 | F350LP | (0.59) | 0.846 |
WFC3 | F390W | (0.40) | 1.256 |
WFC3 | F438W | (0.43) | 1.168 |
WFC3 | F475W | (0.48) | 1.047 |
WFC3 | F475X | (0.50) | 1.004 |
WFC3 | F555W | (0.53) | 0.920 |
WFC3 | F600LP | (0.74) | 0.574 |
WFC3 | F606W | (0.59) | 0.802 |
WFC3 | F625W | (0.62) | 0.728 |
WFC3 | F775W | (0.76) | 0.530 |
WFC3 | F814W | (0.80) | 0.495 |
WFC3 | F850LP | (0.91) | 0.389 |
ACS | clear | (0.62) | 0.785 |
ACS | F435W | (0.43) | 1.163 |
ACS | F475W | (0.48) | 1.053 |
ACS | F550M | (0.56) | 0.844 |
ACS | F555W | (0.54) | 0.900 |
ACS | F606W | (0.59) | 0.796 |
ACS | F625W | (0.63) | 0.715 |
ACS | F775W | (0.77) | 0.525 |
ACS | F814W | (0.80) | 0.492 |
ACS | F850LP | (0.90) | 0.401 |
DES | g | (0.48) | 1.043 |
DES | r | (0.64) | 0.701 |
DES | i | (0.78) | 0.514 |
DES | z | (0.91) | 0.392 |
DES | Y | (0.99) | 0.341 |
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] | 1.702 | 1.352 | 1.038 | 0.837 | 0.608 | 1.615 | 1.188 | 0.862 | 0.653 | 0.463 | 0.283 | 0.180 | 0.115 | 0.048 |
Galactic Extinction based on H I Column Densities and Galaxy Counts (Burstein & Heiles; 1982AJ.....87.1165B) assuming Rv = 3.1: AB = 0.690 mag
See Notes on Galactic Extinction for important caveats.
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