FOREGROUND GALACTIC EXTINCTION for NGC 2260 (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] | 5.664 | 4.739 | 3.584 | 2.835 | 1.967 | 5.540 | 4.317 | 2.986 | 2.219 | 1.651 | 0.927 | 0.587 | 0.395 | 0.200 |
Show/Hide Aλ magnitudes in all 88 photometric bands based on SF11
Bandpass [µm] | Aλ [mag] |
Landolt | U | (0.35) | 5.664 |
Landolt | B | (0.43) | 4.739 |
Landolt | V | (0.54) | 3.584 |
Landolt | R | (0.64) | 2.835 |
Landolt | I | (0.80) | 1.967 |
CTIO | U | (0.37) | 5.368 |
CTIO | B | (0.43) | 4.759 |
CTIO | V | (0.55) | 3.505 |
CTIO | R | (0.65) | 2.769 |
CTIO | I | (0.80) | 1.981 |
UKIRT | J | (1.25) | 0.927 |
UKIRT | H | (1.66) | 0.587 |
UKIRT | K | (2.19) | 0.395 |
UKIRT | L' | (3.78) | 0.200 |
Gunn | g | (0.52) | 3.809 |
Gunn | r | (0.66) | 2.686 |
Gunn | i | (0.79) | 2.032 |
Gunn | z | (0.91) | 1.613 |
Spinrad | R_S | (0.69) | 2.511 |
Stromgren | u | (0.35) | 5.627 |
Stromgren | b | (0.47) | 4.378 |
Stromgren | v | (0.41) | 4.957 |
Stromgren | beta | (0.49) | 4.160 |
Stromgren | y | (0.55) | 3.511 |
SDSS | u | (0.36) | 5.540 |
SDSS | g | (0.47) | 4.317 |
SDSS | r | (0.62) | 2.986 |
SDSS | i | (0.75) | 2.219 |
SDSS | z | (0.89) | 1.651 |
DSS-II | g | (0.46) | 4.419 |
DSS-II | r | (0.65) | 2.729 |
DSS-II | i | (0.81) | 1.943 |
PS1 | g | (0.49) | 4.146 |
PS1 | r | (0.62) | 2.968 |
PS1 | i | (0.75) | 2.198 |
PS1 | z | (0.87) | 1.728 |
PS1 | y | (0.97) | 1.421 |
PS1 | w | (0.62) | 3.060 |
LSST | u | (0.37) | 5.417 |
LSST | g | (0.48) | 4.231 |
LSST | r | (0.62) | 2.971 |
LSST | i | (0.75) | 2.201 |
LSST | z | (0.87) | 1.729 |
LSST | y | (0.97) | 1.422 |
WFPC2 | F300W | (0.31) | 6.407 |
WFPC2 | F450W | (0.46) | 4.457 |
WFPC2 | F555W | (0.54) | 3.601 |
WFPC2 | F606W | (0.60) | 3.156 |
WFPC2 | F702W | (0.69) | 2.546 |
WFPC2 | F814W | (0.79) | 2.025 |
WFC3 | F105W | (1.04) | 1.266 |
WFC3 | F110W | (1.12) | 1.151 |
WFC3 | F125W | (1.23) | 0.949 |
WFC3 | F140W | (1.37) | 0.801 |
WFC3 | F160W | (1.53) | 0.669 |
WFC3 | F200LP | (0.55) | 3.866 |
WFC3 | F218W | (0.22) | 10.142 |
WFC3 | F225W | (0.24) | 9.134 |
WFC3 | F275W | (0.27) | 7.171 |
WFC3 | F300X | (0.29) | 6.833 |
WFC3 | F336W | (0.34) | 5.820 |
WFC3 | F350LP | (0.59) | 3.430 |
WFC3 | F390W | (0.40) | 5.092 |
WFC3 | F438W | (0.43) | 4.735 |
WFC3 | F475W | (0.48) | 4.245 |
WFC3 | F475X | (0.50) | 4.073 |
WFC3 | F555W | (0.53) | 3.731 |
WFC3 | F600LP | (0.74) | 2.328 |
WFC3 | F606W | (0.59) | 3.252 |
WFC3 | F625W | (0.62) | 2.952 |
WFC3 | F775W | (0.76) | 2.147 |
WFC3 | F814W | (0.80) | 2.008 |
WFC3 | F850LP | (0.91) | 1.579 |
ACS | clear | (0.62) | 3.184 |
ACS | F435W | (0.43) | 4.718 |
ACS | F475W | (0.48) | 4.271 |
ACS | F550M | (0.56) | 3.424 |
ACS | F555W | (0.54) | 3.649 |
ACS | F606W | (0.59) | 3.230 |
ACS | F625W | (0.63) | 2.900 |
ACS | F775W | (0.77) | 2.129 |
ACS | F814W | (0.80) | 1.994 |
ACS | F850LP | (0.90) | 1.625 |
DES | g | (0.48) | 4.231 |
DES | r | (0.64) | 2.844 |
DES | i | (0.78) | 2.085 |
DES | z | (0.91) | 1.591 |
DES | Y | (0.99) | 1.383 |
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] | 6.827 | 5.421 | 4.165 | 3.358 | 2.437 | 6.477 | 4.766 | 3.456 | 2.621 | 1.858 | 1.133 | 0.724 | 0.461 | 0.192 |
See Notes on Galactic Extinction for important caveats.
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