| Space Telescope Science Institute |
| WFC3 Instrument Handbook |
| help@stsci.edu |
Figure A.229: Integrated system throughput for F167N.Figure A.230: Point source S/N vs. V+ABν for the F167N filter, assuming high sky backgrounds and a 3×3 pixel aperture.Figure A.231: Extended source S/N vs. V+ABν for the F167N filter, assuming high sky backgrounds and a source uniformly filling a 1 arcsec2 aperture.
Table A.1: Color corrections ABν to go from Johnson V magnitude to AB magnitude for WFC3 as a function of stellar effective temperature. Teff
Table A.2: Color corrections ABν to go from Johnson V magnitude to AB magnitude for WFC3 as a function of age in an instantaneous burst population.
Table A.3: Color corrections ABν to go from Johnson V magnitude to AB magnitude for WFC3 as a function of age in a population with constant star formation.