  The tip of the red giant (TRGB) is a standardizable candle and is
identifiable as the discontinuity at the bright extreme of the red giant branch
(RGB) stars in color-magnitude diagram (CMD) space. The TRGB-based distance
method has been calibrated and used to measured distances to galaxies out to
$D\leq20$ Mpc with the $I$-band equivalent Hubble Space Telescope ($HST$)
$F814W$ filter, and as an important rung in the distance ladder to measure the
Hubble constant, $H_0$. In the infrared (IR), the TRGB apparent magnitude
ranges from $1-2$ magnitudes brighter than in the optical, and now with the IR
James Webb Space Telescope ($JWST$) observatory the feasible distance range of
the TRGB method can be extended to $\sim50$ Mpc. However, in the IR the TRGB
luminosity depends to varying degrees on stellar metallicity and age. In this
study we standardize the TRGB luminosity using stellar colors as a proxy for
metallicity/age to derive color-based corrections for the $JWST$ Near-Infrared
Camera (NIRCam) short wavelength (SW) filters $F090W$, $F115W$, $F150W$ and the
long wavelength (LW) filters $F277W$, $F356W,$ and $F444W$. We provide
recommended filter combinations for distance measurements depending on the
requisite precision. For science requiring high precision ($\leq1\%$ in
distance) and robustness we recommend measuring the TRGB in $F090W$ vs
$F090W-F150W$ or $F115W$ vs. $F115W-F277W$ with the caveat that even with
$JWST$ long integration times will be necessary at further distances. If lower
precision ($>1.5\%$ in distance) can be tolerated, or if shorter integration
times are desirable, we recommend measuring the TRGB in either $F115W$ or
$F150W$ paired with $F356W$. We do not recommend $F444W$ for precision TRGB
measurements due to its lower angular resolution.
