  We present 3.6 and 4.5 um photometry for a set of 61 standard stars observed
by Spitzer's Infrared Spectrograph (IRS). The photometry was obtained with the
Infrared Array Camera (IRAC) on Spitzer in order to help tie the calibration of
IRAC and the IRS, which had been anchored to the calibration of the Multiband
Infrared Photometer for Spitzer (MIPS). The wavelength range of the IRS data
only slightly overlaps with the IRAC 4.5 um band and not at all with the 3.6 um
band. Therefore, we generated synthetic spectra from spectral templates of
stars with the same spectral types and luminosity classes as our sample stars,
normalized to the IRS data at 6-7 um, and compared those to the observed
photometry. The new IRAC observations of IRS standard stars demonstrate that
the two instruments are calibrated to within 1% of each other.
