Determination of the Cosmic Infrared Background from COBE/FIRAS and
  Planck HFI Observations
  New determinations are presented of the cosmic infrared background monopole
brightness in the Planck HFI bands from 100 GHz to 857 GHz. Planck was not
designed to measure the monopole component of sky brightness, so
cross-correlation of the 2015 HFI maps with COBE/FIRAS data is used to
recalibrate the zero level of the HFI maps. For the HFI 545 and 857 GHz maps,
the brightness scale is also recalibrated. Correlation of the recalibrated HFI
maps with a linear combination of Galactic H I and H alpha data is used to
separate the Galactic foreground emission and determine the cosmic infrared
background brightness in each of the HFI bands. We obtain CIB values of 0.007
+- 0.014, 0.010 +- 0.019, 0.060 +- 0.023, 0.149 +- 0.017, 0.371 +- 0.018, and
0.576 +- 0.034 MJy/sr at 100, 143, 217, 353, 545, and 857 GHz, respectively.
The estimated uncertainties for the 353 to 857 GHz bands are about 3 to 6 times
smaller than those of previous direct CIB determinations at these frequencies.
Our results are compared with integrated source brightness results from
selected recent submillimeter and millimeter wavelength imaging surveys.
