  We present observations of HDCO and H2CO emission toward a sample of 15 Class
0 protostars in the Orion A and B clouds. Of these, eleven protostars are
Herschel-identified PACS Bright Red Sources (PBRS) and four are previously
identified protostars. Our observations revealed the chemical properties of the
PBRS envelope for the first time. The column densities of HDCO and H2CO are
derived from single dish observations at an angular resolution of ~20 arcsec
(~8400 AU). The degree of deuteration in H2CO ([HDCO]/[H2CO]) was estimated to
range from 0.03 to 0.31. The deuterium fractionation of most PBRS (70%) is
similar to that of the non-PBRS sources. Three PBRS (30%) exhibit high
deuterium fractionation, larger than 0.15. The large variation of the deuterium
fractionation of H2CO in the whole PBRS sample may reflect the diversity in the
initial conditions of star forming cores. There is no clear correlation between
the [HDCO]/[H2CO] ratio and the evolutionary sequence of protostars.
