Kinematic signatures of reverberation mapping of close binaries of
  supermassive black holes in active galactic nuclei. II. Atlas of
  two-dimensional transfer functions
  Most large galaxies harbor supermassive black holes (SMBHs) in their centers,
and galaxies merge. Consequently, binary SMBHs should be common in galactic
nuclei. However, close binaries of SMBH (CB-SMBHs) with sub-parsec separation
cannot be imaged directly using current facilities. Some indirect signatures,
such as periodic signals in light curves and double peaks in emission-line
profile, have been used to find CB-SMBH candidates, but ambiguities still exist
and no definitive conclusions can be made. We have recently proposed a new
method focusing on kinematic signatures that can be derived from reverberation
mapping of CB-SMBHs, one that offers a promising avenue to address this
important problem. In this paper, we calculated models for a wide range of
parameters, but BLRs of two BHs are close but still not merged. The purpose of
this supplementary paper is to provide an atlas of two-dimensional transfer
functions of CB-SMBHs with a wide range of orbital and geometrical parameters
to aid more efficient identification of CB-SMBH candidates in reverberation
mapping data.
