Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies:
  Supplemental Material
  This is the Supplemental Material to Kormendy and Ho 2013, ARAA, 51, 511
(arXiv:1304.7762). Section S1 summarizes indirect methods that are used to
estimate black hole (BH) masses for galaxies with active nuclei (AGNs). Section
S2 lists the observational criteria that are used to classify classical and
pseudo bulges. The (pseudo)bulge classifications used in the main paper are not
based on physical interpretation; rather, they are based on these observational
criteria. Section S3 supplements the BH database in Section 5 of the main paper
and Section S4 here. It discusses corrections to galaxy and BH parameters, most
importantly to 2MASS K-band apparent magnitudes. It presents evidence that
corrections are needed because 2MASS misses light at large radii when the
images of galaxies subtend large angles on the sky or have shallow outer
brightness gradients. Section S4 reproduces essentially verbatim the first part
of Section 5 in the main paper, the BH database. It includes the list of BH and
host-galaxy properties (Tables 2 and 3). Its most important purpose is to
provide all of the notes on individual objects.
