  E+A galaxies have been interpreted as post-starburst galaxies based on the
presence of strong Balmer absorption lines combined with the absence of major
emission lines ([OII] nor H$\alpha$). As a population of galaxies in the midst
of the transformation, E+A galaxies has been subject to an intense research
activity. It has been, however, difficult to investigate E+A galaxies
statistically since E+A galaxies are an extremely rare population of galaxies
($<$1% of all galaxies in the local Universe).
  Here, we present a large catalog of 564 E+A (post-starburst) galaxies
carefully selected from half million spectra of the Sloan Digital Sky Survey
Data Release 5. We define E+A galaxies as those with H$\delta$ equivalent width
$>$5\AA and no detectable emission in [OII] $and$ H$\alpha$. The catalog
contains 564 E+A galaxies, and thus, is one of the largest of the kind to date.
In addition, we have included the H$\alpha$ line in the selection to remove
dusty star-forming galaxies, which could have contaminated previous [OII]-based
samples of E+A galaxies up to 52%. Thus, the catalog is one of the most
homogeneous, let alone its size. The catalog presented here can be used for
follow-up observations and statistical analyses of this rare population of
galaxies.
