@book{FLOUD:1990:HHAHNS,
   AUTHOR = {Floud, Roderick and Wachter, Kenneth and Gregory, Annabel},
    TITLE = {Height, Health, and History: Nutritional Status in the United
             Kingdom, 1750-1980},
     YEAR = {1990},
PUBLISHER = {Cambridge University Press},
  ADDRESS = {Cambridge, UK},
     ISBN = {0521029988, 9780521029988},
    PAGES = {378},
      URL = {http://www.cambridge.org/catalogue/catalogue.asp?isbn=0521029988},
  EDNOTES = {<bookdetails>ISBNs appear to correspond to 2006 edition},
   }

        

@proceedings{WACHTER:1990:TFOM,
    TITLE = {The Future of Meta-Analysis},
     ISBN = {0871548909, 9780871548900},
   EDITOR = {Wachter, Kenneth W. and Straf, Miron L.},
     YEAR = {1990},
PUBLISHER = {Russel Sage Foundation},
  ADDRESS = {New York, NY},
    PAGES = {210},
     NOTE = {Workshop on the Future of Meta-Analysis, convened in October 1986
             by the Committee on National Statistics (CNSTAT) of the National
             Research Council},
   }

        

@article{NAJITA:1990:DOBAEG,
   AUTHOR = {Najita, Joan and Silk, Joseph and Wachter, K.W.},
    TITLE = {Dust obscuration by an evolving galaxy population},
  JOURNAL = {The Astrophysical Journal},
   VOLUME = {348},
     YEAR = {1990},
    PAGES = {383--397},
       ID = {info:doi/10.1086/168248},
 ABSTRACT = {The effect of an evolving luminosity function (LF) on the ability
             of foreground galaxies to obscure background sources is discussed,
             using the Press--Schechter/CDM standard evolving LF model. Galaxies
             are modeled as simplified versions of local spirals and Poisson
             statistics are used to estimate the fraction of sky covered by
             intervening dusty galaxies and the mean optical depths due to these
             galaxies. The results are compared to those obtained in the case of
             nonevolving luminosity function in a low-density universe. It is
             found that evolution of the galaxy LF does not allow the quasar
             dust obscuration hypothesis to be sustained for dust disks with
             plausible sizes. Even in a low-density universe, where evolution at
             $z =$ less than 10 is unimportant, large disk radii are needed to
             achieve the desired obscuring effect. The mean fraction of sky
             covered is presented as a function of the redshift z along with
             adequate diagram illustrations.},
   }