  We summarize the detection rates at wavelengths other than optical for
\~99,000 galaxies from the Sloan Digital Sky Survey (SDSS) Data Release 1
``main'' spectroscopic sample. The analysis is based on positional
cross-correlation with source catalogs from ROSAT, 2MASS, IRAS, GB6, FIRST,
NVSS and WENSS surveys. We find that the rest-frame UV-IR broad-band galaxy
SEDs form a remarkably uniform, nearly one parameter, family. As an example,
the SDSS u and r band data, supplemented with redshift, can be used to predict
K band magnitudes measured by 2MASS with an rms scatter of only 0.2 mag; when
measurement uncertainties are taken into account, the astrophysical scatter
appears not larger than ~0.1 mag.
