SDSS Galaxy Survey
Key to modern extragalactic surveys is to measure the redshift of the object, via spectral means. By redshift we mean the increase in the wavelength of the electromagnetic radiation (i.e. the light) received by a detector compared with the wavelength emitted by the source, e.g. if the source is moving away from us then the wave will be stretched, if coming towards us it will be compressed. Any increase in wavelength is called “redshift”, even if it occurs in electromagnetic radiation of non-optical wavelengths, such as gamma-rays.
Redshifts surveys in the 1980s and the 1990s (e.g., the CfA, IRAS, and Las campanas surveys) measured thousands to tens of thousands galaxy redshifts. Multifibre technology now allows us to measure redshifts of millions of galaxies. One of these such surveys uses data obtained with the Sloan Digital Sky Survey (SDSS). The SDSS is a U.S.-Japan-Germany joint project to image a quarter of the Celestial Sphere at high Galactic latitude as well as to obtain spectra of galaxies and quasars from the imaging data. The dedicated 2.5 meter telescope at Apache Point Observatory. Recently they have released the most detailed survey ever completed (with the release of DR7) - anyone can navigate around the Universe with their navigation tool - so go and give it a go! Oh and here is what the Universe looks like from the SDSS….

The SDSS has made detailed 3D maps of relatively nearby galaxies. The Earth is at the centre of these wedges, and each point represents a galaxy, with the outer circle at a distance of 2 billion light years. The region between the wedges was not mapped by the SDSS because dust in our own galaxy obscures the view of the distant universe in these directions (Illustration: M Blanton/ SDSS)