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This paper bundles 40 contributions by the IceCube collaboration that weresubmitted to the 30th International Cosmic Ray Conference ICRC 2007. Thearticles cover studies on cosmic rays and atmospheric neutrinos, searches fornon-localized, extraterrestrial electron, muon and tau neutrino signals, scansfor steady and intermittent neutrino point sources, searches for dark mattercandidates, magnetic monopoles and other exotic particles, improvements inanalysis techniques, as well as future detector extensions.  The IceCube observatory will be finalized in 2011 to form a cubic-kilometerice-Cherenkov detector at the location of the geographic South Pole. At thepresent state of construction, IceCube consists of 52 paired IceTop surfacetanks and 22 IceCube strings with a total of 1426 Digital Optical Modulesdeployed at depths up to 2350 m. The observatory also integrates the 19 stringAMANDA subdetector, that was completed in 2000 and extends IceCube's reach tolower energies. Before the deployment of IceTop, cosmic air showers wereregistered with the 30 station SPASE-2 surface array.  IceCube's low noise Digital Optical Modules are very reliable, show a uniformresponse and record waveforms of arriving photons that are resolvable withnanosecond precision over a large dynamic range. Data acquisition,reconstruction and simulation software are running in production mode and theanalyses, profiting from the improved data quality and increased overallsensitivity, are well under way.

The IceCube Collaboration: contributions to the 30th International Cosmic Ray Conference (ICRC 2007)