The DArk Matter In Charge-coupled devices (DAMIC) group at the University of Washington tests and packages charge-coupled devices (CCDs) that are used to detect dark matter. The CCD pixel array collects the free electrons that originate from collisions between silicon atoms and outside particles traveling through the CCD. The signal from these electrons is then measured and a two-dimensional image is produced, showing the interaction of the outside particles with the silicon atoms. In order to "see" a dark matter interaction, the CCDs have to be isolated from non-dark matter particles that may pass through. To do this, the experiment is operated 2 km underground and surrounded with lead blocks. However, these measures are in vain if there are radioactive particulates on the packaged CCDs. Radioactive isotopes decay and produce an array of particles, which are detected. One opportunity for particulate contamination is when the CCDs are exposed to the air in the DAMIC cleanroom. Therefore, the cleanliness of the cleanroom must be measured. This is done using a sampling procedure that has been standardized by the International Standards Organization (ISO). We used particle counters to count the number of airborne particulates and then analyzed the data using the ISO classification system. From this, we now know the cleanliness of the DAMIC cleanroom. Additionally, electron microscopy is being used to characterize the particulates that land on the CCDs during the wire-bonding process.