Explore the Galaxy of images with Cloud Vision API
To recap, Cloud Vision API is an image analysis service that's part of Cloud Platform. It enables you to understand the content of images by encapsulating powerful machine learning models in an easy-to-use REST API. It quickly classifies images into thousands of categories, detects individual objects and faces within images, and finds and reads printed words contained within images. It can analyze images uploaded on request or integrate with your image storage on Google Cloud Storage. The Label detection feature costs $2 per 1,000 images, and other features cost $0.60 per 1,000 images (see pricing). Anyone can start using the API for free for 1,000 images per month.
Discover the Galaxy with Cloud Vision API and ExplorerWhen you access the demo and after clicking on the launch button, you'll discover the "Galaxy" on your Google Chrome (latest version required).
The Galaxy contains approximately 20-25 groups of images whose names (e.g., "Sea," "Snow" and "Vehicle") try to reflect accurately the content of its images.
When you scroll up in a group, you can see thousands of thumbnails of the images surrounding you.
If you click on one thumbnail, you'll see on the right side what Google's machine intelligence system has detected. In the case of the cat image available below, the system is confident that it's seeing “Cat,” “Pet” and “British shorthair” with respective confidence levels of 99%, 99% and 93%.
Using Vision API to get insight from thousands of imagesWhere do the images in Explorer come from? The 80,984 images we used are taken from the Wikimedia Commons, one of the largest repositories of freely usable media. The Commons currently holds more than 650,000 uncategorized images. However, the absence of image description makes it difficult to locate and use these images. This is where Google Cloud Vision API comes into play. This broad, unordered and disparate set of images is a great dataset to demonstrate Vision APIs capabilities.
The mechanics behind GalaxyOne of the challenges in building the demo was to create the Galaxy. This challenge consisted in finding suitable mapping between the output of the Vision API and a 3D space in which each data point represents one single image and belongs to a specific group, called a cluster. Inside this cloud of points, we expect similar images such as “cat” and “dog” to be closer, in comparison to other images such as “vehicle” or “playground.”
One idea is to define a vector representation of every image based on their labels and scores, and apply a dimensionality reduction to shrink the representations of the images into a 3D space. This vector representation consists of a high dimensional vectorization (i.e., usually more than 200 dimensions) of the labels “cat,” “dog,” etc, resulting from a word2vec dictionary called GloVe. The resulting vector for each image is a linear combination of the label word2vec vectors by the corresponding scores.
We now have as many vectors as we have images. In order to visualise this high-dimensional dataset, we used a dimensionality reduction technique called t-Distributed Stochastic Neighbor Embedding (t-SNE). This algorithm transforms each image vector into a 3D vector (x, y, z).
Once the reduction has been performed, we want to detect any clusters (related to the categories: “person,” “chair,” “car” . . .) of the 3D points. To do that, we run a simple K-means algorithm with the Euclidean distance. Each cluster is associated with a color. It's also easy to detect the name of each cluster by taking the most common label among its points.
Jeff Dean’s keynote speech showed that the combination of Cloud Vision API with dimensionality reduction and cluster analysis techniques works effectively to visualize the organization of thousands of images. This approach could be applied for various use cases to build a 3D catalog of an image repository, such as an interactive media explorer for photo libraries, for individuals and professionals. We can’t wait to see how you put it to use in your world.