Big Data in Astronomical scale HDF and HUDF

Scientists in general, and astronomers in particular, have been at the forefront when it comes to dealing with large amounts of data. These days, the “Big Data” community, as it is known, includes almost every scientific endeavor — and even you.

In fact, Big Data is not just about extremely large collections of information hidden in databases inside archives like the Barbara A. Mikulski Archive for Space Telescopes. Big Data includes the hidden data you carry with you all the time in now-ubiquitous smart phones: calendars, photographs, SMS messages, usage information and records of our current and past locations. As we live our lives, we leave behind us a “data exhaust” that tells something about ourselves.

Star-Forming Region LH 95 in the Large Magellanic Cloud


In late 1995, the Hubble Space Telescope took hundreds of exposures of a seemingly empty patch of sky near the constellation of Ursa Major (the Big Dipper). The Hubble Deep Field (HDF), as it is known, uncovered a mystifying collection of about 3,000 galaxies at various stages of their evolution. Most of the galaxies were faint, and from them we began to learn a story about our Universe that had not been told before.


So was the HDF unique? Were we just lucky to observe a crowded but faint patch of sky? To address this question, and determine if indeed the HDF was a “lucky shot,” in 2004  Hubble took a million-second-long exposure in a similarly “empty” patch of sky: The Hubble Ultra Deep Field (HUDF). The result was even more breathtaking. Containing an estimated 10,000 galaxies, the HUDF revealed glimpses of the first galaxies as they emerge from the so-called “dark ages” — the time shortly after the Big Bang when the first stars reheated the cold, dark universe. As with the HDF, the HUDF data was made immediately available to the community, and has spawned hundreds of publications and several follow-up observations.

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