Haleakalā Telescope Images Create World’s Largest Digital Sky SurveyDecember 19, 2016, 7:21 AM HST · Updated December 19, 7:52 AM 0 Comments
The Pan-STARRS project at the University of Hawaii Institute for Astronomy is publicly releasing the world’s largest digital sky survey today compiled using the 1.8 meter telescope atop the summit of Haleakalā on Maui.
In May 2010, it embarked on the survey, the first of its kind to observe the entire sky visible from Hawaii multiple times in many colors of light. The goal was to find moving, transient, and variable objects, including asteroids that could potentially threaten the Earth.
Observatory Director Dr. Ken Chambers says that with the release of the surveys, he expects that scientists, students and even casual users around the world will make many new discoveries about the universe from the wealth of data collected.
“The Pan-STARRS1 Surveys allow anyone to access millions of images and use the database and catalogs containing precision measurements of billions of stars and galaxies,” said Dr. Chambers. “Pan-STARRS has made discoveries from Near Earth Objects and Kuiper Belt Objects in the Solar System to lonely planets between the stars; it has mapped the dust in three dimensions in our galaxy and found new streams of stars; and it has found new kinds of exploding stars and distant quasars in the early universe.”
The catalog contains millions of images compiled over four years and a database of billions of stars and galaxies and is being released via the Space Telescope Science Institute (STScI) in Baltimore, Maryland.
The immense collection contains 2 petabytes of data, which is equivalent to one billion selfies, or one hundred times the total content of Wikipedia.
“Achieving the high quality of the Pan-STARRS1 measurements and maintaining it over such an enormous quantity of data was a unique computational challenge and the results are a tribute to the dedicated efforts of our small team of scientists at the UH IfA and our collaborators who worked to process and calibrate the extraordinary volume of raw image data,” said Dr. Eugene Magnier, lead of the Pan-STARRS Image Processing team.
This research program was undertaken by the PS1 Science Consortium — a collaboration among 10 research institutions in four countries with support from NASA and the National Science Foundation. Consortium observations for the sky survey, mapping everything visible from Hawaiʻi, were completed in April 2014.
“It’s great to see the Pan-STARRS1 data release supported by the National Science Foundation now made available to the general astronomical community,” said Nigel Sharp, program director in NSF’s astronomical sciences division. “I am impressed by the work the team invested to make the best-calibrated and best-characterized data set they could. I eagerly anticipate the science from mining these data.”
The roll-out is being done in two stages. Today’s release is the “Static Sky,” which is the average of each of those individual epochs. For every object, there’s an average value for its position, its brightness, and its colors. In 2017, the second set of data will be released, providing a catalog that gives the information and images for each individual epoch.
“The cooperation between STScI and the Pan-STARRS team at the University of Hawaiʻi has been essential to ensuring that this initial data release is successful,” explained Dr. Marc Postman, Head of the Community Missions office at STScI, and liaison between STScI and the PS1 Consortium. “STScI was a natural partner to host the Pan-STARRS public archive given its extensive experience serving astronomy data to the international community. In advance of the release of the Pan-STARRS data, STScI staff helped perform checks of data quality, helped write archive user documentation, tested and installed the local data storage and database query system, and designed, built and deployed the web-based user interfaces to the archive system.”
The survey data resides in the Mikulski Archive for Space Telescopes, which serves as NASA’s repository for all of its optical and ultraviolet-light observations, some of which date to the early 1970s. It includes all of the observational data from such space astrophysics missions as Hubble, Kepler, GALEX, and a wide variety of other telescopes, as well as several all-sky surveys. Pan-STARRS marks the nineteenth mission to be archived in MAST.