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Astronomers Find Hyperactive Galaxies in the Early Universe

Even some galaxies may have been hyperactive youngsters. Looking almost 11 billion years into the past, astronomers have measured the motions of stars for the first time in a very distant galaxy. They are whirling at a speed of one million miles per hour-about twice the speed of our Sun through the Milky Way. Even stranger, the galaxies are a fraction the size of our Milky Way, and so may have evolved over billions of years into the full-grown galaxies seen around us today. Astronomers are puzzled by how galaxies like these formed. They may be what will eventually become the dense central regions of very large galaxies.

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Around The Institute

Beyond JWST:The Next Steps in UV-Optical-Near IR Astronomy

Beyond JWST
Workshop The Association of Universities for Research in Astronomy (AURA) sponsored a workshop to engage the UV/optical/Near-IR astronomy community to discuss its long-term goals for space-based astronomy and astrophysics. The meeting provided the UVOIR community an opportunity to look forward on a 25-year horizon to identify the scientific opportunities enabled by large and very large space telescopes and to outline a path forward that will form the basis for a community-led report to the 2010 Decadal Review Committee.   Read more...

2009 May Symposium: The Search for Life in the Universe

SM4

The STScI 2009 May Symposium presented discussions of the motivations and expectations for the search for life in the universe in three distance domains that each require markedly different observational approaches and speakers from multiple disciplines: detecting Life within 50 AU of Earth, detecting life within 100 pc of Earth, and detecting life beyond 100 pc from Earth. Read more...

HLA Data Release 3.0

Hubble Legacy Archive DR3.0HLA Data Release 3 Includes New NICMOS Images, ACS Grisms, WFPC2 Source Lists, and Prototype Mosaics.

The Hubble Legacy Archive (HLA) has entered its Data Release 3 (DR3) phase of operation. DR3 features several new products and interface upgrades. Highlights include: improved NICMOS single- and multi-exposure images; extracted spectra from ACS GRISM data; source lists for most WFPC2 visits; and a few prototype mosaics from multi-visit ACS data.

The HLA project is a collaboration between the Space Telescope Science Institute, the Space Telescope European Coordinating Facility, and the Canadian Astronomy Data Centre.  Read more...

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