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Ground Layer Turbulence Monitoring on the Mauna Kea Summit Ridge
Issued: 24 August 2005
Requests for RFP Due: 9 September 2005
The Board of Directors has adopted a resolution that addresses the next steps in the process to design and deploy some of the major instruments that emerged from the multi-year process of discussions. This has been a stimulating process, with the initial phase culminating in the report Scientific Horizons at the Gemini Observatory: Exploring a Universe of Matter, Energy, and Life, which is available here on the Gemini website.
For Immediate Release
August 10, 2005
July 29, 2005
Figure 1: Artist's conception of how 2003 UB313 might look from space
Following the recent announcement from NOAO regarding upcoming changes in the level and type of support for IRAF, we wish to reassure our user community that we will continue to fully support and develop our data reduction package. Further, we are taking steps towards improving our support and development effort. Also, over the last few months, we have been exploring the feasibility of a transition to PyRAF and Python.
Gemini will make every effort to minimize the impact this new NOAO direction could have on our users.
Imaging by Gemini North's Michelle mid-infrared imager/spectrograph has allowed an international team of researchers to isolate and characterize the dusty remains of the supernova remnant SN 2002hh some 20 million light-years away. Led by UK astronomer Michael Barlow (University College London), the team imaged SN 2002hh in the relatively nearby galaxy NGC 6946 to study the dust expelled (and/or created) during the supernova explosion.