Re: Halo: Reach Full Movie Download In Italian Hd
Rubie Mccloughan
A staircase with unusually high steps leads to a terrace separated from the rest of the roof by a low wall. I take off my shoes and step over. I slowly reach the center, moving cautiously, afraid the roof might collapse under my weight. The summer light reflecting on the white paint of the house is so strong that I have to put on my sunglasses.
The new strategic plan includes two new missions for high energy astrophysics: the Gamma Ray Large Area Space Telescope (GLAST; -glast.stanford.edu), a high energy gamma-ray mission devoted to following up the discoveries of EGRET, and the Constellation X-ray Mission (formerly the High Throughput X-ray Spectroscopy mission; ( ), a broad-band high-throughput x-ray astronomy mission for high resolution spectroscopy. However, while these missions may be in the strategic plan, they are not in the NASA budget. It will take all our ingenuity and a formidable effort in public outreach over the next two years to capture the imagination of the decision makers at NASA, the Office of Management and Budget (OMB), and Congress.
An important part of this outreach effort is the public appearance of our science results in the press. The newspaper and television stories that came out of the Estes Park HEAD meeting were gratifying. We would like particularly to applaud Lynn Cominsky for her extraordinary efforts as HEAD press officer. If you have a scientific result from a NASA program, we encourage you to consider a press release from your home institution and, perhaps, NASA. In the near future, we plan to distribute a quick primer on bringing your results to the attention of the media. In the mean time, we suggest you start by contacting the public affairs office at your home institution and the relevant NASA project or program scientist for your research. You may also contact Paul Hertz at NASA headquarters (paul....@hq.nasa.gov).
The Constellation-X is currently in a pre-Phase A study and NASA's Goddard Space Flight Center (GSFC) is directing the study effort. The Constellation-X program office, part of GSFC's Mission Development Office, is responsible for the development of the mission including feasibility and architecture studies, technology development and out reach. The Smithsonian Astrophysical Observatory is a key partner with GSFC in the development of the Constellation X-ray Mission.
Interest by the media in the results presented at the recent HEAD meeting in Estes Park, CO reached new heights this year. We featured two stories - the discovery of a gamma-ray halo at energies greater than 1 GeV using the EGRET experiment on board CGRO, and evidence for relativistic "frame dragging" in timing data from both neutron stars and black hole candidates using the RXTE. The first media event was held on Tuesday, November 4, and featured David Dixon (UC Riverside), Don Kniffen (Hampden-Sydney College and GSFC) and Dieter Hartmann (Clemson University). Dixon's images of the halo and the press release can be found at The story was covered in a front page article in the Los Angeles Times, the Boston Globe, CNN on line, BBC radio, Science News and many other outlets through the AP wire service. Stories are still expected in at least Discover and Sky and Telescope magazines.
My thanks to all the participants in the press conferences, to the press officers at UC Riverside and MIT, and to the support staff from the Conference Connection and Eureka who made it all possible. Please bring any future press-worthy results to my attention for either HEAD meetings, or for AAS meetings, as I will be assisting the AAS press officer (Steve Maran) in getting the word out about exciting high-energy results. I can help you in writing press releases, as well as in communicating your results to interested people at NASA Headquarters (such as Guenter Riegler, see the earlier article.) It is easiest to reach me through e-mail to: ly...@charmian.sonoma.edu.
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