NASA Exoplanet Science Institute Headlines
Announcing the NASA Exoplanet Science Institute
The Michelson Science Center has been renamed the NASA Exoplanet Science Institute (NExScI). NExScI is the science operations and analysis center for NASA's Exoplanet Exploration Program and will continue to support all MSC activities including tools and archives for the exoplanet community, the Sagan program of fellowships and workshops, support of the Keck Interferometer and administration of the NASA Keck telescope time.
Complete agenda with speaker names, participant list, and on-line registration now available! The 2009 Sagan Summer Workshop will be held July 20-24, 2009 at Caltech. It will consist of a series of tutorial discussions covering theory and observations of exoplanetary atmospheres including what we can learn from the planets in our own solar system.
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NExScI announces the release of version 2.0 of the
Visibility Modeling Tool (VMT 2.0). It can be downloaded as a Java executable, or run via a web applet. The VMT 2.0 offers three main new capabilities:
1. Performs visibility predictions for arbitrary brightness maps,
uploaded by the user as FITS images.
2. Of special interest to Keck Interferometer users: Performs a
detailed calculation of the KI Nuller response.
3. Allows users to overplot real or simulated interferometer data,
uploaded by the user in the OI-FITS format (IAU standard).
The 2008-2009
IPAC Newsletter is available with news of NExScI and the wider world of IPAC.
NExScI staff scientist
Solange Ramírez and her collaborators have found young stellar objects in the center of our galaxy. The objects are embedded in cocoons of gas and dust, which will eventually flatten to disks that, according to theory, later lump together to form planets.
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NExScI is pleased to introduce the
inaugural class of Sagan Postdoctoral Fellows! The call for the 2010 Fellowships is expected to go out in late summer 2009. Please see the
call for 2009 Sagan Postdoctoral Fellowships for more information.
On-line proposal submission for NASA's portion of the 2010A Keck time will be available in August. Proposals will be due September 16, 2009 at 4 p.m. PST. NASA has opened up the call to a wider range of disciplines. In addition, a portion of the time will be devoted to CoRoT Key Science projects.
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The
NASA Star and Exoplanet Database (NStED) is a stellar and exoplanet archive to support NASA's planet finding and characterization activities. This version significantly improves on the stellar and exoplanet content, allowing detailed searches on 70+ parameters for over 140,000 bright, nearby stars, including all known exoplanet-hosting stars. For more details, see the
NStED page.
KOA serves raw and extracted data products from the High Resolution Echelle Spectrograph (HIRES), with both PI and public access portals. KOA is a collaboration between NASA, NExScI, and the W. M. Keck Observatory.
The Space Interferometer Mission (SIM) and NExScI selected
19 science teams to conduct concept studies to maximize the science return from SIM. These teams met at a
workshop Sept. 24 & 25, 2008 in Pasadena. In addition,
four Astrometry Analysis teams were selected to participate in a demonstration of SIM's astrometric analysis of multiple-planet exoplanet systems.