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            • Gemini as the Ultimate Time Domain Follow-up Machine: Understanding the Nearest Cosmic Explosions
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            • Roasting Marshmallows: Disentangling Composition & Climate in Hot Jupiter Atmospheres through High-Resolution Thermal Emission Cross-Correlation Spectroscopy
            • Investigating the Activity Drivers of Small Bodies in the Centaur-to-Jupiter-Family Transition
            • Subaru Intensive Program: g-band Imaging for Science with Euclid and UNIONS
            • Exploring the Diversity of Exoplanet Atmospheres at High Spectral Resolution
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            • Validation and Characterization of Exoplanets with Gemini High-Resolution Imaging
            • Monitoring Seasonal Reversal in Uranus' Upper Atmosphere
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            • ZF2K: The First Exploration of the K-Band Window and a Complete Census of Massive Galaxies at 4 < z < 6
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Gemini Director Announcement

Submitted by admin on April 29, 2011
  • Read more about Gemini Director Announcement

AURA announced that Doug Simons, Director of the Gemini Observatory, will step down at the end of his term on May 18, 2011. The full announcement is available at http://www.aura-astronomy.org/news/news.asp?newsID=259

Conceptual Design Studies for a Gemini High-Resolution Optical Spectrograph

Submitted by nlevenson on April 6, 2011
  • Read more about Conceptual Design Studies for a Gemini High-Resolution Optical Spectrograph
Gemini has issued an announcement of opportunity for conceptual design studies of a high-resolution optical spectrograph.  Please see the complete announcement at the Federal Business Opportunities site, solicitation number N310386.

Gemini IRAF package compatibility issues

Submitted by sleggett on March 9, 2011
  • Read more about Gemini IRAF package compatibility issues

IRAF COMPATIBILITY ISSUES - FITSUTIL AND IRAF V2.15
March 9, 2011

FITSUTIL Package
The fitsutil package found on iraf.net dates from December 2010. This new version is not compatible with the current (v1.10) release of Gemini IRAF. Instead users who need to install or re-install fitsutil should obtain the file from iraf.noao.edu, http://iraf.noao.edu/iraf/ftp/iraf/extern-v214/.

2011B call for proposals announced

Submitted by sleggett on February 28, 2011
  • Read more about 2011B call for proposals announced

Gemini is now accepting proposals for observing time in Semester 2011B. The proposal deadline is March 31, 2011. A new version of the Phase I Tool (PIT) has been released to support proposal submissions.

2011B PIT released

Submitted by bmiller on February 28, 2011
  • Read more about 2011B PIT released

The Phase I Tool (PIT) for semester 2011B observing proposals has been released. Poor weather and director's time proposals during the remainder of semester 2011A must continue to use the 2011A PIT.

Gemini South 2011A Science Operations

Submitted by nlevenson on January 28, 2011
  • Read more about Gemini South 2011A Science Operations

Last week Gemini passed a major milestone with the beginning of on-sky engineering testing of the Gemini South 50-watt laser.  This event marks the start of commissioning for the Gemini Multi-Conjugate Adaptive Optics System (GeMS).  The plans through the first half of 2011 are intense, with commissioning runs scheduled to occur in one-week blocks from February to May of 2011A, as shown on the Gemini South telescope schedule.

2011A Programs and Schedule Announced

Submitted by sleggett on December 13, 2010
  • Read more about 2011A Programs and Schedule Announced

The Gemini 2011A observing programs have now been announced. Successful PIs will have received email notification. Please check the schedules page for more information.

GPI Call for Letters of Intent for Campaign Science Proposals Announced

Submitted by sleggett on December 9, 2010
  • Read more about GPI Call for Letters of Intent for Campaign Science Proposals Announced

The Gemini Observatory plans to announce a Call for Proposals for Gemini Planet Imager (GPI) Campaign Science. We now request letters of intent from prospective GPI campaign projects.

2011A Observing Tool Released

Submitted by astephens on December 2, 2010
  • Read more about 2011A Observing Tool Released
The Gemini 2011A Observing Tool (OT) is now available for download or via updating an existing installation of the OT. This version is required for 2011A Phase II preparation as well as for fetch/store of any programs in the observing databases.

Phoenix to be removed in January 2011

Submitted by brodgers on November 25, 2010
  • Read more about Phoenix to be removed in January 2011

Phoenix has been a visitor instrument on Gemini South since the beginning of science operations in 2002.  It has been scientifically productive, with an active user community, and the observatory is grateful to NOAO for the long-term loan. However, Gemini is about to commission new Gemini South instrumentation and is actively engaged in a transition to operations without the UK as a partner.  Together, these fundamentally limit both available staff effort and instrument ports, and Gemini can no longer afford to offer Phoenix for regular use.

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International Gemini Observatory

The International Gemini Observatory  provides the astronomical communities in six participant countries with state-of-the-art astronomical facilities that allocate observing time in proportion to each country's contribution. In addition to financial support, each country also contributes significant scientific and technical resources. The national research agencies that form the Gemini partnership include: the US National Science Foundation (NSF), the Canadian National Research Council (NRC), the Chilean Agencia Nacional de Investigación y Desarrollo (ANID), the Brazilian Ministério da Ciência, Tecnologia e Inovação, the Argentinean Ministerio de Ciencia, Tecnología e Innovación, and the Korea Astronomy and Space Institute (KASI). The observatory is managed by the Association of Universities for Research in Astronomy, Inc. (AURA) under a cooperative agreement with the NSF. The NSF also serves as the executive agency for the international partnership.     


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