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            • Gemini as the Ultimate Time Domain Follow-up Machine: Understanding the Nearest Cosmic Explosions
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            • A MAROON-X radial velocity search for planets around the nearest stars
            • A Spectroscopically Complete Census of Faint Transients Observed by the Young Supernova Experiment
            • 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
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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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2014A Phase I Tool update available

Submitted by bmiller on February 3, 2014
  • Read more about 2014A Phase I Tool update available
A new 2014A Phase I Tool (PIT 2014A-SV 2014.1.2) has been released to support 2014A poor weather, director's time, and GPI early science proposals. Changes are described in the PIT Hot News.

Gemini North Unavailable Until January 24, 2014

Submitted by xzhang on December 31, 2013
  • Read more about Gemini North Unavailable Until January 24, 2014

The Gemini North enclosure (left) shown with the crane used for the recent installation of the service platform. This platform will be necessary to make repairs to the failed shutter bearing. Inset shows a closeup of the shutter bearing assembly with the skewed assembly (aqua, at bottom).

Announcement of Opportunity for Large and Long Programs

Submitted by smargheim on December 4, 2013
  • Read more about Announcement of Opportunity for Large and Long Programs

Gemini Observatory announces an opportunity for Large and Long Programs. Eligible PIs are invited to propose scientific investigations to begin observation in the 2014B semester. Letters of Intent are due February 3 2014, and completed proposals are due March 31 2014.  Details and requirements are available in the Announcement of Opportunity.

New version of the Gemini IRAF package released (v1.12)

Submitted by kchiboucas on October 14, 2013
  • Read more about New version of the Gemini IRAF package released (v1.12)
A new version of the Gemini IRAF package (v1.12) has been released. This version is required for processing GSAOI and FLAMINGOS-2 data and includes configuration files and examples. Please see the processing software page for more information.

2013B Observing Tool update available

Submitted by bmiller on September 13, 2013
  • Read more about 2013B Observing Tool update available
A new Observing Tool (OT 2013B.1.2.2) is available via download or the OT auto-update feature. This is a recommended updated, especially for FLAMINGOS-2 PIs. Changes are described in the Release Notes.

2014A Call for Proposals Announced

Submitted by smargheim on August 30, 2013
  • Read more about 2014A Call for Proposals Announced

Gemini is now accepting proposals for observing time in Semester 2014A. The submission deadline varies with partner and ranges from THURSDAY SEPTEMBER 26 TO WEDNESDAY OCTOBER 2 2013. A new version of the Phase I Tool (PIT) has been released to support proposal submissions.

Information about Gemini's next new instrument project

Submitted by admin on August 23, 2013
  • Read more about Information about Gemini's next new instrument project

Read more here:
http://staff.gemini.edu/g43/2013/08/22/geminis-next-new-instrument/

Update on the Gemini High-resolution Optical Spectrograph (GHOS)

Submitted by jpollard on August 20, 2013
  • Read more about Update on the Gemini High-resolution Optical Spectrograph (GHOS)
Gemini has been negotiating with the Australian Astronomical Observatory (AAO) for the continued design and construction of the Gemini High-resolution Optical Spectroraph (GHOS).  The AAO has, in turn, been negotiating with KiwiStar, a subcontractor working on the GHOS spectrograph.  Late in July, the Board of KiwiStar's parent company, Callaghan Innovation, met to review and hopefully approve the final contract so GHOS could get underway.

Gemini Planet Imager (GPI): Cleared for Shipment to Gemini South!

Submitted by jpollard on July 19, 2013
  • Read more about Gemini Planet Imager (GPI): Cleared for Shipment to Gemini South!

In a milestone statement distributed moments ago by the GPI Pre-delivery Acceptance Review Committee, Chair Stephen Goodsell announced that GPI is now clear for shipment from the University of California Santa Cruz to Gemini South in Chile.The Committee’s final report is slated for release on July 26th, but a statement sumarizing the results of the review is available now - GPI Review Committee: Final Day Statement  41 KB

 

2013B Programs and Schedule Announced

Submitted by sleggett on June 17, 2013
  • Read more about 2013B Programs and Schedule Announced

The Gemini 2013B observing programs have now been announced. Successful PIs will receive email notification on June 17 2013. Please check the schedules page for more information. Note that the new Observing Tool must be used to access and update 13B programs.

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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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